Sample records for air temperature wind

  1. Impacts of wind farms on surface air temperatures

    PubMed Central

    Baidya Roy, Somnath; Traiteur, Justin J.

    2010-01-01

    Utility-scale large wind farms are rapidly growing in size and numbers all over the world. Data from a meteorological field campaign show that such wind farms can significantly affect near-surface air temperatures. These effects result from enhanced vertical mixing due to turbulence generated by wind turbine rotors. The impacts of wind farms on local weather can be minimized by changing rotor design or by siting wind farms in regions with high natural turbulence. Using a 25-y-long climate dataset, we identified such regions in the world. Many of these regions, such as the Midwest and Great Plains in the United States, are also rich in wind resources, making them ideal candidates for low-impact wind farms. PMID:20921371

  2. Metabolic response to air temperature and wind in day-old mallards and a standard operative temperature scale

    USGS Publications Warehouse

    Bakken, G.S.; Reynolds, P.S.; Kenow, K.P.; Korschgen, C.E.; Boysen, A.F.

    1999-01-01

    Most duckling mortality occurs during the week following hatching and is often associated with cold, windy, wet weather and scattering of the brood. We estimated the thermoregulatory demands imposed by cold, windy weather on isolated 1-d-old mallard (Anas platyrhynchos) ducklings resting in cover. We measured O-2 consumption and evaporative water loss at air temperatures from 5 degrees to 25 degrees C and wind speeds of 0.1, 0.2, 0.5, and 1.0 mis. Metabolic heat production increased as wind increased or temperature decreased but was less sensitive to wind than that of either adult passerines or small mammals. Evaporative heat loss ranged from 5% to 17% of heat production. Evaporative heal loss and the ratio of evaporative heat loss to metabolic heat production was significantly lower in rest phase. These data were used to define a standard operative temperature (T-es) scale for night or heavy overcast conditions. An increase of wind speed from 0.1 to 1 mis decreased T-es by 3 degrees-5 degrees C.

  3. A note on the correlation between circular and linear variables with an application to wind direction and air temperature data in a Mediterranean climate

    NASA Astrophysics Data System (ADS)

    Lototzis, M.; Papadopoulos, G. K.; Droulia, F.; Tseliou, A.; Tsiros, I. X.

    2018-04-01

    There are several cases where a circular variable is associated with a linear one. A typical example is wind direction that is often associated with linear quantities such as air temperature and air humidity. The analysis of a statistical relationship of this kind can be tested by the use of parametric and non-parametric methods, each of which has its own advantages and drawbacks. This work deals with correlation analysis using both the parametric and the non-parametric procedure on a small set of meteorological data of air temperature and wind direction during a summer period in a Mediterranean climate. Correlations were examined between hourly, daily and maximum-prevailing values, under typical and non-typical meteorological conditions. Both tests indicated a strong correlation between mean hourly wind directions and mean hourly air temperature, whereas mean daily wind direction and mean daily air temperature do not seem to be correlated. In some cases, however, the two procedures were found to give quite dissimilar levels of significance on the rejection or not of the null hypothesis of no correlation. The simple statistical analysis presented in this study, appropriately extended in large sets of meteorological data, may be a useful tool for estimating effects of wind on local climate studies.

  4. High-resolution daily gridded datasets of air temperature and wind speed for Europe

    NASA Astrophysics Data System (ADS)

    Brinckmann, S.; Krähenmann, S.; Bissolli, P.

    2015-08-01

    New high-resolution datasets for near surface daily air temperature (minimum, maximum and mean) and daily mean wind speed for Europe (the CORDEX domain) are provided for the period 2001-2010 for the purpose of regional model validation in the framework of DecReg, a sub-project of the German MiKlip project, which aims to develop decadal climate predictions. The main input data sources are hourly SYNOP observations, partly supplemented by station data from the ECA&D dataset (http://www.ecad.eu). These data are quality tested to eliminate erroneous data and various kinds of inhomogeneities. Grids in a resolution of 0.044° (5 km) are derived by spatial interpolation of these station data into the CORDEX area. For temperature interpolation a modified version of a regression kriging method developed by Krähenmann et al. (2011) is used. At first, predictor fields of altitude, continentality and zonal mean temperature are chosen for a regression applied to monthly station data. The residuals of the monthly regression and the deviations of the daily data from the monthly averages are interpolated using simple kriging in a second and third step. For wind speed a new method based on the concept used for temperature was developed, involving predictor fields of exposure, roughness length, coastal distance and ERA Interim reanalysis wind speed at 850 hPa. Interpolation uncertainty is estimated by means of the kriging variance and regression uncertainties. Furthermore, to assess the quality of the final daily grid data, cross validation is performed. Explained variance ranges from 70 to 90 % for monthly temperature and from 50 to 60 % for monthly wind speed. The resulting RMSE for the final daily grid data amounts to 1-2 °C and 1-1.5 m s-1 (depending on season and parameter) for daily temperature parameters and daily mean wind speed, respectively. The datasets presented in this article are published at http://dx.doi.org/10.5676/DWD_CDC/DECREG0110v1.

  5. Controlled-Temperature Hot-Air Gun

    NASA Technical Reports Server (NTRS)

    Munoz, M. C.

    1986-01-01

    Materials that find applications in wind tunnels first tested in laboratory. Hot-Air Gun differs from commercial units in that flow rate and temperature monitored and controlled. With typical compressed-airsupply pressure of 25 to 38 psi (170 to 260 kPa), flow rate and maximum temperature are 34 stdft3/min (0.96 stdm3/min) and 1,090 degrees F (590 degrees C), respectively. Resembling elaborate but carefully regulated hot-air gun, setup used to apply blasts of air temperatures above 1,500 degrees F (815 degrees C) to test specimens.

  6. Hurricane Isabel, AIRS Infrared and SeaWinds Scatterometer Data Combined

    NASA Image and Video Library

    2003-09-20

    These two images show Hurricane Isabel as viewed by AIRS and SeaWinds scatterometers on NASA ADEOS-2 and QuikScat satellites in September, 2003. AIRS data are used to create global three-dimensional maps of temperature, humidity and clouds, while scatterometers measure surface wind speed and direction. http://photojournal.jpl.nasa.gov/catalog/PIA00429

  7. Evaluation of Vertically Resolved Water Winds from AIRS using Hurricane Katrina

    NASA Technical Reports Server (NTRS)

    Aumann, Hartmut H.; Dobkowski, Edwin C.; Gregorich, David T.

    2005-01-01

    The knowledge of wind velocity as a function of altitude is key to weather forecast improvements. The ability of hyperspectral sounders in principle to measure vertically resolved water winds, which has long been recognized, has been tested with Atmospheric Infrared Sounder (AIRS) data. AIRS retrievals of total column water above 300 mb have been correlated with the radiosonde upper-tropospheric wind velocity and moisture data. The excellent correlation is illustrated with results obtained from hurricane Katrina and from the western United States. AIRS is a hyperspectral infrared sounder in low Earth orbit. It was launched in May 2002. We illustrate the use of AIRS data for the measurement of upper tropospheric water by using the 2387/cm CO2 R-branch channel and the 1551/cm water vapor channel. The 2387/cm channel measures the temperature at 300 mb totally independent of water vapor. The weighting function of the 1551/cm channel peaks at 300 mb only under moist conditions; the peak shifts downward (higher temperature) for less water and upward (lower temperature) for more water. The difference between the brightness temperatures bt2387 and bt1551 cancels the local several degree weather related variability of the temperature and measures the component due to the water vapor at 300 mb.

  8. High-resolution daily gridded data sets of air temperature and wind speed for Europe

    NASA Astrophysics Data System (ADS)

    Brinckmann, Sven; Krähenmann, Stefan; Bissolli, Peter

    2016-10-01

    New high-resolution data sets for near-surface daily air temperature (minimum, maximum and mean) and daily mean wind speed for Europe (the CORDEX domain) are provided for the period 2001-2010 for the purpose of regional model validation in the framework of DecReg, a sub-project of the German MiKlip project, which aims to develop decadal climate predictions. The main input data sources are SYNOP observations, partly supplemented by station data from the ECA&D data set (http://www.ecad.eu). These data are quality tested to eliminate erroneous data. By spatial interpolation of these station observations, grid data in a resolution of 0.044° (≈ 5km) on a rotated grid with virtual North Pole at 39.25° N, 162° W are derived. For temperature interpolation a modified version of a regression kriging method developed by Krähenmann et al.(2011) is used. At first, predictor fields of altitude, continentality and zonal mean temperature are used for a regression applied to monthly station data. The residuals of the monthly regression and the deviations of the daily data from the monthly averages are interpolated using simple kriging in a second and third step. For wind speed a new method based on the concept used for temperature was developed, involving predictor fields of exposure, roughness length, coastal distance and ERA-Interim reanalysis wind speed at 850 hPa. Interpolation uncertainty is estimated by means of the kriging variance and regression uncertainties. Furthermore, to assess the quality of the final daily grid data, cross validation is performed. Variance explained by the regression ranges from 70 to 90 % for monthly temperature and from 50 to 60 % for monthly wind speed. The resulting RMSE for the final daily grid data amounts to 1-2 K and 1-1.5 ms-1 (depending on season and parameter) for daily temperature parameters

  9. Simulation of air-droplet mixed phase flow in icing wind-tunnel

    NASA Astrophysics Data System (ADS)

    Mengyao, Leng; Shinan, Chang; Menglong, Wu; Yunhang, Li

    2013-07-01

    Icing wind-tunnel is the main ground facility for the research of aircraft icing, which is different from normal wind-tunnel for its refrigeration system and spraying system. In stable section of icing wind-tunnel, the original parameters of droplets and air are different, for example, to keep the nozzles from freezing, the droplets are heated while the temperature of air is low. It means that complex mass and heat transfer as well as dynamic interactive force would happen between droplets and air, and the parameters of droplet will acutely change along the passageway. Therefore, the prediction of droplet-air mixed phase flow is necessary in the evaluation of icing researching wind-tunnel. In this paper, a simplified droplet-air mixed phase flow model based on Lagrangian method was built. The variation of temperature, diameter and velocity of droplet, as well as the air flow field, during the flow process were obtained under different condition. With calculating three-dimensional air flow field by FLUENT, the droplet could be traced and the droplet distribution could also be achieved. Furthermore, the patterns about how initial parameters affect the parameters in test section were achieved. The numerical simulation solving the flow and heat and mass transfer characteristics in the mixing process is valuable for the optimization of experimental parameters design and equipment adjustment.

  10. Sensitivity of Global Sea-Air CO2 Flux to Gas Transfer Algorithms, Climatological Wind Speeds, and Variability of Sea Surface Temperature and Salinity

    NASA Technical Reports Server (NTRS)

    McClain, Charles R.; Signorini, Sergio

    2002-01-01

    Sensitivity analyses of sea-air CO2 flux to gas transfer algorithms, climatological wind speeds, sea surface temperatures (SST) and salinity (SSS) were conducted for the global oceans and selected regional domains. Large uncertainties in the global sea-air flux estimates are identified due to different gas transfer algorithms, global climatological wind speeds, and seasonal SST and SSS data. The global sea-air flux ranges from -0.57 to -2.27 Gt/yr, depending on the combination of gas transfer algorithms and global climatological wind speeds used. Different combinations of SST and SSS global fields resulted in changes as large as 35% on the oceans global sea-air flux. An error as small as plus or minus 0.2 in SSS translates into a plus or minus 43% deviation on the mean global CO2 flux. This result emphasizes the need for highly accurate satellite SSS observations for the development of remote sensing sea-air flux algorithms.

  11. Does the recent warming hiatus exist over northern Asia for winter wind chill temperature?

    NASA Astrophysics Data System (ADS)

    Ma, Ying

    2017-04-01

    Wind chill temperature (WCT) describes the joint effect of wind velocity and air temperature on exposed body skin and could support policy makers in designing plans to reduce the risks of notably cold and windy weather. This study examined winter WCT over northern Asia during 1973-2013 by analyzing in situ station data. The winter WCT warming rate over the Tibetan Plateau slowed during 1999-2013 (-0.04 °C/decade) compared with that during 1973-1998 (0.67 °C/decade). The winter WCT warming hiatus has also been observed in the remainder of Northern Asia with trends of 1.11 °C/decade during 1973-1998 but -1.02 °C/decade during 1999-2013, except for the Far East of Russia (FE), where the winter WCT has continued to heat up during both the earlier period of 1973-1998 (0.54 °C/decade) and the recent period of 1999-2013 (0.75 °C/decade). The results indicate that the influence of temperature on winter WCT is greater than that of wind speed over northern Asia. Atmospheric circulation changes associated with air temperature and wind speed were analyzed to identify the causes for the warming hiatus of winter WCT over northern Asia. The distributions of sea level pressure and 500 hPa height anomalies during 1999-2013 transported cold air from the high latitudes to middle latitudes, resulting in low air temperature over Northern Asia except for the Far East of Russia. Over the Tibetan Plateau, the increase in wind speed offset the increase in air temperature during 1999-2013. For the Far East, the southerly wind from the Western Pacific drove the temperature up during the 1999-2013 period via warm advection.

  12. Air temperature, wind speed, and wind direction in the National Petroleum Reserve—Alaska and the Arctic National Wildlife Refuge, 1998–2011

    USGS Publications Warehouse

    Urban, Frank E.; Clow, Gary D.

    2013-01-01

    This report provides air temperature, wind speed, and wind direction data collected on Federal lands in Arctic Alaska over the period August 1998 to July 2011 by the U.S. Department of the Interior's climate monitoring array, part of the Global Terrestrial Network for Permafrost. In addition to presenting data, this report also describes monitoring, data collection, and quality control methodology. This array of 16 monitoring stations spans 68.5°N to 70.5°N and 142.5°W to 161°W, an area of roughly 150,000 square kilometers. Climate summaries are presented along with provisional quality-controlled data. Data collection is ongoing and includes several additional climate variables to be released in subsequent reports, including ground temperature and soil moisture, snow depth, rainfall, up- and downwelling shortwave radiation, and atmospheric pressure. These data were collected by the U.S. Geological Survey in close collaboration with the Bureau of Land Management and the U.S. Fish and Wildlife Service.

  13. Calculations of air cooler for new subsonic wind tunnel

    NASA Astrophysics Data System (ADS)

    Rtishcheva, A. S.

    2017-10-01

    As part of the component development of TsAGI’s new subsonic wind tunnel where the air flow velocity in the closed test section is up to 160 m/sec hydraulic and thermal characteristics of air cooler are calculated. The air cooler is one of the most important components due to its highest hydraulic resistance in the whole wind tunnel design. It is important to minimize its hydraulic resistance to ensure the energy efficiency of wind tunnel fans and the cost-cutting of tests. On the other hand the air cooler is to assure the efficient cooling of air flow in such a manner as to maintain the temperature below 40 °C for seamless operation of measuring equipment. Therefore the relevance of this project is driven by the need to develop the air cooler that would demonstrate low hydraulic resistance of air and high thermal effectiveness of heat exchanging surfaces; insofar as the cooling section must be given up per unit time with the amount of heat Q=30 MW according to preliminary evaluations. On basis of calculation research some variants of air cooler designs are proposed including elliptical tubes, round tubes, and lateral plate-like fins. These designs differ by the number of tubes and plates, geometrical characteristics and the material of finned surfaces (aluminium or cooper). Due to the choice of component configurations a high thermal effectiveness is achieved for finned surfaces. The obtained results form the basis of R&D support in designing the new subsonic wind tunnel.

  14. A large volume 2000 MPA air source for the radiatively driven hypersonic wind tunnel

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

    Constantino, M

    1999-07-14

    An ultra-high pressure air source for a hypersonic wind tunnel for fluid dynamics and combustion physics and chemistry research and development must provide a 10 kg/s pure air flow for more than 1 s at a specific enthalpy of more than 3000 kJ/kg. The nominal operating pressure and temperature condition for the air source is 2000 MPa and 900 K. A radial array of variable radial support intensifiers connected to an axial manifold provides an arbitrarily large total high pressure volume. This configuration also provides solutions to cross bore stress concentrations and the decrease in material strength with temperature. [hypersonic,more » high pressure, air, wind tunnel, ground testing]« less

  15. Thermodynamic characteristics of a novel wind-solar-liquid air energy storage system

    NASA Astrophysics Data System (ADS)

    Ji, W.; Zhou, Y.; Sun, Y.; Zhang, W.; Pan, C. Z.; Wang, J. J.

    2017-12-01

    Due to the nature of fluctuation and intermittency, the utilization of wind and solar power will bring a huge impact to the power grid management. Therefore a novel hybrid wind-solar-liquid air energy storage (WS-LAES) system was proposed. In this system, wind and solar power are stored in the form of liquid air by cryogenic liquefaction technology and thermal energy by solar thermal collector, respectively. Owing to the high density of liquid air, the system has a large storage capacity and no geographic constraints. The WS-LAES system can store unstable wind and solar power for a stable output of electric energy and hot water. Moreover, a thermodynamic analysis was carried out to investigate the best system performance. The result shows that the increases of compressor adiabatic efficiency, turbine inlet pressure and inlet temperature all have a beneficial effect.

  16. Hurricane Frances as Observed by NASA's Spaceborne Atmospheric Infrared Sounder (AIRS) and SeaWinds

    NASA Technical Reports Server (NTRS)

    2004-01-01

    This image shows Hurricane Frances as captured by instruments onboard two different satellites: the AIRS infrared instrument onboard Aqua, and the SeaWinds scatterometer onboard QuikSCAT. Both are JPL-managed instruments. AIRS data are used to create global three-dimensional maps of temperature, humidity and clouds, while scatterometers measure surface wind speed and direction over the ocean.

    The red vectors in the image show Frances' surface winds as measured by SeaWinds on QuikSCAT. The background colors show the temperature of clouds and surface as viewed in the infrared by AIRS, with cooler areas pushing to purple and warmer areas are pushing to red. The color scale on the right gives the temperatures in degrees Kelvin. (The top of the scale, 320 degrees Kelvin, corresponds to 117 degrees Fahrenheit, and the bottom, 180 degrees K is -135 degrees F.) The powerful circulation of this storm is evident from the combined data as well as the development of a clearly-defined central 'eye'. The infrared signal does not penetrate through clouds, so the light blue areas reveal the cold clouds tops associated with strong thunderstorms embedded within the storm. In cloud-free areas the infrared signal comes from Earth's surface, revealing warmer temperatures.

    The power of the SeaWinds scatterometer data set lies in its ability to generate global maps of wind speed and direction, giving us a snapshot of how the atmosphere is circulating. Weather prediction centers, including the Tropical Prediction Center - a branch of NOAA that monitors the creation of ocean-born storms, use scatterometer data to help it 'see' where these storms are brewing so that warnings can be issued and the storms, with often erratic motions, can be tracked.

    While the SeaWinds instrument isn't designed to gather hurricane data, having difficulty seeing the surface in heavy rain, it's data can be used in combination with other data sets to give us an insight into these storms. In

  17. Wind and Temperature Spectrometry of the Upper Atmosphere in Low-Earth Orbit

    NASA Technical Reports Server (NTRS)

    Herrero, Federico

    2011-01-01

    Wind and Temperature Spectrometry (WATS) is a new approach to measure the full wind vector, temperature, and relative densities of major neutral species in the Earth's thermosphere. The method uses an energy-angle spectrometer moving through the tenuous upper atmosphere to measure directly the angular and energy distributions of the air stream that enters the spectrometer. The angular distribution gives the direction of the total velocity of the air entering the spectrometer, and the energy distribution gives the magnitude of the total velocity. The wind velocity vector is uniquely determined since the measured total velocity depends on the wind vector and the orbiting velocity vector. The orbiting spectrometer moves supersonically, Mach 8 or greater, through the air and must point within a few degrees of its orbital velocity vector (the ram direction). Pointing knowledge is critical; for example, pointing errors 0.1 lead to errors of about 10 m/s in the wind. The WATS method may also be applied without modification to measure the ion-drift vector, ion temperature, and relative ion densities of major ionic species in the ionosphere. In such an application it may be called IDTS: Ion-Drift Temperature Spectrometry. A spectrometer-based coordinate system with one axis instantaneously pointing along the ram direction makes it possible to transform the Maxwellian velocity distribution of the air molecules to a Maxwellian energy-angle distribution for the molecular flux entering the spectrometer. This implementation of WATS is called the gas kinetic method (GKM) because it is applied to the case of the Maxwellian distribution. The WATS method follows from the recognition that in a supersonic platform moving at 8,000 m/s, the measurement of small wind velocities in the air on the order of a few 100 m/s and less requires precise knowledge of the angle of incidence of the neutral atoms and molecules. The same is true for the case of ion-drift measurements. WATS also

  18. Assessment of the effects of environmental radiation on wind chill equivalent temperatures.

    PubMed

    Shitzer, Avraham

    2008-09-01

    Combinations of wind-driven convection and environmental radiation in cold weather, make the environment "feel" colder. The relative contributions of these mechanisms, which form the basis for estimating wind chill equivalent temperatures (WCETs), are studied over a wide range of environmental conditions. Distinction is made between direct solar radiation and environmental radiation. Solar radiation, which is not included in the analysis, has beneficial effects, as it counters and offsets some of the effects due to wind and low air temperatures. Environmental radiation effects, which are included, have detrimental effects in enhancing heat loss from the human body, thus affecting the overall thermal sensation due to the environment. The analysis is performed by a simple, steady-state analytical model of human-environment thermal interaction using upper and lower bounds of environmental radiation heat exchange. It is shown that, over a wide range of relevant air temperatures and reported wind speeds, convection heat losses dominate over environmental radiation. At low wind speeds radiation contributes up to about 23% of the overall heat loss from exposed skin areas. Its relative contributions reduce considerably as the time of the exposure prolongs and exposed skin temperatures drop. At still higher wind speeds, environmental radiation effects become much smaller contributing about 5% of the total heat loss. These values fall well within the uncertainties associated with the parameter values assumed in the computation of WCETs. It is also shown that environmental radiation effects may be accommodated by adjusting reported wind speeds slightly above their reported values.

  19. Investigation on wind energy-compressed air power system.

    PubMed

    Jia, Guang-Zheng; Wang, Xuan-Yin; Wu, Gen-Mao

    2004-03-01

    Wind energy is a pollution free and renewable resource widely distributed over China. Aimed at protecting the environment and enlarging application of wind energy, a new approach to application of wind energy by using compressed air power to some extent instead of electricity put forward. This includes: explaining the working principles and characteristics of the wind energy-compressed air power system; discussing the compatibility of wind energy and compressor capacity; presenting the theoretical model and computational simulation of the system. The obtained compressor capacity vs wind power relationship in certain wind velocity range can be helpful in the designing of the wind power-compressed air system. Results of investigations on the application of high-pressure compressed air for pressure reduction led to conclusion that pressure reduction with expander is better than the throttle regulator in energy saving.

  20. Prediction of air temperature for thermal comfort of people in outdoor environments

    NASA Astrophysics Data System (ADS)

    Huang, Jianhua

    2007-05-01

    Current thermal comfort indices do not take into account the effects of wind and body movement on the thermal resistance and vapor resistance of clothing. This may cause public health problem, e.g. cold-related mortality. Based on the energy balance equation and heat exchanges between a clothed body and the outdoor environment, a mathematical model was developed to determine the air temperature at which an average adult, wearing a specific outdoor clothing and engaging in a given activity, attains thermal comfort under outdoor environment condition. The results indicated low clothing insulation, less physical activity and high wind speed lead to high air temperature prediction for thermal comfort. More accurate air temperature prediction is able to prevent wearers from hypothermia under cold conditions.

  1. Variability of Winter Air Temperature in Mid-Latitude Europe

    NASA Technical Reports Server (NTRS)

    Otterman, J.; Ardizzone, J.; Atlas, R.; Bungato, D.; Cierniewski, J.; Jusem, J. C.; Przybylak, R.; Schubert, S.; Starr, D.; Walczewski, J.

    2002-01-01

    The aim of this paper is to report extreme winter/early-spring air temperature (hereinafter temperature) anomalies in mid-latitude Europe, and to discuss the underlying forcing to these interannual fluctuations. Warm advection from the North Atlantic in late winter controls the surface-air temperature, as indicated by the substantial correlation between the speed of the surface southwesterlies over the eastern North Atlantic (quantified by a specific Index Ina) and the 2-meter level air temperatures (hereinafter Ts) over Europe, 45-60 deg N, in winter. In mid-March and subsequently, the correlation drops drastically (quite often it is negative). This change in the relationship between Ts and Ina marks a transition in the control of the surface-air temperature: absorption of insolation replaces the warm advection as the dominant control. This forcing by maritime-air advection in winter was demonstrated in a previous publication, and is re-examined here in conjunction with extreme fluctuations of temperatures in Europe. We analyze here the interannual variability at its extreme by comparing warm-winter/early-spring of 1989/90 with the opposite scenario in 1995/96. For these two December-to-March periods the differences in the monthly mean temperature in Warsaw and Torun, Poland, range above 10 C. Short-term (shorter than a month) fluctuations of the temperature are likewise very strong. We conduct pentad-by-pentad analysis of the surface-maximum air temperature (hereinafter Tmax), in a selected location, examining the dependence on Ina. The increased cloudiness and higher amounts of total precipitable water, corollary effects to the warm low-level advection. in the 1989/90 winter, enhance the positive temperature anomalies. The analysis of the ocean surface winds is based on the Special Sensor Microwave/Imager (SSM/I) dataset; ascent rates, and over land wind data are from the European Centre for Medium-Range Weather Forecasts (ECMWF); maps of 2-m temperature, cloud

  2. Hurricane Frances as Observed by NASA Spaceborne Atmospheric Infrared Sounder AIRS and SeaWinds Scatterometer

    NASA Image and Video Library

    2004-08-30

    This image shows Hurricane Frances in August 2004 as captured by instruments onboard two different NASA satellites: the AIRS infrared instrument onboard Aqua, and the SeaWinds scatterometer onboard QuikSCAT. Both are JPL-managed instruments. AIRS data are used to create global three-dimensional maps of temperature, humidity and clouds, while scatterometers measure surface wind speed and direction over the ocean. The red vectors in the image show Frances' surface winds as measured by SeaWinds on QuikSCAT. The background colors show the temperature of clouds and surface as viewed in the infrared by AIRS, with cooler areas pushing to purple and warmer areas are pushing to red. The color scale on the right gives the temperatures in degrees Kelvin. (The top of the scale, 320 degrees Kelvin, corresponds to 117 degrees Fahrenheit, and the bottom, 180 degrees K is -135 degrees F.) The powerful circulation of this storm is evident from the combined data as well as the development of a clearly-defined central "eye." The infrared signal does not penetrate through clouds, so the light blue areas reveal the cold clouds tops associated with strong thunderstorms embedded within the storm. In cloud-free areas the infrared signal comes from Earth's surface, revealing warmer temperatures. http://photojournal.jpl.nasa.gov/catalog/PIA00435

  3. The relationship between radiant heat, air temperature and thermal comfort at rest and exercise.

    PubMed

    Guéritée, Julien; Tipton, Michael J

    2015-02-01

    The aims of the present work were to investigate the relationships between radiant heat load, air velocity and body temperatures with or without coincidental exercise to determine the physiological mechanisms that drive thermal comfort and thermoregulatory behaviour. Seven male volunteers wearing swimming trunks in 18°C, 22°C or 26°C air were exposed to increasing air velocities up to 3 m s(-1) and self-adjusted the intensity of the direct radiant heat received on the front of the body to just maintain overall thermal comfort, at rest or when cycling (60 W, 60 rpm). During the 30 min of the experiments, skin and rectal temperatures were continuously recorded. We hypothesized that mean body temperature should be maintained stable and the intensity of the radiant heat and the mean skin temperatures would be lower when cycling. In all conditions, mean body temperature was lower when facing winds of 3 m s(-1) than during the first 5 min, without wind. When facing winds, in all but the 26°C air, the radiant heat was statistically higher at rest than when exercising. In 26°C air mean skin temperature was lower at rest than when exercising. No other significant difference was observed. In all air temperatures, high correlation coefficients were observed between the air velocity and the radiant heat load. Other factors that we did not measure may have contributed to the constant overall thermal comfort status despite dropping mean skin and body temperatures. It is suggested that the allowance to behaviourally adjust the thermal environment increases the tolerance of cold discomfort. Copyright © 2014 Elsevier Inc. All rights reserved.

  4. Temperature And Wind Velocity Oscillations Along a Gentle Slope During Sea-Breeze Events

    NASA Astrophysics Data System (ADS)

    Bastin, Sophie; Drobinski, Philippe

    2005-03-01

    The flow structure on a gentle slope at Vallon d’Ol in the northern suburbs of Marseille in southern France has been documented by means of surface wind and temperature measurements collected from 7 June to 14 July 2001 during the ESCOMPTE experiment. The analysis of the time series reveals temperature and wind speed oscillations during several nights (about 60--90 min oscillation period) and several days (about 120-180 min oscillation period) during the whole observing period. Oscillating katabatic winds have been reported in the literature from theoretical, experimental and numerical studies. In the present study, the dynamics of the observed oscillating katabatic winds are in good agreement with the theory.In contrast to katabatic winds, no daytime observations of oscillating anabatic upslope flows have ever been published to our knowledge, probably because of temperature inversion break-up that inhibits upslope winds. The present paper shows that cold air advection by a sea breeze generates a mesoscale horizontal temperature gradient, and hence baroclinicity in the atmosphere, which then allows low-frequency oscillations, similar to a katabatic flow. An expression for the oscillation period is derived that accounts for the contribution of the sea-breeze induced mesoscale horizontal temperature gradient. The theoretical prediction of the oscillation period is compared to the measurements, and good agreement is found. The statistical analysis of the wind flow at Vallon d’Ol shows a dominant north-easterly to easterly flow pattern for nighttime oscillations and a dominant south-westerly flow pattern for daytime oscillations. These results are consistent with published numerical simulation results that show that the air drains off the mountain along the maximum slope direction, which in the studied case is oriented south-west to north-east.

  5. Thermospheric winds and exospheric temperatures from incoherent scatter radar measurements in four seasons

    NASA Technical Reports Server (NTRS)

    Antoniadis, D. A.

    1976-01-01

    The time-dependent equations of neutral air motion are solved subject to three constraints: two of them are the usual upper and lower boundary conditions and the third is the value of the wind-induced ion drift at any given height. Using incoherent radar data, this procedure leads to a fast, direct numerical integration of the two coupled differential equations describing the horizontal wind components and yields time dependent wind profiles and meridional exospheric neutral temperature gradients. The diurnal behavior of the neutral wind system and of the exospheric temperature is presented for two solstice and two equinox days. The data used were obtained by the St. Santin and the Millstone Hill incoherent scatter radars. The derived geographic distributions of the exospheric temperatures are compared with those predicted by the OGO-6 empirical thermospheric model.

  6. Impacts of Wind Farms on Local Land Surface Temperature

    NASA Astrophysics Data System (ADS)

    Zhou, L.; Tian, Y.; Baidya Roy, S.; Thorncroft, C.; Bosart, L. F.; Hu, Y.

    2012-12-01

    The U.S. wind 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 wind's kinetic energy into electricity, wind 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 regional 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 region in West-Central Texas, where four of the world's largest wind 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 wind farms relative to nearby non wind farm regions 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 wind 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 wind farms. This inference is consistent with the increasing number of operational wind turbines with time during the study period, the diurnal and seasonal variations in the frequency of wind speed and direction distribution, and the changes in near-surface atmospheric boundary layer conditions due to wind 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 wind turbine. A regional 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 regional mean

  7. Modified wind chill temperatures determined by a whole body thermoregulation model and human-based facial convective coefficients.

    PubMed

    Shabat, Yael Ben; Shitzer, Avraham; Fiala, Dusan

    2014-08-01

    Wind chill equivalent temperatures (WCETs) were estimated by a modified Fiala's whole body thermoregulation model of a clothed person. Facial convective heat exchange coefficients applied in the computations concurrently with environmental radiation effects were taken from a recently derived human-based correlation. Apart from these, the analysis followed the methodology used in the derivation of the currently used wind chill charts. WCET values are summarized by the following equation:[Formula: see text]Results indicate consistently lower estimated facial skin temperatures and consequently higher WCETs than those listed in the literature and used by the North American weather services. Calculated dynamic facial skin temperatures were additionally applied in the estimation of probabilities for the occurrence of risks of frostbite. Predicted weather combinations for probabilities of "Practically no risk of frostbite for most people," for less than 5 % risk at wind speeds above 40 km h(-1), were shown to occur at air temperatures above -10 °C compared to the currently published air temperature of -15 °C. At air temperatures below -35 °C, the presently calculated weather combination of 40 km h(-1)/-35 °C, at which the transition for risks to incur a frostbite in less than 2 min, is less conservative than that published: 60 km h(-1)/-40 °C. The present results introduce a fundamentally improved scientific basis for estimating facial skin temperatures, wind chill temperatures and risk probabilities for frostbites over those currently practiced.

  8. Modified wind chill temperatures determined by a whole body thermoregulation model and human-based facial convective coefficients

    NASA Astrophysics Data System (ADS)

    Shabat, Yael Ben; Shitzer, Avraham; Fiala, Dusan

    2014-08-01

    Wind chill equivalent temperatures (WCETs) were estimated by a modified Fiala's whole body thermoregulation model of a clothed person. Facial convective heat exchange coefficients applied in the computations concurrently with environmental radiation effects were taken from a recently derived human-based correlation. Apart from these, the analysis followed the methodology used in the derivation of the currently used wind chill charts. WCET values are summarized by the following equation: Results indicate consistently lower estimated facial skin temperatures and consequently higher WCETs than those listed in the literature and used by the North American weather services. Calculated dynamic facial skin temperatures were additionally applied in the estimation of probabilities for the occurrence of risks of frostbite. Predicted weather combinations for probabilities of "Practically no risk of frostbite for most people," for less than 5 % risk at wind speeds above 40 km h-1, were shown to occur at air temperatures above -10 °C compared to the currently published air temperature of -15 °C. At air temperatures below -35 °C, the presently calculated weather combination of 40 km h-1/-35 °C, at which the transition for risks to incur a frostbite in less than 2 min, is less conservative than that published: 60 km h-1/-40 °C. The present results introduce a fundamentally improved scientific basis for estimating facial skin temperatures, wind chill temperatures and risk probabilities for frostbites over those currently practiced.

  9. Combined effects of wind and solar irradiance on the spatial variation of midday air temperature over a mountainous terrain

    NASA Astrophysics Data System (ADS)

    Kim, Soo-Ock; Kim, Jin-Hee; Kim, Dae-Jun; Shim, Kyo Moon; Yun, Jin I.

    2015-08-01

    When the midday temperature distribution in a mountainous region was estimated using data from a nearby weather station, the correction of elevation difference based on temperature lapse caused a large error. An empirical approach reflecting the effects of solar irradiance and advection was suggested in order to increase the reliability of the results. The normalized slope irradiance, which was determined by normalizing the solar irradiance difference between a horizontal surface and a sloping surface from 1100 to 1500 LST on a clear day, and the deviation relationship between the horizontal surface and the sloping surface at the 1500 LST temperature on each day were presented as simple empirical formulas. In order to simulate the phenomenon that causes immigrant air parcels to push out or mix with the existing air parcels in order to decrease the solar radiation effects, an advection correction factor was added to exponentially reduce the solar radiation effect with an increase in wind speed. In order to validate this technique, we estimated the 1500 LST air temperatures on 177 clear days in 2012 and 2013 at 10 sites with different slope aspects in a mountainous catchment and compared these values to the actual measured data. The results showed that this technique greatly improved the error bias and the overestimation of the solar radiation effect in comparison with the existing methods. By applying this technique to the Korea Meteorological Administration's 5-km grid data, it was possible to determine the temperature distribution at a 30-m resolution over a mountainous rural area south of Jiri Mountain National Park, Korea.

  10. Improved spatial monitoring of air temperature in forested complex terrain: an energy-balance based calibration method

    NASA Astrophysics Data System (ADS)

    Kennedy, A. M.; Thomas, C. K.; Pypker, T. G.; Bond, B. J.; Selker, J. S.; Unsworth, M. H.

    2009-12-01

    Fiber-optic distributed temperature sensing (DTS) has great potential for spatial monitoring in hydrology and atmospheric science. DTS systems have an advantage over conventional individual temperature sensors in that thousands of quasi-concurrent temperature measurements may be made along the entire length of a fiber at 1 meter increments by a single instrument, thus increasing measurement precision. However, like any other temperature sensors, the fiber temperature is influenced by energy exchange with its environment, particularly by radiant energy (solar and long-wave) and by wind speed. The objective of this research is to perform an energy-balance based calibration of a DTS fiber system that will reduce the uncertainty of air temperature measurements in open and forested environments. To better understand the physics controlling the fiber temperature reported by the DTS, alternating black and white fiber optic cables were installed on vertical wooden jigs inside a recirculating wind tunnel. A constant irradiance from six 600W halogen lamps was directed on a two meter section of fiber to permit controlled observations of the resulting temperature difference between the black and white fibers as wind speed was varied. The net short and longwave radiation balance of each fiber was measured with an Eppley pyranometer and Kipp and Zonen pyrgeometer. Additionally, accurate air temperature was recorded from a screened platinum resistance thermometer, and sonic anemometers were positioned to record wind speed and turbulence. Relationships between the temperature excess of each fiber, net radiation, and wind speed were developed and will be used to derive correction terms in future field work. Preliminary results indicate that differential heating of fibers (black-white) is driven largely by net radiation with wind having a smaller but consistent effect. Subsequent work will require field verification to confirm that the observed wind tunnel correction algorithms are

  11. Quantifying energy and mass transfer in crop canopies: sensors for measurement of temperature and air velocity

    NASA Technical Reports Server (NTRS)

    Bugbee, B.; Monje, O.; Tanner, B.

    1996-01-01

    Here we report on the in situ performance of inexpensive, miniature sensors that have increased our ability to measure mass and energy fluxes from plant canopies in controlled environments: 1. Surface temperature. Canopy temperature measurements indicate changes in stomatal aperture and thus latent and sensible heat fluxes. Infrared transducers from two manufacturers (Exergen Corporation, Newton, MA; and Everest Interscience, Tucson, AZ, USA) have recently become available. Transducer accuracy matched that of a more expensive hand-held infrared thermometer. 2. Air velocity varies above and within plant canopies and is an important component in mass and energy transfer models. We tested commercially-available needle, heat-transfer anemometers (1 x 50 mm cylinder) that consist of a fine-wire thermocouple and a heater inside a hypodermic needle. The needle is heated and wind speed determined from the temperature rise above ambient. These sensors are particularly useful in measuring the low wind speeds found within plant canopies. 3. Accurate measurements of air temperature adjacent to plant leaves facilitates transport phenomena modeling. We quantified the effect of radiation and air velocity on temperature rise in thermocouples from 10 to 500 micrometers. At high radiation loads and low wind speeds, temperature errors were as large as 7 degrees C above air temperature.

  12. Ice core evidence of rapid air temperature increases since 1960 in alpine areas of the Wind River Range, Wyoming, United States

    USGS Publications Warehouse

    Naftz, D.L.; Susong, D.D.; Schuster, P.F.; Cecil, L.D.; Dettinger, M.D.; Michel, R.L.; Kendall, C.

    2002-01-01

    Site-specific transfer functions relating delta oxygen 18 (δ18O) values in snow to the average air temperature (TA) during storms on Upper Fremont Glacier (UFG) were used in conjunction with δ18O records from UFG ice cores to reconstruct long-term trends in air temperature from alpine areas in the Wind River Range, Wyoming. Transfer functions were determined by using data collected from four seasonal snowpacks (1989-1990, 1997-1998, 1998-1999, and 1999-2000). The timing and amount of each storm was determined from an automated snowpack telemetry (SNOTEL) site, 22 km northeast of UFG, and ~1060 m in elevation below UFG. Statistically significant and positive correlations between δ18O values in the snow and TA were consistently found in three of the four seasonal snowpacks. The snowpack with the poor correlation was deposited in 1997-1998 during the 1997-1998 El Nino Southern Oscillation (ENSO). An ultrasonic snow-depth sensor installed on UFG provided valuable insights into site-specific storms and postdepositional processes that occur on UFG. The timing of storms recorded at the UFG and Cold Springs SNOTEL sites were similar; however, selected storms did not correlate. Snow from storms occurring after mid-October and followed by high winds was most susceptible to redeposition of snow. This removal of lower temperature snowfall could potentially bias the δ18O values preserved in ice core records to environmental conditions reflecting higher air temperatures and lower wind speeds. Transfer functions derived from seasonal snow cover on UFG were used to reconstruct TA values from δ18O values determined from two ice cores collected from UFG. Reconstructed air temperatures from the ice core data indicate an increase in TA of ~3.5oC from the mid-1960s to the early 1990s in the alpine areas of northwestern Wyoming. Reconstructed TA from the ice core records between the end of the Little Ice Age (LIA), mid-1800s, and the early 1990s indicate a TA increase of ~55oC. The

  13. Measuring centimeter-resolution air temperature profiles above land and water using fiber-optic Distributed Temperature Sensing

    NASA Astrophysics Data System (ADS)

    Sigmund, Armin; Pfister, Lena; Olesch, Johannes; Thomas, Christoph K.

    2016-04-01

    The precise determination of near-surface air temperature profiles is of special importance for the characterization of airflows (e.g. cold air) and the quantification of sensible heat fluxes according to the flux-gradient similarity approach. In contrast to conventional multi-sensor techniques, measuring temperature profiles using fiber-optic Distributed Temperature Sensing (DTS) provides thousands of measurements referenced to a single calibration standard at much reduced costs. The aim of this work was to enhance the vertical resolution of Raman scatter DTS measurements up to the centimeter-scale using a novel approach for atmospheric applications: the optical fiber was helically coiled around a meshed fabric. In addition to testing the new fiber geometry, we quantified the measurement uncertainty and demonstrated the benefits of the enhanced-resolution profiles. The fiber-optic cable was coiled around a hollow column consisting of white reinforcing fabric supported by plexiglass rings every meter. Data from two columns of this type were collected for 47 days to measure air temperature vertically over 3.0 and 5.1 m over a gently inclined meadow and over and in a small lake, respectively. Both profiles had a vertical resolution of 1 cm in the lower section near the surface and 5 cm in the upper section with an along-fiber instrument-specific averaging of 1.0 m and a temporal resolution of 30 s. Measurement uncertainties, especially from conduction between reinforcing fabric and fiber-optic cable, were estimated by modeling the fiber temperature via a detailed energy balance approach. Air temperature, wind velocity and radiation components were needed as input data and measured separately. The temperature profiles revealed valuable details, especially in the lowest 1 m above surface. This was best demonstrated for nighttime observations when artefacts due to solar heating did not occur. For example, the dynamics of a cold air layer was detected in a clear night

  14. Temperature inversions and cold-air pools study in Picos de Europa surroundings

    NASA Astrophysics Data System (ADS)

    Iglesias González, Miguel; Yagüe, Carlos; Maqueda, Gregorio

    2017-04-01

    Using surface temperature data from dataloggers located at the bottom of four different high-altitude (2000 m MSL) glaciokarstic depressions in Picos de Europa (Cantabrian Cordillera, Spain) from January 2012 to September 2016, we have analyzed the evolution of more than 200 different cold-air pools events according to different geomorphologic parameters. The ski-view determinates the cold-air pool occurrence and the temperature range, and the depression's depth is a very important factor in the permanent cold-air pools (PCAP) formation. Depending on the structure of the thermal curve, we classified all cold-air pools in each depression by using a conceptual model with eight different modes. With wind and relative humidity data, supplied by a weather station situated near the depressions, and NCAR-NCEP reanalysis data, we have characterized them at mesoscale and synoptic scale. If the ski-view is small enough, we can have undisturbed cold-air pools even though disturbed wind conditions. Snow-covered and non-snow-covered events were measured during the campaign, which allow us to recognize its influence on the temperature inversions. We also identified and analyze several permanent cold-air pools events where December minimum temperature record of -30,6°C in the Iberian Peninsula was measured. We also make a deep analyze of the Iberian Peninsula historical minimal temperature record of -32,7°C, which was measured on February 2016. Finally we use and test a simplified three-layer radiative model to describe and verify the influence of different geomorphologic factors in the cooling process of all the cold-air pools.

  15. Effects of vernal equinox solar eclipse on temperature and wind direction in Switzerland

    NASA Astrophysics Data System (ADS)

    Eugster, Werner; Emmel, Carmen; Wolf, Sebastian; Buchmann, Nina; McFadden, Joseph P.; Whiteman, Charles David

    2017-12-01

    The vernal equinox total solar eclipse of 20 March 2015 produced a maximum occultation of 65.8-70.1 % over Switzerland during the morning hours (09:22 to 11:48 CET). Skies were generally clear over the Swiss Alps due to a persistent high-pressure band between the UK and Russia associated with a rather weak pressure gradient over the continent. To assess the effects of penumbral shading on near-surface meteorology across Switzerland, air temperature data measured at 10 min intervals at 184 MeteoSwiss weather stations were used. Wind speed and direction data were available from 165 of these stations. Additionally, six Swiss FluxNet eddy covariance flux (ECF) sites provided turbulent measurements at 20 Hz resolution. During maximum occultation, the temperature drop was up to 5.8 K at a mountain site where cold air can pool in a topographic depression. The bootstrapped average of the maximum temperature drops of all 184 MeteoSwiss sites during the solar eclipse was 1.51 ± 0.02 K (mean ± SE). A detailed comparison with literature values since 1834 showed a temperature decrease of 2.6 ± 1.7 K (average of all reports), with extreme values up to 11 K. On fair weather days under weak larger-scale pressure gradients, local thermo-topographic wind systems develop that are driven by small-scale pressure and temperature gradients. At one ECF site, the penumbral shading delayed the morning transition from down-valley to up-valley wind conditions. At another site, it prevented this transition from occurring at all. Data from the 165 MeteoSwiss sites measuring wind direction did not show a consistent pattern of wind direction response to the passing of the penumbral shadow. These results suggest that the local topographic setting had an important influence on the temperature drop and the wind flow patterns during the eclipse. A significant cyclonic effect of the passing penumbral shadow was found in the elevation range ≈ 1700-2700 m a. s. l., but

  16. Field Calibration of XAD-Based Passive Air Sampler on the Tibetan Plateau: Wind Influence and Configuration Improvement.

    PubMed

    Gong, Ping; Wang, Xiaoping; Liu, Xiande; Wania, Frank

    2017-05-16

    The passive air sampler based on XAD-2 resin (XAD-PAS) has proven useful for collecting atmospheric persistent organic pollutants (POPs) in remote regions. Whereas laboratory studies have shown that, due to the open bottom of its housing, the passive sampling rate (PSR) of the XAD-PAS is susceptible to wind and other processes causing air turbulence, the sampler has not been calibrated in the field at sites experiencing high winds. In this study, the PSRs of the XAD-PAS were calibrated at three sites on the Tibetan Plateau, covering a wide range in temperature (T), pressure (P) and wind speed (v). At sites with low wind speeds (i.e., in a forest and an urban site), the PSRs are proportional to the ratio T 1.75 / P; at windy sites with an average wind speed above 3 m/s, the influence of v on PSRs cannot be ignored. Moreover, the open bottom of the XAD-PAS housing causes the PSRs to be influenced by wind angle and air turbulence caused by sloped terrain. Field calibration, wind speed measurements, and computational fluid dynamics (CFD) simulations indicate that a modified design incorporating an air spoiler consisting of 4 metal sheets dampens the turbulence caused by wind angle and sloped terrain and caps the PSR at ∼5 m 3 /day, irrespective of ambient wind. Therefore, the original XAD-PAS with an open bottom is suitable for deployment in urban areas and other less windy places, the modified design is preferable in mountain regions and other places where air circulation is complicated and strong.

  17. Development and testing of a portable wind sensitive directional air sampler

    NASA Technical Reports Server (NTRS)

    Deyo, J.; Toma, J.; King, R. B.

    1975-01-01

    A portable wind sensitive directional air sampler was developed as part of an air pollution source identification system. The system is designed to identify sources of air pollution based on the directional collection of field air samples and their analysis for TSP and trace element characteristics. Sources can be identified by analyzing the data on the basis of pattern recognition concepts. The unit, designated Air Scout, receives wind direction signals from an associated wind vane. Air samples are collected on filter slides using a standard high volume air sampler drawing air through a porting arrangement which tracks the wind direction and permits collection of discrete samples. A preset timer controls the length of time each filter is in the sampling position. At the conclusion of the sampling period a new filter is automatically moved into sampling position displacing the previous filter to a storage compartment. Thus the Air Scout may be set up at a field location, loaded with up to 12 filter slides, and left to acquire air samples automatically, according to the wind, at any timer interval desired from 1 to 30 hours.

  18. Solar wind proton temperature-velocity relationship

    NASA Technical Reports Server (NTRS)

    Lopez, R. E.; Freeman, J. W.

    1986-01-01

    Helios 1 data are analyzed to find an experimental fit for the temperature-velocity relationship at 1 AU. It is shown that the proton temperature-velocity changes at a velocity of approximately 500 km/s. Interplanetary dynamic processes, i.e., stream interactions, are shown to affect the temperature-velocity relationships less than 22 percent; the functional form of these relationships appears to be preserved throughout the solar cycle. It is pointed out that any comprehensive model of the solar wind will have to address the difference in the temperature-velocity relationship between the low- and high-speed wind, since this is a product of the acceleration and subsequent heating process generating the solar wind.

  19. 6. VIEW OF FIVEFOOT WIND TUNNEL WITH AIR STRAIGHTENER AND ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    6. VIEW OF FIVE-FOOT WIND TUNNEL WITH AIR STRAIGHTENER AND OPERATOR STATION IN FOREGROUND (1991). - Wright-Patterson Air Force Base, Area B, Building No. 19, Five-Foot Wind Tunnel, Dayton, Montgomery County, OH

  20. Ground-level climate at a peatland wind farm in Scotland is affected by wind turbine operation

    NASA Astrophysics Data System (ADS)

    Armstrong, Alona; Burton, Ralph R.; Lee, Susan E.; Mobbs, Stephen; Ostle, Nicholas; Smith, Victoria; Waldron, Susan; Whitaker, Jeanette

    2016-04-01

    The global drive to produce low-carbon energy has resulted in an unprecedented deployment of onshore wind turbines, representing a significant land use change for wind energy generation with uncertain consequences for local climatic conditions and the regulation of ecosystem processes. Here, we present high-resolution data from a wind farm collected during operational and idle periods that shows the wind farm affected several measures of ground-level climate. Specifically, we discovered that operational wind turbines raised air temperature by 0.18 °C and absolute humidity (AH) by 0.03 g m-3 during the night, and increased the variability in air, surface and soil temperature throughout the diurnal cycle. Further, the microclimatic influence of turbines on air temperature and AH decreased logarithmically with distance from the nearest turbine. These effects on ground-level microclimate, including soil temperature, have uncertain implications for biogeochemical processes and ecosystem carbon cycling, including soil carbon stocks. Consequently, understanding needs to be improved to determine the overall carbon balance of wind energy.

  1. Sensitivity of New England Stream Temperatures to Air Temperature and Precipitation Under Projected Climate

    NASA Astrophysics Data System (ADS)

    Huang, T.; Samal, N. R.; Wollheim, W. M.; Stewart, R. J.; Zuidema, S.; Prousevitch, A.; Glidden, S.

    2015-12-01

    The thermal response of streams and rivers to changing climate will influence aquatic habitat. This study examines the impact that changing climate has on stream temperatures in the Merrimack River, NH/MA USA using the Framework for Aquatic Modeling in the Earth System (FrAMES), a spatially distributed river network model driven by air temperature, air humidity, wind speed, precipitation, and solar radiation. Streamflow and water temperatures are simulated at a 45-second (latitude x longitude) river grid resolution for 135 years under historical and projected climate variability. Contemporary streamflow (Nash-Sutcliffe Coefficient = 0.77) and river temperatures (Nash-Sutcliffe Coefficient = 0.89) matched at downstream USGS gauge data well. A suite of model runs were made in combination with uniformly increased daily summer air temperatures by 2oC, 4 oC and 6 oC as well as adjusted precipitation by -40%, -30%, -20%, -10% and +10% as a sensitivity analysis to explore a broad range of potential future climates. We analyzed the summer stream temperatures and the percent of river length unsuitable for cold to warm water fish habitats. Impacts are greatest in large rivers due to the accumulation of river temperature warming throughout the entire river network. Cold water fish (i.e. brook trout) are most strongly affected while, warm water fish (i.e. largemouth bass) aren't expected to be impacted. The changes in stream temperatures under various potential climate scenarios will provide a better understanding of the specific impact that air temperature and precipitation have on aquatic thermal regimes and habitat.

  2. Investigation of the spatial variability and possible origins of wind-induced air pressure fluctuations responsible for pressure pumping

    NASA Astrophysics Data System (ADS)

    Mohr, Manuel; Laemmel, Thomas; Maier, Martin; Zeeman, Matthias; Longdoz, Bernard; Schindler, Dirk

    2017-04-01

    The exchange of greenhouse gases between the soil and the atmosphere is highly relevant for the climate of the Earth. Recent research suggests that wind-induced air pressure fluctuations can alter the soil gas transport and therefore soil gas efflux significantly. Using a newly developed method, we measured soil gas transport in situ in a well aerated forest soil. Results from these measurements showed that the commonly used soil gas diffusion coefficient is enhanced up to 30% during periods of strong wind-induced air pressure fluctuations. The air pressure fluctuations above the forest floor are only induced at high above-canopy wind speeds (> 5 m s-1) and lie in the frequency range 0.01-0.1 Hz. Moreover, the amplitudes of air pressure fluctuations in this frequency range show a clear quadratic dependence on mean above-canopy wind speed. However, the origin of these wind-induced pressure fluctuations is still unclear. Airflow measurements and high-precision air pressure measurements were conducted at three different vegetation-covered sites (conifer forest, deciduous forest, grassland) to investigate the spatial variability of dominant air pressure fluctuations, their origin and vegetation-dependent characteristics. At the conifer forest site, a vertical profile of air pressure fluctuations was measured and an array consisting of five pressure sensors were installed at the forest floor. At the grassland site, the air pressure measurements were compared with wind observations made by ground-based LIDAR and spatial temperature observations from a fibre-optic sensing network (ScaleX Campaign 2016). Preliminary results show that at all sites the amplitudes of relevant air pressure fluctuations increase with increasing wind speed. Data from the array measurements reveal that there are no time lags between the air pressure signals of different heights, but a time lag existed between the air pressure signals of the sensors distributed laterally on the forest floor

  3. Weather and climate needs for Lidar observations from space and concepts for their realization. [wind, temperature, moisture, and pressure data needs

    NASA Technical Reports Server (NTRS)

    Atlas, D.; Korb, C. L.

    1980-01-01

    The spectrum of weather and climate needs for Lidar observations from space is discussed with emphasis on the requirements for wind, temperature, moisture, and pressure data. It is shown that winds are required to realistically depict all atmospheric scales in the tropics and the smaller scales at higher latitudes, where both temperature and wind profiles are necessary. The need for means to estimate air-sea exchanges of sensible and latent heat also is noted. A concept for achieving this through a combination of Lidar cloud top heights and IR cloud top temperatures of cloud streets formed during cold air outbreaks over the warmer ocean is outlined. Recent theoretical feasibility studies concerning the profiling of temperatures, pressure, and humidity by differential absorption Lidar (DIAL) from space and expected accuracies are reviewed. An alternative approach to Doppler Lidar wind measurements also is presented. The concept involves the measurement of the displacement of the aerosol backscatter pattern, at constant heights, between two successive scans of the same area, one ahead of the spacecraft and the other behind it a few minutes later. Finally, an integrated space Lidar system capable of measuring temperature, pressure, humidity, and winds which combines the DIAL methods with the aerosol pattern displacement concept is described.

  4. Numerical investigation of air flow in a supersonic wind tunnel

    NASA Astrophysics Data System (ADS)

    Drozdov, S. M.; Rtishcheva, A. S.

    2017-11-01

    In the framework of TsAGI’s supersonic wind tunnel modernization program aimed at improving flow quality and extending the range of test regimes it was required to design and numerically validate a new test section and a set of shaped nozzles: two flat nozzles with flow Mach number at nozzle exit M=4 and M=5 and two axisymmetric nozzles with M=5 and M=6. Geometric configuration of the nozzles, the test section (an Eiffel chamber) and the diffuser was chosen according to the results of preliminary calculations of two-dimensional air flow in the wind tunnel circuit. The most important part of the work are three-dimensional flow simulation results obtained using ANSYS Fluent software. The following flow properties were investigated: Mach number, total and static pressure, total and static temperature and turbulent viscosity ratio distribution, heat flux density at wind tunnel walls (for high-temperature flow regimes). It is demonstrated that flow perturbations emerging from the junction of the nozzle with the test section and spreading down the test section behind the boundaries of characteristic rhomb’s reverse wedge are nearly impossible to eliminate. Therefore, in order to perform tests under most uniform flow conditions, the model’s center of rotation and optical window axis should be placed as close to the center of the characteristic rhomb as possible. The obtained results became part of scientific and technical basis of supersonic wind tunnel design process and were applied to a generalized class of similar wind tunnels.

  5. Errors of five-day mean surface wind and temperature conditions due to inadequate sampling

    NASA Technical Reports Server (NTRS)

    Legler, David M.

    1991-01-01

    Surface meteorological reports of wind components, wind speed, air temperature, and sea-surface temperature from buoys located in equatorial and midlatitude regions are used in a simulation of random sampling to determine errors of the calculated means due to inadequate sampling. Subsampling the data with several different sample sizes leads to estimates of the accuracy of the subsampled means. The number N of random observations needed to compute mean winds with chosen accuracies of 0.5 (N sub 0.5) and 1.0 (N sub 1,0) m/s and mean air and sea surface temperatures with chosen accuracies of 0.1 (N sub 0.1) and 0.2 (N sub 0.2) C were calculated for each 5-day and 30-day period in the buoy datasets. Mean values of N for the various accuracies and datasets are given. A second-order polynomial relation is established between N and the variability of the data record. This relationship demonstrates that for the same accuracy, N increases as the variability of the data record increases. The relationship is also independent of the data source. Volunteer-observing ship data do not satisfy the recommended minimum number of observations for obtaining 0.5 m/s and 0.2 C accuracy for most locations. The effect of having remotely sensed data is discussed.

  6. A Wind Energy Powered Wireless Temperature Sensor Node

    PubMed Central

    Zhang, Chuang; He, Xue-Feng; Li, Si-Yu; Cheng, Yao-Qing; Rao, Yang

    2015-01-01

    A wireless temperature sensor node composed of a piezoelectric wind energy harvester, a temperature sensor, a microcontroller, a power management circuit and a wireless transmitting module was developed. The wind-induced vibration energy harvester with a cuboid chamber of 62 mm × 19.6 mm × 10 mm converts ambient wind energy into electrical energy to power the sensor node. A TMP102 temperature sensor and the MSP430 microcontroller are used to measure the temperature. The power management module consists of LTC3588-1 and LT3009 units. The measured temperature is transmitted by the nRF24l01 transceiver. Experimental results show that the critical wind speed of the harvester was about 5.4 m/s and the output power of the harvester was about 1.59 mW for the electrical load of 20 kΩ at wind speed of 11.2 m/s, which was sufficient to power the wireless sensor node to measure and transmit the temperature every 13 s. When the wind speed increased from 6 m/s to 11.5 m/s, the self-powered wireless sensor node worked normally. PMID:25734649

  7. A wind energy powered wireless temperature sensor node.

    PubMed

    Zhang, Chuang; He, Xue-Feng; Li, Si-Yu; Cheng, Yao-Qing; Rao, Yang

    2015-02-27

    A wireless temperature sensor node composed of a piezoelectric wind energy harvester, a temperature sensor, a microcontroller, a power management circuit and a wireless transmitting module was developed. The wind-induced vibration energy harvester with a cuboid chamber of 62 mm × 19.6 mm × 10 mm converts ambient wind energy into electrical energy to power the sensor node. A TMP102 temperature sensor and the MSP430 microcontroller are used to measure the temperature. The power management module consists of LTC3588-1 and LT3009 units. The measured temperature is transmitted by the nRF24l01 transceiver. Experimental results show that the critical wind speed of the harvester was about 5.4 m/s and the output power of the harvester was about 1.59 mW for the electrical load of 20 kΩ at wind speed of 11.2 m/s, which was sufficient to power the wireless sensor node to measure and transmit the temperature every 13 s. When the wind speed increased from 6 m/s to 11.5 m/s, the self-powered wireless sensor node worked normally.

  8. Effects of open-air temperature on air temperature inside biological safety cabinet.

    PubMed

    Umemura, Masayuki; Shigeno, Katsuro; Yamamura, Keiko; Osada, Takashi; Soda, Midori; Yamada, Kiyofumi; Ando, Yuichi; Wakiya, Yoshifumi

    2011-02-14

    In Japan, biological safety cabinets (BSCs) are normally used by medical staff while handling antineoplastic agents. We have also set up a class II B2 BSC at the Division of Chemotherapy for Outpatients. The air temperature inside this BSC, however, decreases in winter. We assumed that this decrease is caused by the intake of open-air. Therefore, we investigated the effects of low open-air temperature on the BSC temperature and the time of admixtures of antineoplastic agents. The studies were conducted from January 1 to March 31, 2008. The outdoor air temperature was measured in the shade near the intake nozzle of the BSC and was compared with the BSC temperature. The correlation between the outdoor air temperature and the BSC temperature, the dissolution time of cyclophosphamide (CPA) and gemcitabine (GEM), and accurate weight measurement of epirubicin (EPI) solution were investigated for low and normal BSC temperatures. The BSC temperature was correlated with the open-air temperature for open-air temperatures of 5-20°C (p < 0.0001). The dissolution of CPA and GEM at these temperatures was significantly delayed as compared to that at 25°C (p < 0.01 and p < 0.0001, respectively). The weight measurement of EPI solution using a syringe method lacks accuracy because of its high coefficient of viscosity at low temperatures (p < 0.01). These results suggest that the BSC temperature decreases below room temperature in winter when air is drawn from outdoors. We showed that the BSC temperature affects the dissolution rate of antineoplastic agents. Further, we suggested that the BSC temperature drop might delay the affair of the admixtures of antineoplastic agents and increase the waiting time of outpatients for chemotherapy.

  9. The association of air temperature with cardiac arrhythmias

    NASA Astrophysics Data System (ADS)

    Čulić, Viktor

    2017-11-01

    The body response to meteorological influences may activate pathophysiological mechanisms facilitating the occurrence of cardiac arrhythmias in susceptible patients. Putative underlying mechanisms include changes in systemic vascular resistance and blood pressure, as well as a network of proinflammatory and procoagulant processes. Such a chain reaction probably occurs within the time window of several hours, so use of daily average values of meteorological elements do not seem appropriate for investigation in this area. In addition, overall synoptic situation, and season-specific combinations of meteorological elements and air pollutant levels probably cause the overall effect rather than a single atmospheric element. Particularly strong interrelations have been described among wind speed, air pressure and temperature, relative air humidity, and suspended particulate matter. This may be the main reason why studies examining the association between temperature and ventricular arrhythmias have found linear positive, negative, J-shaped or no association. Further understanding of the pathophysiological adaptation to atmospheric environment may help in providing recommendations for protective measures during "bad" weather conditions in patients with cardiac arrhythmias.

  10. Simultaneous measurements of temperature and density in air flows using UV laser spectroscopy

    NASA Technical Reports Server (NTRS)

    Fletcher, D. G.; Mckenzie, R. L.

    1991-01-01

    The simultaneous measurement of temperature and density using laser-induced fluorescence of oxygen in combination with Q-branch Raman scattering of nitrogen and oxygen is demonstrated in a low-speed air flow. The lowest density and temperature measured in the experiment correspond to the freestream values at Mach 5 in the Ames 3.5-Foot Hypersonic Wind Tunnel for stagnation conditions of 100 atm and 1000 K. The experimental results demonstrate the viability of the optical technique for measurements that support the study of compressible turbulence and the validation of numerical codes in supersonic and hypersonic wind tunnel flows.

  11. An Integrated Approach to Estimate Instantaneous Near-Surface Air Temperature and Sensible Heat Flux Fields during the SEMAPHORE Experiment.

    NASA Astrophysics Data System (ADS)

    Bourras, Denis; Eymard, Laurence; Liu, W. Timothy; Dupuis, Hélène

    2002-03-01

    A new technique was developed to retrieve near-surface instantaneous air temperatures and turbulent sensible heat fluxes using satellite data during the Structure des Echanges Mer-Atmosphere, Proprietes des Heterogeneites Oceaniques: Recherche Experimentale (SEMAPHORE) experiment, which was conducted in 1993 under mainly anticyclonic conditions. The method is based on a regional, horizontal atmospheric temperature advection model whose inputs are wind vectors, sea surface temperature fields, air temperatures around the region under study, and several constants derived from in situ measurements. The intrinsic rms error of the method is 0.7°C in terms of air temperature and 9 W m2 for the fluxes, both at 0.16° × 0.16° and 1.125° × 1.125° resolution. The retrieved air temperature and flux horizontal structures are in good agreement with fields from two operational general circulation models. The application to SEMAPHORE data involves the First European Remote Sensing Satellite (ERS-1) wind fields, Advanced Very High Resolution Radiometer (AVHRR) SST fields, and European Centre for Medium-Range Weather Forecasts (ECMWF) air temperature boundary conditions. The rms errors obtained by comparing the estimations with research vessel measurements are 0.3°C and 5 W m2.

  12. Discussion on fresh air volume in Temperature and Humidity Independent Control of Air-conditioning System

    NASA Astrophysics Data System (ADS)

    Cheng, Xiaolong; Liu, Jinxiang; Wang, Yu; Yuan, Xiaolei; Jin, Hui

    2018-05-01

    The fresh air volume in Temperature and Humidity Independent Control of Air-conditioning System(THIC) of a typical office was comfirmed, under the premise of adopting the refrigeration dehumidifying fresh air unit(7°C/12°C). By detailed calculating the space moisture load and the fresh air volume required for dehumidification in 120 selected major cities in China, it can be inferred that the minimum fresh air volume required for dehumidification in THIC is mainly determined by the local outdoor air moisture and the outdoor wind speed; Then the mathematical fitting software Matlab was used to fit the three parameters, and a simplified formula for calculating the minimum per capita fresh air volume required for dehumidification was obtained; And the indoor relative humidity was simulated by the numerical software Airpak and the results by using the formula data and the data for hygiene were compared to verify the relibility of the simplified formula.

  13. The Use of Red Green Blue Air Mass Imagery to Investigate the Role of Stratospheric Air in a Non-convective Wind Event

    NASA Technical Reports Server (NTRS)

    Berndt, E. B.; Zavodsky, B. T.; Jedlovec, G. J.; Molthan, A. L.

    2013-01-01

    Non-convective wind events commonly occur with passing extratropical cyclones and have significant societal and economic impacts. Since non-convective winds often occur in the absence of specific phenomena such as a thunderstorm, tornado, or hurricane, the public are less likely to heed high wind warnings and continue daily activities. Thus non-convective wind events result in as many fatalities as straight line thunderstorm winds. One physical explanation for non-convective winds includes tropopause folds. Improved model representation of stratospheric air and associated non-convective wind events could improve non-convective wind forecasts and associated warnings. In recent years, satellite data assimilation has improved skill in forecasting extratropical cyclones; however errors still remain in forecasting the position and strength of extratropical cyclones as well as the tropopause folding process. The goal of this study is to determine the impact of assimilating satellite temperature and moisture retrieved profiles from hyperspectral infrared (IR) sounders (i.e. Atmospheric Infrared Sounder (AIRS), Cross-track Infrared and Microwave Sounding Suite (CrIMSS), and Infrared Atmospheric Sounding Interferometer (IASI)) on the model representation of the tropopause fold and an associated high wind event that impacted the Northeast United States on 09 February 2013. Model simulations using the Advanced Research Weather Research and Forecasting Model (ARW) were conducted on a 12-km grid with cycled data assimilation mimicking the operational North American Model (NAM). The results from the satellite assimilation run are compared to a control experiment (without hyperspectral IR retrievals), Modern Era-Retrospective Analysis for Research and Applications (MERRA) reanalysis, and Rapid Refresh analyses.

  14. Investigation of air flow in open-throat wind tunnels

    NASA Technical Reports Server (NTRS)

    Jacobs, Eastman N

    1930-01-01

    Tests were conducted on the 6-inch wind tunnel of the National Advisory Committee for Aeronautics to form a part of a research on open-throat wind tunnels. The primary object of this part of the research was to study a type of air pulsation which has been encountered in open-throat tunnels, and to find the most satisfactory means of eliminating such pulsations. In order to do this it was necessary to study the effects of different variable on all of the important characteristics of the tunnel. This paper gives not only the results of the study of air pulsations and methods of eliminating them, but also the effects of changing the exit-cone diameter and flare and the effects of air leakage from the return passage. It was found that the air pulsations in the 6-inch wind tunnel could be practically eliminated by using a moderately large flare on the exit cone in conjunction with leakage introduced by cutting holes in the exit cone somewhat aft of its minimum diameter.

  15. Novel insights into the dynamics of cold-air drainage and pooling on a gentle slope from fiber-optic distributed temperature sensing

    NASA Astrophysics Data System (ADS)

    Pfister, Lena; Sigmund, Armin; Olesch, Johannes; Thomas, Christoph

    2016-04-01

    Urban climate can benefit from cold-air drainage as it may help alleviate the urban heat island. In contrast, stable cold-air pools can damage plants especially in rural areas. In this study, we examined the dynamics of cold-air drainage and pooling in a peri-urban setting over a period of 47 days along a 170 m long slope with an inclination of 1.3° located in the Ecological Botany Gardens of the University of Bayreuth. Air and soil temperatures were measured using distributed temperature sensing of an 2-dimensional fiber-optic array at six heights (-2 cm to 100 cm) along the slope sampling every 1 min and every 1 m. Ancillary measurements of winds, turbulence intensity and momentum exchange were collected using two ultrasonic anemometers installed at 0.1 m and 17 m height at the center of the transect. We hypothesized that cold-air drainage, here defined as a gravity-driven density flow near the bottom originating from local radiative cooling of the surface, is decoupled from non-local flows and can thus be predicted from the local topography. The nocturnal data were stratified by classes of longwave radiation balance, wind speed, and wind direction at 0.1 m agl. The four most abundant classes were tested further for decoupling of wind velocities and directions between 17 and 0.1 m. We further computed the vertical and horizontal temperature perturbations of the fiber-optic array as evaluated for these cases, as well as subject the temperature data to a multiresolution decomposition to investigate the spatial two-point correlation coefficient along the transect. Finally, the cold pool intensity was calculated. The results revealed none of the four most abundant classes followed classical textbook knowledge of locally produced cold-air drainage. Instead, we found that the near-surface flow was strongly forced by two possibly competing non-local flow modes. The first mode caused weak (< 0.4 ms-1) near-surface winds directed perpendicular to the local slope and

  16. Solar wind temperature observations in the outer heliosphere

    NASA Technical Reports Server (NTRS)

    Gazis, P. R.; Barnes, A.; Mihalov, J. D.; Lazarus, A. J.

    1992-01-01

    The Pioneer 10, Pioneer 11, and Voyager 2 spacecraft are now at heliocentric distances of 50, 32 and 33 AU, and heliographic latitudes of 3.5 deg N, 17 deg N, and 0 deg N, respectively. Pioneer 11 and Voyager 2 are at similar celestial longitudes, while Pioneer l0 is on the opposite side of the sun. The baselines defined by these spacecraft make it possible to resolve radial, longitudinal, and latitudinal variations of solar wind parameters. The solar wind temperature decreases with increasing heliocentric distance out to a distance of 10-15 AU. At larger heliocentric distances, this gradient disappears. These high solar wind temperatures in the outer heliosphere have persisted for at least 10 years, which suggests that they are not a solar cycle effect. The solar wind temperature varied with heliographic latitude during the most recent solar minimum. The solar wind temperature at Pioneer 11 and Voyager 2 was higher than that seen at Pioneer 10 for an extended period of time, which suggests the existence of a large-scale variation of temperature with celestial longitude, but the contribution of transient phenomena is yet to be clarified.

  17. Crowdsourcing urban air temperatures from smartphone battery temperatures

    NASA Astrophysics Data System (ADS)

    Overeem, Aart; Robinson, James C. R.; Leijnse, Hidde; Steeneveld, Gert-Jan; Horn, Berthold K. P.; Uijlenhoet, Remko

    2014-05-01

    Accurate air temperature observations in urban areas are important for meteorology and energy demand planning. They are indispensable to study the urban heat island effect and the adverse effects of high temperatures on human health. However, the availability of temperature observations in cities is often limited. Here we show that relatively accurate air temperature information for the urban canopy layer can be obtained from an alternative, nowadays omnipresent source: smartphones. In this study, battery temperatures were collected by an Android application for smartphones. It has been shown that a straightforward heat transfer model can be employed to estimate daily mean air temperatures from smartphone battery temperatures for eight major cities around the world. The results demonstrate the enormous potential of this crowdsourcing application for real-time temperature monitoring in densely populated areas. Battery temperature data were collected by users of an Android application for cell phones (opensignal.com). The application automatically sends battery temperature data to a server for storage. In this study, battery temperatures are averaged in space and time to obtain daily averaged battery temperatures for each city separately. A regression model, which can be related to a physical model, is employed to retrieve daily air temperatures from battery temperatures. The model is calibrated with observed air temperatures from a meteorological station of an airport located in or near the city. Time series of air temperatures are obtained for each city for a period of several months, where 50% of the data is for independent verification. The methodology has been applied to Buenos Aires, London, Los Angeles, Paris, Mexico City, Moscow, Rome, and Sao Paulo. The evolution of the retrieved air temperatures often correspond well with the observed ones. The mean absolute error of daily air temperatures is less than 2 degrees Celsius, and the bias is within 1 degree

  18. Non-hoop winding effect on bonding temperature of laser assisted tape winding process

    NASA Astrophysics Data System (ADS)

    Zaami, Amin; Baran, Ismet; Akkerman, Remko

    2018-05-01

    One of the advanced methods for production of thermoplastic composite methods is laser assisted tape winding (LATW). Predicting the temperature in LATW process is very important since the temperature at nip-point (bonding line through width) plays a pivotal role in a proper bonding and hence the mechanical performance. Despite the hoop-winding where the nip-point is the straight line, non-hoop winding includes a curved nip-point line. Hence, the non-hoop winding causes somewhat a different power input through laser-rays and-reflections and consequently generates unknown complex temperature profile on the curved nip-point line. Investigating the temperature at the nip-point line is the point of interest in this study. In order to understand this effect, a numerical model is proposed to capture the effect of laser-rays and their reflections on the nip-point temperature. To this end, a 3D optical model considering the objects in LATW process is considered. Then, the power distribution (absorption and reflection) from the optical analysis is used as an input (heat flux distribution) for the thermal analysis. The thermal analysis employs a fully-implicit advection-diffusion model to calculate the temperature on the surfaces. The results are examined to demonstrate the effect of winding direction on the curved nip-point line (tape width) which has not been considered in literature up to now. Furthermore, the results can be used for designing a better and more efficient setup in the LATW process.

  19. Centennial-Scale Relationship Between the Southern Hemisphere Westerly Winds and Temperature

    NASA Astrophysics Data System (ADS)

    Hodgson, D. A.; Perren, B.; Roberts, S. J.; Sime, L. C.; Verleyen, E.; Van Nieuwenhuyze, W.; Vyverman, W.

    2017-12-01

    Recent changes in the intensity and position of the Southern Hemisphere Westerly Winds (SHW) have been implicated in a number of important physical changes in the Southern High Latitudes. These include changes in the efficiency of the Southern Ocean CO2 sink through alterations in ocean circulation, the loss of Antarctic ice shelves through enhanced basal melting, changes in Antarctic sea ice extent, and warming of the Antarctic Peninsula. Many of these changes have far-reaching implications for global climate and sea level rise. Despite the importance of the SHW in global climate, our current understanding of the past and future behaviour of the westerly winds is limited by relatively few reconstructions and measurements of the SHW in their core belt over the Antarctic Circumpolar Current; the region most relevant to Southern Ocean air-sea gas exchange. The aim of this study was to reconstruct changes in the relative strength of the SHW at Marion Island, one of a small number of sub-Antarctic islands that lie in the core of the SHWs. We applied independent diatom- and geochemistry- based methods to track past changes in relative wind intensity. This mutiproxy approach provides a validation that the proxies are responding to the external forcing (the SHW) rather than local (e.g. precipitation ) or internal dynamics. Results show that that the strength of the SHW are intrinsically linked to extratropical temperatures over centennial timescales, with warmer temperatures driving stronger winds. Our findings also suggest that large variations in the path and intensity of the westerly winds are driven by relatively small variations in temperature over these timescales. This means that with continued climate warming, even in the absence of anthropogenic ozone-depletion, we should anticipate large shifts in the SHW, causing stronger, more poleward-intensified winds in the decades and centuries to come, with attendant impacts on ocean circulation, ice shelf stability, and

  20. The Use of Red Green Blue (RGB) Air Mass Imagery to Investigate the Role of Stratospheric Air in a Non-Convective Wind Event

    NASA Technical Reports Server (NTRS)

    Berndt, Emily; Zavodsky, Bradley; Molthan, Andrew; Jedlovec, Gary

    2013-01-01

    AIRS ozone and model PV analysis confirm the stratospheric air in RGB Air Mass imagery. Trajectories confirm winds south of the low were distinct from CCB driven winds. Cross sections connect the tropopause fold, downward motion, and high nearsurface winds. Comparison to conceptual models show Shapiro-Keyser features and sting jet characteristics were observed in a storm that impacted the U.S. East Coast. RGB Air Mass imagery can be used to identify stratospheric air and regions susceptible to tropopause folding and attendant non-convective winds.

  1. Winds over Japan.

    NASA Astrophysics Data System (ADS)

    Plumley, William J.

    1994-01-01

    Before World War II, weather forecasters had little knowledge of upper-air wind patterns above 20000 feet. Data were seldom avai able at these heights, and the need was not great because commercial aircraft seldom flew at these altitudes. The war in the Pacific changed all that. Wind forecasts for 30000 feet plus became urgent to support the XXI Bomber Command in its bombing mission over Japan.The U.S. Army Air Force Pacific Ocean Area (AAFPOA) placed a Weather Central in the Marianas Islands in 1944 (Saipan in 1944 and Guam in 1945) to provide forecasting support for this mission. A forecasting procedure was put into operation that combined the elements known as "single-station forecasting" and an advanced procedure that used "altirmeter corrections" to analyze upper-airdata and make prognoses. Upper-air charts were drawn for constant pressure surfaces rather than constant height surfaces. The constant pressure surfaces were tied together by means of the atmospheric temperature field represented by specific temperature anomalies between pressure surfaces. Wind forecasts over the Marianas-Japan route made use of space cross sections that provided the data to forecast winds at each 5000-ft level to 35000 ft along the mission flight path. The new procedures allowed the forecaster to construct internally consistent meteorological charts in three dimensions in regions of sparse data.Army air force pilots and their crews from the Marianas were among the first to experience the extreme wind conditions now known as the "jet stream". Air force forecasters demonstrated that, with experience, such winds could reasonably be forecast under difficult operational conditions.

  2. Trajectories of thermospheric air parcels flowing over Alaska, reconstructed from ground-based wind measurements

    NASA Astrophysics Data System (ADS)

    Dhadly, Manbharat; Conde, Mark

    2017-06-01

    It is widely presumed that the convective stability and enormous kinematic viscosity of Earth's upper thermosphere hinders development of both horizontal and vertical wind shears and other gradients. Any strong local structure (over scale sizes of several hundreds of kilometers) that might somehow form would be expected to dissipate rapidly. Air flow in such an atmosphere should be relatively simple, and transport effects only slowly disperse and mix air masses. However, our observations show that wind fields in Earth's thermosphere have much more local-scale structure than usually predicated by current modeling techniques, at least at auroral latitudes; they complicate air parcel trajectories enormously, relative to typical expectations. For tracing air parcels, we used wind measurements of an all-sky Scanning Doppler Fabry-Perot interferometer and reconstructed time-resolved two-dimensional maps of the horizontal vector wind field to infer forward and backward air parcel trajectories over time. This is the first comprehensive study to visualize the complex motions of thermospheric air parcels carried through the actual observed local-scale structures in the high-latitude winds. Results show that thermospheric air parcel transport is a very difficult observational problem, because the trajectories followed are very sensitive to the detailed features of the driving wind field. To reconstruct the actual motion of a given air parcel requires wind measurements everywhere along the trajectory followed, with spatial resolutions of 100 km or less, and temporal resolutions of a few minutes or better. Understanding such transport is important, for example, in predicting the global-scale impacts of aurorally generated composition perturbations.

  3. Wind-sea surface temperature-sea ice relationship in the Chukchi-Beaufort Seas during autumn

    NASA Astrophysics Data System (ADS)

    Zhang, Jing; Stegall, Steve T.; Zhang, Xiangdong

    2018-03-01

    Dramatic climate changes, especially the largest sea ice retreat during September and October, in the Chukchi-Beaufort Seas could be a consequence of, and further enhance, complex air-ice-sea interactions. To detect these interaction signals, statistical relationships between surface wind speed, sea surface temperature (SST), and sea ice concentration (SIC) were analyzed. The results show a negative correlation between wind speed and SIC. The relationships between wind speed and SST are complicated by the presence of sea ice, with a negative correlation over open water but a positive correlation in sea ice dominated areas. The examination of spatial structures indicates that wind speed tends to increase when approaching the ice edge from open water and the area fully covered by sea ice. The anomalous downward radiation and thermal advection, as well as their regional distribution, play important roles in shaping these relationships, though wind-driven sub-grid scale boundary layer processes may also have contributions. Considering the feedback loop involved in the wind-SST-SIC relationships, climate model experiments would be required to further untangle the underlying complex physical processes.

  4. Polyurethane foam (PUF) disks passive air samplers: wind effect on sampling rates.

    PubMed

    Tuduri, Ludovic; Harner, Tom; Hung, Hayley

    2006-11-01

    Different passive sampler housings were evaluated for their wind dampening ability and how this might translate to variability in sampler uptake rates. Polyurethane foam (PUF) disk samplers were used as the sampling medium and were exposed to a PCB-contaminated atmosphere in a wind tunnel. The effect of outside wind speed on PUF disk sampling rates was evaluated by exposing polyurethane foam (PUF) disks to a PCB-contaminated air stream in a wind tunnel over air velocities in the range 0 to 1.75 m s-1. PUF disk sampling rates increased gradually over the range 0-0.9 m s-1 at approximately 4.5-14.6 m3 d-1 and then increased sharply to approximately 42 m3 d-1 at approximately 1.75 m s-1 (sum of PCBs). The results indicate that for most field deployments the conventional 'flying saucer' housing adequately dampens the wind effect and will yield approximately time-weighted air concentrations.

  5. 10. INTERIOR VIEW OF WIND TUNNEL (1991). WrightPatterson Air ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    10. INTERIOR VIEW OF WIND TUNNEL (1991). - Wright-Patterson Air Force Base, Area B, Buildings 25 & 24,10-foot & 20-foot Wind Tunnel Complex, Northeast side of block bounded by K, G, Third, & Fifth Streets, Dayton, Montgomery County, OH

  6. 9. INTERIOR VIEW OF WIND TUNNEL (1991). WrightPatterson Air ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    9. INTERIOR VIEW OF WIND TUNNEL (1991). - Wright-Patterson Air Force Base, Area B, Buildings 25 & 24,10-foot & 20-foot Wind Tunnel Complex, Northeast side of block bounded by K, G, Third, & Fifth Streets, Dayton, Montgomery County, OH

  7. 11. INTERIOR VIEW OF WIND TUNNEL (1991). WrightPatterson Air ...

    Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey

    11. INTERIOR VIEW OF WIND TUNNEL (1991). - Wright-Patterson Air Force Base, Area B, Buildings 25 & 24,10-foot & 20-foot Wind Tunnel Complex, Northeast side of block bounded by K, G, Third, & Fifth Streets, Dayton, Montgomery County, OH

  8. Recent recovery of surface wind speed after decadal decrease: a focus on South Korea

    NASA Astrophysics Data System (ADS)

    Kim, JongChun; Paik, Kyungrock

    2015-09-01

    We investigate the multi-decadal variability of observed surface wind speed around South Korea. It is found that surface wind speed exhibits decreasing trend from mid-1950s until 2003, which is similar with the trends reported for other parts of the world. However, the decreasing trend ceases and becomes unclear since then. It is revealed that decreasing wind speed until 2003 is strongly associated with the decreasing trend of the spatial variance in both atmospheric pressure and air temperature across the East Asia for the same period. On the contrary, break of decreasing trend in surface wind speed since 2003 is associated with increasing spatial variance in surface temperature over the East Asia. Ground observation shows that surface wind speed and air temperature exhibit highly negative correlations for both summer and winter prior to 2003. However, since 2003, the correlations differ between seasons. We suggest that mechanisms behind the recent wind speed trend are different between summer and winter. This is on the basis of an interesting finding that air temperature has decreased while surface temperature has increased during winter months since 2003. We hypothesize that such contrasting temperature trends indicate more frequent movement of external cold air mass into the region since 2003. We also hypothesize that increasing summer wind speed is driven by intrusion of warm air mass into the region which is witnessed via increasing spatial variance in surface temperature across East Asia and the fact that both air and surface temperature rise together.

  9. Ceramic and coating applications in the hostile environment of a high temperature hypersonic wind tunnel. [Langley 8-foot high temperature structures tunnel

    NASA Technical Reports Server (NTRS)

    Puster, R. L.; Karns, J. R.; Vasquez, P.; Kelliher, W. C.

    1981-01-01

    A Mach 7, blowdown wind tunnel was used to investigate aerothermal structural phenomena on large to full scale high speed vehicle components. The high energy test medium, which provided a true temperature simulation of hypersonic flow at 24 to 40 km altitude, was generated by the combustion of methane with air at high pressures. Since the wind tunnel, as well as the models, must be protected from thermally induced damage, ceramics and coatings were used extensively. Coatings were used both to protect various wind tunnel components and to improve the quality of the test stream. Planned modifications for the wind tunnel included more extensive use of ceramics in order to minimize the number of active cooling systems and thus minimize the inherent operational unreliability and cost that accompanies such systems. Use of nonintrusive data acquisition techniques, such as infrared radiometry, allowed more widespread use of ceramics for models to be tested in high energy wind tunnels.

  10. An evaluation of the wind chill factor: its development and applicability.

    PubMed

    Bluestein, M

    1998-04-01

    The wind chill factor has become a standard meteorologic term in cold climates. Meteorologic charts provide wind chill temperatures meant to represent the hypothetical air temperature that would, under conditions of no wind, effect the same heat loss from unclothed human skin as does the actual combination of air temperature and wind velocity. As this wind chill factor has social and economic significance, an investigation was conducted on the development of this factor and its applicability based on modern heat transfer principles. The currently used wind chill factor was found to be based on a primitive study conducted by the U.S. Antarctic Service over 50 years ago. The resultant equation for the wind chill temperature assumes an unrealistic constant skin temperature and utilizes heat transfer coefficients that differ markedly from those obtained from equations of modern convective heat transfer methods. The combined effect of these two factors is to overestimate the effect of a given wind velocity and to predict a wind chill temperature that is too low.

  11. An Evaluation of Wind Turbine Technology at Peterson Air Force Base

    DTIC Science & Technology

    2005-03-01

    by the wind speed. Darrieus turbines are ordinarily inexpensive and are used for electricity generation and irrigation. One advantage to a...AN EVALUATION OF WIND TURBINE TECHNOLOGY...02 AN EVALUATION OF WIND TURBINE TECHNOLOGY AT PETERSON AIR FORCE BASE THESIS Presented to the Faculty Department of

  12. Comparison of Vertical Soundings and Sidewall Air Temperature Measurements in a Small Alpine Basin

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

    Whiteman, Charles D.; Eisenbach, Stefan; Pospichal, Bernhard

    2004-11-01

    Tethered balloon soundings from two sites on the floor of a 1-km diameter limestone sinkhole in the Eastern Alps are compared with pseudo-vertical temperature ‘soundings’ from three lines of temperature data loggers on the basin’s northwest, southwest and southeast sidewalls. Under stable nighttime conditions with low background winds, the pseudo-vertical profiles from all three lines were good proxies for free air temperature soundings over the basin center, with a mean nighttime cold temperature bias of about 0.4°C and a standard deviation of 0.4°C. Cold biases were highest in the upper basin where relatively warm air subsides to replace air thatmore » spills out of the basin through the lowest altitude saddle. On a windy night, standard deviations increased to 1 - 2°C. After sunrise, the varying exposures of the data loggers to sunlight made the pseudo-vertical profiles less useful as proxies for free air soundings. The good correspondence between sidewall and free air temperatures during high static stability conditions suggests that sidewall soundings will prove useful in monitoring temperatures and vertical temperature gradients in the sinkhole. The sidewall soundings can produce more frequent profiles at less cost than tethersondes or rawinsondes, and provide valuable advantages for some types of meteorological analyses.« less

  13. Using Distributed Temperature Sensing for measuring vertical temperature profiles and air temperature variance in the roughness sublayer above a forest canopy

    NASA Astrophysics Data System (ADS)

    Schilperoort, B.; Coenders, M.; Savenije, H. H. G.

    2017-12-01

    In recent years, the accuracy and resolution of Distributed Temperature Sensing (DTS) machines has increased enough to expand its use in atmospheric sciences. With DTS the temperature of a fiber optic (FO) cable can be measured with a high frequency (1 Hz) and high resolution (0.30 m), for cable lengths up to kilometers. At our measurement site, a patch of 26 to 30 m tall Douglas Fir in mixed forest, we placed FO cables vertically along a 48 m tall flux tower. This gives a high resolution vertical temperature profile above, through, and below the canopy. By using a `bare' FO cable, with a diameter of 0.25 mm, we are able to measure variations in air temperature at a very small timescale, and are able to measure a vertical profile of the air temperature variance. The vertical temperature profiles can be used to study the formation of the stable boundary layer above and in the canopy at a high resolution. It also shows that a stable layer can develop below the canopy, which is not limited to night time conditions but also occurs during daytime. The high frequency measurements can be used to study the gradient of the variance of air temperature over the height. To study how the flux tower itself affects temperature variance measurements, the `bare' FO cable can be placed horizontally under a support structure away from the flux tower. Lastly, by using the hot-wire anemometer principle with DTS, the measurements can be expanded to also include vertical wind profile.

  14. United States Air Force Academy (USAFA) Vertical Axis Wind Turbine.

    DTIC Science & Technology

    1980-09-01

    Rotors, SAND76-0131. Albuquerque: July 1977. 10. Oliver, R.C. and P.R. Nixon. "Design Procedure for Coupling Savonius and Darrieus Wind Turbines ", Air...May 17-20, 1976. -65- 16. Blackwell, B.F., R.E. Sheldahl, and L.V. Feltz. Wind Tunnel Performance Data for the Darrieus Wind Turbine with NACA 0012...a 5.8 m/s (13 mph) wind . At 100 rpm, the Darrieus turbine would be fully self-sustaining and acceleration would continue to an operating tip speed

  15. Solar wind velocity and temperature in the outer heliosphere

    NASA Technical Reports Server (NTRS)

    Gazis, P. R.; Barnes, A.; Mihalov, J. D.; Lazarus, A. J.

    1994-01-01

    At the end of 1992, the Pioneer 10, Pioneer 11, and Voyager 2 spacecraft were at heliocentric distances of 56.0, 37.3, and 39.0 AU and heliographic latitudes of 3.3 deg N, 17.4 deg N, and 8.6 deg S, respectively. Pioneer 11 and Voyager 2 are at similar celestial longitudes, while Pioneer 10 is on the opposite side of the Sun. All three spacecraft have working plasma analyzers, so intercomparison of data from these spacecraft provides important information about the global character of the solar wind in the outer heliosphere. The averaged solar wind speed continued to exhibit its well-known variation with solar cycle: Even at heliocentric distances greater than 50 AU, the average speed is highest during the declining phase of the solar cycle and lowest near solar minimum. There was a strong latitudinal gradient in solar wind speed between 3 deg and 17 deg N during the last solar minimum, but this gradient has since disappeared. The solar wind temperature declined with increasing heliocentric distance out to a heliocentric distance of at least 20 AU; this decline appeared to continue at larger heliocentric distances, but temperatures in the outer heliosphere were suprisingly high. While Pioneer 10 and Voyager 2 observed comparable solar wind temperatures, the temperature at Pioneer 11 was significantly higher, which suggests the existence of a large-scale variation of temperature with heliographic longitude. There was also some suggestion that solar wind temperatures were higher near solar minimum.

  16. Crowdsourcing urban air temperatures from smartphone battery temperatures

    NASA Astrophysics Data System (ADS)

    Overeem, A.; Robinson, J. C. R.; Leijnse, H.; Steeneveld, G. J.; Horn, B. K. P.; Uijlenhoet, R.

    2013-08-01

    Accurate air temperature observations in urban areas are important for meteorology and energy demand planning. They are indispensable to study the urban heat island effect and the adverse effects of high temperatures on human health. However, the availability of temperature observations in cities is often limited. Here we show that relatively accurate air temperature information for the urban canopy layer can be obtained from an alternative, nowadays omnipresent source: smartphones. In this study, battery temperatures were collected by an Android application for smartphones. A straightforward heat transfer model is employed to estimate daily mean air temperatures from smartphone battery temperatures for eight major cities around the world. The results demonstrate the enormous potential of this crowdsourcing application for real-time temperature monitoring in densely populated areas.

  17. Solar Wind Proton Temperature Anisotropy: Linear Theory and WIND/SWE Observations

    NASA Technical Reports Server (NTRS)

    Hellinger, P.; Travnicek, P.; Kasper, J. C.; Lazarus, A. J.

    2006-01-01

    We present a comparison between WIND/SWE observations (Kasper et al., 2006) of beta parallel to p and T perpendicular to p/T parallel to p (where beta parallel to p is the proton parallel beta and T perpendicular to p and T parallel to p are the perpendicular and parallel proton are the perpendicular and parallel proton temperatures, respectively; here parallel and perpendicular indicate directions with respect to the ambient magnetic field) and predictions of the Vlasov linear theory. In the slow solar wind, the observed proton temperature anisotropy seems to be constrained by oblique instabilities, by the mirror one and the oblique fire hose, contrary to the results of the linear theory which predicts a dominance of the proton cyclotron instability and the parallel fire hose. The fast solar wind core protons exhibit an anticorrelation between beta parallel to c and T perpendicular to c/T parallel to c (where beta parallel to c is the core proton parallel beta and T perpendicular to c and T parallel to c are the perpendicular and parallel core proton temperatures, respectively) similar to that observed in the HELIOS data (Marsch et al., 2004).

  18. Vandenberg Air Force Base Pressure Gradient Wind Study

    NASA Technical Reports Server (NTRS)

    Shafer, Jaclyn A.

    2013-01-01

    Warning category winds can adversely impact day-to-day space lift operations at Vandenberg Air Force Base (VAFB) in California. NASA's Launch Services Program and other programs at VAFB use wind forecasts issued by the 30 Operational Support Squadron Weather Flight (30 OSSWF) to determine if they need to limit activities or protect property such as a launch vehicle. The 30 OSSWF tasked the AMU to develop an automated Excel graphical user interface that includes pressure gradient thresholds between specific observing stations under different synoptic regimes to aid forecasters when issuing wind warnings. This required the AMU to determine if relationships between the variables existed.

  19. Air-sea fluxes of momentum and mass in the presence of wind waves

    NASA Astrophysics Data System (ADS)

    Zülicke, Christoph

    2010-05-01

    An air-sea interaction model (ASIM) is developed including the effect of wind waves on momentum and mass transfer. This includes the derivation of profiles of dissipation rate, flow speed and concentration from a certain height to a certain depth. Simplified assumptions on the turbulent closure, skin - bulk matching and the spectral wave model allow for an analytic treatment. Particular emphasis was put on the inclusion of primary (gravity) waves and secondary (capillary-gravity) waves. The model was tuned to match wall-flow theory and data on wave height and slope. Growing waves reduce the air-side turbulent stress and lead to an increasing drag coefficient. In the sea, breaking waves inject turbulent kinetic energy and accelerate the transfer. Cross-reference with data on wave-related momentum and energy flux, dissipation rate and transfer velocity was sufficient. The evaluation of ASIM allowed for the analytical calculation of bulk formulae for the wind-dependent gas transfer velocity including information on the air-side momentum transfer (drag coefficient) and the sea-side gas transfer (Dalton number). The following regimes have been identified: the smooth waveless regime with a transfer velocity proportional to (wind) × (diffusion)2-3, the primary wave regime with a wind speed dependence proportional to (wind)1-4 × (diffusion)1-2-(waveage)1-4 and the secondary wave regime including a more-than-linear wind speed dependence like (wind)15-8 × (diffusion)1-2 × (waveage)5-8. These findings complete the current understanding of air-sea interaction for medium winds between 2 and 20 m s^-1.

  20. Investigation of the impact of extreme air temperature on river water temperature: case study of the heat episode 2013.

    NASA Astrophysics Data System (ADS)

    Weihs, Philipp; Trimmel, Heidelinde; Goler, Robert; Formayer, Herbert; Holzapfel, Gerda; Rauch, Hans Peter

    2014-05-01

    Water stream temperature is a relevant factor for water quality since it is an important driver of water oxygen content and in turn also reduces or increases stress on the aquatic fauna. The water temperature of streams is determined by the source and inflow water temperature, by the energy balance at the stream surface and by the hydrological regime of the stream. Main factors driving the energy balance of streams are radiation balance and air temperature which influences the sensitive and latent heat flux. The present study investigates the impact of the heat episode of summer 2013 on water temperature of two lowland rivers in south eastern Austria. Within the scope of the project BIO_CLIC routine measurements of water temperature at 33 locations alongside the rivers Pinka and Lafnitz have been performed since spring 2012. In addition meteorological measurements of global shortwave and longwave radiation, air temperature, wind and air humidity have been carried out during this time. For the same time period, data of discharge and water levels of both rivers were provided by the public hydrological office. The heat episode of summer 2013 started, according to the Kysely- definition, on 18 July and lasted until 14 August. The highest air temperature ever recorded in Austria was reported on 8 August at 40.5°C. In Güssing, which is located within the project area, 40.0 °C were recorded. In the lower reaches of the river Pinka, at the station Burg the monthly mean water temperature of August 2013 was with more than 22°C, 1°C higher than the mean water temperature of the same period of the previous years. At the same station, the maximum water temperature of 27.1°C was recorded on 29 July, 9 days prior to the air temperature record. Analysis shows that at the downstream stations the main driving parameter is solar radiation whereas at the upstream stations a better correlation between air temperature and water temperature is obtained. Using the extensive data set

  1. Thermal responses and perceptions under distinct ambient temperature and wind conditions.

    PubMed

    Shimazaki, Yasuhiro; Yoshida, Atsumasa; Yamamoto, Takanori

    2015-01-01

    Wind conditions are widely recognized to influence the thermal states of humans. In this study, we investigated the relationship between wind conditions and thermal perception and energy balance in humans. The study participants were exposed for 20 min to 3 distinct ambient temperatures, wind speeds, and wind angles. During the exposure, the skin temperatures as a physiological reaction and mental reactions of the human body were measured and the energy balance was calculated based on the human thermal-load method. The results indicate that the human thermal load is an accurate indicator of human thermal states under all wind conditions. Furthermore, wind speed and direction by themselves do not account for the human thermal experience. Because of the thermoregulation that occurs to prevent heat loss and protect the core of the body, a low skin temperature was maintained and regional differences in skin temperature were detected under cool ambient conditions. Thus, the human thermal load, which represents physiological parameters such as skin-temperature change, adequately describes the mixed sensation of the human thermal experience. Copyright © 2015 Elsevier Ltd. All rights reserved.

  2. Characteristics of Wind Velocity and Temperature Change Near an Escarpment-Shaped Road Embankment

    PubMed Central

    Kim, Young-Moon; You, Ki-Pyo; You, Jang-Youl

    2014-01-01

    Artificial structures such as embankments built during the construction of highways influence the surrounding airflow. Various types of damage can occur due to changes in the wind velocity and temperature around highway embankments. However, no study has accurately measured micrometeorological changes (wind velocity and temperature) due to embankments. This study conducted a wind tunnel test and field measurement to identify changes in wind velocity and temperature before and after the construction of embankments around roads. Changes in wind velocity around an embankment after its construction were found to be influenced by the surrounding wind velocity, wind angle, and the level difference and distance from the embankment. When the level difference from the embankment was large and the distance was up to 3H, the degree of wind velocity declines was found to be large. In changes in reference wind velocities around the embankment, wind velocity increases were not proportional to the rate at which wind velocities declined. The construction of the embankment influenced surrounding temperatures. The degree of temperature change was large in locations with large level differences from the embankment at daybreak and during evening hours when wind velocity changes were small. PMID:25136681

  3. Characteristics of wind velocity and temperature change near an escarpment-shaped road embankment.

    PubMed

    Kim, Young-Moon; You, Ki-Pyo; You, Jang-Youl

    2014-01-01

    Artificial structures such as embankments built during the construction of highways influence the surrounding airflow. Various types of damage can occur due to changes in the wind velocity and temperature around highway embankments. However, no study has accurately measured micrometeorological changes (wind velocity and temperature) due to embankments. This study conducted a wind tunnel test and field measurement to identify changes in wind velocity and temperature before and after the construction of embankments around roads. Changes in wind velocity around an embankment after its construction were found to be influenced by the surrounding wind velocity, wind angle, and the level difference and distance from the embankment. When the level difference from the embankment was large and the distance was up to 3H, the degree of wind velocity declines was found to be large. In changes in reference wind velocities around the embankment, wind velocity increases were not proportional to the rate at which wind velocities declined. The construction of the embankment influenced surrounding temperatures. The degree of temperature change was large in locations with large level differences from the embankment at daybreak and during evening hours when wind velocity changes were small.

  4. Convective and radiative components of wind chill in sheep: Estimation from meteorological records

    NASA Astrophysics Data System (ADS)

    Brown, D.; Mount, L. E.

    1987-06-01

    Wind chill is defined as the excess of sensible heat loss over what would occur at zero wind speed with other conditions unchanged. Wind chill can be broken down into a part that is determined by air temperature and a radiative part that comprises wind-dependent effects on additional long-wave radiative exchange and on solar radiation (by reducing solar warming). Radiative exchange and gain from solar radiation are affected by changes that are produced by wind in both surface and fleece insulations. Coefficients are derived for (a) converting the components of sensible heat exchange (air-temperature-dependent including both convective and associated long-wave radiative, additional long-wave radiative and solar) into the components of the total heat loss that are associated with wind and (b) for calculating equivalent air temperature changes. The coefficients contain terms only in wind speed, wetting of the fleece and fleece depth; these determine the external insulation. Calculation from standard meteorological records, using Plymouth and Aberdeen in 1973 as examples, indicate that in April September 1973 at Plymouth reduction in effective solar warming constituted 28% of the 24-h total wind chill, and 7% in the other months of the year combined; at Aberdeen the corresponding percentages were 25% and 6%. Mean hour-of-day estimates for the months of April and October showed that at midday reduction in solar warming due to wind rose to the order of half the air-temperature-dependent component of wind chill, with a much smaller effect in January. For about six hours at midday in July reduction in solar warming due to wind was similar in magnitude to the air-temperature-dependent component. It is concluded that realistic estimates of wind chill cannot be obtained unless the effect of solar radiation is taken into account. Failure to include solar radiation results not only in omitting solar warming but also in omitting the effects of wind in reducing that warming. The

  5. An atlas of monthly mean distributions of SSMI surface wind speed, AVHRR/2 sea surface temperature, AMI surface wind velocity, TOPEX/POSEIDON sea surface height, and ECMWF surface wind velocity during 1993

    NASA Technical Reports Server (NTRS)

    Halpern, D.; Fu, L.; Knauss, W.; Pihos, G.; Brown, O.; Freilich, M.; Wentz, F.

    1995-01-01

    The following monthly mean global distributions for 1993 are presented with a common color scale and geographical map: 10-m height wind speed estimated from the Special Sensor Microwave Imager (SSMI) on a United States (U.S.) Air Force Defense Meteorological Satellite Program (DMSP) spacecraft; sea surface temperature estimated from the Advanced Very High Resolution Radiometer (AVHRR/2) on a U.S. National Oceanic and Atmospheric Administration (NOAA) satellite; 10-m height wind speed and direction estimated from the Active Microwave Instrument (AMI) on the European Space Agency (ESA) European Remote Sensing (ERS-1) satellite; sea surface height estimated from the joint U.S.-France Topography Experiment (TOPEX)/POSEIDON spacecraft; and 10-m height wind speed and direction produced by the European Center for Medium-Range Weather Forecasting (ECMWF). Charts of annual mean, monthly mean, and sampling distributions are displayed.

  6. The Use of Red Green Blue Air Mass Imagery to Investigate the Role of Stratospheric Air in a Non-Convective Wind Event

    NASA Technical Reports Server (NTRS)

    Berndt, E. B.; Zavodsky, B. T.; Moltham, A. L.; Folmer, M. J.; Jedlovec, G. J.

    2014-01-01

    The investigation of non-convective winds associated with passing extratropical cyclones and the formation of the sting jet in North Atlantic cyclones that impact Europe has been gaining interest. Sting jet research has been limited to North Atlantic cyclones that impact Europe because it is known to occur in Shapiro-Keyser cyclones and theory suggests it does not occur in Norwegian type cyclones. The global distribution of sting jet cyclones is unknown and questions remain as to whether cyclones with Shapiro-Keyser characteristics that impact the United States develop features similar to the sting jet. Therefore unique National Aeronautics and Space Administration (NASA) products were used to analyze an event that impacted the Northeast United States on 09 February 2013. Moderate Resolution Imaging Spectroradiometer (MODIS) Red Green Blue (RGB) Air Mass imagery and Atmospheric Infrared Sounder (AIRS) ozone data were used in conjunction with NASA's global Modern Era-Retrospective Analysis for Research and Applications (MERRA) reanalysis and higher-resolution regional 13-km Rapid Refresh (RAP) data to analyze the role of stratospheric air in producing high winds. The RGB Air Mass imagery and a new AIRS ozone anomaly product were used to confirm the presence of stratospheric air. Plan view and cross sectional plots of wind, potential vorticity, relative humidity, omega, and frontogenesis were used to analyze the relationship between stratospheric air and high surface winds during the event. Additionally, the Hybrid Single Particle Lagrangian Integrated Trajectory (HYSPLIT) model was used to plot trajectories to determine the role of the conveyor belts in producing the high winds. Analyses of new satellite products, such as the RGB Air Mass imagery, show the utility of future GOES-R products in forecasting non-convective wind events.

  7. High Lapse Rates in AIRS Retrieved Temperatures in Cold Air Outbreaks

    NASA Technical Reports Server (NTRS)

    Fetzer, Eric J.; Kahn, Brian; Olsen, Edward T.; Fishbein, Evan

    2004-01-01

    The Atmospheric Infrared Sounder (AIRS) experiment, on NASA's Aqua spacecraft, uses a combination of infrared and microwave observations to retrieve cloud and surface properties, plus temperature and water vapor profiles comparable to radiosondes throughout the troposphere, for cloud cover up to 70%. The high spectral resolution of AIRS provides sensitivity to important information about the near-surface atmosphere and underlying surface. A preliminary analysis of AIRS temperature retrievals taken during January 2003 reveals extensive areas of superadiabatic lapse rates in the lowest kilometer of the atmosphere. These areas are found predominantly east of North America over the Gulf Stream, and, off East Asia over the Kuroshio Current. Accompanying the high lapse rates are low air temperatures, large sea-air temperature differences, and low relative humidities. Imagery from a Visible / Near Infrared instrument on the AIRS experiment shows accompanying clouds. These lines of evidence all point to shallow convection in the bottom layer of a cold air mass overlying warm water, with overturning driven by heat flow from ocean to atmosphere. An examination of operational radiosondes at six coastal stations in Japan shows AIRS to be oversensitive to lower tropospheric lapse rates due to systematically warm near-surface air temperatures. The bias in near-surface air temperature is seen to be independent of sea surface temperature, however. AIRS is therefore sensitive to air-sea temperature difference, but with a warm atmospheric bias. A regression fit to radiosondes is used to correct AIRS near-surface retrieved temperatures, and thereby obtain an estimate of the true atmosphere-ocean thermal contrast in five subtropical regions across the north Pacific. Moving eastward, we show a systematic shift in this air-sea temperature differences toward more isothermal conditions. These results, while preliminary, have implications for our understanding of heat flow from ocean to

  8. Surface wind, pressure and temperature fields near tornadic and non-tornadic narrow cold-frontal rainbands

    NASA Astrophysics Data System (ADS)

    Clark, Matthew; Parker, Douglas

    2014-05-01

    Narrow cold frontal rainbands (NCFRs) occur frequently in the UK and other parts of northwest Europe. At the surface, the passage of an NCFR is often marked by a sharp wind veer, abrupt pressure increase and a rapid temperature decrease. Tornadoes and other instances of localised wind damage sometimes occur in association with meso-gamma-scale vortices (sometimes called misocyclones) that form along the zone of abrupt horizontal wind veer (and associated vertical vorticity) at the leading edge of the NCFR. Using one-minute-resolution data from a mesoscale network of automatic weather stations, surface pressure, wind and temperature fields in the vicinity of 12 NCFRs (five of which were tornadic) have been investigated. High-resolution surface analyses were obtained by mapping temporal variations in the observed parameters to equivalent spatial variations, using a system velocity determined by analysis of the radar-observed movement of NCFR precipitation segments. Substantial differences were found in the structure of surface wind and pressure fields close to tornadic and non-tornadic NCFRs. Tornadic NCFRs exhibited a large wind veer (near 90°) and strong pre- and post-frontal winds. These attributes were associated with large vertical vorticity and horizontal convergence across the front. Tornadoes typically occurred where vertical vorticity and horizontal convergence were increasing. Here, we present surface analyses from selected cases, and draw comparisons between the tornadic and non-tornadic NCFRs. Some Doppler radar observations will be presented, illustrating the development of misocyclones along parts of the NCFR that exhibit strong, and increasing, vertical vorticity stretching. The influence of the stability of the pre-frontal air on the likelihood of tornadoes will also be discussed.

  9. Air temperature recordings in infant incubators.

    PubMed Central

    Aynsley-Green, A; Roberton, N R; Rolfe, P

    1975-01-01

    Air temperatures were continuously recorded inside four incubators with proportional heating control and six incubators with on/off heating cycles, during routine use. The air temperatures in the former were constant throughout, with a gradient between the roof and above-mattress air temperature not exceeding 1 degree C. In contrast, the recordings from the latter models showed a regular cyclical oscillation, the duration of the cycle varying from 14 to 44 minutes. Each incubator had a characteristic profile. The roof air temperature could vary by as much as 7-1 degrees C and the above-mattress air temperature by as much as 2-6 degrees C during the cycle. The oscillation persisted in the air temperatures recorded inside an open-ended hemicylindrical heat shield when used inside these incubators, but was markedly reduced inside a closed-ended heat shield, Carbon dioxide concentration did not increase significantly inside the latter. Images FIG. 1 FIG. 2 PMID:1147654

  10. Relationships Between the Bulk-Skin Sea Surface Temperature Difference, Wind, and Net Air-Sea Heat Flux

    NASA Technical Reports Server (NTRS)

    Emery, William J.; Castro, Sandra L.; Lindstrom, Eric (Technical Monitor)

    2002-01-01

    The primary purpose of this project was to evaluate and improve models for the bulk-skin temperature difference to the point where they could accurately and reliably apply under a wide variety of environmental conditions. To accomplish this goal, work was conducted in three primary areas. These included production of an archive of available data sets containing measurements of the skin and bulk temperatures and associated environmental conditions, evaluation of existing skin layer models using the compiled data archive, and additional theoretical work on the development of an improved model using the data collected under diverse environmental conditions. In this work we set the basis for a new physical model of renewal type, and propose a parameterization for the temperature difference across the cool skin of the ocean in which the effects of thermal buoyancy, wind stress, and microscale breaking are all integrated by means of the appropriate renewal time scales. Ideally, we seek to obtain a model that will accurately apply under a wide variety of environmental conditions. A summary of the work in each of these areas is included in this report. A large amount of work was accomplished under the support of this grant. The grant supported the graduate studies of Sandra Castro and the preparation of her thesis which will be completed later this year. This work led to poster presentations at the 1999 American Geophysical Union Fall Meeting and 2000 IGARSS meeting. Additional work will be presented in a talk at this year's American Meteorological Society Air-Sea Interaction Meeting this May. The grant also supported Sandra Castro during a two week experiment aboard the R/P Flip (led by Dr. Andrew Jessup of the Applied Physics Laboratory) to help obtain additional shared data sets and to provide Sandra with a fundamental understanding of the physical processes needed in the models. In a related area, the funding also partially supported Dr. William Emery and Daniel

  11. Optical air data systems and methods

    NASA Technical Reports Server (NTRS)

    Spaeth, Lisa G. (Inventor); O'Brien, Martin (Inventor); Tang, Shoou-yu (Inventor); Acott, Phillip E. (Inventor); Caldwell, Loren M. (Inventor)

    2011-01-01

    Systems and methods for sensing air includes at least one, and in some embodiments three, transceivers for projecting the laser energy as laser radiation to the air. The transceivers are scanned or aligned along several different axes. Each transceiver receives laser energy as it is backscattered from the air. A computer processes signals from the transceivers to distinguish molecular scattered laser radiation from aerosol scattered laser radiation and determines air temperatures, wind speeds, and wind directions based on the scattered laser radiation. Applications of the system to wind power site evaluation, wind turbine control, traffic safety, general meteorological monitoring and airport safety are presented.

  12. The climate and air-quality benefits of wind and solar power in the United States

    NASA Astrophysics Data System (ADS)

    Millstein, Dev; Wiser, Ryan; Bolinger, Mark; Barbose, Galen

    2017-09-01

    Wind and solar energy reduce combustion-based electricity generation and provide air-quality and greenhouse gas emission benefits. These benefits vary dramatically by region and over time. From 2007 to 2015, solar and wind 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 wind and solar climate and air-quality benefits evolved during this time period. We find cumulative wind 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-trade 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 (wind) and 4.0 ¢ kWh-1 (solar).

  13. Statistical Correction of Air Temperature Forecasts for City and Road Weather Applications

    NASA Astrophysics Data System (ADS)

    Mahura, Alexander; Petersen, Claus; Sass, Bent; Gilet, Nicolas

    2014-05-01

    The method for statistical correction of air /road surface temperatures forecasts was developed based on analysis of long-term time-series of meteorological observations and forecasts (from HIgh Resolution Limited Area Model & Road Conditions Model; 3 km horizontal resolution). It has been tested for May-Aug 2012 & Oct 2012 - Mar 2013, respectively. The developed method is based mostly on forecasted meteorological parameters with a minimal inclusion of observations (covering only a pre-history period). Although the st iteration correction is based taking into account relevant temperature observations, but the further adjustment of air and road temperature forecasts is based purely on forecasted meteorological parameters. The method is model independent, e.g. it can be applied for temperature correction with other types of models having different horizontal resolutions. It is relatively fast due to application of the singular value decomposition method for matrix solution to find coefficients. Moreover, there is always a possibility for additional improvement due to extra tuning of the temperature forecasts for some locations (stations), and in particular, where for example, the MAEs are generally higher compared with others (see Gilet et al., 2014). For the city weather applications, new operationalized procedure for statistical correction of the air temperature forecasts has been elaborated and implemented for the HIRLAM-SKA model runs at 00, 06, 12, and 18 UTCs covering forecast lengths up to 48 hours. The procedure includes segments for extraction of observations and forecast data, assigning these to forecast lengths, statistical correction of temperature, one-&multi-days statistical evaluation of model performance, decision-making on using corrections by stations, interpolation, visualisation and storage/backup. Pre-operational air temperature correction runs were performed for the mainland Denmark since mid-April 2013 and shown good results. Tests also showed

  14. Growth responses of male broilers subjected to increasing air velocities at high ambient temperatures and a high dew point.

    PubMed

    Dozier, W A; Lott, B D; Branton, S L

    2005-06-01

    This study examined live performance responses of male broilers to increasing air velocity of 120 and 180 m/min reared under high cyclic temperatures (25-35-25 degrees C) with a 23 degrees C dew point from 21 to 49 d. Birds were reared in an environmental facility containing 2 wind tunnels (4 pens/tunnel) and 6 floor pens (control). At 21 d, 53 birds were placed in each pen of the wind tunnels and control group, respectively, and growth performance was determined weekly. Increasing air velocity from 120 to 180 m/min improved BW and BW gain from 29 to 35, 36 to 42, and 43 to 49 d of age leading to a cumulative advantage of 287 g in BW gain and a 10-point difference in feed conversion from 21 to 49 d of age. Subjecting birds to air velocity improved growth rate, feed consumption, and feed conversion at each weekly interval from 28 to 49 d over the control birds. These results indicate that male broilers approximating 2.0 to 3.0 kg respond to an air velocity of 180 m/min when exposed to high cyclic temperatures.

  15. Propagation Effects of Wind and Temperature on Acoustic Ground Contour Levels

    NASA Technical Reports Server (NTRS)

    Heath, Stephanie L.; McAninch, Gerry L.

    2006-01-01

    Propagation characteristics for varying wind and temperature atmospheric conditions are identified using physically-limiting propagation angles to define shadow boundary regions. These angles are graphically illustrated for various wind and temperature cases using a newly developed ray-tracing propagation code.

  16. Emissions and temperature benefits: The role of wind power in China.

    PubMed

    Duan, Hongbo

    2017-01-01

    As a non-fossil technology, wind power has an enormous advantage over coal because of its role in climate change mitigation. Therefore, it is important to investigate how substituting wind power for coal-fired electricity will affect emission reductions, changes in radiative forcing and rising temperatures, particularly in the context of emission limits. We developed an integrated methodology that includes two parts: an energy-economy-environmental (3E) integrated model and an emission-temperature response model. The former is used to simulate the dynamic relationships between economic output, wind energy and greenhouse gas (GHG) emissions; the latter is used to evaluate changes in radiative forcing and warming. Under the present development projection, wind energy cannot serve as a major force in curbing emissions, even under the strictest space-restraining scenario. China's temperature contribution to global warming will be up to 21.76% if warming is limited to 2 degrees. With the wind-for-coal power substitution, the corresponding contribution to global radiative forcing increase and temperature rise will decrease by up to 10% and 6.57%, respectively. Substituting wind power for coal-fired electricity has positive effects on emission reductions and warming control. However, wind energy alone is insufficient for climate change mitigation. It forms an important component of the renewable energy portfolio used to combat global warming. Copyright © 2016 Elsevier Inc. All rights reserved.

  17. Temporal and radial variation of the solar wind temperature-speed relationship

    NASA Astrophysics Data System (ADS)

    Elliott, H. A.; Henney, C. J.; McComas, D. J.; Smith, C. W.; Vasquez, B. J.

    2012-09-01

    The solar wind temperature (T) and speed (V) are generally well correlated at ˜1 AU, except in Interplanetary Coronal Mass Ejections where this correlation breaks down. We perform a comprehensive analysis of both the temporal and radial variation in the temperature-speed (T-V) relationship of the non-transient wind, and our analysis provides insight into both the causes of the T-V relationship and the sources of the temperature variability. Often at 1 AU the speed-temperature relationship is well represented by a single linear fit over a speed range spanning both the slow and fast wind. However, at times the fast wind from coronal holes can have a different T-V relationship than the slow wind. A good example of this was in 2003 when there was a very large and long-lived outward magnetic polarity coronal hole at low latitudes that emitted wind with speeds as fast as a polar coronal hole. The long-lived nature of the hole made it possible to clearly distinguish that some holes can have a different T-V relationship. In an earlier ACE study, we found that both the compressions and rarefactions T-V curves are linear, but the compression curve is shifted to higher temperatures. By separating compressions and rarefactions prior to determining the radial profiles of the solar wind parameters, the importance of dynamic interactions on the radial evolution of the solar wind parameters is revealed. Although the T-V relationship at 1 AU is often well described by a single linear curve, we find that the T-V relationship continually evolves with distance. Beyond ˜2.5 AU the differences between the compressions and rarefactions are quite significant and affect the shape of the overall T-V distribution to the point that a simple linear fit no longer describes the distribution well. Since additional heating of the ambient solar wind outside of interaction regions can be associated with Alfvénic fluctuations and the turbulent energy cascade, we also estimate the heating rate

  18. Retrieval of air temperatures from crowd-sourced battery temperatures of cell phones

    NASA Astrophysics Data System (ADS)

    Overeem, Aart; Robinson, James; Leijnse, Hidde; Uijlenhoet, Remko; Steeneveld, Gert-Jan; Horn, Berthold K. P.

    2013-04-01

    Accurate air temperature observations are important for urban meteorology, for example to study the urban heat island and adverse effects of high temperatures on human health. The number of available temperature observations is often relatively limited. A new development is presented to derive temperature information for the urban canopy from an alternative source: cell phones. Battery temperature data were collected by users of an Android application for cell phones (opensignal.com). The application automatically sends battery temperature data to a server for storage. In this study, battery temperatures are averaged in space and time to obtain daily averaged battery temperatures for each city separately. A regression model, which can be related to a physical model, is employed to retrieve daily air temperatures from battery temperatures. The model is calibrated with observed air temperatures from a meteorological station of an airport located in or near the city. Time series of air temperatures are obtained for each city for a period of several months, where 50% of the data is for independent verification. Results are presented for Buenos Aires, London, Los Angeles, Paris, Mexico City, Moscow, Rome, and Sao Paulo. The evolution of the retrieved air temperatures often correspond well with the observed ones. The mean absolute error of daily air temperatures is less than 2 degrees Celsius, and the bias is within 1 degree Celsius. This shows that monitoring air temperatures employing an Android application holds great promise. Since 75% of the world's population has a cell phone, 20% of the land surface of the earth has cellular telephone coverage, and 500 million devices use the Android operating system, there is a huge potential for measuring air temperatures employing cell phones. This could eventually lead to real-time world-wide temperature maps.

  19. Analysis of TIMS performance subjected to simulated wind blast

    NASA Technical Reports Server (NTRS)

    Jaggi, S.; Kuo, S.

    1992-01-01

    The results of the performance of the Thermal Infrared Multispectral Scanner (TIMS) when it is subjected to various wind conditions in the laboratory are described. Various wind conditions were simulated using a 24 inch fan or combinations of air jet streams blowing toward either or both of the blackbody surfaces. The fan was used to simulate a large volume of air flow at moderate speeds (up to 30 mph). The small diameter air jets were used to probe TIMS system response in reaction to localized wind perturbations. The maximum nozzle speed of the air jet was 60 mph. A range of wind directions and speeds were set up in the laboratory during the test. The majority of the wind tests were conducted under ambient conditions with the room temperature fluctuating no more than 2 C. The temperature of the high speed air jet was determined to be within 1 C of the room temperature. TIMS response was recorded on analog tape. Additional thermistor readouts of the blackbody temperatures and thermocouple readout of the ambient temperature were recorded manually to be compared with the housekeeping data recorded on the tape. Additional tests were conducted under conditions of elevated and cooled room temperatures. The room temperature was varied between 19.5 to 25.5 C in these tests. The calibration parameters needed for quantitative analysis of TIMS data were first plotted on a scanline-by-scanline basis. These parameters are the low and high blackbody temperature readings as recorded by the TIMS and their corresponding digitized count values. Using these values, the system transfer equations were calculated. This equation allows us to compute the flux for any video count by computing the slope and intercept of the straight line that relates the flux to the digital count. The actual video of the target (the lab floor in this case) was then compared with a simulated target. This simulated target was assumed to be a blackbody at emissivity of .95 degrees and the temperature was

  20. The effect of humidity on ionic wind velocity in ambient air

    NASA Astrophysics Data System (ADS)

    Chen, She; Nobelen, J. C. P. Y.; Nijdam, S.

    2016-09-01

    Due to the evolution of portable electronics and LED lightning system, advances in air cooling technologies must also keep pace. Active cooling by ionic wind, which is usually generated by corona discharge, can greatly reduce the noise and lifetime issues compared to the mechanical fans. The wind is induced when a gas discharge is formed, and neutral molecules gain their energy by the momentum transfer of ion-neutral collisions. However, there is few discussion about the effect of gas composition such as humidity on the wind generation and the physical mechanism is not clear. In the experiment, a positive 5-20 kV DC voltage is applied to the needle-cylinder electrodes with separation of 20 mm. The ionic wind velocity is measured by hot wire anemometry. As the relative humidity (RH) in the ambient air increases, the velocity is found to be severely inhibited. The current is also measured between the cylinder electrode and earth. The results show that the DC component of corona current decreases when RH increases. Since both the discharge current and the ion mobility are reduced when RH increases, their combined effects determine the ionic wind velocity. This work is supported by STW project 13651.

  1. Importance of air-sea interaction on wind waves, storm surge and hurricane simulations

    NASA Astrophysics Data System (ADS)

    Chen, Yingjian; Yu, Xiping

    2017-04-01

    It was reported from field observations that wind stress coefficient levels off and even decreases when the wind speed exceeds 30-40 m/s. We propose a wave boundary layer model (WBLM) based on the momentum and energy conservation equations. Taking into account the physical details of the air-sea interaction process as well as the energy dissipation due to the presence of sea spray, this model successfully predicts the decreasing tendency of wind stress coefficient. Then WBLM is embedded in the current-wave coupled model FVCOM-SWAVE to simulate surface waves and storm surge under the forcing of hurricane Katrina. Numerical results based on WBLM agree well with the observed data of NDBC buoys and tide gauges. Sensitivity analysis of different wind stress evaluation methods also shows that large anomalies of significant wave height and surge elevation are captured along the passage of hurricane core. The differences of the local wave height are up to 13 m, which is in accordance with the general knowledge that the ocean dynamic processes under storm conditions are very sensitive to the amount of momentum exchange at the air-sea interface. In the final part of the research, the reduced wind stress coefficient is tested in the numerical forecast of hurricane Katrina. A parabolic formula fitted to WBLM is employed in the atmosphere-ocean coupled model COAWST. Considering the joint effects of ocean cooling and reduced wind drag, the intensity metrics - the minimum sea level pressure and the maximum 10 m wind speed - are in good inconsistency with the best track result. Those methods, which predict the wind stress coefficient that increase or saturate in extreme wind condition, underestimate the hurricane intensity. As a whole, we unify the evaluation methods of wind stress in different numerical models and yield reasonable results. Although it is too early to conclude that WBLM is totally applicable or the drag coefficient does decrease for high wind speed, our current

  2. 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.

  3. Spatial variability of chilling temperature in Turkey and its effect on human comfort

    NASA Astrophysics Data System (ADS)

    Toros, H.; Deniz, A.; Şaylan, L.; Şen, O.; Baloğlu, M.

    2005-03-01

    Air temperature, absolute humidity and wind speed are the most important meteorological parameters that affect human thermal comfort. Because of heat loss, the human body feels air temperatures different to actual temperatures. Wind speed is the most practical element for consideration in terms of human comfort. In winter, due to the strong wind speeds, the sensible temperature is generally colder than the air temperature. This uncomfortable condition can cause problems related to tourism, heating and cooling. In this study, the spatial and temporal distributions of cooling temperatures and Wind Chill Index (WCI) are analyzed for Turkey, and their effect on the human body is considered. In this paper, monthly cooling temperatures between October and March in the years 1929 to 1990 are calculated by using measured temperature and wind speed at 79 stations in Turkey. The influence of wind chill is especially observed in the regions of the Aegean, west and middle Black Sea and east and central Anatolia. The wind chill in these regions has an uncomfortable effect on the human body. Usually, the WCI value is higher in western, northern and central Anatolia than in other regions.

  4. Air Modeling - Observational Meteorological Data

    EPA Pesticide Factsheets

    Observed meteorological data for use in air quality modeling consist of physical parameters that are measured directly by instrumentation, and include temperature, dew point, wind direction, wind speed, cloud cover, cloud layer(s), ceiling height,

  5. Voyager observations of solar wind proton temperature - 1-10 AU

    NASA Technical Reports Server (NTRS)

    Gazis, P. R.; Lazarus, A. J.

    1982-01-01

    Simultaneous measurements are made of the solar wind proton temperatures by the Voyager 1 and 2 spacecraft, far from earth, and the IMP 8 spacecraft in earth orbit. This technique permits a separation of radial and temporal variations of solar wind parameters. The average value of the proton temperature between 1 and 9 AU is observed to decrease as r (the heliocentric radius) to the -(0.7 + or - 0.2). This is slower than would be expected for adiabatic expansion. A detailed examination of the solar wind stream structure shows that considerable heating occurs at the interface between high and low speed streams.

  6. Emissions and temperature benefits: The role of wind power in China

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

    Duan, Hongbo, E-mail: hbduan@ucas.ac.cn

    Background: As a non-fossil technology, wind power has an enormous advantage over coal because of its role in climate change mitigation. Therefore, it is important to investigate how substituting wind power for coal-fired electricity will affect emission reductions, changes in radiative forcing and rising temperatures, particularly in the context of emission limits. Methods: We developed an integrated methodology that includes two parts: an energy-economy-environmental (3E) integrated model and an emission-temperature response model. The former is used to simulate the dynamic relationships between economic output, wind energy and greenhouse gas (GHG) emissions; the latter is used to evaluate changes in radiativemore » forcing and warming. Results: Under the present development projection, wind energy cannot serve as a major force in curbing emissions, even under the strictest space-restraining scenario. China's temperature contribution to global warming will be up to 21.76% if warming is limited to 2 degrees. With the wind-for-coal power substitution, the corresponding contribution to global radiative forcing increase and temperature rise will decrease by up to 10% and 6.57%, respectively. Conclusions: Substituting wind power for coal-fired electricity has positive effects on emission reductions and warming control. However, wind energy alone is insufficient for climate change mitigation. It forms an important component of the renewable energy portfolio used to combat global warming. - Highlights: • We assess the warming benefits associated with substitution of wind power for coal. • The effect of emission space limits on climate responses is deeply examined. • China is responsible for at most 21.76% of global warming given the 2-degree target. • Wind power alone may not be sufficient to face the challenge of climate change. • A fertile policy soil and an aggressive plan are necessary to boost renewables.« less

  7. Attaining a steady air stream in wind tunnels

    NASA Technical Reports Server (NTRS)

    Prandtl, L

    1933-01-01

    Many experimental arrangements of varying kind involve the problems of assuring a large, steady air stream both as to volume and to time. For this reason a separate discussion of the methods by which this is achieved should prove of particular interest. Motors and blades receive special attention and a review of existent wind tunnels is also provided.

  8. Musical Intonation of Wind Instruments and Temperature

    ERIC Educational Resources Information Center

    Zendri, G.; Valdan, M.; Gratton, L. M.; Oss, S.

    2015-01-01

    Wind musical instruments are affected in their intonation by temperature. We show how to account for these effects in a simple experiment, and provide results in languages accessible to both physics and music professionals.

  9. Musical intonation of wind instruments and temperature

    NASA Astrophysics Data System (ADS)

    Zendri, G.; Valdan, M.; Gratton, L. M.; Oss, S.

    2015-05-01

    Wind musical instruments are affected in their intonation by temperature. We show how to account for these effects in a simple experiment, and provide results in languages accessible to both physics and music professionals.

  10. Wind variability and sheltering effects on measurements and modeling of air-water exchange for a small lake

    NASA Astrophysics Data System (ADS)

    Markfort, Corey D.; Resseger, Emily; Porté-Agel, Fernando; Stefan, Heinz

    2014-05-01

    Lakes with a surface area of less than 10 km2 account for over 50% of the global cumulative lake surface water area, and make up more than 99% of the total number of global lakes, ponds, and wetlands. Within the boreal regions as well as some temperate and tropical areas, a significant proportion of land cover is characterized by lakes or wetlands, which can have a dramatic effect on land-atmosphere fluxes as well as the local and regional energy budget. Many of these small water bodies are surrounded by complex terrain and forest, which cause the wind blowing over a small lake or wetland to be highly variable. Wind mixing of the lake surface layer affects thermal stratification, surface temperature and air-water gas transfer, e.g. O2, CO2, and CH4. As the wind blows from the land to the lake, wake turbulence behind trees and other shoreline obstacles leads to a recirculation zone and enhanced turbulence. This wake flow results in the delay of the development of wind shear stress on the lake surface, and the fetch required for surface shear stress to fully develop may be ~O(1 km). Interpretation of wind measurements made on the lake is hampered by the unknown effect of wake turbulence. We present field measurements designed to quantify wind variability over a sheltered lake. The wind data and water column temperature profiles are used to evaluate a new method to quantify wind sheltering of lakes that takes into account lake size, shape and the surrounding landscape features. The model is validated against field data for 36 Minnesota lakes. Effects of non-uniform sheltering and lake shape are also demonstrated. The effects of wind sheltering must be included in lake models to determine the effect of wind-derived energy inputs on lake stratification, surface gas transfer, lake water quality, and fish habitat. These effects are also important for correctly modeling momentum, heat, moisture and trace gas flux to the atmosphere.

  11. Wind and Wind Stress Measurements in HiRes

    DTIC Science & Technology

    2008-09-30

    to design the experimental system to be conducted on R /P FLIP. Data from a past experiment are also being analyzed with respect to processes...For the HiRes experiment on R /P FLIP, the air temperature profile will be measured along with wind stress, surface heat flux, sea surface...the best as it registered the lower ambient temperature. In preparation for the HiRes experiment onboard R /P FLIP a mast prototype was built in

  12. Forecasting Cool Season Daily Peak Winds at Kennedy Space Center and Cape Canaveral Air Force Station

    NASA Technical Reports Server (NTRS)

    Barrett, Joe, III; Short, David; Roeder, William

    2008-01-01

    The expected peak wind speed for the day is an important element in the daily 24-Hour and Weekly Planning Forecasts issued by the 45th Weather Squadron (45 WS) for planning operations at Kennedy Space Center (KSC) and Cape Canaveral Air Force Station (CCAFS). The morning outlook for peak speeds also begins the warning decision process for gusts ^ 35 kt, ^ 50 kt, and ^ 60 kt from the surface to 300 ft. The 45 WS forecasters have indicated that peak wind speeds are a challenging parameter to forecast during the cool season (October-April). The 45 WS requested that the Applied Meteorology Unit (AMU) develop a tool to help them forecast the speed and timing of the daily peak and average wind, from the surface to 300 ft on KSC/CCAFS during the cool season. The tool must only use data available by 1200 UTC to support the issue time of the Planning Forecasts. Based on observations from the KSC/CCAFS wind tower network, surface observations from the Shuttle Landing Facility (SLF), and CCAFS upper-air soundings from the cool season months of October 2002 to February 2007, the AMU created multiple linear regression equations to predict the timing and speed of the daily peak wind speed, as well as the background average wind speed. Several possible predictors were evaluated, including persistence, the temperature inversion depth, strength, and wind speed at the top of the inversion, wind gust factor (ratio of peak wind speed to average wind speed), synoptic weather pattern, occurrence of precipitation at the SLF, and strongest wind in the lowest 3000 ft, 4000 ft, or 5000 ft. Six synoptic patterns were identified: 1) surface high near or over FL, 2) surface high north or east of FL, 3) surface high south or west of FL, 4) surface front approaching FL, 5) surface front across central FL, and 6) surface front across south FL. The following six predictors were selected: 1) inversion depth, 2) inversion strength, 3) wind gust factor, 4) synoptic weather pattern, 5) occurrence of

  13. An atlas of monthly mean distributions of SSMI surface wind speed, ARGOS buoy drift, AVHRR/2 sea surface temperature, and ECMWF surface wind components during 1990

    NASA Technical Reports Server (NTRS)

    Halpern, D.; Knauss, W.; Brown, O.; Wentz, F.

    1993-01-01

    The following monthly mean global distributions for 1990 are proposed with a common color scale and geographical map: 10-m height wind speed estimated from the Special Sensor Microwave Imager (SSMI) on a United States (US) Air Force Defense Meteorological Satellite Program (DMSP) spacecraft; sea surface temperature estimated from the advanced very high resolution radiometer (AVHRR/2) on a U.S. National Oceanic and Atmospheric Administration (NOAA) spacecraft; Cartesian components of free drifting buoys which are tracked by the ARGOS navigation system on NOAA satellites; and Cartesian components on the 10-m height wind vector computed by the European Center for Medium-Range Weather Forecasting (ECMWF). Charts of monthly mean value, sampling distribution, and standard deviation values are displayed. Annual mean distributions are displayed.

  14. An atlas of monthly mean distributions of SSMI surface wind speed, ARGOS buoy drift, AVHRR/2 sea surface temperature, and ECMWF surface wind components during 1991

    NASA Technical Reports Server (NTRS)

    Halpern, D.; Knauss, W.; Brown, O.; Wentz, F.

    1993-01-01

    The following monthly mean global distributions for 1991 are presented with a common color scale and geographical map: 10-m height wind speed estimated from the Special Sensor Microwave Imager (SSMI) on a United States Air Force Defense Meteorological Satellite Program (DMSP) spacecraft; sea surface temperature estimated from the advanced very high resolution radiometer (AVHRR/2) on a U.S. National Oceanic and Atmospheric Administration (NOAA) spacecraft; Cartesian components of free-drifting buoys which are tracked by the ARGOS navigation system on NOAA satellites; and Cartesian components of the 10-m height wind vector computed by the European Center for Medium-Range Weather Forecasting (ECMWF). Charts of monthly mean value, sampling distribution, and standard deviation value are displayed. Annual mean distributions are displayed.

  15. Response of water temperatures and stratification to changing climate in three lakes with different morphometry

    NASA Astrophysics Data System (ADS)

    Magee, Madeline R.; Wu, Chin H.

    2017-12-01

    Water temperatures and stratification are important drivers for ecological and water quality processes within lake systems, and changes in these with increases in air temperature and changes to wind speeds may have significant ecological consequences. To properly manage these systems under changing climate, it is important to understand the effects of increasing air temperatures and wind speed changes in lakes of different depths and surface areas. In this study, we simulate three lakes that vary in depth and surface area to elucidate the effects of the observed increasing air temperatures and decreasing wind speeds on lake thermal variables (water temperature, stratification dates, strength of stratification, and surface heat fluxes) over a century (1911-2014). For all three lakes, simulations showed that epilimnetic temperatures increased, hypolimnetic temperatures decreased, the length of the stratified season increased due to earlier stratification onset and later fall overturn, stability increased, and longwave and sensible heat fluxes at the surface increased. Overall, lake depth influences the presence of stratification, Schmidt stability, and differences in surface heat flux, while lake surface area influences differences in hypolimnion temperature, hypolimnetic heating, variability of Schmidt stability, and stratification onset and fall overturn dates. Larger surface area lakes have greater wind mixing due to increased surface momentum. Climate perturbations indicate that our larger study lakes have more variability in temperature and stratification variables than the smaller lakes, and this variability increases with larger wind speeds. For all study lakes, Pearson correlations and climate perturbation scenarios indicate that wind speed has a large effect on temperature and stratification variables, sometimes greater than changes in air temperature, and wind can act to either amplify or mitigate the effect of warmer air temperatures on lake thermal

  16. Effects of air temperature and discharge on Upper Mississippi River summer water temperatures

    USGS Publications Warehouse

    Gray, Brian R.; Robertson, Dale M.; Rogala, James T.

    2018-01-01

    Recent interest in the potential effects of climate change has prompted studies of air temperature and precipitation associations with water temperatures in rivers and streams. We examined associations between summer surface water temperatures and both air temperature and discharge for 5 reaches of the Upper Mississippi River during 1994–2011. Water–air temperature associations at a given reach approximated 1:1 when estimated under an assumption of reach independence but declined to approximately 1:2 when water temperatures were permitted to covary among reaches and were also adjusted for upstream air temperatures. Estimated water temperature–discharge associations were weak. An apparently novel feature of this study is that of addressing changes in associations between water and air temperatures when both are correlated among reaches.

  17. Warm layer and cool skin corrections for bulk water temperature measurements for air-sea interaction studies

    NASA Astrophysics Data System (ADS)

    Alappattu, Denny P.; Wang, Qing; Yamaguchi, Ryan; Lind, Richard J.; Reynolds, Mike; Christman, Adam J.

    2017-08-01

    The sea surface temperature (SST) relevant to air-sea interaction studies is the temperature immediately adjacent to the air, referred to as skin SST. Generally, SST measurements from ships and buoys are taken at depths varies from several centimeters to 5 m below the surface. These measurements, known as bulk SST, can differ from skin SST up to O(1°C). Shipboard bulk and skin SST measurements were made during the Coupled Air-Sea Processes and Electromagnetic ducting Research east coast field campaign (CASPER-East). An Infrared SST Autonomous Radiometer (ISAR) recorded skin SST, while R/V Sharp's Surface Mapping System (SMS) provided bulk SST from 1 m water depth. Since the ISAR is sensitive to sea spray and rain, missing skin SST data occurred in these conditions. However, SMS measurement is less affected by adverse weather and provided continuous bulk SST measurements. It is desirable to correct the bulk SST to obtain a good representation of the skin SST, which is the objective of this research. Bulk-skin SST difference has been examined with respect to meteorological factors associated with cool skin and diurnal warm layers. Strong influences of wind speed, diurnal effects, and net longwave radiation flux on temperature difference are noticed. A three-step scheme is established to correct for wind effect, diurnal variability, and then for dependency on net longwave radiation flux. Scheme is tested and compared to existing correction schemes. This method is able to effectively compensate for multiple factors acting to modify bulk SST measurements over the range of conditions experienced during CASPER-East.

  18. In situ observations of the influence of a large onshore wind farm on near-surface temperature, turbulence intensity and wind speed profiles

    NASA Astrophysics Data System (ADS)

    Smith, Craig M.; Barthelmie, R. J.; Pryor, S. C.

    2013-09-01

    Observations of wakes from individual wind turbines and a multi-megawatt wind energy installation in the Midwestern US indicate that directly downstream of a turbine (at a distance of 190 m, or 2.4 rotor diameters (D)), there is a clear impact on wind speed and turbulence intensity (TI) throughout the rotor swept area. However, at a downwind distance of 2.1 km (26 D downstream of the closest wind turbine) the wake of the whole wind farm is not evident. There is no significant reduction of hub-height wind speed or increase in TI especially during daytime. Thus, in high turbulence regimes even very large wind installations may have only a modest impact on downstream flow fields. No impact is observable in daytime vertical potential temperature gradients at downwind distances of >2 km, but at night the presence of the wind farm does significantly decrease the vertical gradients of potential temperature (though the profile remains stably stratified), largely by increasing the temperature at 2 m.

  19. Observing Equatorial Thermospheric Winds and Temperatures with a New Mapping Technique

    NASA Astrophysics Data System (ADS)

    Faivre, M. W.; Meriwether, J. W.; Sherwood, P.; Veliz, O.

    2005-12-01

    Application of the Fabry-Perot interferometer (FPI) at Arequipa, Peru (16.4S, 71.4 W) to measure the Doppler shifts and Doppler broadenings in the equatorial O(1D) 630-nm nightglow has resulted in numerous detections of a large-scale thermospheric phenomenon called the Midnight Temperature Maximum (MTM). A recent detector upgrade with a CCD camera has improved the accuracy of these measurements by a factor of 5. Temperature increases of 50 to 150K have been measured during nights in April and July, 2005, with error bars less than 10K after averaging in all directions. Moreover, the meridional wind measurements show evidence for a flow reversal from equatorward to poleward near local midnight for such events. A new observing strategy based upon the pioneering work of Burnside et al.[1981] maps the equatorial wind and temperature fields by observing in eight equally-spaced azimuth directions, each with a zenith angle of 60 degrees. Analysis of the data obtained with this technique gives the mean wind velocities in the meridional and zonal directions as well as the horizontal gradients of the wind field for these directions. Significant horizontal wind gradients are found for the meridional direction but not for the zonal direction. The zonal wind blows eastward throughout the night with a maximum speed of ~150 m/s near the middle of the night and then decreases towards zero just before dawn. In general, the fastest poleward meridional wind is observed near mid-evening. By the end of the night, the meridional flow tends to be more equatorward at speeds of about 50 m/s. Using the assumption that local time and longitude are equivalent over a period of 30 minutes, a map of the horizontal wind field vector field is constructed over a range of 12 degrees latitude centered at 16.5 S. Comparison between MTM nights and quiet nights (no MTM) revealed significant differences in the horizontal wind fields. Using the method of Fourier decomposition of the line-of-sight winds

  20. Cabin air temperature of parked vehicles in summer conditions: life-threatening environment for children and pets calculated by a dynamic model

    NASA Astrophysics Data System (ADS)

    Horak, Johannes; Schmerold, Ivo; Wimmer, Kurt; Schauberger, Günther

    2017-10-01

    In vehicles that are parked, no ventilation and/or air conditioning takes place. If a vehicle is exposed to direct solar radiation, an immediate temperature rise occurs. The high cabin air temperature can threaten children and animals that are left unattended in vehicles. In the USA, lethal heat strokes cause a mean death rate of 37 children per year. In addition, temperature-sensitive goods (e.g. drugs in ambulances and veterinary vehicles) can be adversely affected by high temperatures. To calculate the rise of the cabin air temperature, a dynamic model was developed that is driven by only three parameters, available at standard meteorological stations: air temperature, global radiation and wind velocity. The transition from the initial temperature to the constant equilibrium temperature depends strongly on the configuration of the vehicle, more specifically on insulation, window area and transmission of the glass, as well as on the meteorological conditions. The comparison of the model with empirical data showed good agreement. The model output can be applied to assess the heat load of children and animals as well as temperature-sensitive goods, which are transported and/or stored in a vehicle.

  1. Internal gravity wave-atmospheric wind interaction - A cause of clear air turbulence.

    NASA Technical Reports Server (NTRS)

    Bekofske, K.; Liu, V. C.

    1972-01-01

    The interaction between an internal gravity wave (IGW) and a vertical wind shear is discussed as a possible cause in the production of clear air turbulence in the free atmosphere. It is shown that under certain typical condition the interaction of an IGW with a background wind shear near a critical level provides a mechanism for depositing sufficient momentum in certain regions of the atmosphere to significantly increase the local mean wind shear and to lead to the production of turbulence.

  2. A space-based climatology of diurnal MLT tidal winds, temperatures and densities from UARS wind measurements

    NASA Astrophysics Data System (ADS)

    Svoboda, Aaron A.; Forbes, Jeffrey M.; Miyahara, Saburo

    2005-11-01

    A self-consistent global tidal climatology, useful for comparing and interpreting radar observations from different locations around the globe, is created from space-based Upper Atmosphere Research Satellite (UARS) horizontal wind measurements. The climatology created includes tidal structures for horizontal winds, temperature and relative density, and is constructed by fitting local (in latitude and height) UARS wind data at 95 km to a set of basis functions called Hough mode extensions (HMEs). These basis functions are numerically computed modifications to Hough modes and are globally self-consistent in wind, temperature, and density. We first demonstrate this self-consistency with a proxy data set from the Kyushu University General Circulation Model, and then use a linear weighted superposition of the HMEs obtained from monthly fits to the UARS data to extrapolate the global, multi-variable tidal structure. A brief explanation of the HMEs’ origin is provided as well as information about a public website that has been set up to make the full extrapolated data sets available.

  3. Air temperature gradient in large industrial hall

    NASA Astrophysics Data System (ADS)

    Karpuk, Michał; Pełech, Aleksander; Przydróżny, Edward; Walaszczyk, Juliusz; Szczęśniak, Sylwia

    2017-11-01

    In the rooms with dominant sensible heat load, volume airflow depends on many factors incl. pre-established temperature difference between exhaust and supply airflow. As the temperature difference is getting higher, airflow volume drops down, consequently, the cost of AHU is reduced. In high industrial halls with air exhaust grids located under the ceiling additional temperature gradient above working zone should be taken into consideration. In this regard, experimental research of the vertical air temperature gradient in high industrial halls were carried out for the case of mixing ventilation system The paper presents the results of air temperature distribution measurements in high technological hall (mechanically ventilated) under significant sensible heat load conditions. The supply airflow was delivered to the hall with the help of the swirl diffusers while exhaust grids were located under the hall ceiling. Basing on the air temperature distribution measurements performed on the seven pre-established levels, air temperature gradient in the area between 2.0 and 7.0 m above the floor was calculated and analysed.

  4. Vertical profiles of wind and temperature by remote acoustical sounding

    NASA Technical Reports Server (NTRS)

    Fox, H. L.

    1969-01-01

    An acoustical method was investigated for obtaining meteorological soundings based on the refraction due to the vertical variation of wind and temperature. The method has the potential of yielding horizontally averaged measurements of the vertical variation of wind and temperature up to heights of a few kilometers; the averaging takes place over a radius of 10 to 15 km. An outline of the basic concepts and some of the results obtained with the method are presented.

  5. (abstract) Ulysses Solar Wind Ion Temperatures: Radial, Latitudinal, and Dynamical Dependencies

    NASA Technical Reports Server (NTRS)

    Goldstein, B. E.; Smith, E. J.; Gosling, J. T.; McComas, D. J.; Balogh, A.

    1996-01-01

    Observations of the Ulysses SWOOPS plasma experiment are used to determine the dependencies of solar wind ion temperatures upon radial distance, speed, and other parameters, and to estimate solar wind heating. Comparisons with three dimensional temperature estimates determined from the ion spectra by a least squares fitting program will be provided (only small samples of data have been reduced with this program).

  6. Wind-chill-equivalent temperatures: regarding the impact due to the variability of the environmental convective heat transfer coefficient.

    PubMed

    Shitzer, Avraham

    2006-03-01

    The wind-chill index (WCI), developed in Antarctica in the 1940s and recently updated by the weather services in the USA and Canada, expresses the enhancement of heat loss in cold climates from exposed body parts, e.g., face, due to wind. The index provides a simple and practical means for assessing the thermal effects of wind on humans outdoors. It is also used for indicating weather conditions that may pose adverse risks of freezing at subfreezing environmental temperatures. Values of the WCI depend on a number of parameters, i.e, temperatures, physical properties of the air, wind speed, etc., and on insolation and evaporation. This paper focuses on the effects of various empirical correlations used in the literature for calculating the convective heat transfer coefficients between humans and their environment. Insolation and evaporation are not included in the presentation. Large differences in calculated values among these correlations are demonstrated and quantified. Steady-state wind-chill-equivalent temperatures (WCETs) are estimated by a simple, one-dimensional heat-conducting hollow-cylindrical model using these empirical correlations. Partial comparison of these values with the published "new" WCETs is presented. The variability of the estimated WCETs, due to different correlations employed to calculate them, is clearly demonstrated. The results of this study clearly suggest the need for establishing a "gold standard" for estimating convective heat exchange between exposed body elements and the cold and windy environment. This should be done prior to the introduction and adoption of further modifications to WCETs and indices. Correlations to estimate the convective heat transfer coefficients between exposed body parts of humans in windy and cold environments influence the WCETs and need to be standardized.

  7. 14 CFR 23.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 14 Aeronautics and Space 1 2012-01-01 2012-01-01 false Carburetor air temperature controls. 23... Powerplant Powerplant Controls and Accessories § 23.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature control for each engine. ...

  8. 14 CFR 23.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 14 Aeronautics and Space 1 2011-01-01 2011-01-01 false Carburetor air temperature controls. 23... Powerplant Powerplant Controls and Accessories § 23.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature control for each engine. ...

  9. 14 CFR 23.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2014 CFR

    2014-01-01

    ... 14 Aeronautics and Space 1 2014-01-01 2014-01-01 false Carburetor air temperature controls. 23... Powerplant Powerplant Controls and Accessories § 23.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature control for each engine. ...

  10. 14 CFR 23.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2013 CFR

    2013-01-01

    ... 14 Aeronautics and Space 1 2013-01-01 2013-01-01 false Carburetor air temperature controls. 23... Powerplant Powerplant Controls and Accessories § 23.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature control for each engine. ...

  11. 14 CFR 23.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 14 Aeronautics and Space 1 2010-01-01 2010-01-01 false Carburetor air temperature controls. 23... Powerplant Powerplant Controls and Accessories § 23.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature control for each engine. ...

  12. Winds and temperatures of the Arctic middle atmosphere during January measured by Doppler lidar

    NASA Astrophysics Data System (ADS)

    Hildebrand, Jens; Baumgarten, Gerd; Fiedler, Jens; Lübken, Franz-Josef

    2017-11-01

    We present an extensive data set of simultaneous temperature and wind measurements in the Arctic middle atmosphere. It consists of more than 300 h of Doppler Rayleigh lidar observations obtained during three January seasons (2012, 2014, and 2015) and covers the altitude range from 30 km up to about 85 km. The data set reveals large year-to-year variations in monthly mean temperatures and winds, which in 2012 are affected by a sudden stratospheric warming. The temporal evolution of winds and temperatures after that warming are studied over a period of 2 weeks, showing an elevated stratopause and the reformation of the polar vortex. The monthly mean temperatures and winds are compared to data extracted from the Integrated Forecast System of the European Centre for Medium-Range Weather Forecasts (ECMWF) and the Horizontal Wind Model (HWM07). Lidar and ECMWF data show good agreement of mean zonal and meridional winds below ≈ 55 km altitude, but we also find mean temperature, zonal wind, and meridional wind differences of up to 20 K, 20 m s-1, and 5 m s-1, respectively. Differences between lidar observations and HWM07 data are up to 30 m s-1. From the fluctuations of temperatures and winds within single nights we extract the potential and kinetic gravity wave energy density (GWED) per unit mass. It shows that the kinetic GWED is typically 5 to 10 times larger than the potential GWED, the total GWED increases with altitude with a scale height of ≈ 16 km. Since temporal fluctuations of winds and temperatures are underestimated in ECMWF, the total GWED is underestimated as well by a factor of 3-10 above 50 km altitude. Similarly, we estimate the energy density per unit mass for large-scale waves (LWED) from the fluctuations of nightly mean temperatures and winds. The total LWED is roughly constant with altitude. The ratio of kinetic to potential LWED varies with altitude over 2 orders of magnitude. LWEDs from ECMWF data show results similar to the lidar data. From the

  13. Design and optimization of resistance wire electric heater for hypersonic wind tunnel

    NASA Astrophysics Data System (ADS)

    Rehman, Khurram; Malik, Afzaal M.; Khan, I. J.; Hassan, Jehangir

    2012-06-01

    The range of flow velocities of high speed wind tunnels varies from Mach 1.0 to hypersonic order. In order to achieve such high speed flows, a high expansion nozzle is employed in the converging-diverging section of wind tunnel nozzle. The air for flow is compressed and stored in pressure vessels at temperatures close to ambient conditions. The stored air is dried and has minimum amount of moisture level. However, when this air is expanded rapidly, its temperature drops significantly and liquefaction conditions can be encountered. Air at near room temperature will liquefy due to expansion cooling at a flow velocity of more than Mach 4.0 in a wind tunnel test section. Such liquefaction may not only be hazardous to the model under test and wind tunnel structure; it may also affect the test results. In order to avoid liquefaction of air, a pre-heater is employed in between the pressure vessel and the converging-diverging section of a wind tunnel. A number of techniques are being used for heating the flow in high speed wind tunnels. Some of these include the electric arc heating, pebble bed electric heating, pebble bed natural gas fired heater, hydrogen burner heater, and the laser heater mechanisms. The most common are the pebble bed storage type heaters, which are inefficient, contaminating and time consuming. A well designed electrically heating system can be efficient, clean and simple in operation, for accelerating the wind tunnel flow up to Mach 10. This paper presents CFD analysis of electric preheater for different configurations to optimize its design. This analysis has been done using ANSYS 12.1 FLUENT package while geometry and meshing was done in GAMBIT.

  14. New results on equatorial thermospheric winds and temperatures from Ethiopia, Africa

    NASA Astrophysics Data System (ADS)

    Tesema, Fasil; Mesquita, Rafael; Meriwether, John; Damtie, Baylie; Nigussie, Melessew; Makela, Jonathan; Fisher, Daniel; Harding, Brian; Yizengaw, Endawoke; Sanders, Samuel

    2017-03-01

    Measurements of equatorial thermospheric winds, temperatures, and 630 nm relative intensities were obtained using an imaging Fabry-Perot interferometer (FPI), which was recently deployed at Bahir Dar University in Ethiopia (11.6° N, 37.4° E, 3.7° N magnetic). The results obtained in this study cover 6 months (53 nights of useable data) between November 2015 and April 2016. The monthly-averaged values, which include local winter and equinox seasons, show the magnitude of the maximum monthly-averaged zonal wind is typically within the range of 70 to 90 ms-1 and is eastward between 19:00 and 21:00 LT. Compared to prior studies of the equatorial thermospheric wind for this local time period, the magnitude is considerably weaker as compared to the maximum zonal wind speed observed in the Peruvian sector but comparable to Brazilian FPI results. During the early evening, the meridional wind speeds are 30 to 50 ms-1 poleward during the winter months and 10 to 25 ms-1 equatorward in the equinox months. The direction of the poleward wind during the winter months is believed to be mainly caused by the existence of the interhemispheric wind flow from the summer to winter hemispheres. An equatorial wind surge is observed later in the evening and is shifted to later local times during the winter months and to earlier local times during the equinox months. Significant night-to-night variations are also observed in the maximum speed of both zonal and meridional winds. The temperature observations show the midnight temperature maximum (MTM) to be generally present between 00:30 and 02:00 LT. The amplitude of the MTM was ˜ 110 K in January 2016 with values smaller than this in the other months. The local time difference between the appearance of the MTM and a pre-midnight equatorial wind was generally 60 to 180 min. A meridional wind reversal was also observed after the appearance of the MTM (after 02:00 LT). Climatological models, HWM14 and MSIS-00, were compared to the

  15. Application of fuzzy logic to the control of wind tunnel settling chamber temperature

    NASA Technical Reports Server (NTRS)

    Gwaltney, David A.; Humphreys, Gregory L.

    1994-01-01

    The application of Fuzzy Logic Controllers (FLC's) to the control of nonlinear processes, typically controlled by a human operator, is a topic of much study. Recent application of a microprocessor-based FLC to the control of temperature processes in several wind tunnels has proven to be very successful. The control of temperature processes in the wind tunnels requires the ability to monitor temperature feedback from several points and to accommodate varying operating conditions in the wind tunnels. The FLC has an intuitive and easily configurable structure which incorporates the flexibility required to have such an ability. The design and implementation of the FLC is presented along with process data from the wind tunnels under automatic control.

  16. Toward an Educational Sphereology: Air, Wind, and Materialist Pedagogy

    ERIC Educational Resources Information Center

    Ford, Derek R.; Zhao, Weili

    2018-01-01

    It's not uncommon for people to make reference to atmospheres, including in relationship with educational spaces. In this article, we investigate educational atmospheres by turning to Western and Chinese literature on the air and wind. We pursue this task in three phases. First, we examine the Western literature to see the possible strings of…

  17. Effect of real-time boundary wind conditions on the air flow and pollutant dispersion in an urban street canyon—Large eddy simulations

    NASA Astrophysics Data System (ADS)

    Zhang, Yun-Wei; Gu, Zhao-Lin; Cheng, Yan; Lee, Shun-Cheng

    2011-07-01

    Air flow and pollutant dispersion characteristics in an urban street canyon are studied under the real-time boundary conditions. A new scheme for realizing real-time boundary conditions in simulations is proposed, to keep the upper boundary wind conditions consistent with the measured time series of wind data. The air flow structure and its evolution under real-time boundary wind conditions are simulated by using this new scheme. The induced effect of time series of ambient wind conditions on the flow structures inside and above the street canyon is investigated. The flow shows an obvious intermittent feature in the street canyon and the flapping of the shear layer forms near the roof layer under real-time wind conditions, resulting in the expansion or compression of the air mass in the canyon. The simulations of pollutant dispersion show that the pollutants inside and above the street canyon are transported by different dispersion mechanisms, relying on the time series of air flow structures. Large scale air movements in the processes of the air mass expansion or compression in the canyon exhibit obvious effects on pollutant dispersion. The simulations of pollutant dispersion also show that the transport of pollutants from the canyon to the upper air flow is dominated by the shear layer turbulence near the roof level and the expansion or compression of the air mass in street canyon under real-time boundary wind conditions. Especially, the expansion of the air mass, which features the large scale air movement of the air mass, makes more contribution to the pollutant dispersion in this study. Comparisons of simulated results under different boundary wind conditions indicate that real-time boundary wind conditions produces better condition for pollutant dispersion than the artificially-designed steady boundary wind conditions.

  18. 40 CFR 91.309 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 40 Protection of Environment 20 2014-07-01 2013-07-01 true Engine intake air temperature... Provisions § 91.309 Engine intake air temperature measurement. (a) Engine intake air temperature measurement... the supply system or in the air stream entering the engine. (b) The temperature measurements must be...

  19. 40 CFR 91.309 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 40 Protection of Environment 21 2012-07-01 2012-07-01 false Engine intake air temperature... Provisions § 91.309 Engine intake air temperature measurement. (a) Engine intake air temperature measurement... the supply system or in the air stream entering the engine. (b) The temperature measurements must be...

  20. 40 CFR 91.309 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 40 Protection of Environment 21 2013-07-01 2013-07-01 false Engine intake air temperature... Provisions § 91.309 Engine intake air temperature measurement. (a) Engine intake air temperature measurement... the supply system or in the air stream entering the engine. (b) The temperature measurements must be...

  1. 40 CFR 91.309 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 40 Protection of Environment 20 2011-07-01 2011-07-01 false Engine intake air temperature... Provisions § 91.309 Engine intake air temperature measurement. (a) Engine intake air temperature measurement... the supply system or in the air stream entering the engine. (b) The temperature measurements must be...

  2. Simulating air temperature in an urban street canyon in all weather conditions using measured data at a reference meteorological station

    NASA Astrophysics Data System (ADS)

    Erell, E.; Williamson, T.

    2006-10-01

    A model is proposed that adapts data from a standard meteorological station to provide realistic site-specific air temperature in a city street exposed to the same meso-scale environment. In addition to a rudimentary description of the two sites, the canyon air temperature (CAT) model requires only inputs measured at standard weather stations; yet it is capable of accurately predicting the evolution of air temperature in all weather conditions for extended periods. It simulates the effect of urban geometry on radiant exchange; the effect of moisture availability on latent heat flux; energy stored in the ground and in building surfaces; air flow in the street based on wind above roof height; and the sensible heat flux from individual surfaces and from the street canyon as a whole. The CAT model has been tested on field data measured in a monitoring program carried out in Adelaide, Australia, in 2000-2001. After calibrating the model, predicted air temperature correlated well with measured data in all weather conditions over extended periods. The experimental validation provides additional evidence in support of a number of parameterisation schemes incorporated in the model to account for sensible heat and storage flux.

  3. 14 CFR 29.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 14 Aeronautics and Space 1 2012-01-01 2012-01-01 false Carburetor air temperature controls. 29.1157 Section 29.1157 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF... Accessories § 29.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  4. 14 CFR 25.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2012 CFR

    2012-01-01

    ... 14 Aeronautics and Space 1 2012-01-01 2012-01-01 false Carburetor air temperature controls. 25.1157 Section 25.1157 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF... Accessories § 25.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  5. 14 CFR 29.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 14 Aeronautics and Space 1 2011-01-01 2011-01-01 false Carburetor air temperature controls. 29.1157 Section 29.1157 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF... Accessories § 29.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  6. 14 CFR 25.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2011 CFR

    2011-01-01

    ... 14 Aeronautics and Space 1 2011-01-01 2011-01-01 false Carburetor air temperature controls. 25.1157 Section 25.1157 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF... Accessories § 25.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  7. 14 CFR 29.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 14 Aeronautics and Space 1 2010-01-01 2010-01-01 false Carburetor air temperature controls. 29... TRANSPORTATION AIRCRAFT AIRWORTHINESS STANDARDS: TRANSPORT CATEGORY ROTORCRAFT Powerplant Powerplant Controls and Accessories § 29.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  8. 14 CFR 25.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2010 CFR

    2010-01-01

    ... 14 Aeronautics and Space 1 2010-01-01 2010-01-01 false Carburetor air temperature controls. 25... TRANSPORTATION AIRCRAFT AIRWORTHINESS STANDARDS: TRANSPORT CATEGORY AIRPLANES Powerplant Powerplant Controls and Accessories § 25.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  9. 14 CFR 29.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2014 CFR

    2014-01-01

    ... 14 Aeronautics and Space 1 2014-01-01 2014-01-01 false Carburetor air temperature controls. 29.1157 Section 29.1157 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF... Accessories § 29.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  10. 14 CFR 29.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2013 CFR

    2013-01-01

    ... 14 Aeronautics and Space 1 2013-01-01 2013-01-01 false Carburetor air temperature controls. 29.1157 Section 29.1157 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF... Accessories § 29.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  11. 14 CFR 25.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2013 CFR

    2013-01-01

    ... 14 Aeronautics and Space 1 2013-01-01 2013-01-01 false Carburetor air temperature controls. 25.1157 Section 25.1157 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF... Accessories § 25.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  12. 14 CFR 25.1157 - Carburetor air temperature controls.

    Code of Federal Regulations, 2014 CFR

    2014-01-01

    ... 14 Aeronautics and Space 1 2014-01-01 2014-01-01 false Carburetor air temperature controls. 25.1157 Section 25.1157 Aeronautics and Space FEDERAL AVIATION ADMINISTRATION, DEPARTMENT OF... Accessories § 25.1157 Carburetor air temperature controls. There must be a separate carburetor air temperature...

  13. Effects of ambient air temperature, humidity, and wind speed on seminal traits in Braford and Nellore bulls at the Brazilian Pantanal

    NASA Astrophysics Data System (ADS)

    Menegassi, Silvio Renato Oliveira; Pereira, Gabriel Ribas; Bremm, Carolina; Koetz, Celso; Lopes, Flávio Guiselli; Fiorentini, Eduardo Custódio; McManus, Concepta; Dias, Eduardo Antunes; da Rocha, Marcela Kuczynski; Lopes, Rubia Branco; Barcellos, Júlio Otávio Jardim

    2016-11-01

    The aim of this study was to evaluate the bioclimatic thermal stress assessed by Equivalent Temperature Index (ETI) and Temperature Humidity Index (THI) on Braford and Nellore bulls sperm quality during the reproductive seasons at the tropical region in the Brazilian Pantanal. We used 20 bulls aged approximately 24 months at the beginning of the study. Five ejaculates per animal were collected using an electroejaculator. Temperature, air humidity, and wind speed data were collected every hour from the automatic weather station at the National Institute of Meteorology. Infrared thermography images data were collected to assess the testicular temperature gradient in each animal. Data were analyzed with ANOVA using MIXED procedure of SAS and means were compared using Tukey's HSD test. The THI and ETI at 12 days (epididymal transit) were higher in January (89.7 and 28.5, respectively) and February (90.0 and 29.0, respectively) compared to other months ( P < 0.01). Total seminal defects differ only in Bradford bulls between the months of November and February. Nellore bulls had lower major defects (MaD) and total defects (TD) compared to Braford. Nellore bulls showed correlation between minor defects (MiD) and THI for 30 days (0.90) and 18 days (0.88; P < 0.05). Braford bulls showed correlation for MaD (0.89) in ETI for 12 days ( P < 0.05). Infrared thermography showed no difference between animals. Reproductive response to environmental changes is a consequence of Nellore and Braford adaptation to climate stress conditions. Both THI and ETI environmental indexes can be used to evaluate the morphological changes in the seminal parameters in Nellore or Braford bulls; however, more experiments should be performed focusing on larger sample numbers and also in reproductive assessment during the consecutive years to assess fertility potential.

  14. Arctic Strato-Mesospheric Temperature and Wind Variations

    NASA Technical Reports Server (NTRS)

    Schmidlin, F. J.; Goldberg, R. A.

    2004-01-01

    Upper stratosphere and mesosphere rocket measurements are actively used to investigate interaction between the neutral, electrical, and chemical atmospheres and between lower and upper layers of these regions. Satellite temperature measurements from HALOE and from inflatable falling spheres complement each other and allow illustrations of the annual cycle to 85 km altitude. Falling sphere wind and temperature measurements reveal variability that differs as a function of altitude, location, and time. We discuss the state of the Arctic atmosphere during the summer 2002 (Andoya, Norway) and winter 2003 (ESRANGE, Sweden) campaigns of MaCWAVE. Balloon-borne profiles to 30 km altitude and sphere profiles between 50 and 90 km show unique small-scale structure. Nonetheless, there are practical implications that additional measurements are very much needed to complete the full vertical profile picture. Our discussion concentrates on the distribution of temperature and wind and their variability. However, reliable measurements from other high latitude NASA programs over a number of years are available to help properly calculate mean values and the distribution of the individual measurements. Since the available rocket data in the Arctic's upper atmosphere are sparse the results we present are basically a snapshot of atmospheric structure.

  15. A Method to Quantify the Wind and Non-wind Contribution to Year-to-year Air Quality Variation and its Application in China

    NASA Astrophysics Data System (ADS)

    LI, Y.; Lau, A. K. H.; Wong, A.; Fung, J. C. H.

    2017-12-01

    Changes in emissions and wind are often identified as the two dominant factors contributing to year-to-year variations in the concentration of primary pollutants. However, because changes in wind and emissions are intertwined, it has been difficult to quantitatively differentiate their effects on air quality directly from observed data. In particular, if the annual mean concentration of pollutants is higher than the previous year, it is difficult to identify whether the deterioration in air quality is caused by wind blowing from more polluted regions or an increase in contributing emissions. In this paper, based on wind and pollution roses, we propose a method to differentiate the effects of wind and non-wind (e.g., emissions) changes using direct observation. An index (L) is first defined to quantify the validity of the linear decomposition. The method is then validated by idealized experiments, numerical experiments and a two-year observation dataset from an actual emissions control program. Finally, we demonstrate the proposed method by studying long-term PM10 variations in Hong Kong during 2000-2011. We find that for most of the period, the linear decomposition of the changes in annual PM10 is valid (up to 90% confidence) and is dominated by the change in non-wind effects (e.g., emissions), whereas the average absolute effect from the wind variability is about 20%. Sensitivity analyses also suggest that our method should work in any location as long as the observed wind and pollution data have sufficient duration and resolution to resolve the corresponding wind and pollution roses. The method is applied for estimating the control effectiveness of the intervention programs in the Shanghai Expo, the longest socioeconomic international event held in China. The results show that integrated effect of control policies taken for improving the air quality in Shanghai are significantly effective for PM10 reduction and also effective for SO2 reduction, whereas the

  16. Peak Wind Forecasts for the Launch-Critical Wind Towers on Kennedy Space Center/Cape Canaveral Air Force Station, Phase IV

    NASA Technical Reports Server (NTRS)

    Crawford, Winifred

    2011-01-01

    This final report describes the development of a peak wind forecast tool to assist forecasters in determining the probability of violating launch commit criteria (LCC) at Kennedy Space Center (KSC) and Cape Canaveral Air Force Station (CCAFS). The peak winds arc an important forecast clement for both the Space Shuttle and Expendable Launch Vehicle (ELV) programs. The LCC define specific peak wind thresholds for each launch operation that cannot be exceeded in order to ensure the safety of the vehicle. The 45th Weather Squadron (45 WS) has found that peak winds are a challenging parameter to forecast, particularly in the cool season months of October through April. Based on the importance of forecasting peak winds, the 45 WS tasked the Applied Meteorology Unit (AMU) to update the statistics in the current peak-wind forecast tool to assist in forecasting LCC violations. The tool includes onshore and offshore flow climatologies of the 5-minute mean and peak winds and probability distributions of the peak winds as a function of the 5-minute mean wind speeds.

  17. Ocean Winds and Turbulent Air-Sea Fluxes Inferred From Remote Sensing

    NASA Technical Reports Server (NTRS)

    Bourassa, Mark A.; Gille, Sarah T.; Jackson, Daren L.; Roberts, J. Brent; Wick, Gary A.

    2010-01-01

    Air-sea turbulent fluxes determine the exchange of momentum, heat, freshwater, and gas between the atmosphere and ocean. These exchange processes are critical to a broad range of research questions spanning length scales from meters to thousands of kilometers and time scales from hours to decades. Examples are discussed (section 2). The estimation of surface turbulent fluxes from satellite is challenging and fraught with considerable errors (section 3); however, recent developments in retrievals (section 3) will greatly reduce these errors. Goals for the future observing system are summarized in section 4. Surface fluxes are defined as the rate per unit area at which something (e.g., momentum, energy, moisture, or CO Z ) is transferred across the air/sea interface. Wind- and buoyancy-driven surface fluxes are called surface turbulent fluxes because the mixing and transport are due to turbulence. Examples of nonturbulent processes are radiative fluxes (e.g., solar radiation) and precipitation (Schmitt et al., 2010). Turbulent fluxes are strongly dependent on wind speed; therefore, observations of wind speed are critical for the calculation of all turbulent surface fluxes. Wind stress, the vertical transport of horizontal momentum, also depends on wind direction. Stress is very important for many ocean processes, including upper ocean currents (Dohan and Maximenko, 2010) and deep ocean currents (Lee et al., 2010). On short time scales, this horizontal transport is usually small compared to surface fluxes. For long-term processes, transport can be very important but again is usually small compared to surface fluxes.

  18. Variation and co-variation of PM10, particle number concentration, NOx and NO2 in the urban air - Relationships with wind speed, vertical temperature gradient and weather type

    NASA Astrophysics Data System (ADS)

    Grundström, M.; Hak, C.; Chen, D.; Hallquist, M.; Pleijel, H.

    2015-11-01

    Atmospheric ultrafine particles (UFP; diameter < 0.1 μm) represent a growing global health concern in urban environments and has a strong link to traffic related emissions. UFP is usually the dominating fraction of atmospheric particle number concentrations (PNC) despite being a minor part of total particle mass. The aim of this study was to empirically investigate the relationship between PNC and other air pollutants (NOX, NO2 and PM10) in the urban environment and their dependence on meteorology and weather type, using the Lamb Weather Type (LWT) classification scheme. The study was carried out in Gothenburg, Sweden, at an urban background site during April 2007-May 2008. It was found that daily average [PNC] correlated very well with [NOx] (R2 = 0.73) during inversion days, to a lesser extent with [NO2] (R2 = 0.58) and poorly with [PM10] (R2 = 0.07). Both PNC and NOx had similar response patterns to wind speed and to the strength of temperature inversions. PNC displayed two regimes, one strongly correlated to NOx and a second poorly correlated to NOx which was characterised by high wind speed. For concentration averages based on LWTs, the PNC-[NOx] relationship remained strong (R2 = 0.70) where the windy LWT W deviated noticeably. Exclusion of observations with wind speed >5 ms-1 or ΔT < 0 °C from LWTs produced more uniform and stronger relationships (R2 = 0.90; R2 = 0.93). Low wind speeds and positive vertical temperature gradients were most common during LWTs A, NW, N and NE. These weather types were also associated with the highest daily means of NOx (∼30 ppb) and PNC (∼10 000 # cm-3). A conclusion from this study is that NOx (but not PM10) is a good proxy for PNC especially during calm and stable conditions and that LWTs A, NW, N and NE are high risk weather types for elevated NOx and PNC.

  19. Wind effect on PV module temperature: Analysis of different techniques for an accurate estimation.

    NASA Astrophysics Data System (ADS)

    Schwingshackl, Clemens; Petitta, Marcello; Ernst Wagner, Jochen; Belluardo, Giorgio; Moser, David; Castelli, Mariapina; Zebisch, Marc; Tetzlaff, Anke

    2013-04-01

    In this abstract a study on the influence of wind to model the PV module temperature is presented. This study is carried out in the framework of the PV-Alps INTERREG project in which the potential of different photovoltaic technologies is analysed for alpine regions. The PV module temperature depends on different parameters, such as ambient temperature, irradiance, wind speed and PV technology [1]. In most models, a very simple approach is used, where the PV module temperature is calculated from NOCT (nominal operating cell temperature), ambient temperature and irradiance alone [2]. In this study the influence of wind speed on the PV module temperature was investigated. First, different approaches suggested by various authors were tested [1], [2], [3], [4], [5]. For our analysis, temperature, irradiance and wind data from a PV test facility at the airport Bolzano (South Tyrol, Italy) from the EURAC Institute of Renewable Energies were used. The PV module temperature was calculated with different models and compared to the measured PV module temperature at the single panels. The best results were achieved with the approach suggested by Skoplaki et al. [1]. Preliminary results indicate that for all PV technologies which were tested (monocrystalline, amorphous, microcrystalline and polycrystalline silicon and cadmium telluride), modelled and measured PV module temperatures show a higher agreement (RMSE about 3-4 K) compared to standard approaches in which wind is not considered. For further investigation the in-situ measured wind velocities were replaced with wind data from numerical weather forecast models (ECMWF, reanalysis fields). Our results show that the PV module temperature calculated with wind data from ECMWF is still in very good agreement with the measured one (R² > 0.9 for all technologies). Compared to the previous analysis, we find comparable mean values and an increasing standard deviation. These results open a promising approach for PV module

  20. Trend analysis of air temperature and precipitation time series over Greece: 1955-2010

    NASA Astrophysics Data System (ADS)

    Marougianni, G.; Melas, D.; Kioutsioukis, I.; Feidas, H.; Zanis, P.; Anandranistakis, E.

    2012-04-01

    In this study, a database of air temperature and precipitation time series from the network of Hellenic National Meteorological Service has been developed in the framework of the project GEOCLIMA, co-financed by the European Union and Greek national funds through the Operational Program "Competitiveness and Entrepreneurship" of the Research Funding Program COOPERATION 2009. Initially, a quality test was applied to the raw data and then missing observations have been imputed with a regularized, spatial-temporal expectation - maximization algorithm to complete the climatic record. Next, a quantile - matching algorithm was applied in order to verify the homogeneity of the data. The processed time series were used for the calculation of temporal annual and seasonal trends of air temperature and precipitation. Monthly maximum and minimum surface air temperature and precipitation means at all available stations in Greece were analyzed for temporal trends and spatial variation patterns for the longest common time period of homogenous data (1955 - 2010), applying the Mann-Kendall test. The majority of the examined stations showed a significant increase in the summer maximum and minimum temperatures; this could be possibly physically linked to the Etesian winds, because of the less frequent expansion of the low over the southeastern Mediterranean. Summer minimum temperatures have been increasing at a faster rate than that of summer maximum temperatures, reflecting an asymmetric change of extreme temperature distributions. Total annual precipitation has been significantly decreased at the stations located in western Greece, as well as in the southeast, while the remaining areas exhibit a non-significant negative trend. This reduction is very likely linked to the positive phase of the NAO that resulted in an increase in the frequency and persistence of anticyclones over the Mediterranean.

  1. Prediction of facial cooling while walking in cold wind.

    PubMed

    Tikuisis, Peter; Ducharme, Michel B; Brajkovic, Dragan

    2007-09-01

    A dynamic model of cheek cooling has been modified to account for increased skin blood circulation of individuals walking in cold wind. This was achieved by modelling the cold-induced vasodilation response to cold as a varying blood perfusion term, which provided a source of convective heat to the skin tissues of the model. Physiologically-valid blood perfusion was fitted to replicate the cheek skin temperature responses of 12 individuals experimentally exposed to air temperatures from -10 to 10 degrees C at wind speeds from 2 to 8 ms(-1). Resultant cheek skin temperatures met goodness-of-fit criteria and implications on wind chill predictions are discussed.

  2. Wind-chill-equivalent temperatures: regarding the impact due to the variability of the environmental convective heat transfer coefficient

    NASA Astrophysics Data System (ADS)

    Shitzer, Avraham

    2006-03-01

    The wind-chill index (WCI), developed in Antarctica in the 1940s and recently updated by the weather services in the USA and Canada, expresses the enhancement of heat loss in cold climates from exposed body parts, e.g., face, due to wind. The index provides a simple and practical means for assessing the thermal effects of wind on humans outdoors. It is also used for indicating weather conditions that may pose adverse risks of freezing at subfreezing environmental temperatures. Values of the WCI depend on a number of parameters, i.e, temperatures, physical properties of the air, wind speed, etc., and on insolation and evaporation. This paper focuses on the effects of various empirical correlations used in the literature for calculating the convective heat transfer coefficients between humans and their environment. Insolation and evaporation are not included in the presentation. Large differences in calculated values among these correlations are demonstrated and quantified. Steady-state wind-chill-equivalent temperatures (WCETs) are estimated by a simple, one-dimensional heat-conducting hollow-cylindrical model using these empirical correlations. Partial comparison of these values with the published “new” WCETs is presented. The variability of the estimated WCETs, due to different correlations employed to calculate them, is clearly demonstrated. The results of this study clearly suggest the need for establishing a “gold standard” for estimating convective heat exchange between exposed body elements and the cold and windy environment. This should be done prior to the introduction and adoption of further modifications to WCETs and indices. Correlations to estimate the convective heat transfer coefficients between exposed body parts of humans in windy and cold environments influence the WCETs and need to be standardized.

  3. Simulation of the Impact of New Air-Based Ocean Surface Wind Measurements on H*Wind Analyses

    NASA Technical Reports Server (NTRS)

    Miller, Timothy; Atlas, Robert; Black, Peter; Case, Jonathan; Chen, Shuyi; Hood, Robbie; Jones, Linwood; Ruff, Chris; Uhlhorn, Eric

    2008-01-01

    The H'Wind analysis, a product of the Hurricane Research Division of NOAA's Atlantic Oceanographic and Meteorological Laboratory, brings together wind measurements from a variety of observation platforms into an objective analysis of the distribution of wind speeds in a tropical cyclone. This product is designed to improve understanding of the extent and strength of the wind field, and to improve the assessment of hurricane intensity. See http://www.aoml.noaa.gov/hrd/data sub/wind.html. The Hurricane Imaging Radiometer (HIRad) is a new airborne microwave remote sensor for hurricane observations that is currently under development by NASA Marshall Space Flight Center, NOAA Hurricane Research Division, the University of Central Florida and the University of Michigan. HIRad is being designed to enhance the real-time airborne ocean surface winds observation capabilities of NOAA and USAF Weather Squadron hurricane hunter aircraft using the operational airborne Stepped Frequency Microwave Radiometer (SFMR). Unlike SFMR, which measures wind speed and rain rate along the ground track directly beneath the aircraft, HIRad will provide images of the surface wind and rain field over a wide swath (approx. 3 x the aircraft altitude). The instrument is described in a paper presented to the Hurricanes and Tropical Meteorology Symposium. The present paper describes a set of Observing System Simulation Experiments (OSSEs) in which measurements from the new instrument as well as those from existing instruments (air, surface, and space-based) are simulated from the output of a numerical model from the University of Miami and those results are used to construct H*Wind analyses. Evaluations will be presented on the impact of the HIRad instrument on H'Wind analyses, both in terms of adding it to the full suite of current measurements, as well as using it to replace instrument(s) that may not be functioning at the future tame the HIRad instrument is implemented.

  4. Air/sea DMS gas transfer in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed

    NASA Astrophysics Data System (ADS)

    Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.

    2013-05-01

    Shipboard measurements of eddy covariance DMS air/sea fluxes and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas transfer coefficients (k660) show a linear dependence on mean horizontal wind speed at wind speeds up to 11 m s-1. At higher wind speeds the relationship between k660 and wind speed weakens. At high winds, measured DMS fluxes were lower than predicted based on the linear relationship between wind speed and interfacial stress extrapolated from low to intermediate wind speeds. In contrast, the transfer coefficient for sensible heat did not exhibit this effect. The apparent suppression of air/sea gas flux at higher wind speeds appears to be related to sea state, as determined from shipboard wave measurements. These observations are consistent with the idea that long waves suppress near surface water side turbulence, and decrease interfacial gas transfer. This effect may be more easily observed for DMS than for less soluble gases, such as CO2, because the air/sea exchange of DMS is controlled by interfacial rather than bubble-mediated gas transfer under high wind speed conditions.

  5. Low-temperature forced-air drying of Appalachian hardwoods

    Treesearch

    Donald G. Cuppett; E. Paul Craft

    1975-01-01

    Low-temperature forced-air drying involves drying green lumber in heated buildings with forced-air circulation and partial control of temperature and humidity conditions. The lumber is dried to about 20 percent moisture content at dry-bulb temperatures of 70º to 110ºF and with air velocities of 300 to 600 feet per minute. Equipment, methods, and...

  6. The Radial Variation of the Solar Wind Temperature-Speed Relationship

    NASA Astrophysics Data System (ADS)

    Elliott, H. A.; McComas, D. J.

    2010-12-01

    Generally, the solar wind temperature (T) and speed (V) are well correlated except in Interplanetary Coronal Mass Ejections where this correlation breaks down. We have shown that at 1 AU the speed-temperature relationship is often well represented by a linear fit for a speed range spanning both the slow and fast wind. By examining all of the ACE and OMNI measurements, we found that when coronal holes are large the fast wind can have a different T-V relationship than the slow wind. The best example of this was in 2003 when there was a very large and long-lived outward polarity coronal hole at low latitudes. The long-lived nature of the hole made it possible to clearly distinguish that large holes can have a different T-V relationship. We found it to be rare that holes are large enough and last long enough to have enough data points to clearly demonstrate this effect. In this study we compare the 2003 coronal hole observations from ACE with the Ulysses polar coronal hole measurements. In an even earlier ACE study we found that both the compressions and rarefactions curves are linear, but the compression curve is shifted to higher temperatures. In this presentation we use Helios, Ulysses, and ACE measurements to examine how the T-V relationship varies with distance. The dynamic evolution of the solar wind parameters is revealed when we first separate compressions and rarefactions and then determine the radial profiles of the solar wind parameters. We find that T-V relationship varies with distance and in particular beyond 3 AU the differences between the compressions and rarefactions are quite important and at such distances a simple linear fit does not represent the T-V distribution very well.

  7. Distinct wind convergence patterns in the Mexico City basin due to the interaction of the gap winds with the synoptic flow

    NASA Astrophysics Data System (ADS)

    de Foy, B.; Clappier, A.; Molina, L. T.; Molina, M. J.

    2006-04-01

    Mexico City lies in a high altitude basin where air quality and pollutant fate is strongly influenced by local winds. The combination of high terrain with weak synoptic forcing leads to weak and variable winds with complex circulation patterns. A gap wind entering the basin in the afternoon leads to very different wind convergence lines over the city depending on the meteorological conditions. Surface and upper-air meteorological observations are analysed during the MCMA-2003 field campaign to establish the meteorological conditions and obtain an index of the strength and timing of the gap wind. A mesoscale meteorological model (MM5) is used in combination with high-resolution satellite data for the land surface parameters and soil moisture maps derived from diurnal ground temperature range. A simple method to map the lines of wind convergence both in the basin and on the regional scale is used to show the different convergence patterns according to episode types. The gap wind is found to occur on most days of the campaign and is the result of a temperature gradient across the southern basin rim which is very similar from day to day. Momentum mixing from winds aloft into the surface layer is much more variable and can determine both the strength of the flow and the pattern of the convergence zones. Northerly flows aloft lead to a weak jet with an east-west convergence line that progresses northwards in the late afternoon and early evening. Westerlies aloft lead to both stronger gap flows due to channelling and winds over the southern and western basin rim. This results in a north-south convergence line through the middle of the basin starting in the early afternoon. Improved understanding of basin meteorology will lead to better air quality forecasts for the city and better understanding of the chemical regimes in the urban atmosphere.

  8. Comparison of MODIS Land Surface Temperature and Air Temperature over the Continental USA Meteorological Stations

    NASA Technical Reports Server (NTRS)

    Zhang, Ping; Bounoua, Lahouari; Imhoff, Marc L.; Wolfe, Robert E.; Thome, Kurtis

    2014-01-01

    The National Land Cover Database (NLCD) Impervious Surface Area (ISA) and MODIS Land Surface Temperature (LST) are used in a spatial analysis to assess the surface-temperature-based urban heat island's (UHIS) signature on LST amplitude over the continental USA and to make comparisons to local air temperatures. Air-temperature-based UHIs (UHIA), calculated using the Global Historical Climatology Network (GHCN) daily air temperatures, are compared with UHIS for urban areas in different biomes during different seasons. NLCD ISA is used to define urban and rural temperatures and to stratify the sampling for LST and air temperatures. We find that the MODIS LST agrees well with observed air temperature during the nighttime, but tends to overestimate it during the daytime, especially during summer and in nonforested areas. The minimum air temperature analyses show that UHIs in forests have an average UHIA of 1 C during the summer. The UHIS, calculated from nighttime LST, has similar magnitude of 1-2 C. By contrast, the LSTs show a midday summer UHIS of 3-4 C for cities in forests, whereas the average summer UHIA calculated from maximum air temperature is close to 0 C. In addition, the LSTs and air temperatures difference between 2006 and 2011 are in agreement, albeit with different magnitude.

  9. Wind tunnel

    NASA Technical Reports Server (NTRS)

    Wilson, E. M. (Inventor)

    1969-01-01

    A supersonic wind wind tunnel is described for testing several air foils mounted in a row. A test section of a wind tunnel contains means for mounting air foil sections in a row, means for rotating each section about an axis so that the angle of attack of each section changes with the other sections, and means for rotating the row with respect to the air stream so that the row forms an oblique angle with the air stream.

  10. Integration of Wind Turbines with Compressed Air Energy Storage

    NASA Astrophysics Data System (ADS)

    Arsie, I.; Marano, V.; Rizzo, G.; Moran, M.

    2009-08-01

    Some of the major limitations of renewable energy sources are represented by their low power density and intermittent nature, largely depending upon local site and unpredictable weather conditions. These problems concur to increase the unit costs of wind power, so limiting their diffusion. By coupling storage systems with a wind farm, some of the major limitations of wind power, such as a low power density and an unpredictable nature, can be overcome. After an overview on storage systems, the Compressed Air Energy Storage (CAES) is analyzed, and the state of art on such systems is discussed. A Matlab/Simulink model of a hybrid power plant consisting of a wind farm coupled with CAES is then presented. The model has been successfully validated starting from the operating data of the McIntosh CAES Plant in Alabama. Time-series neural network-based wind speed forecasting are employed to determine the optimal daily operation strategy for the storage system. A detailed economic analysis has been carried out: investment and maintenance costs are estimated based on literature data, while operational costs and revenues are calculated according to energy market prices. As shown in the paper, the knowledge of the expected available energy is a key factor to optimize the management strategies of the proposed hybrid power plant, allowing to obtain environmental and economic benefits.

  11. ELECTRONIC BIVANE WIND DIRECTION INDICATOR

    DOEpatents

    Moses, H.

    1961-05-01

    An apparatus is described for determining and recording three dimensional wind vectors. The apparatus comprises a rotatably mounted azimuthal wind component sensing head and an elevational wind component sensing head mounted to the azimuthal head and adapted to rotate therewith in the azimuthal plane and independently in the elevational plane. A heat source and thermocouples disposed thereabout are mounted within each of the sensing heads, the thermocouples providing electrical signals responsive to the temperature differential created by the passage of air through the sensing tuhes. The thermocouple signals are applied to drive mechanisms which position the sensing heads to a null wind position. Recording means are provided responsive to positional data from the drive mechanisms which are a measurement of the three dimensional wind vectors.

  12. The numerical modeling the sensitivity of coastal wind and ozone concentration to different SST forcing

    NASA Astrophysics Data System (ADS)

    Choi, Hyun-Jung; Lee, Hwa Woon; Jeon, Won-Bae; Lee, Soon-Hwan

    2012-01-01

    This study evaluated an atmospheric and air quality model of the spatial variability in low-level coastal winds and ozone concentration, which are affected by sea surface temperature (SST) forcing with different thermal gradients. Several numerical experiments examined the effect of sea surface SST forcing on the coastal atmosphere and air quality. In this study, the RAMS-CAMx model was used to estimate the sensitivity to two different resolutions of SST forcing during the episode day as well as to simulate the low-level coastal winds and ozone concentration over a complex coastal area. The regional model reproduced the qualitative effect of SST forcing and thermal gradients on the coastal flow. The high-resolution SST derived from NGSST-O (New Generation Sea Surface Temperature Open Ocean) forcing to resolve the warm SST appeared to enhance the mean response of low-level winds to coastal regions. These wind variations have important implications for coastal air quality. A higher ozone concentration was forecasted when SST data with a high resolution was used with the appropriate limitation of temperature, regional wind circulation, vertical mixing height and nocturnal boundary layer (NBL) near coastal areas.

  13. Analysis of vector wind change with respect to time for Vandenberg Air Force Base, California

    NASA Technical Reports Server (NTRS)

    Adelfang, S. I.

    1978-01-01

    A statistical analysis of the temporal variability of wind vectors at 1 km altitude intervals from 0 to 27 km altitude taken from a 10-year data sample of twice-daily rawinsode wind measurements over Vandenberg Air Force Base, California is presented.

  14. Simulation of ideal-gas flow by nitrogen and other selected gases at cryogenic temperatures. [transonic flow in cryogenic wind tunnels

    NASA Technical Reports Server (NTRS)

    Hall, R. M.; Adcock, J. B.

    1981-01-01

    The real gas behavior of nitrogen, the gas normally used in transonic cryogenic tunnels, is reported for the following flow processes: isentropic expansion, normal shocks, boundary layers, and interactions between shock waves and boundary layers. The only difference in predicted pressure ratio between nitrogen and an ideal gas which may limit the minimum operating temperature of transonic cryogenic wind tunnels occur at total pressures approaching 9 atm and total temperatures 10 K below the corresponding saturation temperature. These pressure differences approach 1 percent for both isentropic expansions and normal shocks. Alternative cryogenic test gases were also analyzed. Differences between air and an ideal diatomic gas are similar in magnitude to those for nitrogen and should present no difficulty. However, differences for helium and hydrogen are over an order of magnitude greater than those for nitrogen or air. It is concluded that helium and cryogenic hydrogen would not approximate the compressible flow of an ideal diatomic gas.

  15. Passive air sampling using semipermeable membrane devices at different wind-speeds in situ calibrated by performance reference compounds.

    PubMed

    Söderström, Hanna S; Bergqvist, Per-Anders

    2004-09-15

    Semipermeable membrane devices (SPMDs) are passive samplers used to measure the vapor phase of organic pollutants in air. This study tested whether extremely high wind-speeds during a 21-day sampling increased the sampling rates of polycyclic aromatic hydrocarbons (PAHs) and polychlorinated biphenyls (PCBs), and whether the release of performance reference compounds (PRCs) was related to the uptakes at different wind-speeds. Five samplers were deployed in an indoor, unheated, and dark wind tunnel with different wind-speeds at each site (6-50 m s(-1)). In addition, one sampler was deployed outside the wind tunnel and one outside the building. To test whether a sampler, designed to reduce the wind-speeds, decreased the uptake and release rates, each sampler in the wind tunnel included two SPMDs positioned inside a protective device and one unprotected SPMD outside the device. The highest amounts of PAHs and PCBs were found in the SPMDs exposed to the assumed highest wind-speeds. Thus, the SPMD sampling rates increased with increasing wind-speeds, indicating that the uptake was largely controlled by the boundary layer at the membrane-air interface. The coefficient of variance (introduced by the 21-day sampling and the chemical analysis) for the air concentrations of three PAHs and three PCBs, calculated using the PRC data, was 28-46%. Thus, the PRCs had a high ability to predict site effects of wind and assess the actual sampling situation. Comparison between protected and unprotected SPMDs showed that the sampler design reduced the wind-speed inside the devices and thereby the uptake and release rates.

  16. Estimation of Surface Air Temperature from MODIS 1km Resolution Land Surface Temperature Over Northern China

    NASA Technical Reports Server (NTRS)

    Shen, Suhung; Leptoukh, Gregory G.; Gerasimov, Irina

    2010-01-01

    Surface air temperature is a critical variable to describe the energy and water cycle of the Earth-atmosphere system and is a key input element for hydrology and land surface models. It is a very important variable in agricultural applications and climate change studies. This is a preliminary study to examine statistical relationships between ground meteorological station measured surface daily maximum/minimum air temperature and satellite remotely sensed land surface temperature from MODIS over the dry and semiarid regions of northern China. Studies were conducted for both MODIS-Terra and MODIS-Aqua by using year 2009 data. Results indicate that the relationships between surface air temperature and remotely sensed land surface temperature are statistically significant. The relationships between the maximum air temperature and daytime land surface temperature depends significantly on land surface types and vegetation index, but the minimum air temperature and nighttime land surface temperature has little dependence on the surface conditions. Based on linear regression relationship between surface air temperature and MODIS land surface temperature, surface maximum and minimum air temperatures are estimated from 1km MODIS land surface temperature under clear sky conditions. The statistical errors (sigma) of the estimated daily maximum (minimum) air temperature is about 3.8 C(3.7 C).

  17. How the Plant Temperature Links to the Air Temperature in the Desert Plant Artemisia ordosica.

    PubMed

    Yu, Ming-Han; Ding, Guo-Dong; Gao, Guang-Lei; Sun, Bao-Ping; Zhao, Yuan-Yuan; Wan, Li; Wang, De-Ying; Gui, Zi-Yang

    2015-01-01

    Plant temperature (Tp) is an important indicator of plant health. To determine the dynamics of plant temperature and self-cooling ability of the plant, we measured Tp in Artemisia ordosica in July, in the Mu Us Desert of Northwest China. Related factors were also monitored to investigate their effects on Tp, including environmental factors, such as air temperature (Ta), relative humidity, wind speed; and physiological factors, such as leaf water potential, sap flow, and water content. The results indicate that: 1) Tp generally changes in conjunction with Ta mainly, and varies with height and among the plant organs. Tp in the young branches is most constant, while it is the most sensitive in the leaves. 2) Correlations between Tp and environmental factors show that Tp is affected mainly by Ta. 3) The self-cooling ability of the plant was effective by midday, with Tp being lower than Ta. 4) Increasing sap flow and leaf water potential showed that transpiration formed part of the mechanism that supported self-cooling. Increased in water conductance and specific heat at midday may be additional factors that contribute to plant cooling ability. Therefore, our results confirmed plant self-cooling ability. The response to high temperatures is regulated by both transpiration speed and an increase in stem water conductance. This study provides quantitative data for plant management in terms of temperature control. Moreover, our findings will assist species selection with taking plant temperature as an index.

  18. Air-sea dimethylsulfide (DMS) gas transfer in the North Atlantic: evidence for limited interfacial gas exchange at high wind speed

    NASA Astrophysics Data System (ADS)

    Bell, T. G.; De Bruyn, W.; Miller, S. D.; Ward, B.; Christensen, K.; Saltzman, E. S.

    2013-11-01

    Shipboard measurements of eddy covariance dimethylsulfide (DMS) air-sea fluxes and seawater concentration were carried out in the North Atlantic bloom region in June/July 2011. Gas transfer coefficients (k660) show a linear dependence on mean horizontal wind speed at wind speeds up to 11 m s-1. At higher wind speeds the relationship between k660 and wind speed weakens. At high winds, measured DMS fluxes were lower than predicted based on the linear relationship between wind speed and interfacial stress extrapolated from low to intermediate wind speeds. In contrast, the transfer coefficient for sensible heat did not exhibit this effect. The apparent suppression of air-sea gas flux at higher wind speeds appears to be related to sea state, as determined from shipboard wave measurements. These observations are consistent with the idea that long waves suppress near-surface water-side turbulence, and decrease interfacial gas transfer. This effect may be more easily observed for DMS than for less soluble gases, such as CO2, because the air-sea exchange of DMS is controlled by interfacial rather than bubble-mediated gas transfer under high wind speed conditions.

  19. Low-latitude Temperatures, Pressures, and Winds on Saturn from Cassini Radio Occultations

    NASA Astrophysics Data System (ADS)

    Flasar, F. M.; Schinder, P. J.; Kliore, A. J.; French, R. G.; Marouf, E. A.; Nagy, A.; Rappaport, N. J.; Anabtawi, A.; Asmar, S.; Barbinis, E.; Fleischman, D. U.; Goltz, G. L.; Johnston, D. V.; Rochblatt, D.; McGhee, C. A.

    2005-12-01

    We present results from 12 ingress and egress soundings done within 10 degrees of Saturn's equator. Above the 100-mbar level, near the tropopause, the vertical profiles of temperature are marked by undulatory structure that may be associated with vertically propagating waves. Below the 200-mbar level, in the upper troposphere, the vertical profiles are smoother, and the overall trend of temperatures is to increase away from the equator. This implies a decay of the zonal winds with altitude. The zonal winds can actually be inferred directly from the meridional gradient in pressure, without the need of a boundary condition on the winds. We summarize results of these calculations. This is of interest because recent cloud tracking studies have indicated lower equatorial winds than found earlier, but whether this indicates a real change in the winds at a given altitude or a change in the altitudes of the features tracked is controversial.

  20. AIRS Retrieved Temperature Isotherms over Southern Europe

    NASA Image and Video Library

    2002-09-08

    AIRS Retrieved Temperature Isotherms over Southern Europe viewed from the west, September 8, 2002. The isotherms in this map made from AIRS onboard NASA Aqua satellite data show regions of the same temperature in the atmosphere. http://photojournal.jpl.nasa.gov/catalog/PIA00513

  1. 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 ...

  2. A generalized model for the air-sea transfer of dimethyl sulfide at high wind speeds

    NASA Astrophysics Data System (ADS)

    Vlahos, Penny; Monahan, Edward C.

    2009-11-01

    The air-sea exchange of dimethyl sulfide (DMS) is an important component of ocean biogeochemistry and global climate models. Both laboratory experiments and field measurements of DMS transfer rates have shown that the air-sea flux of DMS is analogous to that of other significant greenhouse gases such as CO2 at low wind speeds (<10 m/s) but that these DMS transfer rates may diverge from other gases as wind speeds increase. Herein we provide a mechanism that predicts the attenuation of DMS transfer rates at high wind speeds. The model is based on the amphiphilic nature of DMS that leads to transfer delay at the water-bubble interface and becomes significant at wind speeds above >10 m/s. The result is an attenuation of the dimensionless Henry's Law constant (H) where (Heff = H/(1 + (Cmix/Cw) ΦB) by a solubility enhancement Cmix/Cw, and the fraction of bubble surface area per m2 surface ocean.

  3. A 20-KW Wind Energy Conversion System (WECS) at the Marine Corps Air Station, Kaneohe, Hawaii.

    DTIC Science & Technology

    1983-01-01

    of propellers and that vertical-axis wind turbines would be more efficient. Several turbines such as the Darrieus and gyro-mill, of this type are... wind turbines , wind systems siting, alternate energy systems, remote site power generation. 20 ABSTRACT (Con!,,u,. - r r... .. do I(3 lI - d #,d e...Corps Air Station (MCAS) Kaneohe Bay, Hawaii. The wind turbine generator chosen for the evaluation was a horizontal-axis-propeller- downwind rotor

  4. Kinetic instabilities in the solar wind driven by temperature anisotropies

    NASA Astrophysics Data System (ADS)

    Yoon, Peter H.

    2017-12-01

    The present paper comprises a review of kinetic instabilities that may be operative in the solar wind, and how they influence the dynamics thereof. The review is limited to collective plasma instabilities driven by the temperature anisotropies. To limit the scope even further, the discussion is restricted to the temperature anisotropy-driven instabilities within the model of bi-Maxwellian plasma velocity distribution function. The effects of multiple particle species or the influence of field-aligned drift will not be included. The field-aligned drift or beam is particularly prominent for the solar wind electrons, and thus ignoring its effect leaves out a vast portion of important physics. Nevertheless, for the sake of limiting the scope, this effect will not be discussed. The exposition is within the context of linear and quasilinear Vlasov kinetic theories. The discussion does not cover either computer simulations or data analyses of observations, in any systematic manner, although references will be made to published works pertaining to these methods. The scientific rationale for the present analysis is that the anisotropic temperatures associated with charged particles are pervasively detected in the solar wind, and it is one of the key contemporary scientific research topics to correctly characterize how such anisotropies are generated, maintained, and regulated in the solar wind. The present article aims to provide an up-to-date theoretical development on this research topic, largely based on the author's own work.

  5. CFD simulation research on residential indoor air quality.

    PubMed

    Yang, Li; Ye, Miao; He, Bao-Jie

    2014-02-15

    Nowadays people are excessively depending on air conditioning to create a comfortable indoor environment, but it could cause some health problems in a long run. In this paper, wind velocity field, temperature field and air age field in a bedroom with wall-hanging air conditioning running in summer are analyzed by CFD numerical simulation technology. The results show that wall-hanging air conditioning system can undertake indoor heat load and conduct good indoor thermal comfort. In terms of wind velocity, air speed in activity area where people sit and stand is moderate, most of which cannot feel wind flow and meet the summer indoor wind comfort requirement. However, for air quality, there are local areas without ventilation and toxic gases not discharged in time. Therefore it is necessary to take effective measures to improve air quality. Compared with the traditional measurement method, CFD software has many advantages in simulating indoor environment, so it is hopeful for humans to create a more comfortable, healthy living environment by CFD in the future. Copyright © 2013 Elsevier B.V. All rights reserved.

  6. Consideration of Conductive Motor Winding Materials at Room and Elevated Temperatures

    NASA Technical Reports Server (NTRS)

    de Groh, Henry C., III

    2015-01-01

    A brief history of conductive motor winding materials is presented, comparing various metal motor winding materials and their properties in terms of conductivity, density and cost. The proposed use of carbon nanotubes (CNTs) and composites incorporating CNTs is explored as a potential way to improve motor winding conductivity, density, and reduce motor size which are important to electric aircraft technology. The conductivity of pure Cu, a CNT yarn, and a dilute Cu-CNT composite was measured at room temperature and at several temperatures up to 340 C. The conductivity of the Cu-CNT composite was about 3 percent lower than pure copper's at all temperatures measured. The conductivity of the CNT yarn was about 200 times lower than copper's, however, the yarn's conductivity dropped less with increasing temperature compared to Cu. It is believed that the low conductivity of the yarn is due primarily to high interfacial resistances and the presence of CNTs with low, semiconductor like electrical properties (s-CNT). It is believed the conductivity of the CNT-Cu composite could be improved by not using s-CNT, and instead using only CNTs with high, metallic like electrical properties (m-CNT); and by increasing the vol% m-CNTs.

  7. Wind driven vertical transport in a vegetated, wetland water column with air-water gas exchange

    NASA Astrophysics Data System (ADS)

    Poindexter, C.; Variano, E. A.

    2010-12-01

    Flow around arrays of cylinders at low and intermediate Reynolds numbers has been studied numerically, analytically and experimentally. Early results demonstrated that at flow around randomly oriented cylinders exhibits reduced turbulent length scales and reduced diffusivity when compared to similarly forced, unimpeded flows (Nepf 1999). While horizontal dispersion in flows through cylinder arrays has received considerable research attention, the case of vertical dispersion of reactive constituents has not. This case is relevant to the vertical transfer of dissolved gases in wetlands with emergent vegetation. We present results showing that the presence of vegetation can significantly enhance vertical transport, including gas transfer across the air-water interface. Specifically, we study a wind-sheared air-water interface in which randomly arrayed cylinders represent emergent vegetation. Wind is one of several processes that may govern physical dispersion of dissolved gases in wetlands. Wind represents the dominant force for gas transfer across the air-water interface in the ocean. Empirical relationships between wind and the gas transfer coefficient, k, have been used to estimate spatial variability of CO2 exchange across the worlds’ oceans. Because wetlands with emergent vegetation are different from oceans, different model of wind effects is needed. We investigated the vertical transport of dissolved oxygen in a scaled wetland model built inside a laboratory tank equipped with an open-ended wind tunnel. Plastic tubing immersed in water to a depth of approximately 40 cm represented emergent vegetation of cylindrical form such as hard-stem bulrush (Schoenoplectus acutus). After partially removing the oxygen from the tank water via reaction with sodium sulfite, we used an optical probe to measure dissolved oxygen at mid-depth as the tank water re-equilibrated with the air above. We used dissolved oxygen time-series for a range of mean wind speeds to estimate the

  8. 40 CFR 89.325 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... 40 Protection of Environment 21 2013-07-01 2013-07-01 false Engine intake air temperature... Test Equipment Provisions § 89.325 Engine intake air temperature measurement. (a) Engine intake air temperature measurement must be made within 122 cm of the engine. The measurement location must be made either...

  9. 40 CFR 89.325 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... 40 Protection of Environment 20 2011-07-01 2011-07-01 false Engine intake air temperature... Test Equipment Provisions § 89.325 Engine intake air temperature measurement. (a) Engine intake air temperature measurement must be made within 122 cm of the engine. The measurement location must be made either...

  10. 40 CFR 89.325 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... 40 Protection of Environment 20 2014-07-01 2013-07-01 true Engine intake air temperature... Test Equipment Provisions § 89.325 Engine intake air temperature measurement. (a) Engine intake air temperature measurement must be made within 122 cm of the engine. The measurement location must be made either...

  11. 40 CFR 89.325 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... 40 Protection of Environment 21 2012-07-01 2012-07-01 false Engine intake air temperature... Test Equipment Provisions § 89.325 Engine intake air temperature measurement. (a) Engine intake air temperature measurement must be made within 122 cm of the engine. The measurement location must be made either...

  12. Spatiotemporal structure of wind farm-atmospheric boundary layer interactions

    NASA Astrophysics Data System (ADS)

    Cervarich, Matthew; Baidya Roy, Somnath; Zhou, Liming

    2013-04-01

    Wind power is currently one of the fastest growing energy sources in the world. Most of the growth is in the utility sector consisting of large wind farms with numerous industrial-scale wind turbines. Wind turbines act as a sink of mean kinetic energy and a source of turbulent kinetic energy in the atmospheric boundary layer (ABL). In doing so, they modify the ABL profiles and land-atmosphere exchanges of energy, momentum, mass and moisture. This project explores theses interactions using remote sensing data and numerical model simulations. The domain is central Texas where 4 of the world's largest wind farms are located. A companion study of seasonally-averaged Land Surface Temperature data from the Moderate Resolution Imaging Spectroradiometer (MODIS) on TERRA and AQUA satellites shows a warming signal at night and a mixed cooling/warming signal during the daytime within the wind farms. In the present study, wind farm-ABL interactions are simulated with the Weather Research and Forecasting (WRF) model. The simulations show that the model is capable of replicating the observed signal in land surface temperature. Moreover, similar warming/cooling effect, up to 1C, was observed in seasonal mean 2m air temperature as well. Further analysis show that enhanced turbulent mixing in the rotor wakes is responsible for the impacts on 2m and surface air temperatures. The mixing is due to 2 reasons: (i) turbulent momentum transport to compensate the momentum deficit in the wakes of the turbines and (ii) turbulence generated due to motion of turbine rotors. Turbulent mixing also alters vertical profiles of moisture. Changes in land-atmosphere temperature and moisture gradient and increase in turbulent mixing leads to more than 10% change in seasonal mean surface sensible and latent heat flux. Given the current installed capacity and the projected installation across the world, wind farms are likely becoming a major driver of anthropogenic land use change on Earth. Hence

  13. Pattern recognition methods and air pollution source identification. [based on wind direction

    NASA Technical Reports Server (NTRS)

    Leibecki, H. F.; King, R. B.

    1978-01-01

    Directional air samplers, used for resolving suspended particulate matter on the basis of time and wind direction were used to assess the feasibility of characterizing and identifying emission source types in urban multisource environments. Filters were evaluated for 16 elements and X-ray fluorescence methods yielded elemental concentrations for direction, day, and the interaction of direction and day. Large numbers of samples are necessary to compensate for large day-to-day variations caused by wind perturbations and/or source changes.

  14. 40 CFR 89.325 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 40 Protection of Environment 20 2010-07-01 2010-07-01 false Engine intake air temperature measurement. 89.325 Section 89.325 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY (CONTINUED) AIR... Test Equipment Provisions § 89.325 Engine intake air temperature measurement. (a) Engine intake air...

  15. A simplified method for calculating temperature time histories in cryogenic wind tunnels

    NASA Technical Reports Server (NTRS)

    Stallings, R. L., Jr.; Lamb, M.

    1976-01-01

    Average temperature time history calculations of the test media and tunnel walls for cryogenic wind tunnels have been developed. Results are in general agreement with limited preliminary experimental measurements obtained in a 13.5-inch pilot cryogenic wind tunnel.

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

    NASA Astrophysics Data System (ADS)

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

    2017-06-01

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

  17. Sea spray contributions to the air-sea fluxes at moderate and hurricane wind speeds

    NASA Astrophysics Data System (ADS)

    Mueller, J. A.; Veron, F.

    2009-12-01

    At sufficiently high wind speed conditions, the surface of the ocean separates to form a substantial number of sea spray drops, which can account for a significant fraction of the total air-sea surface area and thus make important contributions to the aggregate air-sea momentum, heat and mass fluxes. Although consensus around the qualitative impacts of these drops has been building in recent years, the quantification of their impacts has remained elusive. Ultimately, the spray-mediated fluxes depend on three controlling factors: the number and size of drops formed at the surface, the duration of suspension within the atmospheric marine boundary layer, and the rate of momentum, heat and mass transfer between the drops and the atmosphere. While the latter factor can be estimated from an established, physically-based theory, the estimates for the former two are not well established. Using a recent, physically-based model of the sea spray source function along with the results from Lagrangian stochastic simulations of individual drops, we estimate the aggregate spray-mediated fluxes, finding reasonable agreement with existing models and estimates within the empirical range of wind speed conditions. At high wind speed conditions that are outside the empirical range, however, we find somewhat lower spray-mediated fluxes than previously reported in the literature, raising new questions about the relative air-sea fluxes at high wind speeds as well as the development and sustainment of hurricanes.

  18. 40 CFR 91.309 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... measurement. 91.309 Section 91.309 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY (CONTINUED) AIR... Provisions § 91.309 Engine intake air temperature measurement. (a) Engine intake air temperature measurement must be made within 100 cm of the air-intake of the engine. The measurement location must be either in...

  19. Wind tunnel pressurization and recovery system

    NASA Technical Reports Server (NTRS)

    Pejack, Edwin R.; Meick, Joseph; Ahmad, Adnan; Lateh, Nordin; Sadeq, Omar

    1988-01-01

    The high density, low toxicity characteristics of refrigerant-12 (dichlorofluoromethane) make it an ideal gas for wind tunnel testing. Present limitations on R-12 emissions, set to slow the rate of ozone deterioration, pose a difficult problem in recovery and handling of large quantities of R-12. This preliminary design is a possible solution to the problem of R-12 handling in wind tunnel testing. The design incorporates cold temperature condensation with secondary purification of the R-12/air mixture by adsorption. Also discussed is the use of Freon-22 as a suitable refrigerant for the 12 foot wind tunnel.

  20. NARSTO PAC2001 GVRD CAPMON AIR QUAL DATA

    Atmospheric Science Data Center

    2018-04-09

    NARSTO PAC2001 GVRD CAPMON AIR QUAL DATA Project Title:  NARSTO Discipline:  ... Order:   E arthdata Search Parameters:  Air Temperature Humidity Upper Level Winds Ozone Aerosol Particle ... Data:  Spatial Coverage: Canada Pacific 2001 Air Quality Study SCAR-B Block:  SCAR-B ...

  1. Comparison of different statistical modelling approaches for deriving spatial air temperature patterns in an urban environment

    NASA Astrophysics Data System (ADS)

    Straub, Annette; Beck, Christoph; Breitner, Susanne; Cyrys, Josef; Geruschkat, Uta; Jacobeit, Jucundus; Kühlbach, Benjamin; Kusch, Thomas; Richter, Katja; Schneider, Alexandra; Umminger, Robin; Wolf, Kathrin

    2017-04-01

    Frequently spatial variations of air temperature of considerable magnitude occur within urban areas. They correspond to varying land use/land cover characteristics and vary with season, time of day and synoptic conditions. These temperature differences have an impact on human health and comfort directly by inducing thermal stress as well as indirectly by means of affecting air quality. Therefore, knowledge of the spatial patterns of air temperature in cities and the factors causing them is of great importance, e.g. for urban planners. A multitude of studies have shown statistical modelling to be a suitable tool for generating spatial air temperature patterns. This contribution presents a comparison of different statistical modelling approaches for deriving spatial air temperature patterns in the urban environment of Augsburg, Southern Germany. In Augsburg there exists a measurement network for air temperature and humidity currently comprising 48 stations in the city and its rural surroundings (corporately operated by the Institute of Epidemiology II, Helmholtz Zentrum München, German Research Center for Environmental Health and the Institute of Geography, University of Augsburg). Using different datasets for land surface characteristics (Open Street Map, Urban Atlas) area percentages of different types of land cover were calculated for quadratic buffer zones of different size (25, 50, 100, 250, 500 m) around the stations as well for source regions of advective air flow and used as predictors together with additional variables such as sky view factor, ground level and distance from the city centre. Multiple Linear Regression and Random Forest models for different situations taking into account season, time of day and weather condition were applied utilizing selected subsets of these predictors in order to model spatial distributions of mean hourly and daily air temperature deviations from a rural reference station. Furthermore, the different model setups were

  2. Teaching Air Pollution in an Authentic Context

    NASA Astrophysics Data System (ADS)

    Mandrikas, Achilleas; Stavrou, Dimitrios; Skordoulis, Constantine

    2017-04-01

    This paper describes a teaching-learning sequence (TLS) about air pollution and the findings resulting from its implementation by pre-service elementary teachers (PET) currently undergraduate students of the Department of Primary Education in the National and Kapodistrian University of Athens, Greece. The TLS focused on the relation of air pollution with wind and topography in local conditions. An authentic context was provided to the students based on daily up-to-date meteorological data via the Internet in order to estimate air pollution. The results are encouraging given that PET can correlate wind and concentration of air pollutants through reading specialized angular diagrams and weather maps, can recognize the correlation of topography in the concentration of air pollutants, and can describe temperature inversion. However, the PET demonstrated clear difficulties in ability of orientation, in wind naming, and in interpretation of symbols on weather map. Finally, the implications on teaching air pollution are discussed.

  3. Calibrating airborne measurements of airspeed, pressure and temperature using a Doppler laser air-motion sensor

    NASA Astrophysics Data System (ADS)

    Cooper, W. A.; Spuler, S. M.; Spowart, M.; Lenschow, D. H.; Friesen, R. B.

    2014-03-01

    A new laser air-motion sensor measures the true airspeed with an uncertainty of less than 0.1 m s-1 (standard error) and so reduces uncertainty in the measured component of the relative wind along the longitudinal axis of the aircraft to about the same level. The calculated pressure expected from that airspeed at the inlet of a pitot tube then provides a basis for calibrating the measurements of dynamic and static pressure, reducing standard-error uncertainty in those measurements to less than 0.3 hPa and the precision applicable to steady flight conditions to about 0.1 hPa. These improved measurements of pressure, combined with high-resolution measurements of geometric altitude from the Global Positioning System, then indicate (via integrations of the hydrostatic equation during climbs and descents) that the offset and uncertainty in temperature measurement for one research aircraft are +0.3 ± 0.3 °C. For airspeed, pressure and temperature these are significant reductions in uncertainty vs. those obtained from calibrations using standard techniques. Finally, it is shown that the new laser air-motion sensor, combined with parametrized fits to correction factors for the measured dynamic and ambient pressure, provides a measurement of temperature that is independent of any other temperature sensor.

  4. The impact of draught related to air velocity, air temperature and workload.

    PubMed

    Griefahn, B; Künemund, C; Gehring, U

    2001-08-01

    This experimental study was designed to test the hypotheses that the effects of draught increase with higher air velocity, with lower air temperature, and with lower workload. Thirty healthy young males were exposed to horizontal draught during 55 min while they operated an arm ergometer in a standing posture. Air velocity, air temperature, and workload were varied in 3 steps each, between 11 and 23 degrees C, 0.1 and 0.3 m/s, and 104 to 156 W/m2, respectively. The 27 combinations were distributed over subjects in a fractional factorial 3(3)-design. The participants were clothed for thermal neutrality. Workload was measured at the end of the sessions by respirometry. Draught-induced annoyance was determined every 5 min, separately for 10 body sites. Corresponding skin temperature was also recorded. The hypotheses were verified for the influence of air velocity and air temperature. Regarding workload, local heat production is probably decisive, meaning that draft-induced local annoyance is inversely related to workload in active but independent from workload in non-active body areas. To improve the situation for the workers concerned it is suggested to apply protective gloves that cover an as great area of the forearms as possible and to limit airflows to mean velocities of less than 0.2 m/s (with turbulence intensities of 50%).

  5. Comparison of MODIS-derived land surface temperature with air temperature measurements

    NASA Astrophysics Data System (ADS)

    Georgiou, Andreas; Akçit, Nuhcan

    2017-09-01

    Air surface temperature is an important parameter for a wide range of applications such as agriculture, hydrology and climate change studies. Air temperature data is usually obtained from measurements made in meteorological stations, providing only limited information about spatial patterns over wide areas. The use of remote sensing data can help overcome this problem, particularly in areas with low station density, having the potential to improve the estimation of air surface temperature at both regional and global scales. Land Surface (skin) Temperatures (LST) derived from Moderate Resolution Imaging Spectroradiometer (MODIS) sensor aboard the Terra and Aqua satellite platforms provide spatial estimates of near-surface temperature values. In this study, LST values from MODIS are compared to groundbased near surface air (Tair) measurements obtained from 14 observational stations during 2011 to 2015, covering coastal, mountainous and urban areas over Cyprus. Combining Terra and Aqua LST-8 Day and Night acquisitions into a mean monthly value, provide a large number of LST observations and a better overall agreement with Tair. Comparison between mean monthly LSTs and mean monthly Tair for all sites and all seasons pooled together yields a very high correlation and biases. In addition, the presented high standard deviation can be explained by the influence of surface heterogeneity within MODIS 1km2 grid cells, the presence of undetected clouds and the inherent difference between LST and Tair. However, MODIS LST data proved to be a reliable proxy for surface temperature and mostly for studies requiring temperature reconstruction in areas with lack of observational stations.

  6. The Resistance of Spheres in Wind Tunnels and In Air

    NASA Technical Reports Server (NTRS)

    Bacon, D L; Reid, E G

    1924-01-01

    To supplement the standardization tests now in progress at several laboratories, a broad investigation of the resistance of spheres in wind tunnels and free air has been carried out by the National Advisory Committee for Aeronautics. The subject has been classed in aerodynamic research, and in consequence there is available a great mass of data from previous investigations. This material was given careful consideration in laying out the research, and explanation of practically all the disagreement between former experiments has resulted. A satisfactory confirmation of Reynolds law has been accomplished, the effect of means of support determined, the range of experiment greatly extended by work in the new variable density wind tunnel, and the effects of turbulence investigated by work in the tunnels and by towing and dropping tests in free air. It is concluded that the erratic nature of most of the previous work is due to support interference and differing turbulence conditions. While the question of support has been investigated thoroughly, a systematic and comprehensive study of the effects of scale and quality of turbulence will be necessary to complete the problem, as this phase was given only general treatment.

  7. THz limb sounder (TLS) for lower thermospheric wind, oxygen density, and temperature

    NASA Astrophysics Data System (ADS)

    Wu, Dong L.; Yee, Jeng-Hwa; Schlecht, Erich; Mehdi, Imran; Siles, Jose; Drouin, Brian J.

    2016-07-01

    Neutral winds are one of the most critical measurements in the lower thermosphere and E region ionosphere (LTEI) for understanding complex electrodynamic processes and ion-neutral interactions. We are developing a high-sensitivity, low-power, noncryogenic 2.06 THz Schottky receiver to measure wind profiles at 100-140 km. The new technique, THz limb sounder (TLS), aims to measure LTEI winds by resolving the wind-induced Doppler shift of 2.06 THz atomic oxygen (OI) emissions. As a transition between fine structure levels in the ground electronic state, the OI emission is in local thermodynamic equilibrium (LTE) at altitudes up to 350 km. This LTE property, together with day-and-night capability and small line-of-sight gradient, makes the OI limb sounding a very attractive technique for neutral wind observations. In addition to the wind measurement, TLS can also retrieve [OI] density and neutral temperature in the LTEI region. TLS leverages rapid advances in THz receiver technologies including subharmonically pumped (SHP) mixers and Schottky-diode-based power multipliers. Current SHP Schottky receivers have produced good sensitivity for THz frequencies at ambient environment temperatures (120-150 K), which are achievable through passively cooling in spaceflight. As an emerging technique, TLS can fill the critical data gaps in the LTEI neutral wind observations to enable detailed studies on the coupling and dynamo processes between charged and neutral molecules.

  8. THz Limb Sounder (TLS) for Lower Thermospheric Wind, Oxygen Density, and Temperature

    NASA Technical Reports Server (NTRS)

    Wu, Dong L.; Yee, Jeng-Hwa; Schlecht, Erich; Mehdi, Imran; Siles, Jose; Drouin, Brian J.

    2016-01-01

    Neutral winds are one of the most critical measurements in the lower thermosphere and E region ionosphere (LTEI) for understanding complex electrodynamic processes and ion-neutral interactions. We are developing a high-sensitivity, low-power, noncryogenic 2.06 THz Schottky receiver to measure wind profiles at 100-140 km. The new technique, THz limb sounder (TLS), aims to measure LTEI winds by resolving the wind-induced Doppler shift of 2.06 THz atomic oxygen (OI) emissions. As a transition between fine structure levels in the ground electronic state, the OI emission is in local thermodynamic equilibrium(LTE) at altitudes up to 350km. This LTE property, together with day-and-night capability and small line-of-sight gradient, makes the OI limb sounding a very attractive technique for neutral wind observations. In addition to the wind measurement, TLS can also retrieve [OI] density and neutral temperature in the LTEI region. TLS leverages rapid advances in THz receiver technologies including subharmonically pumped (SHP)mixers and Schottky-diode-based power multipliers. Current SHP Schottky receivers have produced good sensitivity for THz frequencies at ambient environment temperatures (120-150 K), which are achievable through passively cooling in spaceflight. As an emerging technique, TLS can fill the critical data gaps in the LTEI neutral wind observations to enable detailed studies on the coupling and dynamo processes between charged and neutral molecules.

  9. Calibrating airborne measurements of airspeed, pressure and temperature using a Doppler laser air-motion sensor

    NASA Astrophysics Data System (ADS)

    Cooper, W. A.; Spuler, S. M.; Spowart, M.; Lenschow, D. H.; Friesen, R. B.

    2014-09-01

    A new laser air-motion sensor measures the true airspeed with a standard uncertainty of less than 0.1 m s-1 and so reduces uncertainty in the measured component of the relative wind along the longitudinal axis of the aircraft to about the same level. The calculated pressure expected from that airspeed at the inlet of a pitot tube then provides a basis for calibrating the measurements of dynamic and static pressure, reducing standard uncertainty in those measurements to less than 0.3 hPa and the precision applicable to steady flight conditions to about 0.1 hPa. These improved measurements of pressure, combined with high-resolution measurements of geometric altitude from the global positioning system, then indicate (via integrations of the hydrostatic equation during climbs and descents) that the offset and uncertainty in temperature measurement for one research aircraft are +0.3 ± 0.3 °C. For airspeed, pressure and temperature, these are significant reductions in uncertainty vs. those obtained from calibrations using standard techniques. Finally, it is shown that although the initial calibration of the measured static and dynamic pressures requires a measured temperature, once calibrated these measured pressures and the measurement of airspeed from the new laser air-motion sensor provide a measurement of temperature that does not depend on any other temperature sensor.

  10. Dust-wind interactions can intensify aerosol pollution over eastern China.

    PubMed

    Yang, Yang; Russell, Lynn M; Lou, Sijia; Liao, Hong; Guo, Jianping; Liu, Ying; Singh, Balwinder; Ghan, Steven J

    2017-05-11

    Eastern China has experienced severe and persistent winter haze episodes in recent years due to intensification of aerosol pollution. In addition to anthropogenic emissions, the winter aerosol pollution over eastern China is associated with unusual meteorological conditions, including weaker wind speeds. Here we show, based on model simulations, that during years with decreased wind speed, large decreases in dust emissions (29%) moderate the wintertime land-sea surface air temperature difference and further decrease winds by -0.06 (±0.05) m s -1 averaged over eastern China. The dust-induced lower winds enhance stagnation of air and account for about 13% of increasing aerosol concentrations over eastern China. Although recent increases in anthropogenic emissions are the main factor causing haze over eastern China, we conclude that natural emissions also exert a significant influence on the increases in wintertime aerosol concentrations, with important implications that need to be taken into account by air quality studies.

  11. Dust-wind interactions can intensify aerosol pollution over eastern China

    PubMed Central

    Yang, Yang; Russell, Lynn M.; Lou, Sijia; Liao, Hong; Guo, Jianping; Liu, Ying; Singh, Balwinder; Ghan, Steven J.

    2017-01-01

    Eastern China has experienced severe and persistent winter haze episodes in recent years due to intensification of aerosol pollution. In addition to anthropogenic emissions, the winter aerosol pollution over eastern China is associated with unusual meteorological conditions, including weaker wind speeds. Here we show, based on model simulations, that during years with decreased wind speed, large decreases in dust emissions (29%) moderate the wintertime land–sea surface air temperature difference and further decrease winds by −0.06 (±0.05) m s−1 averaged over eastern China. The dust-induced lower winds enhance stagnation of air and account for about 13% of increasing aerosol concentrations over eastern China. Although recent increases in anthropogenic emissions are the main factor causing haze over eastern China, we conclude that natural emissions also exert a significant influence on the increases in wintertime aerosol concentrations, with important implications that need to be taken into account by air quality studies. PMID:28492276

  12. Incidence of Temperature Inversion and their Impact on Air Quality: A Case Study of Delhi

    NASA Astrophysics Data System (ADS)

    Singh, V. P.

    2016-12-01

    In troposphere, an increase in temperature with the altitude produces stable atmosphere which prohibits the air pollutants dispersion. This study investigates the phenomenon of temperature inversion (TI), Lapse rate (LR) and its effects on air quality in respect of Ozone (O3), CO2, CO & PM2.5 over a megacity- Delhi (Study Time Period: 2006-2012). Because of huge population, urban sprawl and orographic location, this study can be very helpful for Delhi and cities like Delhi. Radiosonde observations for temperature was used for TI calculations over the region. Results indicate that TI generally occurs at 975-850 hPa. Also, the maximum number of inversions occur during winter months (December and January) especially at night time and early mornings. Furthermore, during winter months, the incidence of inversion is highest at both 00UTC and 12UTC while it is least during the monsoon months (July and August) at 00UTC. The LR is maximum in terms of magnitude (i.e. highly negative) during the summer months (May & June) every year indicating the strong heating effects that takes place during the day time in summer and also because the sensible heat flux from the surface to the atmosphere is significant even at 12UTC (i.e. around 5.30 P.M.) The bivariate correlation analysis for air quality variables reveals negative relationship of all air quality variables except O3 with rainfall. A positive relationship of LR with all air quality variables, except O3, was observed indicating the increase in pollutants' concentrations with an increase in LR. The correlation coefficient between LR and air pollutants CO, NO, NO2, PM2.5 were found to be 0.463, 0.346, 0.249 and 0.673 respectively. A negative correlation was found between wind speed and most of the air pollutants. Also, significantly, O3 had been the only air pollutant having a negative relationship with LR (both at 00UTC &12UTC).

  13. Can air temperatures be used to project influences of climate change on stream temperatures?

    NASA Astrophysics Data System (ADS)

    Arismendi, I.; Safeeq, M.; Dunham, J.; Johnson, S. L.

    2013-12-01

    The lack of available in situ stream temperature records at broad spatiotemporal scales have been recognized as a major limiting factor in the understanding of thermal behavior of stream and river systems. This has motivated the promotion of a wide variety of models that use surrogates for stream temperatures including a regression approach that uses air temperature as the predictor variable. We investigate the long-term performance of widely used linear and non-linear regression models between air and stream temperatures to project the latter in future climate scenarios. Specifically, we examine the temporal variability of the parameters that define each of these models in long-term stream and air temperature datasets representing relatively natural and highly human-influenced streams. We selected 25 sites with long-term records that monitored year-round daily measurements of stream temperature (daily mean) in the western United States (California, Oregon, Idaho, Washington, and Alaska). Surface air temperature data from each site was not available. Therefore, we calculated daily mean surface air temperature for each site in contiguous US from a 1/16-degree resolution gridded surface temperature data. Our findings highlight several limitations that are endemic to linear or nonlinear regressions that have been applied in many recent attempts to project future stream temperatures based on air temperature. Our results also show that applications over longer time periods, as well as extrapolation of model predictions to project future stream temperatures are unlikely to be reliable. Although we did not analyze a broad range of stream types at a continental or global extent, our analysis of stream temperatures within the set of streams considered herein was more than sufficient to illustrate a number of specific limitations associated with statistical projections of stream temperature based on air temperature. Radar plots of Nash-Sutcliffe efficiency (NSE) values for

  14. NARSTO EPA SS NEW YORK AIR CHEM PM MET DATA

    Atmospheric Science Data Center

    2018-04-09

    NARSTO EPA SS NEW YORK AIR CHEM PM MET DATA Project Title:  NARSTO ... Nitrogen Oxides Ozone Surface Winds Air Temperature Humidity Solar Irradiance Particulate Matter ... Data Guide Documents:  New York Air Chem Guide CPM Summary Report  (PDF) Nitrate ...

  15. Nonlinear regression method for estimating neutral wind and temperature from Fabry-Perot interferometer data.

    PubMed

    Harding, Brian J; Gehrels, Thomas W; Makela, Jonathan J

    2014-02-01

    The Earth's thermosphere plays a critical role in driving electrodynamic processes in the ionosphere and in transferring solar energy to the atmosphere, yet measurements of thermospheric state parameters, such as wind and temperature, are sparse. One of the most popular techniques for measuring these parameters is to use a Fabry-Perot interferometer to monitor the Doppler width and breadth of naturally occurring airglow emissions in the thermosphere. In this work, we present a technique for estimating upper-atmospheric winds and temperatures from images of Fabry-Perot fringes captured by a CCD detector. We estimate instrument parameters from fringe patterns of a frequency-stabilized laser, and we use these parameters to estimate winds and temperatures from airglow fringe patterns. A unique feature of this technique is the model used for the laser and airglow fringe patterns, which fits all fringes simultaneously and attempts to model the effects of optical defects. This technique yields accurate estimates for winds, temperatures, and the associated uncertainties in these parameters, as we show with a Monte Carlo simulation.

  16. Soil and air temperatures for different habitats in Mount Rainier National Park.

    Treesearch

    Sarah E. Greene; Mark Klopsch

    1985-01-01

    This paper reports air and soil temperature data from 10 sites in Mount Rainier National Park in Washington State for 2- to 5-year periods. Data provided are monthly summaries for day and night mean air temperatures, mean minimum and maximum air temperatures, absolute minimum and maximum air temperatures, range of air temperatures, mean soil temperature, and absolute...

  17. Effect of Initial Mixture Temperature on Flame Speed of Methane-Air, Propane-Air, and Ethylene-Air Mixtures

    NASA Technical Reports Server (NTRS)

    Dugger, Gordon L

    1952-01-01

    Flame speeds based on the outer edge of the shadow cast by the laminar Bunsen cone were determined as functions of composition for methane-air mixtures at initial mixture temperatures ranging from -132 degrees to 342 degrees c and for propane-air and ethylene-air mixtures at initial mixture temperatures ranging from -73 degrees to 344 degrees c. The data showed that maximum flame speed increased with temperature at an increasing rate. The percentage change in flame speed with change in initial temperature for the three fuels followed the decreasing order, methane, propane, and ethylene. Empirical equations were determined for maximum flame speed as a function of initial temperature over the temperature range covered for each fuel. The observed effect of temperature on flame speed for each of the fuels was reasonably well predicted by either the thermal theory as presented by Semenov or the square-root law of Tanford and Pease.

  18. Crowdsourcing urban air temperatures through smartphone battery temperatures in São Paulo, Brazil

    NASA Astrophysics Data System (ADS)

    Droste, Arjan; Pape, Jan-Jaap; Overeem, Aart; Leijnse, Hidde; Steeneveld, Gert-Jan; Van Delden, Aarnout; Uijlenhoet, Remko

    2017-04-01

    Crowdsourcing as a method to obtain and apply vast datasets is rapidly becoming prominent in meteorology, especially for urban areas where traditional measurements are scarce. Earlier studies showed that smartphone battery temperature readings allow for estimating the daily and city-wide air temperature via a straightforward heat transfer model. This study advances these model estimations by studying spatially and temporally smaller scales. The accuracy of temperature retrievals as a function of the number of battery readings is also studied. An extensive dataset of over 10 million battery temperature readings is available for São Paulo (Brazil), for estimating hourly and daily air temperatures. The air temperature estimates are validated with air temperature measurements from a WMO station, an Urban Fluxnet site, and crowdsourced data from 7 hobby meteorologists' private weather stations. On a daily basis temperature estimates are good, and we show they improve by optimizing model parameters for neighbourhood scales as categorized in Local Climate Zones. Temperature differences between Local Climate Zones can be distinguished from smartphone battery temperatures. When validating the model for hourly temperature estimates, initial results are poor, but are vastly improved by using a diurnally varying parameter function in the heat transfer model rather than one fixed value for the entire day. The obtained results show the potential of large crowdsourced datasets in meteorological studies, and the value of smartphones as a measuring platform when routine observations are lacking.

  19. 40 CFR 90.309 - Engine intake air temperature measurement.

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... 40 Protection of Environment 20 2010-07-01 2010-07-01 false Engine intake air temperature measurement. 90.309 Section 90.309 Protection of Environment ENVIRONMENTAL PROTECTION AGENCY (CONTINUED) AIR... Emission Test Equipment Provisions § 90.309 Engine intake air temperature measurement. (a) The measurement...

  20. Improving Forecast Skill by Assimilation of AIRS Temperature Soundings

    NASA Technical Reports Server (NTRS)

    Susskind, Joel; Reale, Oreste

    2010-01-01

    AIRS was launched on EOS Aqua on May 4, 2002, together with AMSU-A and HSB, to form a next generation polar orbiting infrared and microwave atmospheric sounding system. The primary products of AIRS/AMSU-A are twice daily global fields of atmospheric temperature-humidity profiles, ozone profiles, sea/land surface skin temperature, and cloud related parameters including OLR. The AIRS Version 5 retrieval algorithm, is now being used operationally at the Goddard DISC in the routine generation of geophysical parameters derived from AIRS/AMSU data. A major innovation in Version 5 is the ability to generate case-by-case level-by-level error estimates delta T(p) for retrieved quantities and the use of these error estimates for Quality Control. We conducted a number of data assimilation experiments using the NASA GEOS-5 Data Assimilation System as a step toward finding an optimum balance of spatial coverage and sounding accuracy with regard to improving forecast skill. The model was run at a horizontal resolution of 0.5 deg. latitude X 0.67 deg longitude with 72 vertical levels. These experiments were run during four different seasons, each using a different year. The AIRS temperature profiles were presented to the GEOS-5 analysis as rawinsonde profiles, and the profile error estimates delta (p) were used as the uncertainty for each measurement in the data assimilation process. We compared forecasts analyses generated from the analyses done by assimilation of AIRS temperature profiles with three different sets of thresholds; Standard, Medium, and Tight. Assimilation of Quality Controlled AIRS temperature profiles significantly improve 5-7 day forecast skill compared to that obtained without the benefit of AIRS data in all of the cases studied. In addition, assimilation of Quality Controlled AIRS temperature soundings performs better than assimilation of AIRS observed radiances. Based on the experiments shown, Tight Quality Control of AIRS temperature profile performs best

  1. Low temperature air with high IAQ for dry climates

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

    Scofield, C.M.; Des Champs, N.H.

    1995-01-01

    This article describes how low temperature supply air and air-to-air heat exchangers can furnish 100% outdoor air with reduced peak energy demands. The use of low temperature supply air systems in arid climates greatly simplifies the air-conditioning design. Risks associated with moisture migration and sweating of duct and terminal equipment are reduced. Insulation and vapor barrier design requirements are not nearly as critical as they are in the humid, ambient conditions that exist in the eastern United States. The introduction of outdoor air to meet ASHRAE Standard 62-1989 becomes far less taxing on the mechanical cooling equipment because of themore » lower enthalpy levels of the dry western climate. Energy costs to assure indoor air quality (IAQ) are lower than for more tropical climates. In arid regions, maintaining acceptable indoor relative humidity (RH) levels becomes a major IAQ concern. For the western United States, coupling an air-to-air heat exchanger to direct (adiabatic) evaporative coolers can greatly reduce low temperature supply air refrigeration energy requirements and winter humidification costs while ensuring proper ventilation.« less

  2. Piezoelectric transformers for low-voltage generation of gas discharges and ionic winds in atmospheric air

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

    Johnson, Michael J.; Go, David B., E-mail: dgo@nd.edu; Department of Chemical and Biomolecular Engineering, University of Notre Dame, Notre Dame, Indianapolis 46556

    To generate a gas discharge (plasma) in atmospheric air requires an electric field that exceeds the breakdown threshold of ∼30 kV/cm. Because of safety, size, or cost constraints, the large applied voltages required to generate such fields are often prohibitive for portable applications. In this work, piezoelectric transformers are used to amplify a low input applied voltage (<30 V) to generate breakdown in air without the need for conventional high-voltage electrical equipment. Piezoelectric transformers (PTs) use their inherent electromechanical resonance to produce a voltage amplification, such that the surface of the piezoelectric exhibits a large surface voltage that can generate corona-like dischargesmore » on its corners or on adjacent electrodes. In the proper configuration, these discharges can be used to generate a bulk air flow called an ionic wind. In this work, PT-driven discharges are characterized by measuring the discharge current and the velocity of the induced ionic wind with ionic winds generated using input voltages as low as 7 V. The characteristics of the discharge change as the input voltage increases; this modifies the resonance of the system and subsequent required operating parameters.« less

  3. City ventilation of Hong Kong at no-wind conditions

    NASA Astrophysics Data System (ADS)

    Yang, Lina; Li, Yuguo

    We hypothesize that city ventilation due to both thermally-driven mountain slope flows and building surface flows is important in removing ambient airborne pollutants in the high-rise dense city Hong Kong at no-wind conditions. Both spatial and temporal urban surface temperature profiles are an important boundary condition for studying city ventilation by thermal buoyancy. Field measurements were carried out to investigate the diurnal thermal behavior of urban surfaces (mountain slopes, and building exterior walls and roofs) in Hong Kong by using the infrared thermography. The maximum urban surface temperature was measured in the early noon hours (14:00-15:00 h) and the minimum temperature was observed just before sunrise (5:00 h). The vertical surface temperature of the building exterior wall was found to increase with height at daytime and the opposite occurred at nighttime. The solar radiation and the physical properties of the various urban surfaces were found to be important factors affecting the surface thermal behaviors. The temperature difference between the measured maximum and minimum surface temperatures of the four selected exterior walls can be at the highest of 16.7 °C in the early afternoon hours (15:00 h). Based on the measured surface temperatures, the ventilation rate due to thermal buoyancy-induced wall surface flows of buildings and mountain slope winds were estimated through an integral analysis of the natural convection flow over a flat surface. At no-wind conditions, the total air change rate by the building wall flows (2-4 ACH) was found to be 2-4 times greater than that by the slope flows due to mountain surface (1 ACH) due to larger building exterior surface areas and temperature differences with surrounding air. The results provide useful insights into the ventilation of a high-rise dense city at no-wind conditions.

  4. Differences and Similarities in MaCWAVE Summer and Winter Temperatures and Winds

    NASA Technical Reports Server (NTRS)

    Schmidlin, F. J.; Goldberg, R. A.

    2008-01-01

    Small meteorological rockets released inflatable falling spheres during the MaCWAVE Campaign. The Mountain and Convective Waves Ascending Vertically Experiment (MaCWAVE) was carried out in two parts, a summer sequence from Andoya Rocket Range (69N) during July 2002 to examine convective initiation of gravity waves and a winter sequence from ESRANGE (68N) during January 2003 to examine mountain-terrain initiated gravity waves. The sphere-tracked data provided significant information about the variation of temperature and wind from 70 km and above. The changes observed may be considered akin to tidal motion; unfortunately the launch activity was restricted to 12-hour periods, thus the observation of a full diurnal cycle was not possible. During summer, temperature variation was smaller than that observed during winter when peak to null differences reached 15-20 K at 80-85 km. Variation in the zonal winds varied up to 100+mps in summer and winter. Examination of the times of peak wind vs altitude showed that the peak zonal wind occurred approximately two hours ahead of the peak meridional wind. We provide details about the measurements and observed variations.

  5. The impact of changing wind speeds on gas transfer and its effect on global air-sea CO2 fluxes

    NASA Astrophysics Data System (ADS)

    Wanninkhof, R.; Triñanes, J.

    2017-06-01

    An increase in global wind speeds over time is affecting the global uptake of CO2 by the ocean. We determine the impact of changing winds on gas transfer and CO2 uptake by using the recently updated, global high-resolution, cross-calibrated multiplatform wind product (CCMP-V2) and a fixed monthly pCO2 climatology. In particular, we assess global changes in the context of regional wind speed changes that are attributed to large-scale climate reorganizations. The impact of wind on global CO2 gas fluxes as determined by the bulk formula is dependent on several factors, including the functionality of the gas exchange-wind speed relationship and the regional and seasonal differences in the air-water partial pressure of CO2 gradient (ΔpCO2). The latter also controls the direction of the flux. Fluxes out of the ocean are influenced more by changes in the low-to-intermediate wind speed range, while ingassing is impacted more by changes in higher winds because of the regional correlations between wind and ΔpCO2. Gas exchange-wind speed parameterizations with a quadratic and third-order polynomial dependency on wind, each of which meets global constraints, are compared. The changes in air-sea CO2 fluxes resulting from wind speed trends are greatest in the equatorial Pacific and cause a 0.03-0.04 Pg C decade-1 increase in outgassing over the 27 year time span. This leads to a small overall decrease of 0.00 to 0.02 Pg C decade-1 in global net CO2 uptake, contrary to expectations that increasing winds increase net CO2 uptake.Plain Language SummaryThe effects of changing <span class="hlt">winds</span> are isolated from the total change in trends in global <span class="hlt">air</span>-sea CO2 fluxes over the last 27 years. The overall effect of increasing <span class="hlt">winds</span> over time has a smaller impact than expected as the impact in regions of outgassing is greater than for the regions acting as a CO2 sink.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title14-vol1/pdf/CFR-2013-title14-vol1-sec25-1527.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title14-vol1/pdf/CFR-2013-title14-vol1-sec25-1527.pdf"><span>14 CFR 25.1527 - Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-01-01</p> <p>... 14 Aeronautics and Space 1 2013-01-01 2013-01-01 false Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating... Information Operating Limitations § 25.1527 Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude. The extremes of the ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude for which operation is allowed, as limited by...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title14-vol1/pdf/CFR-2011-title14-vol1-sec25-1527.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title14-vol1/pdf/CFR-2011-title14-vol1-sec25-1527.pdf"><span>14 CFR 25.1527 - Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-01-01</p> <p>... 14 Aeronautics and Space 1 2011-01-01 2011-01-01 false Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating... Information Operating Limitations § 25.1527 Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude. The extremes of the ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude for which operation is allowed, as limited by...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title14-vol1/pdf/CFR-2012-title14-vol1-sec25-1527.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title14-vol1/pdf/CFR-2012-title14-vol1-sec25-1527.pdf"><span>14 CFR 25.1527 - Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-01-01</p> <p>... 14 Aeronautics and Space 1 2012-01-01 2012-01-01 false Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating... Information Operating Limitations § 25.1527 Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude. The extremes of the ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude for which operation is allowed, as limited by...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title14-vol1/pdf/CFR-2014-title14-vol1-sec25-1527.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title14-vol1/pdf/CFR-2014-title14-vol1-sec25-1527.pdf"><span>14 CFR 25.1527 - Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-01-01</p> <p>... 14 Aeronautics and Space 1 2014-01-01 2014-01-01 false Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating... Information Operating Limitations § 25.1527 Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude. The extremes of the ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude for which operation is allowed, as limited by...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850035425&hterms=sass&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsass','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850035425&hterms=sass&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsass"><span>Error trends in SASS <span class="hlt">winds</span> as functions of atmospheric stability and sea surface <span class="hlt">temperature</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liu, W. T.</p> <p>1983-01-01</p> <p><span class="hlt">Wind</span> speed measurements obtained with the scatterometer instrument aboard the Seasat satellite are compared equivalent neutral <span class="hlt">wind</span> measurements obtained from ship reports in the western N. Atlantic and eastern N. Pacific where the concentration of ship reports are high and the ranges of atmospheric stability and sea surface <span class="hlt">temperature</span> are large. It is found that at low <span class="hlt">wind</span> speeds the difference between satellite measurements and surface reports depends on sea surface <span class="hlt">temperature</span>. At <span class="hlt">wind</span> speeds higher than 8 m/s the dependence was greatly reduced. The removal of systematic errors due to fluctuations in atmospheric stability reduced the r.m.s. difference from 1.7 m/s to 0.8 m/s. It is suggested that further clarification of the effects of fluctuations in atmospheric stability on Seasat <span class="hlt">wind</span> speed measurements should increase their reliability in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170000762','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170000762"><span>Identifying Stratospheric <span class="hlt">Air</span> Intrusions and Associated Hurricane-Force <span class="hlt">Wind</span> Events over the North Pacific Ocean</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Malloy, Kelsey; Folmer, Michael J.; Phillips, Joseph; Sienkiewicz, Joseph M.; Berndt, Emily</p> <p>2017-01-01</p> <p>Motivation: Ocean data is sparse: reliance on satellite imagery for marine forecasting; Ocean Prediction Center (OPC) –“mariner’s weather lifeline”. Responsible for: Pacific, Atlantic, Pacific Alaska surface analyses –24, 48, 96 hrs.; <span class="hlt">Wind</span> & wave analyses –24, 48, 96 hrs.; Issue warnings, make decisions, Geostationary Operational Environmental Satellite –R Series (now GOES-16), Compared to the old GOES: 3 times spectral resolution, 4 times spatial resolution, 5 times faster coverage; Comparable to Japanese Meteorological Agency’s Himawari-8, used a lot throughout this research. Research Question: How can integrating satellite data imagery and derived products help forecasters improve prognosis of rapid cyclogenesis and hurricane-force <span class="hlt">wind</span> events? Phase I –Identifying stratospheric <span class="hlt">air</span> intrusions: Water Vapor –6.2, 6.9, 7.3 micron channels; Airmass RGB Product; <span class="hlt">AIRS</span>, IASI, NUCAPS total column ozone and ozone anomaly; ASCAT (A/B) and AMSR-2 <span class="hlt">wind</span> data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title40-vol21/pdf/CFR-2013-title40-vol21-sec90-309.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title40-vol21/pdf/CFR-2013-title40-vol21-sec90-309.pdf"><span>40 CFR 90.309 - Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span> measurement.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-07-01</p> <p>... 40 Protection of Environment 21 2013-07-01 2013-07-01 false Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span>... Emission Test Equipment Provisions § 90.309 Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span> measurement. (a) The measurement...) The <span class="hlt">temperature</span> measurements must be accurate to within ±2 °C. ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title40-vol20/pdf/CFR-2014-title40-vol20-sec90-309.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title40-vol20/pdf/CFR-2014-title40-vol20-sec90-309.pdf"><span>40 CFR 90.309 - Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span> measurement.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-07-01</p> <p>... 40 Protection of Environment 20 2014-07-01 2013-07-01 true Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span>... Emission Test Equipment Provisions § 90.309 Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span> measurement. (a) The measurement...) The <span class="hlt">temperature</span> measurements must be accurate to within ±2 °C. ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title40-vol20/pdf/CFR-2011-title40-vol20-sec90-309.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title40-vol20/pdf/CFR-2011-title40-vol20-sec90-309.pdf"><span>40 CFR 90.309 - Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span> measurement.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-07-01</p> <p>... 40 Protection of Environment 20 2011-07-01 2011-07-01 false Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span>... Emission Test Equipment Provisions § 90.309 Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span> measurement. (a) The measurement...) The <span class="hlt">temperature</span> measurements must be accurate to within ±2 °C. ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title40-vol21/pdf/CFR-2012-title40-vol21-sec90-309.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title40-vol21/pdf/CFR-2012-title40-vol21-sec90-309.pdf"><span>40 CFR 90.309 - Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span> measurement.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-07-01</p> <p>... 40 Protection of Environment 21 2012-07-01 2012-07-01 false Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span>... Emission Test Equipment Provisions § 90.309 Engine intake <span class="hlt">air</span> <span class="hlt">temperature</span> measurement. (a) The measurement...) The <span class="hlt">temperature</span> measurements must be accurate to within ±2 °C. ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1035054','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1035054"><span><span class="hlt">Temperature</span> Calculations in the Coastal Modeling System</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-04-01</p> <p>tide) and river discharge at model boundaries, wave radiation stress, and <span class="hlt">wind</span> forcing over a model computational domain. Physical processes calculated...calculated in the CMS using the following meteorological parameters: solar radiation, cloud cover, <span class="hlt">air</span> <span class="hlt">temperature</span>, <span class="hlt">wind</span> speed, and surface water <span class="hlt">temperature</span>...during a clear (i.e., cloudless) sky (Wm-2); CLDC is the cloud cover fraction (0-1.0); SWR is the surface reflection coefficient; and SHDf is the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=69843&keyword=kernel&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=69843&keyword=kernel&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>LOCATING NEARBY SOURCES OF <span class="hlt">AIR</span> POLLUTION BY NONPARAMETRIC REGRESSION OF ATMOSPHERIC CONCENTRATIONS ON <span class="hlt">WIND</span> DIRECTION. (R826238)</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p><p>The relationship of the concentration of <span class="hlt">air</span> pollutants to <span class="hlt">wind</span> direction has been determined by nonparametric regression using a Gaussian kernel. The results are smooth curves with error bars that allow for the accurate determination of the <span class="hlt">wind</span> direction where the concentrat...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920020070&hterms=wind+monitor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dwind%2Bmonitor','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920020070&hterms=wind+monitor&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dwind%2Bmonitor"><span>Error Analysis of <span class="hlt">Wind</span> Measurements for the University of Illinois Sodium Doppler <span class="hlt">Temperature</span> System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pfenninger, W. Matthew; Papen, George C.</p> <p>1992-01-01</p> <p>Four-frequency lidar measurements of <span class="hlt">temperature</span> and <span class="hlt">wind</span> velocity require accurate frequency tuning to an absolute reference and long term frequency stability. We quantify frequency tuning errors for the Illinois sodium system, to measure absolute frequencies and a reference interferometer to measure relative frequencies. To determine laser tuning errors, we monitor the vapor cell and interferometer during lidar data acquisition and analyze the two signals for variations as functions of time. Both sodium cell and interferometer are the same as those used to frequency tune the laser. By quantifying the frequency variations of the laser during data acquisition, an error analysis of <span class="hlt">temperature</span> and <span class="hlt">wind</span> measurements can be calculated. These error bounds determine the confidence in the calculated <span class="hlt">temperatures</span> and <span class="hlt">wind</span> velocities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1213876M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1213876M"><span>Comparison of kinetic and <span class="hlt">air</span> <span class="hlt">temperatures</span> in Budapest aiming applications in weather forecasting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mika, Janos; Nemeth, Akos; Bela Olah, Andras; Dezso, Zsuzsanna</p> <p>2010-05-01</p> <p>Moderate Resolution Imaging Spectroradiometer (MODIS) based kinetic <span class="hlt">temperature</span> data are compared with the surface <span class="hlt">air</span> <span class="hlt">temperature</span> data at the four weather stations in Budapest, Hun-gary. Dependence of these <span class="hlt">temperature</span> characteristics on weather conditions, characterised by macrosynoptic types and by objective weather types, is in the focus of the study. Day- and night-time kinetic <span class="hlt">temperature</span> series are used from the period 2001-2008. Four automatic stations are also used as the surface-based control variables. The four MODIS-pixels, covering one station, each, are the sites of our comparison. One of the four stations has strictly urban situation at the roof level in a strongly built-in region of Budapest. Another one, used as background rural station is at the east-west edge of the town with gar-dened environment. Two other stations are positioned near the river Danube at the northern and southern edges of Budapest, still under mezo-scale effect of the city. The number of elaborated hourly values is 4300-4400 above each pixel, depending on the cloudiness. At the four station automatic observations on <span class="hlt">air</span> <span class="hlt">temperature</span>, cloudiness (=0), relative humidity and <span class="hlt">wind</span>-speed are observed in the hours of the MODIS observations. From these elements <span class="hlt">air</span> <span class="hlt">temperature</span> is used for comparison with the satellite-based kinetic <span class="hlt">temperature</span>, and also as the main components of the Physiologically Equivalent <span class="hlt">Temperature</span> (PET), de-rived to characterise usefulness of the kinetic <span class="hlt">temperature</span>. Our first aim is to specify detailed relationship between the two <span class="hlt">temperatures</span> consider-ing the seasonal and diurnal cycles and synoptic situation. This comparison is also performed by using the PET to establish which kind of <span class="hlt">temperature</span> reminds this human bioclimatic in-dex better. If we could establish effective relationships with the synoptic situations (or weather types) we could use them in two further applications. The first one is the everyday forecasting of dangerous situations within the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED035214.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED035214.pdf"><span>Possible Economies in <span class="hlt">Air</span>-Conditioning by Accepting <span class="hlt">Temperature</span> Swings.</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>Loudon, A. G.; Petherbridge, P.</p> <p></p> <p>Public building <span class="hlt">air</span> conditioning systems, which use constant and varying heat and cooling loads, are compared and investigated. Experiments indicated that constant <span class="hlt">temperature</span> controls based on outside <span class="hlt">air</span> <span class="hlt">temperature</span> alone were inefficient. Ventilating a building with outside <span class="hlt">air</span> and the methods of doing so are cited as being the most economical…</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70120200','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70120200"><span><span class="hlt">Air</span>-sea interactions during strong winter extratropical storms</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nelson, Jill; He, Ruoying; Warner, John C.; Bane, John</p> <p>2014-01-01</p> <p>A high-resolution, regional coupled atmosphere–ocean model is used to investigate strong air–sea interactions during a rapidly developing extratropical cyclone (ETC) off the east coast of the USA. In this two-way coupled system, surface momentum and heat fluxes derived from the Weather Research and Forecasting model and sea surface <span class="hlt">temperature</span> (SST) from the Regional Ocean Modeling System are exchanged via the Model Coupling Toolkit. Comparisons are made between the modeled and observed <span class="hlt">wind</span> velocity, sea level pressure, 10 m <span class="hlt">air</span> <span class="hlt">temperature</span>, and sea surface <span class="hlt">temperature</span> time series, as well as a comparison between the model and one glider transect. Vertical profiles of modeled <span class="hlt">air</span> <span class="hlt">temperature</span> and <span class="hlt">winds</span> in the marine atmospheric boundary layer and <span class="hlt">temperature</span> variations in the upper ocean during a 3-day storm period are examined at various cross-shelf transects along the eastern seaboard. It is found that the air–sea interactions near the Gulf Stream are important for generating and sustaining the ETC. In particular, locally enhanced <span class="hlt">winds</span> over a warm sea (relative to the land <span class="hlt">temperature</span>) induce large surface heat fluxes which cool the upper ocean by up to 2 °C, mainly during the cold <span class="hlt">air</span> outbreak period after the storm passage. Detailed heat budget analyses show the ocean-to-atmosphere heat flux dominates the upper ocean heat content variations. Results clearly show that dynamic air–sea interactions affecting momentum and buoyancy flux exchanges in ETCs need to be resolved accurately in a coupled atmosphere–ocean modeling framework.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080021728','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080021728"><span>Peak <span class="hlt">Wind</span> Tool for General Forecasting</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barrett, Joe H., III; Short, David</p> <p>2008-01-01</p> <p>This report describes work done by the Applied Meteorology Unit (AMU) in predicting peak <span class="hlt">winds</span> at Kennedy Space Center (KSC) and Cape Canaveral <span class="hlt">Air</span> Force Station (CCAFS). The 45th Weather Squadron requested the AMU develop a tool to help them forecast the speed and timing of the daily peak and average <span class="hlt">wind</span>, from the surface to 300 ft on KSC/CCAFS during the cool season. Based on observations from the KSC/CCAFS <span class="hlt">wind</span> tower network , Shuttle Landing Facility (SLF) surface observations, and CCAFS sounding s from the cool season months of October 2002 to February 2007, the AMU created mul tiple linear regression equations to predict the timing and speed of the daily peak <span class="hlt">wind</span> speed, as well as the background average <span class="hlt">wind</span> speed. Several possible predictors were evaluated, including persistence , the <span class="hlt">temperature</span> inversion depth and strength, <span class="hlt">wind</span> speed at the top of the inversion, <span class="hlt">wind</span> gust factor (ratio of peak <span class="hlt">wind</span> speed to average <span class="hlt">wind</span> speed), synoptic weather pattern, occurrence of precipitation at the SLF, and strongest <span class="hlt">wind</span> in the lowest 3000 ft, 4000 ft, or 5000 ft.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRD..11723110S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRD..11723110S"><span>Validation of Mode-S Meteorological Routine <span class="hlt">Air</span> Report aircraft observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Strajnar, B.</p> <p>2012-12-01</p> <p>The success of mesoscale data assimilation depends on the availability of three-dimensional observations with high spatial and temporal resolution. This paper describes an example of such observations, available through Mode-S <span class="hlt">air</span> traffic control system composed of ground radar and transponders on board the aircraft. The meteorological information is provided by interrogation of a dedicated meteorological data register, called Meteorological Routine <span class="hlt">Air</span> Report (MRAR). MRAR provides direct measurements of <span class="hlt">temperature</span> and <span class="hlt">wind</span>, but is only returned by a small fraction of aircraft. The quality of Mode-S MRAR data, collected at the Ljubljana Airport, Slovenia, is assessed by its comparison with AMDAR and high-resolution radiosonde data sets, which enable high- and low-level validation, respectively. The need for temporal smoothing of raw Mode-S MRAR data is also studied. The standard deviation of differences between smoothed Mode-S MRAR and AMDAR is 0.35°C for <span class="hlt">temperature</span>, 0.8 m/s for <span class="hlt">wind</span> speed and below 10 degrees for <span class="hlt">wind</span> direction. The differences with respect to radiosondes are larger, with standard deviations of approximately 1.7°C, 3 m/s and 25 degrees for <span class="hlt">temperature</span>, <span class="hlt">wind</span> speed and <span class="hlt">wind</span> direction, respectively. It is concluded that both <span class="hlt">wind</span> and <span class="hlt">temperature</span> observations from Mode-S MRAR are accurate and therefore potentially very useful for data assimilation in numerical weather prediction models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/15009599','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/15009599"><span>Preliminary Assessment of Potential Avian Interactions at Four Proposed <span class="hlt">Wind</span> Energy Facilities on Vandenberg <span class="hlt">Air</span> Force Base, California</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>The United States <span class="hlt">Air</span> Force (USAF) is investigating whether to install <span class="hlt">wind</span> turbines to provide a supplemental source of electricity at Vandenberg <span class="hlt">Air</span> Force Base (VAFB) near Lompoc, California. As part of that investigation, VAFB sought assistance from the U.S. Department of Energy's National Renewable Energy Laboratory (NREL) to provide a preliminary characterization of the potential risk to wildlife resources (mainly birds and bats) from <span class="hlt">wind</span> turbine installations. With <span class="hlt">wind</span> power development expanding throughout North America and Europe, concerns have surfaced over the number of bird fatalities associated with <span class="hlt">wind</span> turbines. Guidelines developed for the <span class="hlt">wind</span> industry by the Nationalmore » <span class="hlt">Wind</span> Coordinating Committee (NWCC) recommend assessing potential impacts to birds, bats, and other potentially sensitive resources before construction. The primary purpose of an assessment is to identify potential conflicts with sensitive resources, to assist developers with identifying their permitting needs, and to develop strategies to avoid impacts or to mitigate their effects. This report provides a preliminary (Phase I) biological assessment of potential impacts to birds and bats that might result from construction and operation of the proposed <span class="hlt">wind</span> energy facilities on VAFB.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989JApMe..28..545Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989JApMe..28..545Y"><span>A Numerical Model Study of Nocturnal Drainage Flows with Strong <span class="hlt">Wind</span> and <span class="hlt">Temperature</span> Gradients.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamada, T.; Bunker, S.</p> <p>1989-07-01</p> <p>A second-moment turbulence-closure model described in Yamada and Bunker is used to simulate nocturnal drainage flows observed during the 1984 ASCOT field expedition in Brush Creek, Colorado. In order to simulate the observed strong <span class="hlt">wind</span> directional shear and <span class="hlt">temperature</span> gradients, two modifications are added to the model. The strong <span class="hlt">wind</span> directional shear was maintained by introducing a `nudging' term in the equation of motion to guide the modeled <span class="hlt">winds</span> in the layers above the ridge top toward the observed <span class="hlt">wind</span> direction. The second modification was accomplished by reformulating the conservation equation for the potential <span class="hlt">temperature</span> in such a way that only the deviation from the horizontally averaged value was prognostically computed.The vegetation distribution used in this study is undoubtedly crude. Nevertheless, the present simulation suggests that tall tree canopy can play an important role in producing inhomogeneous <span class="hlt">wind</span> distribution, particularly in the levels below the canopy top.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000116508','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000116508"><span>BOREAS AFM-2 Wyoming King <span class="hlt">Air</span> 1994 Aircraft Sounding Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kelly, Robert D.; Hall, Forrest G. (Editor); Knapp, David E. (Editor); Smith, David E. (Technical Monitor)</p> <p>2000-01-01</p> <p>The BOREAS AFM-2 team used the University of Wyoming King <span class="hlt">Air</span> aircraft during IFCs 1, 2, and 3 in 1994 to collected pass-by-pass fluxes (and many other statistics) for the large number of level (constant altitude), straight-line passes used in a variety of flight patterns over the SSA and NSA and areas along the transect between these study areas. The data described here form a second set, namely soundings that were incorporated into nearly every research flight by the King <span class="hlt">Air</span> in 1994. These soundings generally went from near the surface to above the inversion layer. Most were flown immediately after takeoff or immediately after finishing the last flux pattern of that particular day's flights. The parameters that were measured include <span class="hlt">wind</span> direction, <span class="hlt">wind</span> speed, west <span class="hlt">wind</span> component (u), south <span class="hlt">wind</span> component (v), static pressure, <span class="hlt">air</span> dry bulb <span class="hlt">temperature</span>, potential <span class="hlt">temperature</span>, dewpoint, <span class="hlt">temperature</span>, water vapor mixing ratio, and CO2 concentration. Data on the aircraft's location, attitude, and altitude during data collection are also provided. These data are stored in tabular ASCH files. The data files are available on a CD-ROM (see document number 20010000884) or from the Oak Ridge National Laboratory (ORNL) Distributed Active Archive Center (DAAC).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC24F..06D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC24F..06D"><span>Using Analog Ensemble to generate spatially downscaled probabilistic <span class="hlt">wind</span> power forecasts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delle Monache, L.; Shahriari, M.; Cervone, G.</p> <p>2017-12-01</p> <p>We use the Analog Ensemble (AnEn) method to generate probabilistic 80-m <span class="hlt">wind</span> power forecasts. We use data from the NCEP GFS ( 28 km resolution) and NCEP NAM (12 km resolution). We use forecasts data from NAM and GFS, and analysis data from NAM which enables us to: 1) use a lower-resolution model to create higher-resolution forecasts, and 2) use a higher-resolution model to create higher-resolution forecasts. The former essentially increases computing speed and the latter increases forecast accuracy. An aggregated model of the former can be compared against the latter to measure the accuracy of the AnEn spatial downscaling. The AnEn works by taking a deterministic future forecast and comparing it with past forecasts. The model searches for the best matching estimates within the past forecasts and selects the predictand value corresponding to these past forecasts as the ensemble prediction for the future forecast. Our study is based on predicting <span class="hlt">wind</span> speed and <span class="hlt">air</span> density at more than 13,000 grid points in the continental US. We run the AnEn model twice: 1) estimating 80-m <span class="hlt">wind</span> speed by using predictor variables such as <span class="hlt">temperature</span>, pressure, geopotential height, U-component and V-component of <span class="hlt">wind</span>, 2) estimating <span class="hlt">air</span> density by using predictors such as <span class="hlt">temperature</span>, pressure, and relative humidity. We use the <span class="hlt">air</span> density values to correct the standard <span class="hlt">wind</span> power curves for different values of <span class="hlt">air</span> density. The standard deviation of the ensemble members (i.e. ensemble spread) will be used as the degree of difficulty to predict <span class="hlt">wind</span> power at different locations. The value of the correlation coefficient between the ensemble spread and the forecast error determines the appropriateness of this measure. This measure is prominent for <span class="hlt">wind</span> farm developers as building <span class="hlt">wind</span> farms in regions with higher predictability will reduce the real-time risks of operating in the electricity markets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910035691&hterms=sines&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsines','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910035691&hterms=sines&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsines"><span>Mean state densities, <span class="hlt">temperatures</span> and <span class="hlt">winds</span> during the MAC/SINE and MAC/EPSILON campaigns</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Luebken, F.-J.; Von Zahn, U.; Manson, A.; Meek, C.; Hoppe, U.-P.; Schmidlin, F. J.</p> <p>1990-01-01</p> <p>Two field campaigns were conducted, primarily in northern Norway, in the summer and late autumn of 1987; these yielded a total of 41 in situ <span class="hlt">temperature</span> profiles and 67 in situ <span class="hlt">wind</span> profiles. Simultaneously, ground-based measurements were conducted of OH <span class="hlt">temperatures</span> and sodium lidar <span class="hlt">temperatures</span> for 85 and 104 hours, respectively. The summer campaign's mean <span class="hlt">temperature</span> profile exhibited major deviations from the CIRA (1986) reference atmosphere; the differences between this model and the observations are less pronounced in the autumn. Both the summer and autumn mean <span class="hlt">wind</span> profiles were in general agreement with the CIRA model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120016235','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120016235"><span>A Full-Envelope <span class="hlt">Air</span> Data Calibration and Three-Dimensional <span class="hlt">Wind</span> Estimation Method Using Global Output-Error Optimization and Flight-Test Techniques</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Taylor, Brian R.</p> <p>2012-01-01</p> <p>A novel, efficient <span class="hlt">air</span> data calibration method is proposed for aircraft with limited envelopes. This method uses output-error optimization on three-dimensional inertial velocities to estimate calibration and <span class="hlt">wind</span> parameters. Calibration parameters are based on assumed calibration models for static pressure, angle of attack, and flank angle. Estimated <span class="hlt">wind</span> parameters are the north, east, and down components. The only assumptions needed for this method are that the inertial velocities and Euler angles are accurate, the calibration models are correct, and that the steady-state component of <span class="hlt">wind</span> is constant throughout the maneuver. A two-minute maneuver was designed to excite the aircraft over the range of <span class="hlt">air</span> data calibration parameters and de-correlate the angle-of-attack bias from the vertical component of <span class="hlt">wind</span>. Simulation of the X-48B (The Boeing Company, Chicago, Illinois) aircraft was used to validate the method, ultimately using data derived from <span class="hlt">wind</span>-tunnel testing to simulate the un-calibrated <span class="hlt">air</span> data measurements. Results from the simulation were accurate and robust to turbulence levels comparable to those observed in flight. Future experiments are planned to evaluate the proposed <span class="hlt">air</span> data calibration in a flight environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.H43G1319A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.H43G1319A"><span>Near-surface <span class="hlt">temperature</span> lapse rates in a mountainous catchment in the Chilean Andes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ayala; Schauwecker, S.; Pellicciotti, F.; McPhee, J. P.</p> <p>2011-12-01</p> <p> <span class="hlt">temperature</span> in a high elevation catchment. Our main result is that the assumption of a MALR is appropriate to describe the average variability of <span class="hlt">temperature</span> over the entire measurement period (and possibly for daily scales), but that hourly near-surface lapse rates vary considerably and can deviate strongly from the MALR. This diurnal variability in lapse rates is associated with changes in <span class="hlt">wind</span> direction and variations in <span class="hlt">wind</span> velocity. Shallow lapse rates, in particular, occur during the morning, in correspondence to low <span class="hlt">wind</span> speeds and change in <span class="hlt">wind</span> direction from katabatic <span class="hlt">wind</span> to valley <span class="hlt">wind</span> and are associated with a weaker correlation between <span class="hlt">air</span> <span class="hlt">temperature</span> and elevation, while steeper lapse rates (meaning by this that <span class="hlt">temperature</span> decreases more with elevation) closer to the MALR are typical of the afternoon hours from 13.00 on (and correspond to high <span class="hlt">wind</span> speed), and are representative of a more linear dependency between <span class="hlt">air</span> <span class="hlt">temperature</span> and elevation. The steepest LRs, however, occur in the evening at 20.00-21.00, when <span class="hlt">wind</span> velocity drops again and <span class="hlt">wind</span> direction changes from valley <span class="hlt">wind</span> to katabatic <span class="hlt">wind</span>. It is clear that the <span class="hlt">wind</span> regime is the main controls on LRs variability, and it is important to validate these findings with data sets from a second season.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060029193&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dair%2Bmeasurement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060029193&hterms=air+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dair%2Bmeasurement"><span>Sea surface <span class="hlt">temperature</span> measurements with <span class="hlt">AIRS</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Aumann, H.</p> <p>2003-01-01</p> <p>The comparison of global sea surface skin <span class="hlt">temperature</span> derived from cloud-free <span class="hlt">AIRS</span> super window channel at 2616 cm-1 (sst2616) with the Real-Time Global Sea Surface <span class="hlt">Temperature</span> for September 2002 shows surprisingly small standard deviation of 0.44K.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=temperature+AND+influence+AND+HA&pg=2&id=EJ726716','ERIC'); return false;" href="https://eric.ed.gov/?q=temperature+AND+influence+AND+HA&pg=2&id=EJ726716"><span>The Effect of Venue and <span class="hlt">Wind</span> on the Distance of a Hammer Throw</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>Hunter, Iain</p> <p>2005-01-01</p> <p>In track and field, gravity and <span class="hlt">air</span> resistance act on the hammer after it has been released. Both of these forces depend on altitude and latitude. In addition, <span class="hlt">air</span> resistance also depends on <span class="hlt">wind</span>, <span class="hlt">temperature</span>, humidity, and barometric pressure. Often, <span class="hlt">air</span> resistance and varying gravity throughout the earth are not considered when throwing…</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> low values during summer and high values during winter. This variation is mainly explained by the direct effect of <span class="hlt">air</span> <span class="hlt">temperature</span> on atmospheric stability. When the surface <span class="hlt">temperature</span> becomes high, <span class="hlt">air</span> is mixed well in atmospheric boundary layer. This phenomenon leads to vertically low <span class="hlt">wind</span> speed change indicating low <span class="hlt">wind</span> profile parameter. On the contrary, cold surface <span class="hlt">temperature</span> prevents <span class="hlt">air</span> from being mixed well in the boundary layer. This analysis is applied to different regions to see the spatial characteristics of <span class="hlt">wind</span> in UAE. As a next step, a mesoscale model coupled with UAE roughness maps will be used to predict elevated <span class="hlt">wind</span> speed. A micro-scale modeling approach will be also used to capture small-scale <span class="hlt">wind</span> speed variability. This data will be combined with the NCMS data and tailored to the UAE by modeling the effects due to local changes in terrain elevation and local surface roughness changes and obstacles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12..259T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12..259T"><span>Laboratory modeling of <span class="hlt">air</span>-sea interaction under severe <span class="hlt">wind</span> conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Troitskaya, Yuliya; Vasiliy, Kazakov; Nicolay, Bogatov; Olga, Ermakova; Mikhail, Salin; Daniil, Sergeev; Maxim, Vdovin</p> <p>2010-05-01</p> <p><span class="hlt">Wind</span>-wave interaction at extreme <span class="hlt">wind</span> speed is of special interest now in connection with the problem of explanation of the sea surface drag saturation at the <span class="hlt">wind</span> speed exceeding 30 m/s. The idea on saturation (and even reduction) of the coefficient of aerodynamic resistance of the sea surface at hurricane <span class="hlt">wind</span> speed was first suggested by Emanuel (1995) on the basis of theoretical analysis of sensitivity of maximum <span class="hlt">wind</span> speed in a hurricane to the ratio of the enthalpy and momentum exchange coefficients. Both field (Powell, Vickery, Reinhold, 2003, French et al, 2007, Black, et al, 2007) and laboratory (Donelan et al, 2004) experiments confirmed that at hurricane <span class="hlt">wind</span> speed the sea surface drag coefficient is significantly reduced in comparison with the parameterization obtained at moderate to strong <span class="hlt">wind</span> conditions. Two groups of possible theoretical mechanisms for explanation of the effect of the sea surface drag reduction can be specified. In the first group of models developed by Kudryavtsev & Makin (2007) and Kukulka,Hara Belcher (2007), the sea surface drag reduction is explained by peculiarities of the <span class="hlt">air</span> flow over breaking waves. Another approach more appropriate for the conditions of developed sea exploits the effect of sea drops and sprays on the <span class="hlt">wind</span>-wave momentum exchange (Andreas, 2004; Makin, 2005; Kudryavtsev, 2006). The main objective of this work is investigation of factors determining momentum exchange under high <span class="hlt">wind</span> speeds basing on the laboratory experiment in a well controlled environment. The experiments were carried out in the Thermo-Stratified <span class="hlt">WInd</span>-WAve Tank (TSWIWAT) of the Institute of Applied Physics. The parameters of the facility are as follows: airflow 0 - 25 m/s (equivalent 10-m neutral <span class="hlt">wind</span> speed U10 up to 60 m/s), dimensions 10m x 0.4m x 0.7 m, <span class="hlt">temperature</span> stratification of the water layer. Simultaneous measurements of the airflow velocity profiles and <span class="hlt">wind</span> waves were carried out in the wide range of <span class="hlt">wind</span> velocities. Airflow</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110011475','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110011475"><span>Statistical Short-Range Guidance for Peak <span class="hlt">Wind</span> Speed Forecasts at Edwards <span class="hlt">Air</span> Force Base, CA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dreher, Joseph G.; Crawford, Winifred; Lafosse, Richard; Hoeth, Brian; Burns, Kerry</p> <p>2009-01-01</p> <p>The peak <span class="hlt">winds</span> near the surface are an important forecast element for space shuttle landings. As defined in the Flight Rules (FR), there are peak <span class="hlt">wind</span> thresholds that cannot be exceeded in order to ensure the safety of the shuttle during landing operations. The National Weather Service Spaceflight Meteorology Group (SMG) is responsible for weather forecasts for all shuttle landings, and is required to issue surface average and 10-minute peak <span class="hlt">wind</span> speed forecasts. They indicate peak <span class="hlt">winds</span> are a challenging parameter to forecast. To alleviate the difficulty in making such <span class="hlt">wind</span> forecasts, the Applied Meteorology Unit (AMU) developed a PC-based graphical user interface (GUI) for displaying peak <span class="hlt">wind</span> climatology and probabilities of exceeding peak <span class="hlt">wind</span> thresholds for the Shuttle Landing Facility (SLF) at Kennedy Space Center (KSC; Lambert 2003). However, the shuttle occasionally may land at Edwards <span class="hlt">Air</span> Force Base (EAFB) in southern California when weather conditions at KSC in Florida are not acceptable, so SMG forecasters requested a similar tool be developed for EAFB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC21D1126A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC21D1126A"><span>Sensitivity of Great Lakes Ice Cover to <span class="hlt">Air</span> <span class="hlt">Temperature</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Austin, J. A.; Titze, D.</p> <p>2016-12-01</p> <p>Ice cover is shown to exhibit a strong linear sensitivity to <span class="hlt">air</span> <span class="hlt">temperature</span>. Upwards of 70% of ice cover variability on all of the Great Lakes can be explained in terms of <span class="hlt">air</span> <span class="hlt">temperature</span>, alone, and nearly 90% of ice cover variability can be explained in some lakes. Ice cover sensitivity to <span class="hlt">air</span> <span class="hlt">temperature</span> is high, and a difference in seasonally-averaged (Dec-May) <span class="hlt">air</span> <span class="hlt">temperature</span> on the order of 1°C to 2°C can be the difference between a low-ice year and a moderate- to high- ice year. The total amount of seasonal ice cover is most influenced by <span class="hlt">air</span> <span class="hlt">temperatures</span> during the meteorological winter, contemporaneous with the time of ice formation. <span class="hlt">Air</span> <span class="hlt">temperature</span> conditions during the pre-winter conditioning period and during the spring melting period were found to have less of an impact on seasonal ice cover. This is likely due to the fact that there is a negative feedback mechanism when heat loss goes toward cooling the lake, but a positive feedback mechanism when heat loss goes toward ice formation. Ice cover sensitivity relationships were compared between shallow coastal regions of the Great Lakes and similarly shallow smaller, inland lakes. It was found that the sensitivity to <span class="hlt">air</span> <span class="hlt">temperature</span> is similar between these coastal regions and smaller lakes, but that the absolute amount of ice that forms varies significantly between small lakes and the Great Lakes, and amongst the Great Lakes themselves. The Lake Superior application of the ROMS three-dimensional hydrodynamic numerical model verifies a deterministic linear relationship between <span class="hlt">air</span> <span class="hlt">temperature</span> and ice cover, which is also strongest around the period of ice formation. When the Lake Superior bathymetry is experimentally adjusted by a constant vertical multiplier, average lake depth is shown to have a nonlinear relationship with seasonal ice cover, and this nonlinearity may be associated with a nonlinear increase in the lake-wide volume of the surface mixed layer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28501653','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28501653"><span>Incorporating <span class="hlt">wind</span> availability into land use regression modelling of <span class="hlt">air</span> quality in mountainous high-density urban environment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shi, Yuan; Lau, Kevin Ka-Lun; Ng, Edward</p> <p>2017-08-01</p> <p>Urban <span class="hlt">air</span> quality serves as an important function of the quality of urban life. Land use regression (LUR) modelling of <span class="hlt">air</span> quality is essential for conducting health impacts assessment but more challenging in mountainous high-density urban scenario due to the complexities of the urban environment. In this study, a total of 21 LUR models are developed for seven kinds of <span class="hlt">air</span> pollutants (gaseous <span class="hlt">air</span> pollutants CO, NO 2 , NO x , O 3 , SO 2 and particulate <span class="hlt">air</span> pollutants PM 2.5 , PM 10 ) with reference to three different time periods (summertime, wintertime and annual average of 5-year long-term hourly monitoring data from local <span class="hlt">air</span> quality monitoring network) in Hong Kong. Under the mountainous high-density urban scenario, we improved the traditional LUR modelling method by incorporating <span class="hlt">wind</span> availability information into LUR modelling based on surface geomorphometrical analysis. As a result, 269 independent variables were examined to develop the LUR models by using the "ADDRESS" independent variable selection method and stepwise multiple linear regression (MLR). Cross validation has been performed for each resultant model. The results show that <span class="hlt">wind</span>-related variables are included in most of the resultant models as statistically significant independent variables. Compared with the traditional method, a maximum increase of 20% was achieved in the prediction performance of annual averaged NO 2 concentration level by incorporating <span class="hlt">wind</span>-related variables into LUR model development. Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA020223','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA020223"><span>Aircraft Carrier Turbulence Study for Predicting <span class="hlt">Air</span> Flow Dynamics with Increasing <span class="hlt">Wind</span>-Over-Deck Velocities</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1968-03-28</p> <p>AD-A020 223 AIRCRAFT CARRIER TURBULENCE STUDY FOR PREDICTING <span class="hlt">AIR</span> FLOW DYNAMICS WITH INCREASING <span class="hlt">WIND</span>-OVER-DECK VELOCITIES S. Frost Naval <span class="hlt">Air</span>...Copy NAVAL <span class="hlt">AIR</span> ENGINEERING CENTERElPILAOUPHBA, PENNSYLVANIA 19112 Q Had-NG7~ CODE IDEN NO. *OOM 28 MARCH 4fe AIRCRAFT CARRIER TUJRBULENCE STUDY FOR...carrier dynamics. Ike- comirendations for future experimental and theoretical studies are give,. DD 1473 EDITIOIN 0F I NOV SS IS O@SOLETE S - ’i02</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.A11A0809P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.A11A0809P"><span>Observations of <span class="hlt">Air</span> Quality at the Edge of Kathmandu, Nepal, and the Diurnal Cycle of <span class="hlt">Air</span> Pollution In and Around the Kathmandu Valley</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Panday, A. K.; Prinn, R. G.; Regmi, R. P.</p> <p>2006-12-01</p> <p>The Kathmandu Valley is a bowl-shaped basin in the Nepal Himalaya, with a rapidly growing city surrounded by rice fields and steep terraced and forested mountain slopes. The valley's <span class="hlt">air</span> quality is influenced by urban and rural emissions, nocturnal pooling of cold <span class="hlt">air</span>, slope <span class="hlt">winds</span>, and a daily exchange of <span class="hlt">air</span> through mountain passes. To understand these processes and to inform <span class="hlt">air</span> pollution policy in Nepal, we have carried out the most comprehensive study of <span class="hlt">air</span> pollution in Nepal to date. During the 9-month dry season of 2004-2005, we carried out continuous measurements every minute of carbon monoxide, ozone, PM10, <span class="hlt">wind</span> speed, <span class="hlt">wind</span> direction, solar radiation, <span class="hlt">temperature</span>, and humidity on the eastern edge of Kathmandu city, at a site that daily received <span class="hlt">air</span> from both the city and rural areas. We recorded the diurnal cycle of the vertical <span class="hlt">temperature</span> structure and stability with <span class="hlt">temperature</span> loggers on towers and mountains. A sodar measured the mixed layer height and upper-level <span class="hlt">winds</span>. 24-hour simultaneous bag sampling campaigns on mountain peaks, passes, the rural valley, and within the city provided glimpses of the spatial patterns of the diurnal cycle of CO -- a useful tracer of anthropogenic emissions. We measured <span class="hlt">winds</span> on mountain passes and ozone on mountain peaks. At our main measurement site we found a daily-recurring pattern of CO and PM10, with an afternoon low showing rural background levels, even though the arriving <span class="hlt">air</span> had traversed the city. This was followed by an evening peak starting at sunset, a second low late at night, and a morning peak enhanced by re-circulation. Pollutants emitted in the valley only traveled out of the valley between the late morning and sunset. During winter months, rush hour was outside of this period, enhancing the morning and evening peaks. Within the city, ozone dropped to zero at night. At mid-day we observed an ozone peak enhanced by photochemical production when the <span class="hlt">air</span> mass that had been stagnant over the city swept</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/522724','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/522724"><span>Conceptual design for an electron-beam heated hypersonic <span class="hlt">wind</span> tunnel</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>Lipinski, R.J.; Kensek, R.P.</p> <p>1997-07-01</p> <p>There is a need for hypersonic <span class="hlt">wind</span>-tunnel testing at about mach 10 and above using natural <span class="hlt">air</span> and simulating <span class="hlt">temperatures</span> and pressures which are prototypic of flight at 50 km altitude or below. With traditional <span class="hlt">wind</span>-tunnel techniques, gas cooling during expansion results in exit <span class="hlt">temperatures</span> which are too low. Miles, et al., have proposed overcoming this difficulty by heating the <span class="hlt">air</span> with a laser beam as it expands in the <span class="hlt">wind</span>-tunnel nozzle. This report discusses an alternative option of using a high-power electron beam to heat the <span class="hlt">air</span> as it expands. In the e-beam heating concept, the electron beam ismore » injected into the <span class="hlt">wind</span>-tunnel nozzle near the exit and then is guided upstream toward the nozzle throat by a strong axial magnetic field. The beam deposits most of its power in the dense <span class="hlt">air</span> near the throat where the expansion rate is greatest. A conceptual design is presented for a large-scale system which achieves Mach 14 for 0.1 seconds with an exit diameter of 2.8 meters. It requires 450 MW of electron beam power (5 MeV at 90 A). The guiding field is 500 G for most of the transport length and increases to 100 kG near the throat to converge the beam to a 1.0-cm diameter. The beam generator is a DC accelerator using a Marx bank (of capacitors) and a diode stack with a hot cathode. 14 refs. 38 figs., 9 tabs.« 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_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865029','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865029"><span>Tornado type <span class="hlt">wind</span> turbines</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Hsu, Cheng-Ting</p> <p>1984-01-01</p> <p>A tornado type <span class="hlt">wind</span> turbine has a vertically disposed <span class="hlt">wind</span> collecting tower with spaced apart inner and outer walls and a central bore. The upper end of the tower is open while the lower end of the structure is in communication with a <span class="hlt">wind</span> intake chamber. An opening in the <span class="hlt">wind</span> chamber is positioned over a turbine which is in driving communication with an electrical generator. An opening between the inner and outer walls at the lower end of the tower permits radially flowing <span class="hlt">air</span> to enter the space between the inner and outer walls while a vertically disposed opening in the <span class="hlt">wind</span> collecting tower permits tangentially flowing <span class="hlt">air</span> to enter the central bore. A porous portion of the inner wall permits the radially flowing <span class="hlt">air</span> to interact with the tangentially flowing <span class="hlt">air</span> so as to create an intensified vortex flow which exits out of the top opening of the tower so as to create a low pressure core and thus draw <span class="hlt">air</span> through the opening of the <span class="hlt">wind</span> intake chamber so as to drive the turbine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930057203&hterms=air+pressure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dair%2Bpressure','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930057203&hterms=air+pressure&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dair%2Bpressure"><span>An evaluation of Shuttle Entry <span class="hlt">Air</span> Data System (SEADS) flight pressures - Comparisons with <span class="hlt">wind</span> tunnel and theoretical predictions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Henry, M. W.; Wolf, H.; Siemers, Paul M., III</p> <p>1988-01-01</p> <p>The SEADS pressure data obtained from the Shuttle flight 61-C are analyzed in conjunction with the preflight database. Based on <span class="hlt">wind</span> tunnel data, the sensitivity of the Shuttle Orbiter stagnation region pressure distribution to angle of attack and Mach number is demonstrated. Comparisons are made between flight and <span class="hlt">wind</span> tunnel SEADS orifice pressure distributions at several points throughout the re-entry. It is concluded that modified Newtonian theory provides a good tool for the design of a flush <span class="hlt">air</span> data system, furnishing data for determining orifice locations and transducer sizing. Ground-based <span class="hlt">wind</span> tunnel facilities are capable of providing the correction factors necessary for the derivation of accurate <span class="hlt">air</span> data parameters from pressure data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950033279&hterms=homogenization&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dhomogenization','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950033279&hterms=homogenization&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dhomogenization"><span>A PV view of the zonal mean distribution of <span class="hlt">temperature</span> and <span class="hlt">wind</span> in the extratropical troposphere</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sun, De-Zheng; Lindzen, Richard S.</p> <p>1994-01-01</p> <p>The dependence of the <span class="hlt">temperature</span> and <span class="hlt">wind</span> distribution of the zonal mean flow in the extratropical troposphere on the gradient of pontential vorticity along isentropes is examined. The extratropics here refer to the region outside the Hadley circulation. Of particular interest is whether the distribution of <span class="hlt">temperature</span> and <span class="hlt">wind</span> corresponding to a constant potential vorticity (PV) along isentropes resembles the observed, and the implications of PV homogenization along isentropes for the role of the tropics. With the assumption that PV is homogenized along isentropes, it is found that the <span class="hlt">temperature</span> distribution in the extratropical troposphere may be determined by a linear, first-order partial differential equation. When the observed surface <span class="hlt">temperature</span> distribution and tropical lapse rate are used as the boundary conditions, the solution of the equation is close to the observed <span class="hlt">temperature</span> distribution except in the upper troposphere adjacent to the Hadley circulation, where the troposphere with no PV gradient is considerably colder. Consequently, the jet is also stronger. It is also found that the meridional distribution of the balanced zonal <span class="hlt">wind</span> is very sensitive to the meridional distribution of the tropopause <span class="hlt">temperature</span>. The result may suggest that the requirement of the global momentum balance has no practical role in determining the extratropical <span class="hlt">temperature</span> distribution. The authors further investigated the sensitivity of the extratropical troposphere with constant PV along isentropes to changes in conditions at the tropical boundary (the edge of the Hadley circulation). It is found that the <span class="hlt">temperature</span> and <span class="hlt">wind</span> distributions in the extratropical troposphere are sensitive to the vertical distribution of PV at the tropical boundary. With a surface distribution of <span class="hlt">temperature</span> that decreases linearly with latitude, the jet maximum occurs at the tropical boundary and moves with it. The overall pattern of <span class="hlt">wind</span> distribution is not sensitive to the change of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMSH22B..03H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSH22B..03H"><span>IPS analysis on relationship among velocity, density and <span class="hlt">temperature</span> 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>Hayashi, K.; Tokumaru, M.; Fujiki, K.</p> <p>2015-12-01</p> <p>The IPS(Interplanetary Scintillation)-MHD(magnetohydrodynamics) tomography is a method we have developed to determine three-dimensional MHD solution of the solar <span class="hlt">wind</span> that best matches the line-of-sight IPS solar-<span class="hlt">wind</span> speed data (Hayashi et al., 2003). The tomographic approach is an iteration method in which IPS observations are simulated in MHD steady-state solution, then differences between the simulated observation and the actual IPS observation is reduced by modifying solar-<span class="hlt">wind</span> boundary map at 50 solar radii. This forward model needs to assume solar <span class="hlt">wind</span> density and <span class="hlt">temperature</span> as function of speed. We use empirical functions, N(V) and T(V), derived from Helios in-situ measurement data within 0.5 AU in 1970s. For recent years, especially after 2006, these functions yield higher densities and lower <span class="hlt">temperatures</span> than in-situ measurements indicate. To characterize the differences between the simulated and actual solar <span class="hlt">wind</span> plasma, we tune parameters in the functions so that agreements with in-situ data (near the Earth and at Ulysses) will be optimized. This optimization approach can help better simulations of the solar corona and heliosphere, and will help our understandings on roles of magnetic field in solar <span class="hlt">wind</span> heating and acceleration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1353479-value-compressed-air-energy-storage-wind-transmission-constrained-electric-power-systems','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1353479-value-compressed-air-energy-storage-wind-transmission-constrained-electric-power-systems"><span>The value of compressed <span class="hlt">air</span> energy storage with <span class="hlt">wind</span> in transmission-constrained electric power systems</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Denholm, Paul; Sioshansi, Ramteen</p> <p>2009-05-05</p> <p>In this paper, we examine the potential advantages of co-locating <span class="hlt">wind</span> and energy storage to increase transmission utilization and decrease transmission costs. Co-location of <span class="hlt">wind</span> and storage decreases transmission requirements, but also decreases the economic value of energy storage compared to locating energy storage at the load. This represents a tradeoff which we examine to estimate the transmission costs required to justify moving storage from load-sited to <span class="hlt">wind</span>-sited in three different locations in the United States. We examined compressed <span class="hlt">air</span> energy storage (CAES) in three “<span class="hlt">wind</span> by wire” scenarios with a variety of transmission and CAES sizes relative to amore » given amount of <span class="hlt">wind</span>. In the sites and years evaluated, the optimal amount of transmission ranges from 60% to 100% of the <span class="hlt">wind</span> farm rating, with the optimal amount of CAES equal to 0–35% of the <span class="hlt">wind</span> farm rating, depending heavily on <span class="hlt">wind</span> resource, value of electricity in the local market, and the cost of natural gas.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910014871','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910014871"><span><span class="hlt">Temperature</span> lapse rate as an adjunct to <span class="hlt">wind</span> shear detection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zweifil, Terry</p> <p>1991-01-01</p> <p>Several meteorological parameters were examined to determine if measurable atmospheric conditions can improve windshear detection devices. Lapse rate, the <span class="hlt">temperature</span> change with altitude, shows promise as being an important parameter in the prediction of severe <span class="hlt">wind</span> shears. It is easily measured from existing aircraft instrumentation, and it can be important indicator of convective activity including thunderstorms and microbursts. The meteorological theory behind lapse rate measurement is briefly reviewed, and and FAA certified system is described that is currently implemented in the Honeywell <span class="hlt">Wind</span> Shear Detection and Guidance System.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMSA44A..06S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSA44A..06S"><span>Variation of Equatorial F-region Vertical Neutral <span class="hlt">Wind</span> and Neutral <span class="hlt">Temperature</span> during Geomagnetic Storms: Brazil FPI Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sheng, C.; De La Garza, J. L.; Deng, Y.; Makela, J. J.; Fisher, D. J.; Meriwether, J. W.; Mesquita, R.</p> <p>2015-12-01</p> <p>An accurate description of vertical neutral <span class="hlt">winds</span> in the thermosphere is essential to understand how the upper atmosphere responds to the geomagnetic storms. However, vertical <span class="hlt">wind</span> measurements are difficult to obtain and there are still limited data. Recent observation deployments now permit substantial progress on this issue. In this paper, neutral vertical <span class="hlt">wind</span> data from Brazil FPI observations at around 240 km altitude during 2009 to 2015 are used for the study of the equatorial vertical <span class="hlt">wind</span> and neutral <span class="hlt">temperature</span> variation during geomagnetic activity times. First, the observations during several particular storm periods will be analyzed. Secondly, Epoch analysis will be used to bin all the observed events together to investigate the climatological features of vertical <span class="hlt">wind</span> and <span class="hlt">temperature</span> during storms. The results will give us an unprecedented view of the nighttime vertical <span class="hlt">wind</span> and neutral <span class="hlt">temperature</span> variations at low latitudes, which is critical to specify the dynamics of the upper atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918108S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918108S"><span>Variability of <span class="hlt">winds</span> and <span class="hlt">temperature</span> in the Bergen area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schönbein, Daniel; Ólafsson, Haraldur; Asle Olseth, Jan; Furevik, Birgitte</p> <p>2017-04-01</p> <p>In recent years, observations have been made by a dense network of automatic weather stations in the Bergen area in W-Norway (Bergen School of Meteorology). Here, cases are presented that feature large spatial variability in <span class="hlt">winds</span> and <span class="hlt">temperature</span> and the ability of a numerical model to reproduce this variability is assessed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A41A0015W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A41A0015W"><span>Daily Cycle of <span class="hlt">Air</span> <span class="hlt">Temperature</span> and Surface <span class="hlt">Temperature</span> in Stone Forest</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, K.; Li, Y.; Wang, X.; Yuan, M.</p> <p>2013-12-01</p> <p>Urbanization is one of the most profound human activities that impact on climate change. In cities, where are highly artificial areas, the conflict between human activity and natural climate is particularly prominent. Urban areas always have the larger area of impervious land, the higher consumption of greenhouse gases, more emissions of anthropogenic heat and <span class="hlt">air</span> pollution, all contribute to the urban warming phenomena. Understanding the mechanisms causing a variety of phenomena involved in the urban warming is critical to distinguish the anthropogenic effect and natural variation in the climate change. However, the exact dynamics of urban warming were poorly understood, and effective control strategies are not available. Here we present a study of the daily cycle of <span class="hlt">air</span> <span class="hlt">temperature</span> and surface <span class="hlt">temperature</span> in Stone Forest. The specific heat of the stones in the Stone Forest and concrete of the man-made structures within the cities are approximate. Besides, the height of the Stone Forest and the height of buildings within the city are also similar. As a scenic area, the Stone Forest is being preserved and only opened for sightseeing. There is no anthropogenic heat, as well <span class="hlt">air</span> pollution within the Stone Forest. The thermal environment in Stone Forest can be considered to be a simulation of thermal environment in the city, which can reveal the effect of man-made structures on urban thermal environment. We conducted the field studies and numerical analysis in the Stone Forest for 4 typical urban morphology and environment scenarios, including high-rise compact cities, low-rise sparse cities, garden cities and isolated single stone. <span class="hlt">Air</span> <span class="hlt">temperature</span> and relative humidity were measured every half an hour in 15 different locations, which within different spatial distribution of stones and can represent the four urban scenarios respectively. At the same time, an infrared camera was used to take thermal images and get the hourly surface <span class="hlt">temperatures</span> of stones and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870000988','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870000988"><span>A theory for the retrieval of virtual <span class="hlt">temperature</span> from <span class="hlt">winds</span>, radiances and the equations of fluid dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tzvi, G. C.</p> <p>1986-01-01</p> <p>A technique to deduce the virtual <span class="hlt">temperature</span> from the combined use of the equations of fluid dynamics, observed <span class="hlt">wind</span> and observed radiances is described. The <span class="hlt">wind</span> information could come from ground-based sensitivity very high frequency (VHF) Doppler radars and/or from space-borne Doppler lidars. The radiometers are also assumed to be either space-borne and/or ground-based. From traditional radiometric techniques the vertical structure of the <span class="hlt">temperature</span> can be estimated only crudely. While it has been known for quite some time that the virtual <span class="hlt">temperature</span> could be deduced from <span class="hlt">wind</span> information only, such techniques had to assume the infallibility of certain diagnostic relations. The proposed technique is an extension of the Gal-Chen technique. It is assumed that due to modeling uncertainties the equations of fluid dynamics are satisfied only in the least square sense. The retrieved <span class="hlt">temperature</span>, however, is constrained to reproduce the observed radiances. It is shown that the combined use of the three sources of information (<span class="hlt">wind</span>, radiances and fluid dynamical equations) can result in a unique determination of the vertical <span class="hlt">temperature</span> structure with spatial and temporal resolution comparable to that of the observed <span class="hlt">wind</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19780065938&hterms=moderating&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dmoderating','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19780065938&hterms=moderating&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dmoderating"><span>Observations of the convective plume of a lake under cold-<span class="hlt">air</span> advective conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bill, R. G., Jr.; Sutherland, R. A.; Bartholic, J. F.; Chen, E.</p> <p>1978-01-01</p> <p>Moderating effects of Lake Apopka, Florida, on downwind surface <span class="hlt">temperatures</span> were evaluated under cold-<span class="hlt">air</span> advective conditions. Point <span class="hlt">temperature</span> measurements north and south of the lake and data obtained from a thermal scanner flown at 1.6 km indicate that surface <span class="hlt">temperatures</span> directly downwind may be higher than surrounding surface <span class="hlt">temperatures</span> by as much as 5 C under conditions of moderate <span class="hlt">winds</span> (about 4 m/s). No substantial <span class="hlt">temperature</span> effects were observed with surface <span class="hlt">wind</span> speed less than 1 m/s. Fluxes of sensible and latent heat from Lake Apopka were calculated from measurements of lake <span class="hlt">temperature</span>, net radiation, relative humidity, and <span class="hlt">air</span> <span class="hlt">temperature</span> above the lake. Bulk transfer coefficients and the Bowen ratio were calculated and found to be in agreement with reported data for nonadvective conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A33I2498F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A33I2498F"><span>Three-Dimensional <span class="hlt">Temperature</span> and <span class="hlt">Wind</span> Profiles Obtained Using UAV-Based Acoustic Atmospheric Tomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Finn, A.</p> <p>2017-12-01</p> <p>The natural sound generated by an unmanned aerial vehicle is used in conjunction with tomography to remotely sense atmospheric <span class="hlt">temperature</span> and <span class="hlt">wind</span> profiles simultaneously. Sound fields recorded onboard the aircraft and by an array of microphones on the ground are compared and converted to sound speed estimates for the ray paths intersecting the intervening medium. Tomographic inversion is then used to transform these sound speed values into vertical cross-sections and 3D volumes of virtual <span class="hlt">temperature</span> and <span class="hlt">wind</span> vectors, which enables the atmosphere to be visualised and monitored over time up to altitudes of 1,200m and over baselines of up to 600m. This paper reports on results from two short campaigns during which 2D and 3D profiles of <span class="hlt">wind</span> and <span class="hlt">temperature</span> obtained in this way were compared to: measurements taken by co-located mid-range Doppler SODAR and LIDAR; and <span class="hlt">temperature</span> measurements made by instruments carried by unmanned aircraft flying through the intervening atmosphere. Large eddy simulation of daytime atmospheric boundary layers were also used to examine the anticipated performance of the instruments and the nature of any errors. The observations obtained using all systems are shown to correspond closely.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070019319','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070019319"><span>Advanced <span class="hlt">Air</span> Data Systems for Commercial Aircraft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2006-01-01</p> <p>It is possible to get a crude estimate of <span class="hlt">wind</span> speed and direction while driving a car at night in the rain, with the motion of the raindrop reflections in the headlights providing clues about the <span class="hlt">wind</span>. The clues are difficult to interpret, though, because of the relative motions of ground, car, <span class="hlt">air</span>, and raindrops. More subtle interpretation is possible if the rain is replaced by fog, because the tiny droplets would follow the swirling currents of <span class="hlt">air</span> around an illuminated object, like, for example, a walking pedestrian. Microscopic particles in the <span class="hlt">air</span> (aerosols) are better for helping make assessments of the <span class="hlt">wind</span>, and reflective <span class="hlt">air</span> molecules are best of all, providing the most refined measurements. It takes a bright light to penetrate fog, so it is easy to understand how other factors, like replacing the headlights with the intensity of a searchlight, can be advantageous. This is the basic principle behind a lidar system. While a radar system transmits a pulse of radiofrequency energy and interprets the received reflections, a lidar system works in a similar fashion, substituting a near-optical laser pulse. The technique allows the measurement of relative positions and velocities between the transmitter and the <span class="hlt">air</span>, which allows measurements of relative <span class="hlt">wind</span> and of <span class="hlt">air</span> <span class="hlt">temperature</span> (because <span class="hlt">temperature</span> is associated with high-frequency random motions on a molecular level). NASA, as well as the National Oceanic and Atmospheric Administration (NOAA), have interests in this advanced lidar technology, as much of their explorative research requires the ability to measure <span class="hlt">winds</span> and turbulent regions within the atmosphere. Lidar also shows promise for providing warning of turbulent regions within the National Airspace System to allow commercial aircraft to avoid encounters with turbulence and thereby increase the safety of the traveling public. Both agencies currently employ lidar and optical sensing for a variety of weather-related research projects, such as analyzing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120015454','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120015454"><span>Vandenberg <span class="hlt">Air</span> Force Base Upper Level <span class="hlt">Wind</span> Launch Weather Constraints</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shafer, Jaclyn A.; Wheeler, Mark M.</p> <p>2012-01-01</p> <p>The 30th Operational Support Squadron Weather Flight (30 OSSWF) provides comprehensive weather services to the space program at Vandenberg <span class="hlt">Air</span> Force Base (VAFB) in California. One of their responsibilities is to monitor upper-level <span class="hlt">winds</span> to ensure safe launch operations of the Minuteman III ballistic missile. The 30 OSSWF tasked the Applied Meteorology Unit (AMU) to analyze VAFB sounding data with the goal of determining the probability of violating (PoV) their upper-level thresholds for <span class="hlt">wind</span> speed and shear constraints specific to this launch vehicle, and to develop a tool that will calculate the PoV of each constraint on the day of launch. In order to calculate the probability of exceeding each constraint, the AMU collected and analyzed historical data from VAFB. The historical sounding data were retrieved from the National Oceanic and Atmospheric Administration Earth System Research Laboratory archive for the years 1994-2011 and then stratified into four sub-seasons: January-March, April-June, July-September, and October-December. The maximum <span class="hlt">wind</span> speed and 1000-ft shear values for each sounding in each subseason were determined. To accurately calculate the PoV, the AMU determined the theoretical distributions that best fit the maximum <span class="hlt">wind</span> speed and maximum shear datasets. Ultimately it was discovered that the maximum <span class="hlt">wind</span> speeds follow a Gaussian distribution while the maximum shear values follow a lognormal distribution. These results were applied when calculating the averages and standard deviations needed for the historical and real-time PoV calculations. In addition to the requirements outlined in the original task plan, the AMU also included forecast sounding data from the Rapid Refresh model. This information provides further insight for the launch weather officers (LWOs) when determining if a <span class="hlt">wind</span> constraint violation will occur over the next few hours on day of launch. The interactive graphical user interface (GUI) for this project was developed in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050009951&hterms=time+management+skills&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dtime%2Bmanagement%2Bskills','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050009951&hterms=time+management+skills&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dtime%2Bmanagement%2Bskills"><span><span class="hlt">Wind</span> Prediction Accuracy for <span class="hlt">Air</span> Traffic Management Decision Support Tools</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cole, Rod; Green, Steve; Jardin, Matt; Schwartz, Barry; Benjamin, Stan</p> <p>2000-01-01</p> <p>The performance of <span class="hlt">Air</span> Traffic Management and flight deck decision support tools depends in large part on the accuracy of the supporting 4D trajectory predictions. This is particularly relevant to conflict prediction and active advisories for the resolution of conflicts and the conformance with of traffic-flow management flow-rate constraints (e.g., arrival metering / required time of arrival). Flight test results have indicated that <span class="hlt">wind</span> prediction errors may represent the largest source of trajectory prediction error. The tests also discovered relatively large errors (e.g., greater than 20 knots), existing in pockets of space and time critical to ATM DST performance (one or more sectors, greater than 20 minutes), are inadequately represented by the classic RMS aggregate prediction-accuracy studies of the past. To facilitate the identification and reduction of DST-critical <span class="hlt">wind</span>-prediction errors, NASA has lead a collaborative research and development activity with MIT Lincoln Laboratories and the Forecast Systems Lab of the National Oceanographic and Atmospheric Administration (NOAA). This activity, begun in 1996, has focussed on the development of key metrics for ATM DST performance, assessment of <span class="hlt">wind</span>-prediction skill for state of the art systems, and development/validation of system enhancements to improve skill. A 13 month study was conducted for the Denver Center airspace in 1997. Two complementary <span class="hlt">wind</span>-prediction systems were analyzed and compared to the forecast performance of the then standard 60 km Rapid Update Cycle - version 1 (RUC-1). One system, developed by NOAA, was the prototype 40-km RUC-2 that became operational at NCEP in 1999. RUC-2 introduced a faster cycle (1 hr vs. 3 hr) and improved mesoscale physics. The second system, Augmented <span class="hlt">Winds</span> (AW), is a prototype en route <span class="hlt">wind</span> application developed by MITLL based on the Integrated Terminal <span class="hlt">Wind</span> System (ITWS). AW is run at a local facility (Center) level, and updates RUC predictions based on an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatCC...7...58L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatCC...7...58L"><span>Meltwater produced by <span class="hlt">wind</span>-albedo interaction stored in an East Antarctic ice shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lenaerts, J. T. M.; Lhermitte, S.; Drews, R.; Ligtenberg, S. R. M.; Berger, S.; Helm, V.; Smeets, C. J. P. P.; Broeke, M. R. Van Den; van de Berg, W. J.; van Meijgaard, E.; Eijkelboom, M.; Eisen, O.; Pattyn, F.</p> <p>2017-01-01</p> <p>Surface melt and subsequent firn <span class="hlt">air</span> depletion can ultimately lead to disintegration of Antarctic ice shelves causing grounded glaciers to accelerate and sea level to rise. In the Antarctic Peninsula, foehn <span class="hlt">winds</span> enhance melting near the grounding line, which in the recent past has led to the disintegration of the most northerly ice shelves. Here, we provide observational and model evidence that this process also occurs over an East Antarctic ice shelf, where meltwater-induced firn <span class="hlt">air</span> depletion is found in the grounding zone. Unlike the Antarctic Peninsula, where foehn events originate from episodic interaction of the circumpolar westerlies with the topography, in coastal East Antarctica high <span class="hlt">temperatures</span> are caused by persistent katabatic <span class="hlt">winds</span> originating from the ice sheet’s interior. Katabatic <span class="hlt">winds</span> warm and mix the <span class="hlt">air</span> as it flows downward and cause widespread snow erosion, explaining >3 K higher near-surface <span class="hlt">temperatures</span> in summer and surface melt doubling in the grounding zone compared with its surroundings. Additionally, these <span class="hlt">winds</span> expose blue ice and firn with lower surface albedo, further enhancing melt. The in situ observation of supraglacial flow and englacial storage of meltwater suggests that ice-shelf grounding zones in East Antarctica, like their Antarctic Peninsula counterparts, are vulnerable to hydrofracturing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JQSRT.188...52Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JQSRT.188...52Y"><span>Development of a mobile Doppler lidar system for <span class="hlt">wind</span> and <span class="hlt">temperature</span> measurements at 30-70 km</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yan, Zhaoai; Hu, Xiong; Guo, Wenjie; Guo, Shangyong; Cheng, Yongqiang; Gong, Jiancun; Yue, Jia</p> <p>2017-02-01</p> <p>A mobile Doppler lidar system has been developed to simultaneously measure zonal and meridional <span class="hlt">winds</span> and <span class="hlt">temperature</span> from 30 to 70 km. Each of the two zonal and meridional <span class="hlt">wind</span> subsystems employs a 15 W power, 532 nm laser and a 1 m diameter telescope. Iodine vapor filters are used to stabilize laser frequency and to detect the Doppler shift of backscattered signal. The integration method is used for <span class="hlt">temperature</span> measurement. Experiments were carried out using the mobile Doppler lidar in August 2014 at Qinghai, China (91°E, 38°N). The zonal <span class="hlt">wind</span> was measured from 20 to 70 km at a 3 km spatial resolution and 2 h temporal resolution. The measurement error is about 0.5 m/s at 30 km, and 10 m/s at 70 km. In addition, the <span class="hlt">temperature</span> was measured from 30 to 70 km at 1 km spatial resolution and 1 h temporal resolution. The <span class="hlt">temperature</span> measurement error is about 0.4 K at 30 km, and 8.0 K at 70 km. Comparison of the lidar results with the <span class="hlt">temperature</span> of the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER), the zonal <span class="hlt">wind</span> of the Modern-Era Retrospective Analysis for Re-search and Applications (MERRA), and radiosonde zonal <span class="hlt">wind</span> shows good agreement, indicating that the Doppler lidar results are reliable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC51E0850G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC51E0850G"><span>The EUSTACE project: delivering global, daily information on surface <span class="hlt">air</span> <span class="hlt">temperature</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ghent, D.; Rayner, N. A.</p> <p>2017-12-01</p> <p>Day-to-day variations in surface <span class="hlt">air</span> <span class="hlt">temperature</span> affect society in many ways; however, daily surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurements are not available everywhere. A global daily analysis cannot be achieved with measurements made in situ alone, so incorporation of satellite retrievals is needed. To achieve this, in the EUSTACE project (2015-2018, https://www.eustaceproject.eu) we have developed an understanding of the relationships between traditional (land and marine) surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurements and retrievals of surface skin <span class="hlt">temperature</span> from satellite measurements, i.e. Land Surface <span class="hlt">Temperature</span>, Ice Surface <span class="hlt">Temperature</span>, Sea Surface <span class="hlt">Temperature</span> and Lake Surface Water <span class="hlt">Temperature</span>. Here we discuss the science needed to produce a fully-global daily analysis (or ensemble of analyses) of surface <span class="hlt">air</span> <span class="hlt">temperature</span> on the centennial scale, integrating different ground-based and satellite-borne data types. Information contained in the satellite retrievals is used to create globally-complete fields in the past, using statistical models of how surface <span class="hlt">air</span> <span class="hlt">temperature</span> varies in a connected way from place to place. This includes developing new "Big Data" analysis methods as the data volumes involved are considerable. We will present recent progress along this road in the EUSTACE project, i.e.: • identifying inhomogeneities in daily surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurement series from weather stations and correcting for these over Europe; • estimating surface <span class="hlt">air</span> <span class="hlt">temperature</span> over all surfaces of Earth from surface skin <span class="hlt">temperature</span> retrievals; • using new statistical techniques to provide information on higher spatial and temporal scales than currently available, making optimum use of information in data-rich eras. Information will also be given on how interested users can become involved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015IAUGA..2251702B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015IAUGA..2251702B"><span>Thermospheric nighttime <span class="hlt">wind</span> and <span class="hlt">temperature</span> analysis from some 2014 stormy nights monitored at Oukaimeden Observatory by RENOIR instrument</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bounhir, Aziza; Benkhaldoun, Zouhair; Kaab, Mohamed; Makela, Jonathan J.; Harding, Brian; Fisher, Daniel J.; Lagheryeb, Amine; Khalifa, Malki; Lazrek, Mohamed; Daassou, Ahmed</p> <p>2015-08-01</p> <p>In this paper we report on the thermospheric <span class="hlt">winds</span> and <span class="hlt">temperatures</span> over Oukaimeden Observatory in Morocco in some stormy nights during the year 2014. These results are based on Fabry-Perot interferometer (FPI) measurements of Doppler shifts and Doppler broadenings of the 630.0nm spectral emission and pertain to the lower thermosphere region, near 250km altitude. This FPI is a part of RENOIR experiment installed thanks to scientific cooperation program with university of Illinois Urbana (USA).The storm energy input modify the global circulation in the thermosphere resulting in significant changes in the ionospheric plasma properties. Thermospheric and ionospheric storms are closely connected.We first set up the climatological behavior of the thermospheric <span class="hlt">winds</span> and <span class="hlt">temperature</span> during quiet nights. These results will be presented in this session in a separate abstract (M. Kaab & Z. Benkhaldoun et al) . Then we investigate the departure of the <span class="hlt">winds</span> and the <span class="hlt">temperatures</span> from their climatological behavior during some magnetic storms. The <span class="hlt">winds</span> present many features. We can notice westward <span class="hlt">winds</span> and an enhancement of the equatorward <span class="hlt">winds</span> with sometimes an appearance of a poleward component. We also notice a significant increase of the <span class="hlt">temperature</span> that last several hours. By looking trough the geomagnetic indices we investigate the delay of thermospheric storm time in our region and its effects on the <span class="hlt">winds</span> and <span class="hlt">temperature</span> patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70122722','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70122722"><span>Can <span class="hlt">air</span> <span class="hlt">temperature</span> be used to project influences of climate change on stream <span class="hlt">temperature</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>Arismendi, Ivan; Safeeq, Mohammad; Dunham, Jason B.; Johnson, Sherri L.</p> <p>2014-01-01</p> <p>Worldwide, lack of data on stream <span class="hlt">temperature</span> has motivated the use of regression-based statistical models to predict stream <span class="hlt">temperatures</span> based on more widely available data on <span class="hlt">air</span> <span class="hlt">temperatures</span>. Such models have been widely applied to project responses of stream <span class="hlt">temperatures</span> under climate change, but the performance of these models has not been fully evaluated. To address this knowledge gap, we examined the performance of two widely used linear and nonlinear regression models that predict stream <span class="hlt">temperatures</span> based on <span class="hlt">air</span> <span class="hlt">temperatures</span>. We evaluated model performance and temporal stability of model parameters in a suite of regulated and unregulated streams with 11–44 years of stream <span class="hlt">temperature</span> data. Although such models may have validity when predicting stream <span class="hlt">temperatures</span> within the span of time that corresponds to the data used to develop them, model predictions did not transfer well to other time periods. Validation of model predictions of most recent stream <span class="hlt">temperatures</span>, based on <span class="hlt">air</span> temperature–stream <span class="hlt">temperature</span> relationships from previous time periods often showed poor performance when compared with observed stream <span class="hlt">temperatures</span>. Overall, model predictions were less robust in regulated streams and they frequently failed in detecting the coldest and warmest <span class="hlt">temperatures</span> within all sites. In many cases, the magnitude of errors in these predictions falls within a range that equals or exceeds the magnitude of future projections of climate-related changes in stream <span class="hlt">temperatures</span> reported for the region we studied (between 0.5 and 3.0 °C by 2080). The limited ability of regression-based statistical models to accurately project stream <span class="hlt">temperatures</span> over time likely stems from the fact that underlying processes at play, namely the heat budgets of <span class="hlt">air</span> and water, are distinctive in each medium and vary among localities and through time.</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://hdl.handle.net/2060/20130010089','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130010089"><span>A Peak <span class="hlt">Wind</span> Probability Forecast Tool for Kennedy Space Center and Cape Canaveral <span class="hlt">Air</span> Force Station</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Crawford, Winifred; Roeder, William</p> <p>2008-01-01</p> <p>This conference abstract describes the development of a peak <span class="hlt">wind</span> forecast tool to assist forecasters in determining the probability of violating launch commit criteria (LCC) at Kennedy Space Center (KSC) and Cape Canaveral <span class="hlt">Air</span> Force Station (CCAFS) in east-central Florida. The peak <span class="hlt">winds</span> are an important forecast element for both the Space Shuttle and Expendable Launch Vehicle (ELV) programs. The LCC define specific peak <span class="hlt">wind</span> thresholds for each launch operation that cannot be exceeded in order to ensure the safety of the vehicle. The 45th Weather Squadron (45 WS) has found that peak <span class="hlt">winds</span> are a challenging parameter to forecast, particularly in the cool season months of October through April. Based on the importance of forecasting peak <span class="hlt">winds</span>, the 45 WS tasked the Applied Meteorology Unit (AMU) to develop a short-range peak-<span class="hlt">wind</span> forecast tool to assist in forecasting LCC violatioas.The tool will include climatologies of the 5-minute mean end peak <span class="hlt">winds</span> by month, hour, and direction, and probability distributions of the peak <span class="hlt">winds</span> as a function of the 5-minute mean <span class="hlt">wind</span> speeds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014BoLMe.150..381W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BoLMe.150..381W"><span>Numerical Simulations of Laminar <span class="hlt">Air</span>-Water Flow of a Non-linear Progressive Wave at Low <span class="hlt">Wind</span> Speed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wen, X.; Mobbs, S.</p> <p>2014-03-01</p> <p>A numerical simulation for two-dimensional laminar <span class="hlt">air</span>-water flow of a non-linear progressive water wave with large steepness is performed when the background <span class="hlt">wind</span> speed varies from zero to the wave phase speed. It is revealed that in the water the difference between the analytical solution of potential flow and numerical solution of viscous flow is very small, indicating that both solutions of the potential flow and viscous flow describe the water wave very accurately. In the <span class="hlt">air</span> the solutions of potential and viscous flows are very different due to the effects of viscosity. The velocity distribution in the airflow is strongly influenced by the background <span class="hlt">wind</span> speed and it is found that three <span class="hlt">wind</span> speeds, , (the maximum orbital velocity of a water wave), and (the wave phase speed), are important in distinguishing different features of the flow patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29369893','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29369893"><span>Effects of Ambient <span class="hlt">Temperature</span> and Forced-<span class="hlt">air</span> Warming on Intraoperative Core <span class="hlt">Temperature</span>: A Factorial Randomized Trial.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pei, Lijian; Huang, Yuguang; Xu, Yiyao; Zheng, Yongchang; Sang, Xinting; Zhou, Xiaoyun; Li, Shanqing; Mao, Guangmei; Mascha, Edward J; Sessler, Daniel I</p> <p>2018-05-01</p> <p>The effect of ambient <span class="hlt">temperature</span>, with and without active warming, on intraoperative core <span class="hlt">temperature</span> remains poorly characterized. The authors determined the effect of ambient <span class="hlt">temperature</span> on core <span class="hlt">temperature</span> changes with and without forced-<span class="hlt">air</span> warming. In this unblinded three-by-two factorial trial, 292 adults were randomized to ambient <span class="hlt">temperatures</span> 19°, 21°, or 23°C, and to passive insulation or forced-<span class="hlt">air</span> warming. The primary outcome was core <span class="hlt">temperature</span> change between 1 and 3 h after induction. Linear mixed-effects models assessed the effects of ambient <span class="hlt">temperature</span>, warming method, and their interaction. A 1°C increase in ambient <span class="hlt">temperature</span> attenuated the negative slope of core <span class="hlt">temperature</span> change 1 to 3 h after anesthesia induction by 0.03 (98.3% CI, 0.01 to 0.06) °Ccore/(h°Cambient) (P < 0.001), for patients who received passive insulation, but not for those warmed with forced-<span class="hlt">air</span> (-0.01 [98.3% CI, -0.03 to 0.01] °Ccore/[h°Cambient]; P = 0.40). Final core <span class="hlt">temperature</span> at the end of surgery increased 0.13°C (98.3% CI, 0.07 to 0.20; P < 0.01) per degree increase in ambient <span class="hlt">temperature</span> with passive insulation, but was unaffected by ambient <span class="hlt">temperature</span> during forced-<span class="hlt">air</span> warming (0.02 [98.3% CI, -0.04 to 0.09] °Ccore/°Cambient; P = 0.40). After an average of 3.4 h of surgery, core <span class="hlt">temperature</span> was 36.3° ± 0.5°C in each of the forced-<span class="hlt">air</span> groups, and ranged from 35.6° to 36.1°C in passively insulated patients. Ambient intraoperative <span class="hlt">temperature</span> has a negligible effect on core <span class="hlt">temperature</span> when patients are warmed with forced <span class="hlt">air</span>. The effect is larger when patients are passively insulated, but the magnitude remains small. Ambient <span class="hlt">temperature</span> can thus be set to comfortable levels for staff in patients who are actively warmed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15859404','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15859404"><span>[Dust storms trend in the Capital Circle of China over the past 50 years and its correlation with <span class="hlt">temperature</span>, precipitation and <span class="hlt">wind</span>].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Yu-fu; Tang, Hai-ping</p> <p>2005-01-01</p> <p>The trends of number of dust storm days of the selected 11 meteorological stations from their established year to 2000 as well as their correlations with <span class="hlt">temperature</span>, precipitation and <span class="hlt">wind</span> are revealed. The number of dust storm days of the Capital Circle of China is distinctly variable in space and time. The numbers of dust storm days of the western area are far more than those of the eastern area. The interannual variability of number of dust storm days is remarkable. The number of dust storm days of the following 7 stations, Erlianhaote, Abaga, Xilinhaote, Fengning, Zhangjiakou, Huailai and Beijing, declined along the past decades, but those of the other four stations had no significant upward or downward trends. There is a marked seasonality of the number of dust storm days, and the maximum was in April. The correlation between number of dust storm days and number of days of mean <span class="hlt">wind</span> velocity > 5 m/s, which is critical <span class="hlt">wind</span> velocity to entrain sand into the <span class="hlt">air</span>, was strongest among the three climatic factor. There were significant positive correlations between the number of dust storm days and number of days of mean <span class="hlt">wind</span> velocity > 5 m/s in 6 stations. The second strongest climatic factor correlated with the number of dust storm days is <span class="hlt">temperature</span>. There are significant negative correlations between the number of dust storm days and mean annual <span class="hlt">temperature</span>, mean winter <span class="hlt">temperature</span>, mean spring <span class="hlt">temperature</span> in 3 or 4 stations. The correlation between the number of dust storm days and precipitation is weakest. Only one station, Zhurihe, showes significant negative correlation between the number of dust storm days and spring rainfall. There are 4 stations whose number of dust storm days don't significantly correlate with the climate. In the end, the spatial-temporal variability of dust storms and its relation with climate in the Capital Circle of China were discussed thoroughly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/985400','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/985400"><span>Freezing <span class="hlt">temperature</span> of finger skin.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wilson, O; Goldman, R F; Molnar, G W</p> <p>1976-10-01</p> <p>In 45 subjects, 154 frostnips of the finger were induced by cooling in <span class="hlt">air</span> at -15 degrees C with various <span class="hlt">wind</span> speeds. The mean supercooled skin <span class="hlt">temperature</span> at which frostnip appeared was -9.4 degrees C. The mean skin <span class="hlt">temperature</span> rise due to heat of fusion at ice crystallization was 5.3 degrees C. The skin <span class="hlt">temperature</span> rose to what was termed the apparent freezing point. The relation of this point to the supercooled skin <span class="hlt">temperature</span> was analyzed for the three <span class="hlt">wind</span> speeds used. An apparent freezing point for a condition of no supercooling was calculated, estimating the highest <span class="hlt">temperature</span> at which skin freezes at a given <span class="hlt">wind</span> speed. The validity of the obtained differences in apparent freezing point was tested by an analysis of covariance. Although not statistically significant, the data suggest that the apparent freezing point with no supercooling decreases with increasing <span class="hlt">wind</span> velocity. The highest calculated apparent freezing point at -15 degrees C and 6.8 m/s was 1.2 degrees C lower than the true freezing point for skin previously determined in brine, which is a statistically significant difference.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912697R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912697R"><span>The EUSTACE project: delivering global, daily information on surface <span class="hlt">air</span> <span class="hlt">temperature</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rayner, Nick</p> <p>2017-04-01</p> <p>Day-to-day variations in surface <span class="hlt">air</span> <span class="hlt">temperature</span> affect society in many ways; however, daily surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurements are not available everywhere. A global daily analysis cannot be achieved with measurements made in situ alone, so incorporation of satellite retrievals is needed. To achieve this, in the EUSTACE project (2015-June 2018, https://www.eustaceproject.eu) we are developing an understanding of the relationships between traditional (land and marine) surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurements and retrievals of surface skin <span class="hlt">temperature</span> from satellite measurements, i.e. Land Surface <span class="hlt">Temperature</span>, Ice Surface <span class="hlt">Temperature</span>, Sea Surface <span class="hlt">Temperature</span> and Lake Surface Water <span class="hlt">Temperature</span>. Here we discuss the science needed to produce a fully-global daily analysis (or ensemble of analyses) of surface <span class="hlt">air</span> <span class="hlt">temperature</span> on the centennial scale, integrating different ground-based and satellite-borne data types. Information contained in the satellite retrievals is used to create globally-complete fields in the past, using statistical models of how surface <span class="hlt">air</span> <span class="hlt">temperature</span> varies in a connected way from place to place. As the data volumes involved are considerable, such work needs to include development of new "Big Data" analysis methods. We will present recent progress along this road in the EUSTACE project: 1. providing new, consistent, multi-component estimates of uncertainty in surface skin <span class="hlt">temperature</span> retrievals from satellites; 2. identifying inhomogeneities in daily surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurement series from weather stations and correcting for these over Europe; 3. estimating surface <span class="hlt">air</span> <span class="hlt">temperature</span> over all surfaces of Earth from surface skin <span class="hlt">temperature</span> retrievals; 4. using new statistical techniques to provide information on higher spatial and temporal scales than currently available, making optimum use of information in data-rich eras. Information will also be given on how interested users can become involved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC51D1201G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC51D1201G"><span>The EUSTACE project: delivering global, daily information on surface <span class="hlt">air</span> <span class="hlt">temperature</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ghent, D.; Rayner, N. A.</p> <p>2016-12-01</p> <p>Day-to-day variations in surface <span class="hlt">air</span> <span class="hlt">temperature</span> affect society in many ways; however, daily surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurements are not available everywhere. A global daily analysis cannot be achieved with measurements made in situ alone, so incorporation of satellite retrievals is needed. To achieve this, in the EUSTACE project (2015-June 2018, https://www.eustaceproject.eu) we are developing an understanding of the relationships between traditional (land and marine) surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurements and retrievals of surface skin <span class="hlt">temperature</span> from satellite measurements, i.e. Land Surface <span class="hlt">Temperature</span>, Ice Surface <span class="hlt">Temperature</span>, Sea Surface <span class="hlt">Temperature</span> and Lake Surface Water <span class="hlt">Temperature</span>. Here we discuss the science needed to produce a fully-global daily analysis (or ensemble of analyses) of surface <span class="hlt">air</span> <span class="hlt">temperature</span> on the centennial scale, integrating different ground-based and satellite-borne data types. Information contained in the satellite retrievals is used to create globally-complete fields in the past, using statistical models of how surface <span class="hlt">air</span> <span class="hlt">temperature</span> varies in a connected way from place to place. As the data volumes involved are considerable, such work needs to include development of new "Big Data" analysis methods. We will present recent progress along this road in the EUSTACE project, i.e.: • providing new, consistent, multi-component estimates of uncertainty in surface skin <span class="hlt">temperature</span> retrievals from satellites; • identifying inhomogeneities in daily surface <span class="hlt">air</span> <span class="hlt">temperature</span> measurement series from weather stations and correcting for these over Europe; • estimating surface <span class="hlt">air</span> <span class="hlt">temperature</span> over all surfaces of Earth from surface skin <span class="hlt">temperature</span> retrievals; • using new statistical techniques to provide information on higher spatial and temporal scales than currently available, making optimum use of information in data-rich eras. Information will also be given on how interested users can become involved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19780043820&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DMagnetic%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19780043820&hterms=Magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DMagnetic%2Benergy"><span>Design of single-<span class="hlt">winding</span> energy-storage reactors for dc-to-dc converters using <span class="hlt">air</span>-gapped magnetic-core structures</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ohri, A. K.; Wilson, T. G.; Owen, H. A., Jr.</p> <p>1977-01-01</p> <p>A procedure is presented for designing <span class="hlt">air</span>-gapped energy-storage reactors for nine different dc-to-dc converters resulting from combinations of three single-<span class="hlt">winding</span> power stages for voltage stepup, current stepup and voltage stepup/current stepup and three controllers with control laws that impose constant-frequency, constant transistor on-time and constant transistor off-time operation. The analysis, based on the energy-transfer requirement of the reactor, leads to a simple relationship for the required minimum volume of the <span class="hlt">air</span> gap. Determination of this minimum <span class="hlt">air</span> gap volume then permits the selection of either an <span class="hlt">air</span> gap or a cross-sectional core area. Having picked one parameter, the minimum value of the other immediately leads to selection of the physical magnetic structure. Other analytically derived equations are used to obtain values for the required turns, the inductance, and the maximum rms <span class="hlt">winding</span> current. The design procedure is applicable to a wide range of magnetic material characteristics and physical configurations for the <span class="hlt">air</span>-gapped magnetic structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880013119','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880013119"><span>Monthly mean global climatology of <span class="hlt">temperature</span>, <span class="hlt">wind</span>, geopotential height, and pressure for 0 - 120 km</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fleming, Eric L.; Chandra, Sushil; Schoeberl, Mark R.; Barnett, John J.</p> <p>1988-01-01</p> <p>A monthly mean climatology is presented of <span class="hlt">temperature</span>, <span class="hlt">wind</span>, and geopotential height with nearly pole-to-pole coverage (80 S to 80 N) for 0 to 210 km, which can be used as a function of altitude and pressure. The purpose is to provide a reference for various atmospheric research and analysis activities. Data sources and methods of computation are described; in general, hydrostatic and thermal <span class="hlt">wind</span> balance are maintained at all levels and latitudes. As observed in a series of cross-sectional plots, this climatology accurately reproduces most of the characteristic features of the atmosphere such as equatorial <span class="hlt">wind</span> and the general structure of the tropopause, stratopause, and mesopause. A series of zonal <span class="hlt">wind</span> profiles is also represented comparing this climatological <span class="hlt">wind</span> with monthly mean climatological direct <span class="hlt">wind</span> measurements in the upper mesosphere and lower thermosphere. The <span class="hlt">temperature</span> and zonal <span class="hlt">wind</span> climatology at stratospheric levels is compared with corresponding data from the National Meteorological Center, and general agreement is observed between the two data sets. Tables of the climatological values as a function of latitude and height for each month are contained in Appendix B, and are also available in floppy disk.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080023396&hterms=Summer&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DSummer','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080023396&hterms=Summer&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DSummer"><span>Differences and Similarities between Summer and Winter <span class="hlt">Temperatures</span> and <span class="hlt">Winds</span> during MaCWAVE</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schmidlin, F. J.; Goldberg, R. A.</p> <p>2008-01-01</p> <p>The Mountain and Convective Waves Ascending Vertically Experiment (MaCWAVE) was carried out in two sequences: one during the summer from the Andoya Rocket Range (69N) during July 2002 to examine convective initiation of gravity waves. The second was a winter sequence from ESRANGE (68N) during January 2003 to examine mountain-initiated waves. Inflatable falling spheres released from small meteorological rockets provided significant information about the variation of <span class="hlt">temperature</span> and <span class="hlt">wind</span> from 50 km and higher. The small rocket launch activity was restricted to 12-hour periods that inhibited observing a full diurnal cycle, nonetheless, the time-history of the measurements have provided information about tidal motion. During summer, <span class="hlt">temperature</span> variation was smaller than observed during winter when peak differences reached 15-20 K at 80-85 km. variation in zonal <span class="hlt">winds</span> varied up to more than 100 mps in summer and winter. Times of <span class="hlt">wind</span> vs. altitude showed that the peak zonal component occurred approximately two hours ahead of the peak meridional <span class="hlt">wind</span>. Measurement details and the observed variations are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27370122','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27370122"><span>Characterization of <span class="hlt">air</span> <span class="hlt">temperature</span> in modern ion chambers due to phantom geometry and ambient <span class="hlt">temperature</span> changes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saenz, Daniel L; Kirby, Neil; Gutiérrez, Alonso N</p> <p>2016-07-01</p> <p><span class="hlt">Temperature</span> and pressure corrections are necessary to account for the varying mass of <span class="hlt">air</span> in the sensitive volume of a vented ionization chamber (IC) when performing absolute dose measurements. Locations commonly used to measure the presumed IC <span class="hlt">air</span> <span class="hlt">temperature</span> may not accurately represent the chamber cavity <span class="hlt">air</span> <span class="hlt">temperature</span>, and phantoms undergoing <span class="hlt">temperature</span> changes further compound the problem. Prior studies have characterized thermal equilibrium in separate phantoms for Farmer chambers alone. However, the purpose of this study was to characterize the cavity <span class="hlt">air</span> <span class="hlt">temperature</span> dependence on changes in the ambient <span class="hlt">temperature</span> and phantom geometry configuration for a wider and more modern variety of chambers to determine if previously published wait times apply to these chambers as well. Thermal conduction properties were experimentally investigated by modifying a PTW 0.3 cm(3) Semiflex IC with a thermocouple replacing the central electrode. <span class="hlt">Air</span> cavity <span class="hlt">temperature</span> versus time was recorded in three phantom geometries characteristic of common absolute dose measurements. The phantoms were (15 ± 1) °C before measurement with an IC at the treatment vault <span class="hlt">temperature</span> of (21 ± 1) °C. Simulations were conducted to provide a theoretical basis for the measurements and to simulate <span class="hlt">temperature</span> response of a PTW PinPoint® and Farmer chamber. The simulation methods were first validated by comparison with measured Semiflex chamber thermal response curves before extension to the other chambers. Two thermal equilibria curves were recorded on different time scales. IC <span class="hlt">temperature</span> initially dropped to the colder phantom <span class="hlt">temperature</span> but subsequently increased as the phantom itself equilibrated with the warmer room <span class="hlt">temperature</span>. In a large phantom of dimensions (25.5 × 25.5 × 23.4) cm(3), 3 min was required before the IC <span class="hlt">temperature</span> reached within 0.5 °C of its equilibrium within the phantom. Similarly, wait times of 2 min were needed for 7.5 and 2 cm slab phantoms. Recording</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1788c0024A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1788c0024A"><span>Effect of water <span class="hlt">temperature</span> and <span class="hlt">air</span> stream velocity on performance of direct evaporative <span class="hlt">air</span> cooler for thermal comfort</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aziz, Azridjal; Mainil, Rahmat Iman; Mainil, Afdhal Kurniawan; Listiono, Hendra</p> <p>2017-01-01</p> <p>The aim of this work was to determine the effects of water <span class="hlt">temperature</span> and <span class="hlt">air</span> stream velocity on the performance of direct evaporative <span class="hlt">air</span> cooler (DEAC) for thermal comfort. DEAC system requires the lower cost than using vapor compression refrigeration system (VCRS), because VCRS use a compressor to circulate refrigerant while DEAC uses a pump for circulating water in the cooling process to achieve thermal comfort. The study was conducted by varying the water <span class="hlt">temperature</span> (10°C, 20°C, 30°C, 40°C, and 50°C) at different <span class="hlt">air</span> stream velocity (2,93 m/s, 3.9 m/s and 4,57 m/s). The results show that the relative humidity (RH) in test room tends to increase with the increasing of water <span class="hlt">temperature</span>, while on the variation of <span class="hlt">air</span> stream velocity, RH remains constant at the same water <span class="hlt">temperature</span>, because the amount of water that evaporates increase with the increasing water <span class="hlt">temperature</span>. The cooling effectiveness (CE) increase with the increasing of <span class="hlt">air</span> stream velocity where the higher CE was obtained at lower water <span class="hlt">temperature</span> (10°C) with high <span class="hlt">air</span> velocity (4,57m/s). The lower room <span class="hlt">temperature</span> (26°C) was achieved at water <span class="hlt">temperature</span> 10°C and <span class="hlt">air</span> stream velocity 4.57 m/s with the relative humidity 85,87%. DEAC can be successfully used in rooms that have smoothly <span class="hlt">air</span> circulation to fulfill the indoor thermal comfort.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B31A0518T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B31A0518T"><span>Observed impacts of <span class="hlt">wind</span> farms on land surface <span class="hlt">temperature</span> in Inner Mongolia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tang, B.; Zhao, X.; Wu, D.; Zhao, W.; Wei, H.</p> <p>2015-12-01</p> <p>Abstract: The <span class="hlt">wind</span> turbine industry in china has experienced a dramatic increase in recent years and <span class="hlt">wind</span> farms (WFs) have an impact on the underlying surface conditions of climate system. This paper assesses the impacts of <span class="hlt">wind</span> farms by analyzing the variations of the land surface <span class="hlt">temperature</span> (LST) data for the period of 2003-2014 over a region consisted of 1097 turbines in the Huitengxile <span class="hlt">Wind</span> Farm, the largest <span class="hlt">wind</span> farm in Asia. We first compare the spatial coupling between the geographic layouts of the WFs and the spatial patterns of LST changes of two periods (post- versus pre- <span class="hlt">wind</span> turbines construction) and then employ the difference of LST between WF pixels and surrounding non-WF pixels to quantify the effects of WFs. The results reveal that the LST at daytime increases by 0.52-0.86°C in winter, spring and autumn and decreases by about 0.56°C in summer over the WFs on average, with the spatial pattern of this warming or cooling generally coupled with the geographic distribution of the <span class="hlt">wind</span> turbines, while the changes in LST at nighttime are much noisier. The daytime LST warming or cooling effects vary with seasons, and the strongest warming and tightest spatial coupling are in autumn months of September-November. The seasonal variations in albedo due to the construction of <span class="hlt">wind</span> turbines are primarily responsible for the daytime LST changes. Areal mean decreases in winter, spring and autumn and increase in summer in albedo are observed over the WFs and the spatial pattern and magnitude of the changes in albedo couple very well with the layouts of the <span class="hlt">wind</span> turbines. The increase (decrease) in albedo over the WFs indicates that WFs across the Huitengxile grassland absorb less (more) incoming radiation, thus resulting in a decrease (increase) in LST at daytime. The inter-annual variations in areal mean LST differences at daytime are highly correlated with those in areal mean albedo differences for all four seasons (R2=0.48~0.67). Our findings are in contrast</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840014950','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840014950"><span><span class="hlt">Wind</span> and solar powered turbine</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wells, I. D.; Koh, J. L.; Holmes, M. (Inventor)</p> <p>1984-01-01</p> <p>A power generating station having a generator driven by solar heat assisted ambient <span class="hlt">wind</span> is described. A first plurality of radially extendng <span class="hlt">air</span> passages direct ambient <span class="hlt">wind</span> to a radial flow <span class="hlt">wind</span> turbine disposed in a centrally located opening in a substantially disc-shaped structure. A solar radiation collecting surface having black bodies is disposed above the fist plurality of <span class="hlt">air</span> passages and in communication with a second plurality of radial <span class="hlt">air</span> passages. A cover plate enclosing the second plurality of radial <span class="hlt">air</span> passages is transparent so as to permit solar radiation to effectively reach the black bodies. The second plurality of <span class="hlt">air</span> passages direct ambient <span class="hlt">wind</span> and thermal updrafts generated by the black bodies to an axial flow turbine. The rotating shaft of the turbines drive the generator. The solar and <span class="hlt">wind</span> drien power generating system operates in electrical cogeneration mode with a fuel powered prime mover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1916285M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1916285M"><span>Influence of <span class="hlt">wind</span>-induced <span class="hlt">air</span> pressure fluctuations on topsoil gas concentrations within a Scots pine forest</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohr, Manuel; Laemmel, Thomas; Maier, Martin; Schindler, Dirk</p> <p>2017-04-01</p> <p>Commonly it is assumed that soil gas transport is dominated by molecular diffusion. Few recent studies indicate that the atmosphere above the soil triggers non-diffusive gas transport processes in the soil, which can enhance soil gas transport and therefore soil gas efflux significantly. During high <span class="hlt">wind</span> speed conditions, the so called pressure pumping effect has been observed: the enhancement of soil gas transport through dynamic changes in the <span class="hlt">air</span> pressure field above the soil. However, the amplitudes and frequencies of the <span class="hlt">air</span> pressure fluctuations responsible for pressure pumping are still uncertain. Moreover, an in situ observation of the pressure pumping effect is still missing. To investigate the pressure pumping effect, airflow measurements above and below the canopy of a Scots pine forest and high-precision relative <span class="hlt">air</span> pressure measurements were conducted in the below-canopy space and in the soil over a measurement period of 16 weeks. To monitor the soil gas transport, a newly developed gas measurement system was used. The gas measurement system continuously injects helium as a tracer gas into the soil until a diffusive steady state is reached. With the steady state concentration profile of the tracer gas, it is possible to inversely model the gas diffusion coefficient profile of the soil. If the gas diffusion coefficient profile differed from steady state, we deduced that the soil gas transport is not only diffusive, but also influenced by non-diffusive processes. Results show that the occurrence of small <span class="hlt">air</span> pressure fluctuations is strongly dependent on the mean above-canopy <span class="hlt">wind</span> speed. The <span class="hlt">wind</span>-induced <span class="hlt">air</span> pressure fluctuations have mean amplitudes up to 10 Pa and lie in the frequency range 0.01-0.1 Hz. To describe the pumping motion of the <span class="hlt">air</span> pressure field, the pressure pumping coefficient (PPC) was defined as the mean change in pressure per second. The PPC shows a clear quadratic dependence on mean above-canopy <span class="hlt">wind</span> speed. Empirical modelling of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1034104','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1034104"><span>System and method for monitoring and controlling stator <span class="hlt">winding</span> <span class="hlt">temperature</span> in a de-energized AC motor</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Lu, Bin [Kenosha, WI; Luebke, Charles John [Sussex, WI; Habetler, Thomas G [Snellville, GA; Zhang, Pinjia [Atlanta, GA; Becker, Scott K [Oak Creek, WI</p> <p>2011-12-27</p> <p>A system and method for measuring and controlling stator <span class="hlt">winding</span> <span class="hlt">temperature</span> in an AC motor while idling is disclosed. The system includes a circuit having an input connectable to an AC source and an output connectable to an input terminal of a multi-phase AC motor. The circuit further includes a plurality of switching devices to control current flow and terminal voltages in the multi-phase AC motor and a controller connected to the circuit. The controller is configured to activate the plurality of switching devices to create a DC signal in an output of the motor control device corresponding to an input to the multi-phase AC motor, determine or estimate a stator <span class="hlt">winding</span> resistance of the multi-phase AC motor based on the DC signal, and estimate a stator <span class="hlt">temperature</span> from the stator <span class="hlt">winding</span> resistance. <span class="hlt">Temperature</span> can then be controlled and regulated by DC injection into the stator <span class="hlt">windings</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1740864','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1740864"><span>The lagged effect of cold <span class="hlt">temperature</span> and <span class="hlt">wind</span> chill on cardiorespiratory mortality in Scotland</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Carder, M; McNamee, R; Beverland, I; Elton, R; Cohen, G; Boyd, J; Agius, R</p> <p>2005-01-01</p> <p>Aims: To investigate the lagged effects of cold <span class="hlt">temperature</span> on cardiorespiratory mortality and to determine whether "<span class="hlt">wind</span> chill" is a better predictor of these effects than "dry bulb" <span class="hlt">temperature</span>. Methods: Generalised linear Poisson regression models were used to investigate the relation between mortality and "dry bulb" and "<span class="hlt">wind</span> chill" <span class="hlt">temperatures</span> in the three largest Scottish cities (Glasgow, Edinburgh, and Aberdeen) between January 1981 and December 2001. Effects of <span class="hlt">temperature</span> on mortality (lags up to one month) were quantified. Analyses were conducted for the whole year and by season (cool and warm seasons). Main results: <span class="hlt">Temperature</span> was a significant predictor of mortality with the strongest association observed between <span class="hlt">temperature</span> and respiratory mortality. There was a non-linear association between mortality and <span class="hlt">temperature</span>. Mortality increased as <span class="hlt">temperatures</span> fell throughout the range, but the rate of increase was steeper at <span class="hlt">temperatures</span> below 11°C. The association between <span class="hlt">temperature</span> and mortality persisted at lag periods beyond two weeks but the effect size generally decreased with increasing lag. For <span class="hlt">temperatures</span> below 11°C, a 1°C drop in the daytime mean <span class="hlt">temperature</span> on any one day was associated with an increase in mortality of 2.9% (95% CI 2.5 to 3.4), 3.4% (95% CI 2.6 to 4.1), 4.8% (95% CI 3.5 to 6.2) and 1.7% (95% CI 1.0 to 2.4) over the following month for all cause, cardiovascular, respiratory, and "other" cause mortality respectively. The effect of <span class="hlt">temperature</span> on mortality was not observed to be significantly modified by season. There was little indication that "<span class="hlt">wind</span> chill" <span class="hlt">temperature</span> was a better predictor of mortality than "dry bulb" <span class="hlt">temperature</span>. Conclusions: Exposure to cold <span class="hlt">temperature</span> is an important public health problem in Scotland, particularly for those dying from respiratory disease. PMID:16169916</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29210407','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29210407"><span>Three-dimensional vapor intrusion modeling approach that combines <span class="hlt">wind</span> and stack effects on indoor, atmospheric, and subsurface domains.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shirazi, Elham; Pennell, Kelly G</p> <p>2017-12-13</p> <p>Vapor intrusion (IV) exposure risks are difficult to characterize due to the role of atmospheric, building and subsurface processes. This study presents a three-dimensional VI model that extends the common subsurface fate and transport equations to incorporate <span class="hlt">wind</span> and stack effects on indoor <span class="hlt">air</span> pressure, building <span class="hlt">air</span> exchange rate (AER) and indoor contaminant concentration to improve VI exposure risk estimates. The model incorporates three modeling programs: (1) COMSOL Multiphysics to model subsurface fate and transport processes, (2) CFD0 to model atmospheric <span class="hlt">air</span> flow around the building, and (3) CONTAM to model indoor <span class="hlt">air</span> quality. The combined VI model predicts AER values, zonal indoor <span class="hlt">air</span> pressures and zonal indoor <span class="hlt">air</span> contaminant concentrations as a function of <span class="hlt">wind</span> speed, <span class="hlt">wind</span> direction and outdoor and indoor <span class="hlt">temperature</span>. Steady state modeling results for a single-story building with a basement demonstrate that <span class="hlt">wind</span> speed, <span class="hlt">wind</span> direction and opening locations in a building play important roles in changing the AER, indoor <span class="hlt">air</span> pressure, and indoor <span class="hlt">air</span> contaminant concentration. Calculated indoor <span class="hlt">air</span> pressures ranged from approximately -10 Pa to +4 Pa depending on weather conditions and building characteristics. AER values, mass entry rates and indoor <span class="hlt">air</span> concentrations vary depending on weather conditions and building characteristics. The presented modeling approach can be used to investigate the relationship between building features, AER, building pressures, soil gas concentrations, indoor <span class="hlt">air</span> concentrations and VI exposure risks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26121613','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26121613"><span>Observed Thermal Impacts of <span class="hlt">Wind</span> Farms Over Northern Illinois.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Slawsky, Lauren M; Zhou, Liming; Baidya Roy, Somnath; Xia, Geng; Vuille, Mathias; Harris, Ronald A</p> <p>2015-06-25</p> <p>This paper assesses impacts of three <span class="hlt">wind</span> farms in northern Illinois using land surface <span class="hlt">temperature</span> (LST) data from the Moderate Resolution Imaging Spectroradiometer (MODIS) instruments onboard the Terra and Aqua satellites for the period 2003-2013. Changes in LST between two periods (before and after construction of the <span class="hlt">wind</span> turbines) and between <span class="hlt">wind</span> farm pixels and nearby non-<span class="hlt">wind</span>-farm pixels are quantified. An areal mean increase in LST by 0.18-0.39 °C is observed at nighttime over the <span class="hlt">wind</span> farms, with the geographic distribution of this warming effect generally spatially coupled with the layout of the <span class="hlt">wind</span> turbines (referred to as the spatial coupling), while there is no apparent impact on daytime LST. The nighttime LST warming effect varies with seasons, with the strongest warming in winter months of December-February, and the tightest spatial coupling in summer months of June-August. Analysis of seasonal variations in <span class="hlt">wind</span> speed and direction from weather balloon sounding data and Automated Surface Observing System hourly observations from nearby stations suggest stronger <span class="hlt">winds</span> correspond to seasons with greater warming and larger downwind impacts. The early morning soundings in Illinois are representative of the nighttime boundary layer and exhibit strong <span class="hlt">temperature</span> inversions across all seasons. The strong and relatively shallow inversion in summer leaves warm <span class="hlt">air</span> readily available to be mixed down and spatially well coupled with the turbine. Although the warming effect is strongest in winter, the spatial coupling is more erratic and spread out than in summer. These results suggest that the observed warming signal at nighttime is likely due to the net downward transport of heat from warmer <span class="hlt">air</span> aloft to the surface, caused by the turbulent mixing in the wakes of the spinning turbine rotor blades.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4541818','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4541818"><span>Observed Thermal Impacts of <span class="hlt">Wind</span> Farms Over Northern Illinois</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Slawsky, Lauren M.; Zhou, Liming; Baidya Roy, Somnath; Xia, Geng; Vuille, Mathias; Harris, Ronald A.</p> <p>2015-01-01</p> <p>This paper assesses impacts of three <span class="hlt">wind</span> farms in northern Illinois using land surface <span class="hlt">temperature</span> (LST) data from the Moderate Resolution Imaging Spectroradiometer (MODIS) instruments onboard the Terra and Aqua satellites for the period 2003–2013. Changes in LST between two periods (before and after construction of the <span class="hlt">wind</span> turbines) and between <span class="hlt">wind</span> farm pixels and nearby non-<span class="hlt">wind</span>-farm pixels are quantified. An areal mean increase in LST by 0.18–0.39 °C is observed at nighttime over the <span class="hlt">wind</span> farms, with the geographic distribution of this warming effect generally spatially coupled with the layout of the <span class="hlt">wind</span> turbines (referred to as the spatial coupling), while there is no apparent impact on daytime LST. The nighttime LST warming effect varies with seasons, with the strongest warming in winter months of December-February, and the tightest spatial coupling in summer months of June-August. Analysis of seasonal variations in <span class="hlt">wind</span> speed and direction from weather balloon sounding data and Automated Surface Observing System hourly observations from nearby stations suggest stronger <span class="hlt">winds</span> correspond to seasons with greater warming and larger downwind impacts. The early morning soundings in Illinois are representative of the nighttime boundary layer and exhibit strong <span class="hlt">temperature</span> inversions across all seasons. The strong and relatively shallow inversion in summer leaves warm <span class="hlt">air</span> readily available to be mixed down and spatially well coupled with the turbine. Although the warming effect is strongest in winter, the spatial coupling is more erratic and spread out than in summer. These results suggest that the observed warming signal at nighttime is likely due to the net downward transport of heat from warmer <span class="hlt">air</span> aloft to the surface, caused by the turbulent mixing in the wakes of the spinning turbine rotor blades. PMID:26121613</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC54C..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC54C..04H"><span>Ice Surface <span class="hlt">Temperature</span> Variability in the Polar Regions and the Relationships to 2 Meter <span class="hlt">Air</span> <span class="hlt">Temperatures</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoyer, J.; Madsen, K. S.; Englyst, P. N.</p> <p>2017-12-01</p> <p>Determining the surface and near surface <span class="hlt">air</span> <span class="hlt">temperature</span> from models or observations in the Polar Regions is challenging due to the extreme conditions and the lack of in situ observations. The errors in near surface <span class="hlt">temperature</span> products are typically larger than for other regions of the world, and the potential for using Earth Observations is large. As part of the EU project, EUSTACE, we have developed empirical models for the relationship between the satellite observed skin ice <span class="hlt">temperatures</span> and 2m <span class="hlt">air</span> <span class="hlt">temperatures</span>. We use the Arctic and Antarctic Sea and sea ice Surface <span class="hlt">Temperatures</span> from thermal Infrared satellite sensors (AASTI) reanalysis to estimate daily surface <span class="hlt">air</span> <span class="hlt">temperature</span> over land ice and sea ice for the Arctic and the Antarctic. Large efforts have been put into collecting and quality controlling in situ observations from various data portals and research projects. The reconstruction is independent of numerical weather prediction models and thus provides an important alternative to modelled <span class="hlt">air</span> <span class="hlt">temperature</span> estimates. The new surface <span class="hlt">air</span> <span class="hlt">temperature</span> data record has been validated against more than 58.000 independent in situ measurements for the four surface types: Arctic sea ice, Greenland ice sheet, Antarctic sea ice and Antarctic ice sheet. The average correlations are 92-97% and average root mean square errors are 3.1-3.6°C for the four surface types. The root mean square error includes the uncertainty of the in-situ measurement, which ranges from 0.5 to 2°C. A comparison with ERA-Interim shows a consistently better performance of the satellite based <span class="hlt">air</span> <span class="hlt">temperatures</span> than the ERA-Interim for the Greenland ice sheet, when compared against observations not used in any of the two estimates. This is encouraging and demonstrates the values of these products. In addition, the procedure presented here works on satellite observations that are available in near real time and this opens up for a near real time estimation of the surface <span class="hlt">air</span> <span class="hlt">temperature</span> over</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1398195-impacts-interactive-dust-its-direct-radiative-forcing-interannual-variations-temperature-precipitation-winter-over-east-asia-impacts-dust-iavs-temperature','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1398195-impacts-interactive-dust-its-direct-radiative-forcing-interannual-variations-temperature-precipitation-winter-over-east-asia-impacts-dust-iavs-temperature"><span>Impacts of interactive dust and its direct radiative forcing on interannual variations of <span class="hlt">temperature</span> and precipitation in winter over East Asia: Impacts of Dust on IAVs of <span class="hlt">Temperature</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>Lou, Sijia; Russell, Lynn M.; Yang, Yang</p> <p></p> <p>We used 150-year pre-industrial simulations of the Community Earth System Model (CESM) to quantify the impacts of interactively-modeled dust emissions on the interannual variations of <span class="hlt">temperature</span> and precipitation over East Asia during the East Asian Winter Monsoon (EAWM) season. The simulated December-January-February dust column burden and dust optical depth are lower over northern China in the strongest EAWM years than those of the weakest years, with regional mean values lower by 38.3% and 37.2%, respectively. The decrease in dust over the dust source regions (the Taklamakan and Gobi Deserts) and the downwind region (such as the North China Plain) leadsmore » to an increase in direct radiative forcing (RF) both at the surface and top of atmosphere by up to 1.5 and 0.75 W m-2, respectively. The effects of EAWM-related variations in surface <span class="hlt">winds</span>, precipitation and their effects on dust emissions and wet removal contribute about 67% to the total dust-induced variations of direct RF at the surface and partly offset the cooling that occurs with the EAWM strengthening by heating the surface. The variations of surface <span class="hlt">air</span> <span class="hlt">temperature</span> induced by the changes in <span class="hlt">wind</span> and dust emissions increase by 0.4-0.6 K over eastern coastal China, northeastern China, and Japan, which weakens the impact of EAWM on surface <span class="hlt">air</span> <span class="hlt">temperature</span> by 3–18% in these regions. The warming results from the combined effects of changes in direct RF and easterly <span class="hlt">wind</span> anomalies that bring warm <span class="hlt">air</span> from the ocean to these regions. Moreover, the feedback of the changes in <span class="hlt">wind</span> on dust emissions weakens the variations of the sea level pressure gradient on the Siberian High while enhancing the Maritime Continent Low. Therefore, cold <span class="hlt">air</span> is prevented from being transported from Siberia, Kazakhstan, western and central China to the western Pacific Ocean and decreases surface <span class="hlt">air</span> <span class="hlt">temperature</span> by 0.6 K and 2 K over central China and the Tibetan Plateau, respectively. Over eastern coastal China, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ThEng..63..329M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ThEng..63..329M"><span>Startup of <span class="hlt">air</span>-cooled condensers and dry cooling towers at low <span class="hlt">temperatures</span> of the cooling <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Milman, O. O.; Ptakhin, A. V.; Kondratev, A. V.; Shifrin, B. A.; Yankov, G. G.</p> <p>2016-05-01</p> <p>The problems of startup and performance of <span class="hlt">air</span>-cooled condensers (ACC) and dry cooling towers (DCT) at low cooling <span class="hlt">air</span> <span class="hlt">temperatures</span> are considered. Effects of the startup of the ACC at sub-zero <span class="hlt">temperatures</span> are described. Different options of the ACC heating up are analyzed, and examples of existing technologies are presented (electric heating, heating up with hot <span class="hlt">air</span> or steam, and internal and external heating). The use of additional heat exchanging sections, steam tracers, in the DCT design is described. The need for high power in cases of electric heating and heating up with hot <span class="hlt">air</span> is noted. An experimental stand for research and testing of the ACC startup at low <span class="hlt">temperatures</span> is described. The design of the three-pass ACC unit is given, and its advantages over classical single-pass design at low <span class="hlt">temperatures</span> are listed. The formation of ice plugs inside the heat exchanging tubes during the start-up of ACC and DCT at low cooling <span class="hlt">air</span> <span class="hlt">temperatures</span> is analyzed. Experimental data on the effect of the steam flow rate, steam nozzle distance from the heat-exchange surface, and their orientation in space on the metal <span class="hlt">temperature</span> were collected, and test results are analyzed. It is noted that the surface <span class="hlt">temperature</span> at the end of the heat up is almost independent from its initial <span class="hlt">temperature</span>. Recommendations for the safe start-up of ACCs and DCTs are given. The heating flow necessary to sufficiently heat up heat-exchange surfaces of ACCs and DCTs for the safe startup is estimated. The technology and the process of the heat up of the ACC with the heating steam external supply are described by the example of the startup of the full-scale section of the ACC at sub-zero <span class="hlt">temperatures</span> of the cooling <span class="hlt">air</span>, and the advantages of the proposed start-up technology are confirmed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS31A1997S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS31A1997S"><span>Comparison of Sea-<span class="hlt">Air</span> CO2 Flux Estimates Using Satellite-Based Versus Mooring <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>Sutton, A. J.; Sabine, C. L.; Feely, R. A.; Wanninkhof, R. H.</p> <p>2016-12-01</p> <p>The global ocean is a major sink of anthropogenic CO2, absorbing approximately 27% of CO2 emissions since the beginning of the industrial revolution. Any variation or change in the ocean CO2 sink has implications for future climate. Observations of sea-<span class="hlt">air</span> CO2 flux have relied primarily on ship-based underway measurements of partial pressure of CO2 (pCO2) combined with satellite, model, or multi-platform <span class="hlt">wind</span> products. Direct measurements of ΔpCO2 (seawater - <span class="hlt">air</span> pCO2) and <span class="hlt">wind</span> speed from moored platforms now allow for high-resolution CO2 flux time series. Here we present a comparison of CO2 flux calculated from moored ΔpCO2 measured on four moorings in different biomes of the Pacific Ocean in combination with: 1) Cross-Calibrated Multi-Platform (CCMP) <span class="hlt">winds</span> or 2) <span class="hlt">wind</span> speed measurements made on ocean reference moorings excluded from the CCMP dataset. Preliminary results show using CCMP <span class="hlt">winds</span> overestimates CO2 flux on average by 5% at the Kuroshio Extension Observatory, Ocean Station Papa, WHOI Hawaii Ocean Timeseries Station, and Stratus. In general, CO2 flux seasonality follows patterns of seawater pCO2 and SST with periods of CO2 outgassing during summer and CO2 uptake during winter at these locations. Any offsets or seasonal biases in CCMP <span class="hlt">winds</span> could impact global ocean sink estimates using this data product. Here we present patterns and trends between the two CO2 flux estimates and discuss the potential implications for tracking variability and change in global ocean CO2 uptake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PApGe.tmp.1266S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PApGe.tmp.1266S"><span><span class="hlt">Wind</span>-Induced <span class="hlt">Air</span>-Flow Patterns in an Urban Setting: Observations and Numerical Modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sattar, Ahmed M. A.; Elhakeem, Mohamed; Gerges, Bishoy N.; Gharabaghi, Bahram; Gultepe, Ismail</p> <p>2018-04-01</p> <p>City planning can have a significant effect on <span class="hlt">wind</span> flow velocity patterns and thus natural ventilation. Buildings with different heights are roughness elements that can affect the near- and far-field <span class="hlt">wind</span> flow velocity. This paper aims at investigating the impact of an increase in building height on the nearby velocity fields. A prototype urban setting of buildings with two different heights (25 and 62.5 cm) is built up and placed in a <span class="hlt">wind</span> tunnel. <span class="hlt">Wind</span> flow velocity around the buildings is mapped at different heights. <span class="hlt">Wind</span> tunnel measurements are used to validate a 3D-numerical Reynolds averaged Naviers-Stokes model. The validated model is further used to calculate the <span class="hlt">wind</span> flow velocity patterns for cases with different building heights. It was found that increasing the height of some buildings in an urban setting can lead to the formation of large horseshoe vortices and eddies around building corners. A separation area is formed at the leeward side of the building, and the recirculation of <span class="hlt">air</span> behind the building leads to the formation of slow rotation vortices. The opposite effect is observed in the wake (cavity) region of the buildings, where both the cavity length and width are significantly reduced, and this resulted in a pronounced increase in the <span class="hlt">wind</span> flow velocity. A significant increase in the <span class="hlt">wind</span> flow velocity in the wake region of tall buildings with a value of up to 30% is observed. The spatially averaged velocities around short buildings also increased by 25% compared to those around buildings with different heights. The increase in the height of some buildings is found to have a positive effect on the <span class="hlt">wind</span> ventilation at the pedestrian level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990004150','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990004150"><span><span class="hlt">Temperature</span> Tunable <span class="hlt">Air</span>-Gap Etalon Filter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Krainak, Michael A.; Stephen, Mark A.; Lunt, David L.</p> <p>1998-01-01</p> <p>We report on experimental measurements of a <span class="hlt">temperature</span> tuned <span class="hlt">air</span>-gap etalon filter. The filter exhibits <span class="hlt">temperature</span> dependent wavelength tuning of 54 pm/C. It has a nominal center wavelength of 532 nm. The etalon filter has a 27 pm optical bandpass and 600 pm free spectral range (finesse approximately 22). The experimental results are in close agreement with etalon theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800024075','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800024075"><span>Apparatus for supplying conditioned <span class="hlt">air</span> at a substantially constant <span class="hlt">temperature</span> and humidity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Obler, H. D. (Inventor)</p> <p>1980-01-01</p> <p>The apparatus includes a supply duct coupled to a source of supply <span class="hlt">air</span> for carrying the supply <span class="hlt">air</span> therethrough. A return duct is coupled to the supply duct for carrying return conditioned <span class="hlt">air</span> therethrough. A <span class="hlt">temperature</span> reducing device is coupled to the supply duct for decreasing the <span class="hlt">temperature</span> of the supply and return conditioned <span class="hlt">air</span>. A by-pass duct is coupled to the supply duct for selectively directing portions of the supply and return conditioned <span class="hlt">air</span> around the <span class="hlt">temperature</span> reducing device. Another by-pass duct is coupled to the return duct for selectively directing portions of the return conditioned <span class="hlt">air</span> around the supply duct and the <span class="hlt">temperature</span> reduction device. Controller devices selectively control the flow and amount of mixing of the supply and return conditioned <span class="hlt">air</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EOSTr..94Q.372B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EOSTr..94Q.372B"><span>Crowdsourcing urban <span class="hlt">air</span> <span class="hlt">temperature</span> measurements using smartphones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Balcerak, Ernie</p> <p>2013-10-01</p> <p>Crowdsourced data from cell phone battery <span class="hlt">temperature</span> sensors could be used to contribute to improved real-time, high-resolution <span class="hlt">air</span> <span class="hlt">temperature</span> estimates in urban areas, a new study shows. <span class="hlt">Temperature</span> observations in cities are in some cases currently limited to a few weather stations, but there are millions of smartphone users in many cities. The batteries in cell phones have <span class="hlt">temperature</span> sensors to avoid damage to the phone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A31H0154J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A31H0154J"><span>Weekly Oscillation of Daily Climatology of <span class="hlt">Air</span> <span class="hlt">Temperature</span>: Implication for Anthropogenic Attribution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jiang, S.; Wang, K.</p> <p>2016-12-01</p> <p>During national holiday and weekend, human activity and anthropogenic emission are expected to be much less than those during workday. Therefore, the contrast of environmental factors (i.e., <span class="hlt">air</span> <span class="hlt">temperature</span> and <span class="hlt">air</span> quality) between national holiday (or weekend) and workday has been attributed to anthropogenic impact. For example, daily maximum (Tmax), minimum (Tmin) and mean (Tmean) <span class="hlt">air</span> <span class="hlt">temperatures</span> during the Chinese Spring Festival holiday were found to be 0. 6°C less than those of nearby workdays. We evaluated the contrasts using daily meteorological observations collected at 2479 stations in China from 1961 to 2015. The contrasts were evaluated with two methods. The first directly compared <span class="hlt">air</span> <span class="hlt">temperatures</span> between Chinese Spring Festival holiday and nearby workdays. The second first composited a daily climatology of <span class="hlt">air</span> <span class="hlt">temperatures</span> centered on the first day of Chinese Spring Festival holiday, and the seasonal cycles of <span class="hlt">air</span> <span class="hlt">temperatures</span> were then removed using polynomial regressions. The average of the derived daily deviation of <span class="hlt">air</span> <span class="hlt">temperatures</span> can be regarded as anthropogenic impact of Chinese Spring Festival holiday. We found that these two methods obtained nearly the same results. However, we found that the so-called anthropogenic impact during Chinese Spring Festival was not unique because the daily deviations of <span class="hlt">air</span> <span class="hlt">temperatures</span> had obvious weekly oscillations. The daily deviations of <span class="hlt">air</span> <span class="hlt">temperature</span> had periods of 7 days and 9 days, which explain 60% of the variance of daily deviations of Tmax, Tmin, and Tmean. These results indicate that the so-called anthropogenic impacts are primarily caused by natural variability, i.e., weekly oscillations of the <span class="hlt">air</span> <span class="hlt">temperatures</span>. This study also has great implication for the studies on weekend effect of the environmental factors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.2333B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.2333B"><span>On the importance of high-frequency <span class="hlt">air-temperature</span> fluctuations for spectroscopic corrections of open-path carbon dioxide flux measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bogoev, Ivan; Helbig, Manuel; Sonnentag, Oliver</p> <p>2015-04-01</p> <p> systematic errors in the CO2 density measurements. Under conditions of high positive or negative sensible heat flux, <span class="hlt">air-temperature</span> fluctuations are correlated with fluctuations of the vertical <span class="hlt">wind</span> component and can lead to significant biases in the CO2 flux estimates. This study demonstrates that sonically derived fast-response <span class="hlt">air</span> <span class="hlt">temperature</span> in the optical sensing path of an OP gas analyzer can replace the slow-response measurements from the <span class="hlt">temperature</span> sensor as a scaling parameter in the calibration model to correct for these <span class="hlt">air</span> <span class="hlt">temperature</span>-induced spectroscopic effects. Our approach is evaluated by comparison between different OP and CP gas analyzer-based eddy-covariance systems in ecosystems with low CO2 uptake under a range of sensible heat flux regimes and varying meteorological parameters. We show that ignoring high-frequency spectroscopic effects can lead to false interpretations of net ecosystem CO2 exchange for specific site and environmental conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1715292B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1715292B"><span>Statistical modeling of urban <span class="hlt">air</span> <span class="hlt">temperature</span> distributions under different synoptic conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beck, Christoph; Breitner, Susanne; Cyrys, Josef; Hald, Cornelius; Hartz, Uwe; Jacobeit, Jucundus; Richter, Katja; Schneider, Alexandra; Wolf, Kathrin</p> <p>2015-04-01</p> <p>Within urban areas <span class="hlt">air</span> <span class="hlt">temperature</span> may vary distinctly between different locations. These intra-urban <span class="hlt">air</span> <span class="hlt">temperature</span> variations partly reach magnitudes that are relevant with respect to human thermal comfort. Therefore and furthermore taking into account potential interrelations with other health related environmental factors (e.g. <span class="hlt">air</span> quality) it is important to estimate spatial patterns of intra-urban <span class="hlt">air</span> <span class="hlt">temperature</span> distributions that may be incorporated into urban planning processes. In this contribution we present an approach to estimate spatial <span class="hlt">temperature</span> distributions in the urban area of Augsburg (Germany) by means of statistical modeling. At 36 locations in the urban area of Augsburg <span class="hlt">air</span> <span class="hlt">temperatures</span> are measured with high temporal resolution (4 min.) since December 2012. These 36 locations represent different typical urban land use characteristics in terms of varying percentage coverages of different land cover categories (e.g. impervious, built-up, vegetated). Percentage coverages of these land cover categories have been extracted from different sources (Open Street Map, European Urban Atlas, Urban Morphological Zones) for regular grids of varying size (50, 100, 200 meter horizonal resolution) for the urban area of Augsburg. It is well known from numerous studies that land use characteristics have a distinct influence on <span class="hlt">air</span> <span class="hlt">temperature</span> and as well other climatic variables at a certain location. Therefore <span class="hlt">air</span> <span class="hlt">temperatures</span> at the 36 locations are modeled utilizing land use characteristics (percentage coverages of land cover categories) as predictor variables in Stepwise Multiple Regression models and in Random Forest based model approaches. After model evaluation via cross-validation appropriate statistical models are applied to gridded land use data to derive spatial urban <span class="hlt">air</span> <span class="hlt">temperature</span> distributions. Varying models are tested and applied for different seasons and times of the day and also for different synoptic conditions (e.g. clear and calm</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018FrES..tmp...16Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018FrES..tmp...16Z"><span>Estimation of <span class="hlt">wind</span> speeds inside Super Typhoon Nepartak from AMSR2 low-frequency brightness <span class="hlt">temperatures</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, Lei; Yin, Xiaobin; Shi, Hanqing; Wang, Zhenzhan; Xu, Qing</p> <p>2018-04-01</p> <p>Accurate estimations of typhoon-level <span class="hlt">winds</span> are highly desired over the western Pacific Ocean. A <span class="hlt">wind</span> speed retrieval algorithm is used to retrieve the <span class="hlt">wind</span> speeds within Super Typhoon Nepartak (2016) using 6.9- and 10.7-GHz brightness <span class="hlt">temperatures</span> from the Japanese Advanced Microwave Scanning Radiometer 2 (AMSR2) sensor on board the Global Change Observation Mission-Water 1 (GCOM-W1) satellite. The results show that the retrieved <span class="hlt">wind</span> speeds clearly represent the intensification process of Super Typhoon Nepartak. A good agreement is found between the retrieved <span class="hlt">wind</span> speeds and the Soil Moisture Active Passive <span class="hlt">wind</span> speed product. The mean bias is 0.51 m/s, and the root-mean-square difference is 1.93 m/s between them. The retrieved maximum <span class="hlt">wind</span> speeds are 59.6 m/s at 04:45 UTC on July 6 and 71.3 m/s at 16:58 UTC on July 6. The two results demonstrate good agreement with the results reported by the China Meteorological Administration and the Joint Typhoon Warning Center. In addition, Feng-Yun 2G (FY-2G) satellite infrared images, Feng-Yun 3C (FY-3C) microwave atmospheric sounder data, and AMSR2 brightness <span class="hlt">temperature</span> images are also used to describe the development and structure of Super Typhoon Nepartak.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ThApC.132..857L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ThApC.132..857L"><span>An analysis of spatial representativeness of <span class="hlt">air</span> <span class="hlt">temperature</span> monitoring stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Suhua; Su, Hongbo; Tian, Jing; Wang, Weizhen</p> <p>2018-05-01</p> <p>Surface <span class="hlt">air</span> <span class="hlt">temperature</span> is an essential variable for monitoring the atmosphere, and it is generally acquired at meteorological stations that can provide information about only a small area within an r m radius ( r-neighborhood) of the station, which is called the representable radius. In studies on a local scale, ground-based observations of surface <span class="hlt">air</span> <span class="hlt">temperatures</span> obtained from scattered stations are usually interpolated using a variety of methods without ascertaining their effectiveness. Thus, it is necessary to evaluate the spatial representativeness of ground-based observations of surface <span class="hlt">air</span> <span class="hlt">temperature</span> before conducting studies on a local scale. The present study used remote sensing data to estimate the spatial distribution of surface <span class="hlt">air</span> <span class="hlt">temperature</span> using the advection-energy balance for <span class="hlt">air</span> <span class="hlt">temperature</span> (ADEBAT) model. Two target stations in the study area were selected to conduct an analysis of spatial representativeness. The results showed that one station (AWS 7) had a representable radius of about 400 m with a possible error of less than 1 K, while the other station (AWS 16) had the radius of about 250 m. The representable radius was large when the heterogeneity of land cover around the station was small.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PSST...27e5021C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PSST...27e5021C"><span>The effect of DC voltage polarity on ionic <span class="hlt">wind</span> in ambient <span class="hlt">air</span> for cooling purposes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, She; van den Berg, R. G. W.; Nijdam, S.</p> <p>2018-05-01</p> <p>Gas flows can be induced by gas discharges like DC coronas because neutral molecules gain momentum by ion-neutral collisions. This can be used for active cooling and has advantages over mechanical fans. We investigate ionic <span class="hlt">wind</span> by a DC corona discharge under different conditions with an emphasis on the effects of voltage polarity and the transition between different discharge regimes. We also consider the gas <span class="hlt">temperature</span> of a DC corona which is important when it is to be used for cooling purposes. Although DC coronas are usually characterized as low <span class="hlt">temperature</span> plasmas, gas heating can have a significant impact on flow generation, especially at higher operating voltages. In this paper, a 5–20 kV DC voltage of positive and negative polarity is applied to a needle–cylinder electrode. The ionic <span class="hlt">wind</span> velocity at the exit of the cylinder electrode is measured by hot wire anemometry and the emission spectrum is used to study the gas <span class="hlt">temperature</span>. It is found that the flow velocity induced by positive coronas is higher than that by negative coronas for voltages above 10–15 kV, which is also demonstrated by a phenomenological EHD force model. Furthermore, a heated column is observed by Schlieren technique for both voltage polarities. An improved self-consistent ionic <span class="hlt">wind</span> model considering heat transfer is built to study the <span class="hlt">temperature</span> distribution. The simulation results indicate that the gas flow velocity is lower on the symmetry axis when the <span class="hlt">temperature</span> gradient is taken into account, something which is usually ignored in ionic <span class="hlt">wind</span> simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A33G0328S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A33G0328S"><span>Windblown Dust and <span class="hlt">Air</span> Quality Under a Changing Climate in the Pacific Northwest</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharratt, B. S.; Tatarko, J.; Abatzoglou, J. T.; Fox, F.; Huggins, D. R.</p> <p>2016-12-01</p> <p><span class="hlt">Wind</span> erosion is a concern for sustainable agriculture and societal health in the US Pacific Northwest. Indeed, <span class="hlt">wind</span> erosion continues to cause exceedances of the National Ambient <span class="hlt">Air</span> Quality Standard for PM10 in the region. Can we expect <span class="hlt">air</span> quality to deteriorate or improve as climate changes? Will <span class="hlt">wind</span> erosion escalate in the future under a warmer and drier climate as forecast for Australia, southern prairies of Canada, northern China, and United States Corn Belt and Colorado Plateau? To answer these questions, we used 18 global climate models, cropping systems simulation model (CropSyst), and the <span class="hlt">Wind</span> Erosion Prediction System (WEPS) to simulate the complex interactions among climate, crop production, and <span class="hlt">wind</span> erosion. These simulations were carried out in eastern Washington where <span class="hlt">wind</span> erosion of agricultural lands contribute to poor <span class="hlt">air</span> quality in the region. Our results suggest that an increase in <span class="hlt">temperature</span> and CO2 concentration, coupled with nominal increases in precipitation, will enhance biomass production and reduce soil and PM10 losses by the mid-21st century. This study reveals that climate change may reduce the risk of <span class="hlt">wind</span> erosion and improve <span class="hlt">air</span> quality in the Inland Pacific Northwest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29689465','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29689465"><span>Two-way effect modifications of <span class="hlt">air</span> pollution and <span class="hlt">air</span> <span class="hlt">temperature</span> on total natural and cardiovascular mortality in eight European urban areas.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Kai; Wolf, Kathrin; Breitner, Susanne; Gasparrini, Antonio; Stafoggia, Massimo; Samoli, Evangelia; Andersen, Zorana Jovanovic; Bero-Bedada, Getahun; Bellander, Tom; Hennig, Frauke; Jacquemin, Bénédicte; Pekkanen, Juha; Hampel, Regina; Cyrys, Josef; Peters, Annette; Schneider, Alexandra</p> <p>2018-07-01</p> <p>Although epidemiological studies have reported associations between mortality and both ambient <span class="hlt">air</span> pollution and <span class="hlt">air</span> <span class="hlt">temperature</span>, it remains uncertain whether the mortality effects of <span class="hlt">air</span> pollution are modified by <span class="hlt">temperature</span> and vice versa. Moreover, little is known on the interactions between ultrafine particles (diameter ≤ 100 nm, UFP) and <span class="hlt">temperature</span>. We investigated whether the short-term associations of particle number concentration (PNC in the ultrafine range (≤100 nm) or total PNC ≤ 3000 nm, as a proxy for UFP), particulate matter ≤ 2.5 μm (PM 2.5 ) and ≤ 10 μm (PM 10 ), and ozone with daily total natural and cardiovascular mortality were modified by <span class="hlt">air</span> <span class="hlt">temperature</span> and whether <span class="hlt">air</span> pollution levels affected the <span class="hlt">temperature</span>-mortality associations in eight European urban areas during 1999-2013. We first analyzed <span class="hlt">air</span> <span class="hlt">temperature</span>-stratified associations between <span class="hlt">air</span> pollution and total natural (nonaccidental) and cardiovascular mortality as well as <span class="hlt">air</span> pollution-stratified <span class="hlt">temperature</span>-mortality associations using city-specific over-dispersed Poisson additive models with a distributed lag nonlinear <span class="hlt">temperature</span> term in each city. All models were adjusted for long-term and seasonal trend, day of the week, influenza epidemics, and population dynamics due to summer vacation and holidays. City-specific effect estimates were then pooled using random-effects meta-analysis. Pooled associations between <span class="hlt">air</span> pollutants and total and cardiovascular mortality were overall positive and generally stronger at high relatively compared to low <span class="hlt">air</span> <span class="hlt">temperatures</span>. For example, on days with high <span class="hlt">air</span> <span class="hlt">temperatures</span> (>75th percentile), an increase of 10,000 particles/cm 3 in PNC corresponded to a 2.51% (95% CI: 0.39%, 4.67%) increase in cardiovascular mortality, which was significantly higher than that on days with low <span class="hlt">air</span> <span class="hlt">temperatures</span> (<25th percentile) [-0.18% (95% CI: -0.97%, 0.62%)]. On days with high <span class="hlt">air</span> pollution (>50th percentile), both heat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1046108','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1046108"><span><span class="hlt">Wind</span> flow through shrouded <span class="hlt">wind</span> turbines</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-03-01</p> <p>were so patient with me during this process, sometimes spending hours in the <span class="hlt">wind</span> tunnel room with me while I performed what seemed like endless runs ...disorderly <span class="hlt">wind</span> velocities that result from the rotating turbine blades . In 2011, a study conducted by the White House Office of Science and...targets, and scattering target returns” [4]. Furthermore, the shadowing effects from spinning <span class="hlt">wind</span> turbine blades can adversely impact <span class="hlt">air</span>-traffic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eosweb.larc.nasa.gov/project/narsto/narsto_epa_ss_st_louis_air_chem_pm_met_data_table','SCIGOV-ASDC'); return false;" href="https://eosweb.larc.nasa.gov/project/narsto/narsto_epa_ss_st_louis_air_chem_pm_met_data_table"><span>NARSTO EPA SS ST LOUIS <span class="hlt">AIR</span> CHEM PM MET DATA</span></a></p> <p><a target="_blank" href="http://eosweb.larc.nasa.gov/">Atmospheric Science Data Center </a></p> <p></p> <p>2018-04-09</p> <p>... <span class="hlt">Winds</span> Precipitation Amount Surface Pressure Solar Radiation Surface <span class="hlt">Air</span> <span class="hlt">Temperature</span> Particulates Trace Metals ... Earth Related Data:  Environmental Protection Agency Supersites St. Louis SCAR-B Block:  ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130012628','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130012628"><span>Developing a Peak <span class="hlt">Wind</span> Probability Forecast Tool for Kennedy Space Center and Cape Canaveral <span class="hlt">Air</span> Force Station</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lambert, WInifred; Roeder, William</p> <p>2007-01-01</p> <p>This conference presentation describes the development of a peak <span class="hlt">wind</span> forecast tool to assist forecasters in determining the probability of violating launch commit criteria (LCC) at Kennedy Space Center (KSC) and Cape Canaveral <span class="hlt">Air</span> Force Station (CCAFS) in east-central Florida. The peak <span class="hlt">winds</span> are an important forecast element for both the Space Shuttle and Expendable Launch Vehicle (ELV) programs. The LCC define specific peak <span class="hlt">wind</span> thresholds for each launch operation that cannot be exceeded in order to ensure the safety of the vehicle. The 45th Weather Squadron (45 WS) has found that peak <span class="hlt">winds</span> are a challenging parameter to forecast, particularly in the cool season months of October through April. Based on the importance of forecasting peak <span class="hlt">winds</span>, the 45 WS tasked the Applied Meteorology Unit (AMU) to develop a short-range peak-<span class="hlt">wind</span> forecast tool to assist in forecasting LCC violations. The tool will include climatologies of the 5-minute mean and peak <span class="hlt">winds</span> by month, hour, and direction, and probability distributions of the peak <span class="hlt">winds</span> as a function of the 5-minute mean <span class="hlt">wind</span> speeds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29255277','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29255277"><span>Satellite Observations of Imprint of Oceanic Current on <span class="hlt">Wind</span> Stress by <span class="hlt">Air</span>-Sea Coupling.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Renault, Lionel; McWilliams, James C; Masson, Sebastien</p> <p>2017-12-18</p> <p>Mesoscale eddies are present everywhere in the ocean and partly determine the mean state of the circulation and ecosystem. The current feedback on the surface <span class="hlt">wind</span> stress modulates the <span class="hlt">air</span>-sea transfer of momentum by providing a sink of mesoscale eddy energy as an atmospheric source. Using nine years of satellite measurements of surface stress and geostrophic currents over the global ocean, we confirm that the current-induced surface stress curl is linearly related to the current vorticity. The resulting coupling coefficient between current and surface stress (s τ [N s m -3 ]) is heterogeneous and can be roughly expressed as a linear function of the mean surface <span class="hlt">wind</span>. s τ expresses the sink of eddy energy induced by the current feedback. This has important implications for <span class="hlt">air</span>-sea interaction and implies that oceanic mean and mesoscale circulations and their effects on surface-layer ventilation and carbon uptake are better represented in oceanic models that include this feedback.</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/2007AGUFM.U52A..06T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.U52A..06T"><span>The Turbulent Structure of the Atmosphere: Vorticity, <span class="hlt">Winds</span> and <span class="hlt">Temperature</span> Emerge From Molecular Motion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tuck, A. F.; Hovde, S. J.; Lovejoy, S.; Schertzer, D.</p> <p>2007-12-01</p> <p>Application of generalized scale invariance to horizontal airborne observations of <span class="hlt">winds</span>, <span class="hlt">temperature</span>, ozone and humidity reveals the atmosphere as a random, non-Gaussian Levy process, having mean scaling exponents H (conservation), C1 (intermittency) and alpha (Levy) of 0.56, 0.05 and 1.6 respectively in the cases of <span class="hlt">winds</span> and <span class="hlt">temperature</span>. A correlation between the intermittency of <span class="hlt">temperature</span> and the ozone photodissociation rate in the Arctic lower stratosphere is interpreted in terms of the ring currents of non-equilibrium statistical mechanics in which vortices, fluid dynamical behavior, emerge from thermalized populations of Maxwellian molecules subjected to an anisotropy in the form of a flux. The emergence of jet streams and the definition of atmospheric <span class="hlt">temperature</span> are examined in the light of these results. The vertical scaling of <span class="hlt">wind</span>, <span class="hlt">temperature</span> and humidity is examined through the depth of the troposphere using data observed by GPS dropsondes from the NOAA Gulfstream 4 aircraft over the eastern Pacific Ocean in boreal winter. The results exclude isotropic turbulence in the atmosphere, and reveal the structure of static, moist static and dynamic (Richardson number) stabilities to be sparse fractal sets. Each stable layer contains a set of smaller scale unstable sublayers, each of which in turn contains a set of stable sub-sublayers and so on. The moist static stability scales differently to the dry static stability in the lower troposphere. As with the 'horizontal' data, the 'vertical' data reveal a correlation between H for horizontal <span class="hlt">wind</span> and measures of jet stream strength. It is pointed out that these results provide potentially a new way of testing numerical models of the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15536131','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15536131"><span>The influence of large-scale <span class="hlt">wind</span> power on global climate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Keith, David W; Decarolis, Joseph F; Denkenberger, David C; Lenschow, Donald H; Malyshev, Sergey L; Pacala, Stephen; Rasch, Philip J</p> <p>2004-11-16</p> <p>Large-scale use of <span class="hlt">wind</span> power can alter local and global climate by extracting kinetic energy and altering turbulent transport in the atmospheric boundary layer. We report climate-model simulations that address the possible climatic impacts of <span class="hlt">wind</span> power at regional to global scales by using two general circulation models and several parameterizations of the interaction of <span class="hlt">wind</span> turbines with the boundary layer. We find that very large amounts of <span class="hlt">wind</span> power can produce nonnegligible climatic change at continental scales. Although large-scale effects are observed, <span class="hlt">wind</span> power has a negligible effect on global-mean surface <span class="hlt">temperature</span>, and it would deliver enormous global benefits by reducing emissions of CO(2) and <span class="hlt">air</span> pollutants. Our results may enable a comparison between the climate impacts due to <span class="hlt">wind</span> power and the reduction in climatic impacts achieved by the substitution of <span class="hlt">wind</span> for fossil fuels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010cosp...38.1357P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010cosp...38.1357P"><span>Thermal zonal <span class="hlt">winds</span> in the Venus mesosphere from the Venus Express <span class="hlt">temperature</span> soundings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Piccialli, Arianna; Titov, Dmitri; Tellmann, Silvia; Migliorini, Alessandra; Read, Peter; Grassi, Davide; Paetzold, Martin; Haeusler, Bernd; Piccioni, Giuseppe; Drossart, Pierre</p> <p></p> <p>The Venus mesosphere (60-100 km altitude) is a transition region characterized by extremely complex dynamics: strong retrograde zonal <span class="hlt">winds</span> dominate in the troposphere and lower meso-sphere while a solar-antisolar circulation can be observed in the upper mesosphere. The super-rotation extends from the surface up to the cloud top (˜65 km altitude) with <span class="hlt">wind</span> speeds of only a few meters per second near the surface and reaching a maximum value of ˜100 m s-1 at cloud top, corresponding to a rotation period of ˜4 Earth days (˜60 times faster than Venus itself). The solar-antisolar circulation is driven by the day-night contrast in solar heating, and occurs above 110 km altitude with speeds of 120 m s-1 . The processes responsible for maintain-ing the zonal super-rotation in the lower atmosphere and its transition to the solar-antisolar circulation in the upper atmosphere are still poorly understood (Schubert et al.,2007). Different techniques have been used to obtain direct observations of <span class="hlt">wind</span> at various altitudes: tracking of clouds in ultraviolet (UV) and near infrared (NIR) images give information on <span class="hlt">wind</span> speeds at the cloud top (Moissl et al., 2009; Sanchez-Lavega et al., 2008) and within the clouds (˜47 km, ˜61 km) (Sanchez-Lavega et al., 2008) while ground-based measurements of Doppler shifts in the CO2 band at 10 µm (Sornig et al., 2008) and in several CO millimiter lines (Rengel et al., 2008) provide <span class="hlt">wind</span> speeds above the clouds up to ˜110 km altitude. The deep atmosphere from the surface up to the cloud top has been investigated through the Doppler tracking of descent probes and balloons (Counselman et al., 1980; Kerzhanovich and Limaye, 1985). In the mesosphere, between 45-85 km of altitude, where direct observations of <span class="hlt">wind</span> are not possible, the zonal <span class="hlt">wind</span> field can be derived from the vertical <span class="hlt">temperature</span> structure using a special approximation of the thermal <span class="hlt">wind</span> equation: based on cyclostrophic balance. Previous studies (Leovy, 1973; Newman et al</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880008244','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880008244"><span>Infrared low-level <span class="hlt">wind</span> shear work</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Adamson, Pat</p> <p>1988-01-01</p> <p>Results of field experiments for the detection of clear <span class="hlt">air</span> disturbance and low level <span class="hlt">wind</span> shear utilizing an infrared airborne system are given in vugraph form. The hits, misses and nuisance alarms scores are given. Information is given on the infrared spatial resolution technique. The popular index of aircraft hazard (F= WX over g - VN over AS) is developed for a remote <span class="hlt">temperature</span> sensor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100036761','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100036761"><span>Weather Research and Forecasting Model <span class="hlt">Wind</span> Sensitivity Study at Edwards <span class="hlt">Air</span> Force Base, CA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Watson, Leela R.; Bauman, William H., III</p> <p>2008-01-01</p> <p>NASA prefers to land the space shuttle at Kennedy Space Center (KSC). When weather conditions violate Flight Rules at KSC, NASA will usually divert the shuttle landing to Edwards <span class="hlt">Air</span> Force Base (EAFB) in Southern California. But forecasting surface <span class="hlt">winds</span> at EAFB is a challenge for the Spaceflight Meteorology Group (SMG) forecasters due to the complex terrain that surrounds EAFB, One particular phenomena identified by SMG is that makes it difficult to forecast the EAFB surface <span class="hlt">winds</span> is called "<span class="hlt">wind</span> cycling". This occurs when <span class="hlt">wind</span> speeds and directions oscillate among towers near the EAFB runway leading to a challenging deorbit bum forecast for shuttle landings. The large-scale numerical weather prediction models cannot properly resolve the <span class="hlt">wind</span> field due to their coarse horizontal resolutions, so a properly tuned high-resolution mesoscale model is needed. The Weather Research and Forecasting (WRF) model meets this requirement. The AMU assessed the different WRF model options to determine which configuration best predicted surface <span class="hlt">wind</span> speed and direction at EAFB, To do so, the AMU compared the WRF model performance using two hot start initializations with the Advanced Research WRF and Non-hydrostatic Mesoscale Model dynamical cores and compared model performance while varying the physics options.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ThApC.tmp..108L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ThApC.tmp..108L"><span><span class="hlt">Air</span> and wet bulb <span class="hlt">temperature</span> lapse rates and their impact on snowmaking in a Pyrenean ski resort</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>López-Moreno, Juan Ignacio; Navarro-Serrano, F.; Azorín-Molina, C.; Sánchez-Navarrete, P.; Alonso-González, E.; Rico, I.; Morán-Tejeda, E.; Buisan, S.; Revuelto, J.; Pons, M.; Vicente-Serrano, S. M.</p> <p>2018-03-01</p> <p>A set of 17 <span class="hlt">air</span> <span class="hlt">temperature</span> and relative humidity sensors were used to analyze the temporal variability of surface <span class="hlt">air</span> <span class="hlt">temperature</span> (Tair), wet bulb <span class="hlt">temperature</span> (Twb), and daily snowmaking hours (SM, number of hours per day with Twb < - 2 °C), lapse rates, and the occurrence of thermal inversions at the Formigal ski resort (Spanish Pyrenees) from December to March during three consecutive ski seasons (2012-2013, 2013-2014, and 2014-2015). The Tair and Twb lapse rates showed strong hourly and daily variability, with both exhibiting almost identical temporal fluctuations. The Twb exhibited average lapse rates that were slightly steeper (- 5.2 °C/km) than those observed for Tair (- 4.9 °C/km). The less steep lapse rates and most thermal inversions were observed in December. Days having less (more) steep Tair and Twb lapse rates were observed under low (high) <span class="hlt">wind</span> speeds and high (low) relative humidity and <span class="hlt">air</span> pressure. The temporal dynamics of the SM lapse rates was more complex, as this involved consideration of the average Tair in the ski resort, in addition to the driving factors of the spatio-temporal variability of Twb. Thus, on a number of cold (warm) days, snowmaking was feasible at all elevations at the ski resort, independently of the slopes of the lapse rates. The SM exhibited an average daily lapse rate of 8.2 h/km, with a progressive trend of increase from December to March. Weather types over the Iberian Peninsula tightly control the driving factors of the Tair, Twb, and SM lapse rates (<span class="hlt">wind</span> speed, relative humidity, and Tair), so the slopes of the lapse rates and the frequency of inversions in relation to elevation for the three variables are very dependent on the occurrence of specific weather types. The less steep lapse rates occurred associated with advections from the southeast, although low lapse rates also occurred during advections from the east and south, and under anticyclonic conditions. The steepest Tair and Twb lapse rates were observed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018alas.confE..29O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018alas.confE..29O"><span>PWV, <span class="hlt">Temperature</span> and <span class="hlt">Wind</span> Statistics at Sites Suitable For mm and Sub-mm Wavelengths Astronomy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Otarola, Angel; Travouillon, Tony; De Breuck, Carlos; Radford, Simon; Matsushita, Satoki; Pérez-Beaupuits, Juan P.</p> <p>2018-01-01</p> <p>Atmospheric water vapor is the main limiting factor of atmospheric transparency in the mm and sub-mm wavelength spectral windows. Thus, dry sites are needed for the installation and successful operation of radio astronomy observatories exploiting those spectral windows. Other parameters that play an important role in the mechanical response of radio telescopes exposed to the environmental conditions are: <span class="hlt">temperature</span>, and in particular <span class="hlt">temperature</span> gradients that induce thermal deformation of mechanical structures, as well as <span class="hlt">wind</span> magnitude that induce pointing jitter affecting this way the required accuracy in the ability to point to a cosmic source during the observations. <span class="hlt">Temperature</span> and <span class="hlt">wind</span> are variables of special consideration when planning the installation and operations of large aperture radio telescopes. This work summarizes the statistics of precipitable water vapor (PWV), <span class="hlt">temperature</span> and <span class="hlt">wind</span> monitored at sites by the costal mountain range, as well as on t he west slope of the Andes mountain range in the region of Antofagasta, Chile. This information could prove useful for the planning of the Atacama Large-Aperture Submm/mm Telescope (AtLast).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title14-vol1/pdf/CFR-2010-title14-vol1-sec25-1527.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title14-vol1/pdf/CFR-2010-title14-vol1-sec25-1527.pdf"><span>14 CFR 25.1527 - Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 14 Aeronautics and Space 1 2010-01-01 2010-01-01 false Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating... TRANSPORTATION AIRCRAFT AIRWORTHINESS STANDARDS: TRANSPORT CATEGORY AIRPLANES Operating Limitations and Information Operating Limitations § 25.1527 Ambient <span class="hlt">air</span> <span class="hlt">temperature</span> and operating altitude. The extremes of...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040171651','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040171651"><span>Intra-seasonal Oscillations (ISO) of Zonal-Mean Meridional <span class="hlt">Winds</span> and <span class="hlt">Temperatures</span> as Measured by UARS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Huang, Frank T.; Mayr, Hans G.; Reber, Carl A.</p> <p>2004-01-01</p> <p>Based on an empirical analysis of measurements with the High Resolution Doppler Imager (HRDI) on the UARS spacecraft in the upper mesosphere (95 km), persistent and regular intra-seasonal oscillations (ISO) with periods of about 2 to 4 months have recently been reported in the zonal-mean meridional <span class="hlt">winds</span>. Similar oscillations have also been discussed independently in a modeling study, and they were attributed to wave-mean-flow interactions. The observed and modeled meridional <span class="hlt">wind</span> ISOs were largely confined to low latitudes. We report here an analysis of concurrent <span class="hlt">temperature</span> measurements on UARS, which produces oscillations similar to those seen in the meridional <span class="hlt">winds</span>. Although the <span class="hlt">temperature</span> oscillations are observed at lower altitudes (55 km), their phase variations with latitude are qualitatively consistent with the inferred properties seen in the meridional <span class="hlt">winds</span> and thus provide independent evidence for the existence of ISOs in the mesosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/7649','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/7649"><span>Soil and <span class="hlt">air</span> <span class="hlt">temperature</span> and biomass after residue treatment.</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>W.B. Fowler; J.D. Helvey</p> <p>1981-01-01</p> <p><span class="hlt">Air</span> <span class="hlt">temperature</span> at 0.5 m and soil <span class="hlt">temperature</span> at 0.01 m were measured during May and early June after forest harvest on four residue treatment sites and a control. Broadcast burning or burning in piles increased daily accumulation of heat in <span class="hlt">air</span> while scattered chips and scarified and cleared treatments were equal to the control (broadcast, untreated slash). During mid...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23977309','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23977309"><span>Using <span class="hlt">wind</span> setdown and storm surge on Lake Erie to calibrate the <span class="hlt">air</span>-sea drag coefficient.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Drews, Carl</p> <p>2013-01-01</p> <p>The <span class="hlt">air</span>-sea drag coefficient controls the transfer of momentum from <span class="hlt">wind</span> to water. In modeling storm surge, this coefficient is a crucial parameter for estimating the surge height. This study uses two strong <span class="hlt">wind</span> events on Lake Erie to calibrate the drag coefficient using the Coupled Ocean Atmosphere Wave Sediment Transport (COAWST) modeling system and the the Regional Ocean Modeling System (ROMS). Simulated waves are generated on the lake with Simulating WAves Nearshore (SWAN). <span class="hlt">Wind</span> setdown provides the opportunity to eliminate wave setup as a contributing factor, since waves are minimal at the upwind shore. The study finds that model results significantly underestimate <span class="hlt">wind</span> setdown and storm surge when a typical open-ocean formulation without waves is used for the drag coefficient. The contribution of waves to <span class="hlt">wind</span> setdown and storm surge is 34.7%. Scattered lake ice also increases the effective drag coefficient by a factor of 1.1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/863380','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/863380"><span>Isokinetic <span class="hlt">air</span> sampler</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Sehmel, George A.</p> <p>1979-01-01</p> <p>An isokinetic <span class="hlt">air</span> sampler includes a filter, a holder for the filter, an <span class="hlt">air</span> pump for drawing <span class="hlt">air</span> through the filter at a fixed, predetermined rate, an inlet assembly for the sampler having an inlet opening therein of a size such that isokinetic <span class="hlt">air</span> sampling is obtained at a particular <span class="hlt">wind</span> speed, a closure for the inlet opening and means for simultaneously opening the closure and turning on the <span class="hlt">air</span> pump when the <span class="hlt">wind</span> speed is such that isokinetic <span class="hlt">air</span> sampling is obtained. A system incorporating a plurality of such samplers provided with <span class="hlt">air</span> pumps set to draw <span class="hlt">air</span> through the filter at the same fixed, predetermined rate and having different inlet opening sizes for use at different <span class="hlt">wind</span> speeds is included within the ambit of the present invention as is a method of sampling <span class="hlt">air</span> to measure airborne concentrations of particulate pollutants as a function of <span class="hlt">wind</span> speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860018627','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860018627"><span>Cryogenic <span class="hlt">wind</span> tunnels: Problems of continuous operation at low <span class="hlt">temperatures</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Faulmann, D.</p> <p>1986-01-01</p> <p>The design of a cryogenic <span class="hlt">wind</span> tunnel which operates continuously, and is capable of attaining transonic speeds at generating pressures of about 3 bars is described. Its stainless steel construction with inside insulation allows for very rapid <span class="hlt">temperature</span> variations promoted by rapid changes in the liquid nitrogen flow. A comparative study of <span class="hlt">temperature</span> measuring probes shows a good reliability of thin sheet thermocouples. To measure fluctuations, only a cold wire makes it possible to record frequencies of about 300 Hz. The use of an integral computer method makes it possible to determine the impact of the wall <span class="hlt">temperature</span> ratio to the adiabatic wall <span class="hlt">temperature</span> for the various parameters characterizing the boundary layer. These cases are processed with positive and negative pressure gradients.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ERL....13c4015W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ERL....13c4015W"><span>Effects of anthropogenic heat due to <span class="hlt">air</span>-conditioning systems on an extreme high <span class="hlt">temperature</span> event in Hong Kong</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.; Li, Y.; Di Sabatino, S.; Martilli, A.; Chan, P. W.</p> <p>2018-03-01</p> <p>Anthropogenic heat flux is the heat generated by human activities in the urban canopy layer, which is considered the main contributor to the urban heat island (UHI). The UHI can in turn increase the use and energy consumption of <span class="hlt">air</span>-conditioning systems. In this study, two effective methods for water-cooling <span class="hlt">air</span>-conditioning systems in non-domestic areas, including the direct cooling system and central piped cooling towers (CPCTs), are physically based, parameterized, and implemented in a weather research and forecasting model at the city scale of Hong Kong. An extreme high <span class="hlt">temperature</span> event (June 23-28, 2016) in the urban areas was examined, and we assessed the effects on the surface thermal environment, the interaction of sea-land breeze circulation and urban heat island circulation, boundary layer dynamics, and a possible reduction of energy consumption. The results showed that both water-cooled <span class="hlt">air</span>-conditioning systems could reduce the 2 m <span class="hlt">air</span> <span class="hlt">temperature</span> by around 0.5 °C-0.8 °C during the daytime, and around 1.5 °C around 7:00-8:00 pm when the planetary boundary layer (PBL) height was confined to a few hundred meters. The CPCT contributed around 80%-90% latent heat flux and significantly increased the water vapor mixing ratio in the atmosphere by around 0.29 g kg-1 on average. The implementation of the two alternative <span class="hlt">air</span>-conditioning systems could modify the heat and momentum of turbulence, which inhibited the evolution of the PBL height (a reduction of 100-150 m), reduced the vertical mixing, presented lower horizontal <span class="hlt">wind</span> speed and buoyant production of turbulent kinetic energy, and reduced the strength of sea breeze and UHI circulation, which in turn affected the removal of <span class="hlt">air</span> pollutants. Moreover, the two alternative <span class="hlt">air</span>-conditioning systems could significantly reduce the energy consumption by around 30% during extreme high <span class="hlt">temperature</span> events. The results of this study suggest potential UHI mitigation strategies and can be extended to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090020627','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090020627"><span>Estimating Mixing Heights Using Microwave <span class="hlt">Temperature</span> Profiler</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nielson-Gammon, John; Powell, Christina; Mahoney, Michael; Angevine, Wayne</p> <p>2008-01-01</p> <p>A paper describes the Microwave <span class="hlt">Temperature</span> Profiler (MTP) for making measurements of the planetary boundary layer thermal structure data necessary for <span class="hlt">air</span> quality forecasting as the Mixing Layer (ML) height determines the volume in which daytime pollution is primarily concentrated. This is the first time that an airborne <span class="hlt">temperature</span> profiler has been used to measure the mixing layer height. Normally, this is done using a radar <span class="hlt">wind</span> profiler, which is both noisy and large. The MTP was deployed during the Texas 2000 <span class="hlt">Air</span> Quality Study (TexAQS-2000). An objective technique was developed and tested for estimating the ML height from the MTP vertical <span class="hlt">temperature</span> profiles. In order to calibrate the technique and evaluate the usefulness of this approach, estimates from a variety of measurements during the TexAQS-2000 were compared. Estimates of ML height were used from radiosondes, radar <span class="hlt">wind</span> profilers, an aerosol backscatter lidar, and in-situ aircraft measurements in addition to those from the MTP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090017609&hterms=information+quality&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dinformation%2Bquality','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090017609&hterms=information+quality&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dinformation%2Bquality"><span>Data Assimilation Experiments Using Quality Controlled <span class="hlt">AIRS</span> Version 5 <span class="hlt">Temperature</span> Soundings</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Susskind, Joel</p> <p>2009-01-01</p> <p>The <span class="hlt">AIRS</span> Science Team Version 5 retrieval algorithm has been finalized and is now operational at the Goddard DAAC in the processing (and reprocessing) of all <span class="hlt">AIRS</span> data. The <span class="hlt">AIRS</span> Science Team Version 5 retrieval algorithm contains a number of significant improvements over Version 4. Two very significant improvements are described briefly below. 1) The <span class="hlt">AIRS</span> Science Team Radiative Transfer Algorithm (RTA) has now been upgraded to accurately account for effects of non-local thermodynamic equilibrium on the <span class="hlt">AIRS</span> observations. This allows for use of <span class="hlt">AIRS</span> observations in the entire 4.3 micron CO2 absorption band in the retrieval algorithm during both day and night. Following theoretical considerations, tropospheric <span class="hlt">temperature</span> profile information is obtained almost exclusively from clear column radiances in the 4.3 micron CO2 band in the <span class="hlt">AIRS</span> Version 5 <span class="hlt">temperature</span> profile retrieval step. These clear column radiances are a derived product that are indicative of radiances <span class="hlt">AIRS</span> channels would have seen if the field of view were completely clear. Clear column radiances for all channels are determined using tropospheric sounding 15 micron CO2 observations. This approach allows for the generation of accurate values of clear column radiances and T(p) under most cloud conditions. 2) Another very significant improvement in Version 5 is the ability to generate accurate case-by-case, level-by-level error estimates for the atmospheric <span class="hlt">temperature</span> profile, as well as for channel-by-channel clear column radiances. These error estimates are used for quality control of the retrieved products. Based on error estimate thresholds, each <span class="hlt">temperature</span> profiles is assigned a characteristic pressure, pg, down to which the profile is characterized as good for use for data assimilation purposes. We have conducted forecast impact experiments assimilating <span class="hlt">AIRS</span> quality controlled <span class="hlt">temperature</span> profiles using the NASA GEOS-5 data assimilation system, consisting of the NCEP GSI analysis coupled with the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018IJEaS.107..145C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018IJEaS.107..145C"><span>Attribution of precipitation changes on ground-<span class="hlt">air</span> <span class="hlt">temperature</span> offset: Granger causality analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cermak, Vladimir; Bodri, Louise</p> <p>2018-01-01</p> <p>This work examines the causal relationship between the value of the ground-<span class="hlt">air</span> <span class="hlt">temperature</span> offset and the precipitation changes for monitored 5-min data series together with their hourly and daily averages obtained at the Sporilov Geophysical Observatory (Prague). Shallow subsurface soil <span class="hlt">temperatures</span> were monitored under four different land cover types (bare soil, sand, short-cut grass and asphalt). The ground surface <span class="hlt">temperature</span> (GST) and surface <span class="hlt">air</span> <span class="hlt">temperature</span> (SAT) offset, Δ T(GST-SAT), is defined as the difference between the <span class="hlt">temperature</span> measured at the depth of 2 cm below the surface and the <span class="hlt">air</span> <span class="hlt">temperature</span> measured at 5 cm above the surface. The results of the Granger causality test did not reveal any evidence of Granger causality for precipitation to ground-<span class="hlt">air</span> <span class="hlt">temperature</span> offsets on the daily scale of aggregation except for the asphalt pavement. On the contrary, a strong evidence of Granger causality for precipitation to the ground-<span class="hlt">air</span> <span class="hlt">temperature</span> offsets was found on the hourly scale of aggregation for all land cover types except for the sand surface cover. All results are sensitive to the lag choice of the autoregressive model. On the whole, obtained results contain valuable information on the delay time of Δ T(GST-SAT) caused by the rainfall events and confirmed the importance of using autoregressive models to understand the ground-<span class="hlt">air</span> <span class="hlt">temperature</span> relationship.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhD...51p4003T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhD...51p4003T"><span>Indoor <span class="hlt">air</span> purification by dielectric barrier discharge combined with ionic <span class="hlt">wind</span>: physical and microbiological investigations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Timmermann, E.; Prehn, F.; Schmidt, M.; Höft, H.; Brandenburg, R.; Kettlitz, M.</p> <p>2018-04-01</p> <p>A non-thermal plasma source based on a surface dielectric barrier discharge (DBD) is developed for purification of recirculating <span class="hlt">air</span> in operating theatres in hospitals. This is a challenging application due to high flow rates, short treatment times and the low threshold for ozone in the ventilated <span class="hlt">air</span>. Therefore, the surface DBD was enhanced in order to generate an ionic <span class="hlt">wind</span>, which can deflect and thus, filter out airborne microorganisms. Electrical and gas diagnostics as well as microbiological experiments were performed in a downscaled plasma source under variation of various electrical parameters, but application-oriented airflow velocity and humidity. The dependence of electrical power and ozone concentration as well as charged particles in the plasma treated <span class="hlt">air</span> on frequency, voltage and relative humidity is presented and discussed. The presence of humidity causes a more conductive dielectric surface and thus a weaker plasma formation, especially at low frequency. The airborne test bacteria, Escherichia coli, showed significant effect to plasma treatment (up to 20% reduction) and to plasma with ionic <span class="hlt">wind</span> (up to 90% removal); especially a configuration with 70% removal and an accompanying ozone concentration of only 360 ppb is promising for future application.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140010876','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140010876"><span>Comparison of Near-Surface <span class="hlt">Air</span> <span class="hlt">Temperatures</span> and MODIS Ice-Surface <span class="hlt">Temperatures</span> at Summit, Greenland (2008-2013)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shuman, Christopher A.; Hall, Dorothy K.; DiGirolamo, Nicolo E.; Mefford, Thomas K.; Schnaubelt, Michael J.</p> <p>2014-01-01</p> <p>We have investigated the stability of the MODerate resolution Imaging Spectroradiometer (MODIS) infrared-derived ice surface <span class="hlt">temperature</span> (IST) data from Terra for use as a climate quality data record. The availability of climate quality <span class="hlt">air</span> <span class="hlt">temperature</span> data (TA) from a NOAA Global Monitoring Division observatory at Greenlands Summit station has enabled this high temporal resolution study of MODIS ISTs. During a 5 year period (July 2008 to August 2013), more than 2500 IST values were compared with 3-minute average TA values derived from the 1-minute data from NOAAs primary 2 m <span class="hlt">air</span> <span class="hlt">temperature</span> sensor. These data enabled an expected small offset between <span class="hlt">air</span> and surface <span class="hlt">temperatures</span> at this the ice sheet location to be investigated over multiple annual cycles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28076196','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28076196"><span>Impacts of Lowered Urban <span class="hlt">Air</span> <span class="hlt">Temperatures</span> on Precursor Emission and Ozone <span class="hlt">Air</span> Quality.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Taha, Haider; Konopacki, Steven; Akbari, Hashem</p> <p>1998-09-01</p> <p>Meteorological, photochemical, building-energy, and power plant simulations were performed to assess the possible precursor emission and ozone <span class="hlt">air</span> quality impacts of decreased <span class="hlt">air</span> <span class="hlt">temperatures</span> that could result from implementing the "cool communities" concept in California's South Coast <span class="hlt">Air</span> Basin (SoCAB). Two pathways are considered. In the direct pathway, a reduction in cooling energy use translates into reduced demand for generation capacity and, thus, reduced precursor emissions from electric utility power plants. In the indirect pathway, reduced <span class="hlt">air</span> <span class="hlt">temperatures</span> can slow the atmospheric production of ozone as well as precursor emission from anthropogenic and biogenic sources. The simulations suggest small impacts on emissions following implementation of cool communities in the SoCAB. In summer, for example, there can be reductions of up to 3% in NO x emissions from in-basin power plants. The photochemical simulations suggest that the <span class="hlt">air</span> quality impacts of these direct emission reductions are small. However, the indirect atmospheric effects of cool communities can be significant. For example, ozone peak concentrations can decrease by up to 11% in summer and population-weighted exceedance exposure to ozone above the California and National Ambient <span class="hlt">Air</span> Quality Standards can decrease by up to 11 and 17%, respectively. The modeling suggests that if these strategies are combined with others, such as mobile-source emission control, the improvements in ozone <span class="hlt">air</span> quality can be substantial.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4223031','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4223031"><span>Characterizing <span class="hlt">Air</span> <span class="hlt">Temperature</span> Changes in the Tarim Basin over 1960–2012</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Peng, Dongmei; Wang, Xiujun; Zhao, Chenyi; Wu, Xingren; Jiang, Fengqing; Chen, Pengxiang</p> <p>2014-01-01</p> <p>There has been evidence of warming rate varying largely over space and between seasons. However, little has been done to evaluate the spatial and temporal variability of <span class="hlt">air</span> <span class="hlt">temperature</span> in the Tarim Basin, northwest China. In this study, we collected daily <span class="hlt">air</span> <span class="hlt">temperature</span> from 19 meteorological stations for the period of 1960–2012, and analyzed annual mean <span class="hlt">temperature</span> (AMT), the annual minimum (Tmin) and maximum <span class="hlt">temperature</span> (Tmax), and mean <span class="hlt">temperatures</span> of all twelve months and four seasons and their anomalies. Trend analyses, standard deviation of the detrended anomaly (SDDA) and correlations were carried out to characterize the spatial and temporal variability of various mean <span class="hlt">air</span> <span class="hlt">temperatures</span>. Our data showed that increasing trend was much greater in the Tmin (0.55°C/10a) than in the AMT (0.25°C/10a) and Tmax (0.12°C/10a), and the fluctuation followed the same order. There were large spatial variations in the increasing trends of both AMT (from −0.09 to 0.43 °C/10a) and Tmin (from 0.15 to 1.12°C/10a). Correlation analyses indicated that AMT had a significantly linear relationship with Tmin and the mean <span class="hlt">temperatures</span> of four seasons. There were also pronounced changes in the monthly <span class="hlt">air</span> <span class="hlt">temperature</span> from November to March at decadal time scale. The seasonality (i.e., summer and winter difference) of <span class="hlt">air</span> <span class="hlt">temperature</span> was stronger during the period of 1960–1979 than over the recent three decades. Our preliminary analyses indicated that local environmental conditions (such as elevation) might be partly responsible for the spatial variability, and large scale climate phenomena might have influences on the temporal variability of <span class="hlt">air</span> <span class="hlt">temperature</span> in the Tarim Basin. In particular, there was a significant correlation between index of El Niño-Southern Oscillation (ENSO) and <span class="hlt">air</span> <span class="hlt">temperature</span> of May (P = 0.004), and between the index of Pacific Decadal Oscillation (PDO) and <span class="hlt">air</span> <span class="hlt">temperature</span> of July (P = 0.026) over the interannual to decadal time scales. PMID</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GRC-1958-C-47803.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GRC-1958-C-47803.html"><span>Preheater in the 10-by 10-Foot Supersonic <span class="hlt">Wind</span> Tunnel</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1958-04-21</p> <p>The 10- by 10-Foot Supersonic <span class="hlt">Wind</span> Tunnel at the NACA Lewis Flight Propulsion Laboratory was built under the Congressional Unitary Plan Act which coordinated <span class="hlt">wind</span> tunnel construction at the NACA, <span class="hlt">Air</span> Force, industry, and universities. The 10- by 10, which began operation in 1956, was the largest of the three NACA tunnels built under the act. Researchers could test engines up to five feet in diameter in the 10- by 10-foot test section. A 250,000-horsepower axial-flow compressor fan can generate airflows up to Mach 3.5 through the test section. The incoming <span class="hlt">air</span> must be dehumidified and cooled so that the proper conditions are present for the test. A large <span class="hlt">air</span> dryer with 1,890 tons of activated alumina soaks up 1.5 tons of water per minute from the airflow. A cooling apparatus equivalent to 250,000 household <span class="hlt">air</span> conditioners is used to cool the <span class="hlt">air</span>. The <span class="hlt">air</span> heater is located just upstream from the test section. Natural gas is combusted in the tunnel to increase the <span class="hlt">air</span> <span class="hlt">temperature</span>. The system could only be employed when the tunnel was run in its closed-circuit propulsion mode.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3747107','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3747107"><span>Using <span class="hlt">Wind</span> Setdown and Storm Surge on Lake Erie to Calibrate the <span class="hlt">Air</span>-Sea Drag Coefficient</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Drews, Carl</p> <p>2013-01-01</p> <p>The <span class="hlt">air</span>-sea drag coefficient controls the transfer of momentum from <span class="hlt">wind</span> to water. In modeling storm surge, this coefficient is a crucial parameter for estimating the surge height. This study uses two strong <span class="hlt">wind</span> events on Lake Erie to calibrate the drag coefficient using the Coupled Ocean Atmosphere Wave Sediment Transport (COAWST) modeling system and the the Regional Ocean Modeling System (ROMS). Simulated waves are generated on the lake with Simulating WAves Nearshore (SWAN). <span class="hlt">Wind</span> setdown provides the opportunity to eliminate wave setup as a contributing factor, since waves are minimal at the upwind shore. The study finds that model results significantly underestimate <span class="hlt">wind</span> setdown and storm surge when a typical open-ocean formulation without waves is used for the drag coefficient. The contribution of waves to <span class="hlt">wind</span> setdown and storm surge is 34.7%. Scattered lake ice also increases the effective drag coefficient by a factor of 1.1. PMID:23977309</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/25304','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/25304"><span>Modifications of highway <span class="hlt">air</span> pollution models for complex geometries, volume II : <span class="hlt">wind</span> tunnel test program.</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>2002-09-01</p> <p>This is volume I1 of a two-volume report of a study to increase the scope and clarity of <span class="hlt">air</span> pollution models for : depressed highway and street canyon sites. It presents the atmospheric <span class="hlt">wind</span> tunnel program conducted to increase the : data base and i...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22086025','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22086025"><span>High-precision diode-laser-based <span class="hlt">temperature</span> measurement for <span class="hlt">air</span> refractive index compensation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hieta, Tuomas; Merimaa, Mikko; Vainio, Markku; Seppä, Jeremias; Lassila, Antti</p> <p>2011-11-01</p> <p>We present a laser-based system to measure the refractive index of <span class="hlt">air</span> over a long path length. In optical distance measurements, it is essential to know the refractive index of <span class="hlt">air</span> with high accuracy. Commonly, the refractive index of <span class="hlt">air</span> is calculated from the properties of the ambient <span class="hlt">air</span> using either Ciddor or Edlén equations, where the dominant uncertainty component is in most cases the <span class="hlt">air</span> <span class="hlt">temperature</span>. The method developed in this work utilizes direct absorption spectroscopy of oxygen to measure the average <span class="hlt">temperature</span> of <span class="hlt">air</span> and of water vapor to measure relative humidity. The method allows measurement of <span class="hlt">temperature</span> and humidity over the same beam path as in optical distance measurement, providing spatially well-matching data. Indoor and outdoor measurements demonstrate the effectiveness of the method. In particular, we demonstrate an effective compensation of the refractive index of <span class="hlt">air</span> in an interferometric length measurement at a time-variant and spatially nonhomogeneous <span class="hlt">temperature</span> over a long time period. Further, we were able to demonstrate 7 mK RMS noise over a 67 m path length using a 120 s sample time. To our knowledge, this is the best <span class="hlt">temperature</span> precision reported for a spectroscopic <span class="hlt">temperature</span> measurement. © 2011 Optical Society of America</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1358504-dust-wind-interactions-can-intensify-aerosol-pollution-over-eastern-china','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1358504-dust-wind-interactions-can-intensify-aerosol-pollution-over-eastern-china"><span>Dust-<span class="hlt">wind</span> interactions can intensify aerosol pollution over eastern China</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Yang, Yang; Russell, Lynn M.; Lou, Sijia; ...</p> <p>2017-05-11</p> <p>Eastern China has experienced severe and persistent winter haze episodes in recent years due to intensification of aerosol pollution, which has adverse impacts on hundreds of millions of people across China1–4. In addition to anthropogenic emissions, the winter aerosol pollution over eastern China is associated with abnormal meteorological conditions, including weaker <span class="hlt">wind</span> speeds5–9. Using a global climate model and a chemical transport model, we show that variations in dust emissions decrease the wintertime land-sea surface <span class="hlt">air</span> <span class="hlt">temperature</span> difference between eastern China and the South China Sea and weaken <span class="hlt">winds</span> below the lowest 10th percentile of <span class="hlt">wind</span> speed by 0.06 mmore » s-1. Here, the weakened <span class="hlt">winds</span> enhance stagnation and account for 13% of the increases in PM2.5 aerosol concentrations over eastern China. Although recent increases in anthropogenic emissions are the main factor causing haze over eastern China, we conclude that natural emissions also exert a significant influence on the increases in wintertime PM2.5 concentrations, with important implications that should be considered in <span class="hlt">air</span> quality studies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1358504','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1358504"><span>Dust-<span class="hlt">wind</span> interactions can intensify aerosol pollution over eastern China</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Yang, Yang; Russell, Lynn M.; Lou, Sijia</p> <p></p> <p>Eastern China has experienced severe and persistent winter haze episodes in recent years due to intensification of aerosol pollution, which has adverse impacts on hundreds of millions of people across China1–4. In addition to anthropogenic emissions, the winter aerosol pollution over eastern China is associated with abnormal meteorological conditions, including weaker <span class="hlt">wind</span> speeds5–9. Using a global climate model and a chemical transport model, we show that variations in dust emissions decrease the wintertime land-sea surface <span class="hlt">air</span> <span class="hlt">temperature</span> difference between eastern China and the South China Sea and weaken <span class="hlt">winds</span> below the lowest 10th percentile of <span class="hlt">wind</span> speed by 0.06 mmore » s-1. Here, the weakened <span class="hlt">winds</span> enhance stagnation and account for 13% of the increases in PM2.5 aerosol concentrations over eastern China. Although recent increases in anthropogenic emissions are the main factor causing haze over eastern China, we conclude that natural emissions also exert a significant influence on the increases in wintertime PM2.5 concentrations, with important implications that should be considered in <span class="hlt">air</span> quality studies.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/46514','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/46514"><span>A physically based analytical spatial <span class="hlt">air</span> <span class="hlt">temperature</span> and humidity model</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Yang Yang; Theodore A. Endreny; David J. Nowak</p> <p>2013-01-01</p> <p>Spatial variation of urban surface <span class="hlt">air</span> <span class="hlt">temperature</span> and humidity influences human thermal comfort, the settling rate of atmospheric pollutants, and plant physiology and growth. Given the lack of observations, we developed a Physically based Analytical Spatial <span class="hlt">Air</span> <span class="hlt">Temperature</span> and Humidity (PASATH) model. The PASATH model calculates spatial solar radiation and heat...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GRC-1944-C-06715.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GRC-1944-C-06715.html"><span>Refrigeration Compressors for the Altitude <span class="hlt">Wind</span> Tunnel</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1944-09-21</p> <p>These compressors inside the Refrigeration Building at the National Advisory Committee for Aeronautics (NACA) Aircraft Engine Research Laboratory were used to generate cold <span class="hlt">temperatures</span> in the Altitude <span class="hlt">Wind</span> Tunnel (AWT) and Icing Research Tunnel. The AWT was a large facility that simulated actual flight conditions at high altitudes. The two primary aspects of altitude simulation are the reduction of the <span class="hlt">air</span> pressure and the decrease of <span class="hlt">temperature</span>. The Icing Research Tunnel was a smaller facility in which water droplets were added to the refrigerated <span class="hlt">air</span> stream to simulate weather conditions that produced ice buildup on aircraft. The military pressured the NACA to complete the tunnels quickly so they could be of use during World War II. The NACA engineers struggled with the design of this refrigeration system, so Willis Carrier, whose Carrier Corporation had pioneered modern refrigeration, took on the project. The Carrier engineers devised the largest cooling system of its kind in the world. The system could lower the tunnels’ <span class="hlt">air</span> <span class="hlt">temperature</span> to –47⁰ F. The cooling system was powered by 14 Carrier and York compressors, seen in this photograph, which were housed in the Refrigeration Building between the two <span class="hlt">wind</span> tunnels. The compressors converted the Freon 12 refrigerant into a liquid. The refrigerant was then pumped into zig-zag banks of cooling coils inside the tunnels’ return leg. The Freon absorbed heat from the airflow as it passed through the coils. The heat was transferred to the cooling water and sent to the cooling tower where it was dissipated into the atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1433253','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1433253"><span>Apparatus and method for maintaining an article at a <span class="hlt">temperature</span> that is less than the <span class="hlt">temperature</span> of the ambient <span class="hlt">air</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>Klett, James; Klett, Lynn</p> <p></p> <p>An apparatus for maintaining the <span class="hlt">temperature</span> of an article at a <span class="hlt">temperature</span> that is below the ambient <span class="hlt">air</span> <span class="hlt">temperature</span> includes an enclosure having an outer wall that defines an interior chamber for holding a volume of sealed <span class="hlt">air</span>. An insert is disposed inside of the chamber and has a body that is made of a porous graphite foam material. A vacuum pump penetrates the outer wall and fluidly connects the sealed <span class="hlt">air</span> in the interior chamber with the ambient <span class="hlt">air</span> outside of the enclosure. The <span class="hlt">temperatures</span> of the insert and article is maintained at <span class="hlt">temperatures</span> that are below the ambientmore » <span class="hlt">air</span> <span class="hlt">temperature</span> when a volume of a liquid is wicked into the pores of the porous insert and the vacuum pump is activated to reduce the pressure of a volume of sealed <span class="hlt">air</span> within the interior chamber to a pressure that is below the vapor pressure of the liquid.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoRL..41.8713F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoRL..41.8713F"><span>Increases in plasma sheet <span class="hlt">temperature</span> with solar <span class="hlt">wind</span> driving during substorm growth phases</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forsyth, C.; Watt, C. E. J.; Rae, I. J.; Fazakerley, A. N.; Kalmoni, N. M. E.; Freeman, M. P.; Boakes, P. D.; Nakamura, R.; Dandouras, I.; Kistler, L. M.; Jackman, C. M.; Coxon, J. C.; Carr, C. M.</p> <p>2014-12-01</p> <p>During substorm growth phases, magnetic reconnection at the magnetopause extracts ~1015 J from the solar <span class="hlt">wind</span> which is then stored in the magnetotail lobes. Plasma sheet pressure increases to balance magnetic flux density increases in the lobes. Here we examine plasma sheet pressure, density, and <span class="hlt">temperature</span> during substorm growth phases using 9 years of Cluster data (>316,000 data points). We show that plasma sheet pressure and <span class="hlt">temperature</span> are higher during growth phases with higher solar <span class="hlt">wind</span> driving, whereas the density is approximately constant. We also show a weak correlation between plasma sheet <span class="hlt">temperature</span> before onset and the minimum SuperMAG AL (SML) auroral index in the subsequent substorm. We discuss how energization of the plasma sheet before onset may result from thermodynamically adiabatic processes; how hotter plasma sheets may result in magnetotail instabilities, and how this relates to the onset and size of the subsequent substorm expansion phase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRA..122.7504D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRA..122.7504D"><span>Coordinated observations of postmidnight irregularities and thermospheric neutral <span class="hlt">winds</span> and <span class="hlt">temperatures</span> at low latitudes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dao, Tam; Otsuka, Yuichi; Shiokawa, Kazuo; Nishioka, Michi; Yamamoto, Mamoru; Buhari, Suhaila M.; Abdullah, Mardina; Husin, Asnawi</p> <p>2017-07-01</p> <p>We investigated a postmidnight field-aligned irregularity (FAI) event observed with the Equatorial Atmosphere Radar at Kototabang (0.2°S, 100.3°E, dip latitude 10.4°S) in Indonesia on the night of 9 July 2010 using a comprehensive data set of both neutral and plasma parameters. We examined the rate of total electron content change index (ROTI) obtained from GPS receivers in Southeast Asia, airglow images detected by an all-sky imager, and thermospheric neutral <span class="hlt">winds</span> and <span class="hlt">temperatures</span> obtained by a Fabry-Perot interferometer at Kototabang. Altitudes of the F layer (h'F) observed by ionosondes at Kototabang, Chiang Mai, and Chumphon were also surveyed. We found that the postmidnight FAIs occurred within plasma bubbles and coincided with kilometer-scale plasma density irregularities. We also observed an enhancement of the magnetically equatorward thermospheric neutral <span class="hlt">wind</span> at the same time as the increase of h'F at low-latitude stations, but h'F at a station near the magnetic equator remained invariant. Simultaneously, a magnetically equatorward gradient of thermospheric <span class="hlt">temperature</span> was identified at Kototabang. The convergence of equatorward neutral <span class="hlt">winds</span> from the Northern and Southern Hemispheres could be associated with a midnight <span class="hlt">temperature</span> maximum occurring around the magnetic equator. Equatorward neutral <span class="hlt">winds</span> can uplift the F layer at low latitudes and increase the growth rate of Rayleigh-Taylor instabilities, causing more rapid extension of plasma bubbles. The equatorward <span class="hlt">winds</span> in both hemispheres also intensify the eastward Pedersen current, so a large polarization electric field generated in the plasma bubble might play an important role in the generation of postmidnight FAIs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...63a2002K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...63a2002K"><span>Discussion on Boiler Efficiency Correction Method with Low <span class="hlt">Temperature</span> Economizer-<span class="hlt">Air</span> Heater System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ke, Liu; Xing-sen, Yang; Fan-jun, Hou; Zhi-hong, Hu</p> <p>2017-05-01</p> <p>This paper pointed out that it is wrong to take the outlet flue gas <span class="hlt">temperature</span> of low <span class="hlt">temperature</span> economizer as exhaust gas <span class="hlt">temperature</span> in boiler efficiency calculation based on GB10184-1988. What’s more, this paper proposed a new correction method, which decomposed low <span class="hlt">temperature</span> economizer-<span class="hlt">air</span> heater system into two hypothetical parts of <span class="hlt">air</span> preheater and pre condensed water heater and take the outlet equivalent gas <span class="hlt">temperature</span> of <span class="hlt">air</span> preheater as exhaust gas <span class="hlt">temperature</span> in boiler efficiency calculation. This method makes the boiler efficiency calculation more concise, with no <span class="hlt">air</span> heater correction. It has a positive reference value to deal with this kind of problem correctly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/9611371','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9611371"><span>Estimation of thermal sensation during varied <span class="hlt">air</span> <span class="hlt">temperature</span> conditions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Katsuura, T; Tabuchi, R; Iwanaga, K; Harada, H; Kikuchi, Y</p> <p>1998-03-01</p> <p>Seven male students were exposed to four varied <span class="hlt">air</span> <span class="hlt">temperature</span> environments: hot (37 degrees C) to neutral (27 degrees C) (HN), neutral to hot (NH), cool (17 degrees C) to neutral (CN), and neutral to cool (NC). The <span class="hlt">air</span> <span class="hlt">temperature</span> was maintained at the first condition for 20 min, then was changed to the second condition after 15 min and was held there for 20 min. Each subject wore a T-shirt, briefs, trunks, and socks. Each sat on a chair and was continuously evaluated for thermal sensation, thermal comfort, and <span class="hlt">air</span> velocity sensation. Some physiological and thermal parameters were also measured every 5 s during the experiment. The correlation between thermal sensation and skin <span class="hlt">temperature</span> at 15 sites was found to be poor. The subjects felt much warmer during the rising phase of the <span class="hlt">air</span> <span class="hlt">temperature</span> (CN, NH) than during the descending phase (HN, NC) at a given mean skin <span class="hlt">temperature</span>. However, thermal sensation at the same heat flux or at the same value of the difference between skin and <span class="hlt">air</span> <span class="hlt">temperature</span> (delta(Tsk - Ta)) was not so different among the four experimental conditions, and the correlation between thermal sensation and heat flux or delta(Tsk - Ta) was fairly good. The multiple regression equation of the thermal sensation (TS) on 15 sites of skin <span class="hlt">temperature</span> (Tsk; degrees C) was calculated and the coefficient of determination (R*2) was found to be 0.656. Higher coefficients of determination were found in the equations of thermal sensation for the heat flux (H; kcal.m-2.h-1) at the right and left thighs of the subjects and on delta(Tsk - Ta) (degrees C) at 4 sites. They were as follows: TS = 2.04 - 0.016 Hright - 0.036 Hleft; R*2 = 0.717, TS = 1.649 + 0.013 delta(Tsk - Ta)UpperArm - 0.036 delta(Tsk - Ta)Chest - 0.223 delta(Tsk - Ta)Thigh-0.083 delta(Tsk - Ta)LowerLeg; R*2 = 0.752, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010OcSci...6..913J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010OcSci...6..913J"><span>A numerical scheme to calculate <span class="hlt">temperature</span> and salinity dependent <span class="hlt">air</span>-water transfer velocities for any gas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Johnson, M. T.</p> <p>2010-10-01</p> <p>The ocean-atmosphere flux of a gas can be calculated from its measured or estimated concentration gradient across the <span class="hlt">air</span>-sea interface and the transfer velocity (a term representing the conductivity of the layers either side of the interface with respect to the gas of interest). Traditionally the transfer velocity has been estimated from empirical relationships with <span class="hlt">wind</span> speed, and then scaled by the Schmidt number of the gas being transferred. Complex, physically based models of transfer velocity (based on more physical forcings than <span class="hlt">wind</span> speed alone), such as the NOAA COARE algorithm, have more recently been applied to well-studied gases such as carbon dioxide and DMS (although many studies still use the simpler approach for these gases), but there is a lack of validation of such schemes for other, more poorly studied gases. The aim of this paper is to provide a flexible numerical scheme which will allow the estimation of transfer velocity for any gas as a function of <span class="hlt">wind</span> speed, <span class="hlt">temperature</span> and salinity, given data on the solubility and liquid molar volume of the particular gas. New and existing parameterizations (including a novel empirical parameterization of the salinity-dependence of Henry's law solubility) are brought together into a scheme implemented as a modular, extensible program in the R computing environment which is available in the supplementary online material accompanying this paper; along with input files containing solubility and structural data for ~90 gases of general interest, enabling the calculation of their total transfer velocities and component parameters. Comparison of the scheme presented here with alternative schemes and methods for calculating <span class="hlt">air</span>-sea flux parameters shows good agreement in general. It is intended that the various components of this numerical scheme should be applied only in the absence of experimental data providing robust values for parameters for a particular gas of interest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1052222','SCIGOV-DOEDE'); return false;" href="https://www.osti.gov/servlets/purl/1052222"><span>NREL National <span class="hlt">Wind</span> Technology Center (NWTC): M2 Tower; Boulder, Colorado (Data)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/dataexplorer">DOE Data Explorer</a></p> <p>Jager, D.; Andreas, A.</p> <p>1996-09-24</p> <p>The National <span class="hlt">Wind</span> Technology Center (NWTC), located at the foot of the Rocky Mountains near Boulder, Colorado, is a world-class research facility managed by NREL for the U.S. Department of Energy. NWTC researchers work with members of the <span class="hlt">wind</span> energy industry to advance <span class="hlt">wind</span> power technologies that lower the cost of <span class="hlt">wind</span> energy through research and development of state-of-the-art <span class="hlt">wind</span> turbine designs. NREL's Measurement and Instrument Data Center provides data from NWTC's M2 tower which are derived from instruments mounted on or near an 82 meter (270 foot) meteorological tower located at the western edge of the NWTC site and about 11 km (7 miles) west of Broomfield, and approximately 8 km (5 miles) south of Boulder, Colorado. The data represent the mean value of readings taken every two seconds and averaged over one minute. The <span class="hlt">wind</span> speed and direction are measured at six heights on the tower and <span class="hlt">air</span> <span class="hlt">temperature</span> is measured at three heights. The dew point <span class="hlt">temperature</span>, relative humidity, barometric pressure, totalized liquid precipitation, and global solar radiation are also available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JHyd..556.1050I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JHyd..556.1050I"><span>Impact of <span class="hlt">air</span> <span class="hlt">temperature</span> on physically-based maximum precipitation estimation through change in moisture holding capacity of <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ishida, K.; Ohara, N.; Kavvas, M. L.; Chen, Z. Q.; Anderson, M. L.</p> <p>2018-01-01</p> <p>Impact of <span class="hlt">air</span> <span class="hlt">temperature</span> on the Maximum Precipitation (MP) estimation through change in moisture holding capacity of <span class="hlt">air</span> was investigated. A series of previous studies have estimated the MP of 72-h basin-average precipitation over the American River watershed (ARW) in Northern California by means of the Maximum Precipitation (MP) estimation approach, which utilizes a physically-based regional atmospheric model. For the MP estimation, they have selected 61 severe storm events for the ARW, and have maximized them by means of the atmospheric boundary condition shifting (ABCS) and relative humidity maximization (RHM) methods. This study conducted two types of numerical experiments in addition to the MP estimation by the previous studies. First, the <span class="hlt">air</span> <span class="hlt">temperature</span> on the entire lateral boundaries of the outer model domain was increased uniformly by 0.0-8.0 °C with 0.5 °C increments for the two severest maximized historical storm events in addition to application of the ABCS + RHM method to investigate the sensitivity of the basin-average precipitation over the ARW to <span class="hlt">air</span> <span class="hlt">temperature</span> rise. In this investigation, a monotonous increase was found in the maximum 72-h basin-average precipitation over the ARW with <span class="hlt">air</span> <span class="hlt">temperature</span> rise for both of the storm events. The second numerical experiment used specific amounts of <span class="hlt">air</span> <span class="hlt">temperature</span> rise that is assumed to happen under future climate change conditions. <span class="hlt">Air</span> <span class="hlt">temperature</span> was increased by those specified amounts uniformly on the entire lateral boundaries in addition to application of the ABCS + RHM method to investigate the impact of <span class="hlt">air</span> <span class="hlt">temperature</span> on the MP estimate over the ARW under changing climate. The results in the second numerical experiment show that <span class="hlt">temperature</span> increases in the future climate may amplify the MP estimate over the ARW. The MP estimate may increase by 14.6% in the middle of the 21st century and by 27.3% in the end of the 21st century compared to the historical period.</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 regional 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 regional 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 <span class="hlt">temperature</span>, and pressure distribution (<span class="hlt">air</span> density). In the context of <span class="hlt">wind</span> power these data are used </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900058734&hterms=correlated+anti-correlated&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dcorrelated%2Banti-correlated','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900058734&hterms=correlated+anti-correlated&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dcorrelated%2Banti-correlated"><span><span class="hlt">Temperature</span> and density anti-correlations in solar <span class="hlt">wind</span> fluctuations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zank, G. P.; Matthaeus, W. H.; Klein, L. W.</p> <p>1990-01-01</p> <p>Recent theoretical investigations of low Mach number flows, that describe two distinct approaches by fluids to the incompressible regime are summarized. The first includes the effects of relatively strong density and <span class="hlt">temperature</span> fluctuations (Type I), while the second places fluctuations in mechanical pressure, density, and <span class="hlt">temperature</span> on an equal footing (Type II). In the latter case, the relations between density and pressure are recovered, whereas the former case yields departures from incompressible behavior in that density and <span class="hlt">temperature</span> fluctuations are predicted to be anti-correlated. It is suggested that nearly incompressible fluids can be classified as either Type I or II, and it is shown that the well-known pressure-balanced structures represent a subclass of static solutions within this classification. Two examples from Voyager data illustrate the potential for observing these distinct nearly incompressible dynamical ordering in the solar <span class="hlt">wind</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatSR...5E8322Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatSR...5E8322Z"><span>From Dust Devil to Sustainable Swirling <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>Zhang, Mingxu; Luo, Xilian; Li, Tianyu; Zhang, Liyuan; Meng, Xiangzhao; Kase, Kiwamu; Wada, Satoshi; Yu, Chuck Wah; Gu, Zhaolin</p> <p>2015-02-01</p> <p>Dust devils are common but meteorologically unique phenomena on Earth and on Mars. The phenomenon produces a vertical vortex motion in the atmosphere boundary layer and often occurs in hot desert regions, especially in the afternoons from late spring to early summer. Dust devils usually contain abundant <span class="hlt">wind</span> energy, for example, a maximum swirling <span class="hlt">wind</span> velocity of up to 25 m/s, with a 15 m/s maximum vertical velocity and 5 m/s maximum near-surface horizontal velocity can be formed. The occurrences of dust devils cannot be used for energy generation because these are generally random and short-lived. Here, a concept of sustained dust-devil-like whirlwind is proposed for the energy generation. A prototype of a circular shed with pre-rotation vanes has been devised to generate the whirlwind flow by heating the <span class="hlt">air</span> inflow into the circular shed. The pre-rotation vanes can provide the <span class="hlt">air</span> inflow with angular momentum. The results of numerical simulations and experiment illustrate a promising potential of the circular shed for generating swirling <span class="hlt">wind</span> energy via the collection of low-<span class="hlt">temperature</span> solar energy.</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://eric.ed.gov/?q=heat+AND+exchange&pg=3&id=EJ582662','ERIC'); return false;" href="https://eric.ed.gov/?q=heat+AND+exchange&pg=3&id=EJ582662"><span>Balloons and Bottles: Activities on <span class="hlt">Air</span>-Sea Heat Exchange.</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>Murphree, Tom</p> <p>1998-01-01</p> <p>Presents an activity designed to demonstrate how heating and cooling an <span class="hlt">air</span> mass affects its <span class="hlt">temperature</span>, volume, density, and pressure. Illustrates how thermal energy can cause atmospheric motion such as expansion, contraction, and <span class="hlt">winds</span>. (Author/WRM)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRD..11810449Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRD..11810449Y"><span>A physically based analytical spatial <span class="hlt">air</span> <span class="hlt">temperature</span> and humidity model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Yang; Endreny, Theodore A.; Nowak, David J.</p> <p>2013-09-01</p> <p>Spatial variation of urban surface <span class="hlt">air</span> <span class="hlt">temperature</span> and humidity influences human thermal comfort, the settling rate of atmospheric pollutants, and plant physiology and growth. Given the lack of observations, we developed a Physically based Analytical Spatial <span class="hlt">Air</span> <span class="hlt">Temperature</span> and Humidity (PASATH) model. The PASATH model calculates spatial solar radiation and heat storage based on semiempirical functions and generates spatially distributed estimates based on inputs of topography, land cover, and the weather data measured at a reference site. The model assumes that for all grids under the same mesoscale climate, grid <span class="hlt">air</span> <span class="hlt">temperature</span> and humidity are modified by local variation in absorbed solar radiation and the partitioning of sensible and latent heat. The model uses a reference grid site for time series meteorological data and the <span class="hlt">air</span> <span class="hlt">temperature</span> and humidity of any other grid can be obtained by solving the heat flux network equations. PASATH was coupled with the USDA iTree-Hydro water balance model to obtain evapotranspiration terms and run from 20 to 29 August 2010 at a 360 m by 360 m grid scale and hourly time step across a 285 km2 watershed including the urban area of Syracuse, NY. PASATH predictions were tested at nine urban weather stations representing variability in urban topography and land cover. The PASATH model predictive efficiency R2 ranged from 0.81 to 0.99 for <span class="hlt">air</span> <span class="hlt">temperature</span> and 0.77 to 0.97 for dew point <span class="hlt">temperature</span>. PASATH is expected to have broad applications on environmental and ecological models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=338181&Lab=NERL&keyword=public+AND+relations&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=338181&Lab=NERL&keyword=public+AND+relations&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Interaction between Soil Moisture and <span class="hlt">Air</span> <span class="hlt">Temperature</span> in the Mississippi River Basin</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Increasing <span class="hlt">air</span> <span class="hlt">temperatures</span> are expected to continue in the future. The relation between soil moisture and near surface <span class="hlt">air</span> <span class="hlt">temperature</span> is significant for climate change and climate extremes. Evaluation of the relations between soil moisture and <span class="hlt">temperature</span> was performed by devel...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.7958A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.7958A"><span>Effects of the Relaxation of Upwelling-Favorable <span class="hlt">Winds</span> on the Diurnal and Semidiurnal Water <span class="hlt">Temperature</span> Fluctuations in the Santa Barbara Channel, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aristizábal, María. F.; Fewings, Melanie R.; Washburn, Libe</p> <p>2017-10-01</p> <p>In the Santa Barbara Channel, California, and around the Northern Channel Islands, water <span class="hlt">temperature</span> fluctuations in the diurnal and semidiurnal frequency bands are intermittent, with amplitudes that vary on time scales of days to weeks. The cause of this intermittency is not well understood. We studied the effects of the barotropic tide, vertical stratification, propagation of coastal-trapped waves, regional <span class="hlt">wind</span> relaxations, and diurnal-band <span class="hlt">winds</span> on the intermittency of the <span class="hlt">temperature</span> fluctuations during 1992-2015. We used <span class="hlt">temperature</span> data from 43 moorings in 10-200 m water depth and <span class="hlt">wind</span> data from two buoys and one land station. Subtidal-frequency changes in vertical stratification explain 20-40% of the intermittency in diurnal and semidiurnal <span class="hlt">temperature</span> fluctuations at time scales of days to weeks. Along the mainland north of Point Conception and at the Northern Channel Islands, the relaxation of upwelling-favorable <span class="hlt">winds</span> substantially increases vertical stratification, accounting for up to 55% of the subtidal-frequency variability in stratification. As a result of the enhanced stratification, <span class="hlt">wind</span> relaxations enhance the diurnal and semidiurnal <span class="hlt">temperature</span> fluctuations at those sites, even though the diurnal-band <span class="hlt">wind</span> forcing decreases during <span class="hlt">wind</span> relaxation. A linear model where the background stratification is advected vertically explains a substantial fraction of the <span class="hlt">temperature</span> fluctuations at most sites. The increase of vertical stratification and subsequent increase in diurnal and semidiurnal <span class="hlt">temperature</span> fluctuations during <span class="hlt">wind</span> relaxation is a mechanism that can supply nutrients to the euphotic zone and kelp forests in the Channel in summer when upwelling is weak.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20110942661&hterms=Tracer&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DTracer','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20110942661&hterms=Tracer&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DTracer"><span>Stratospheric Horizontal Wavenumber Spectra of <span class="hlt">Winds</span>, Potential <span class="hlt">Temperature</span>, and Atmospheric Tracers Observed by High-Altitude Aircraft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bacmeister, Julio T.; Eckermann, Stephen D.; Newman, Paul A.; Lait, Leslie; Chan, K. R.; Loewenstein, Max; Proffitt, Michael H.; Gary, Bruce L.</p> <p>1996-01-01</p> <p>Horizontal wavenumber power spectra of vertical and horizontal <span class="hlt">wind</span> velocities, potential <span class="hlt">temperatures</span>, and ozone and N(2)O mixing ratios, as measured in the mid-stratosphere during 73 ER-2 flights (altitude approx. 20km) are presented. The velocity and potential <span class="hlt">temperature</span> spectra in the 100 to 1-km wavelength range deviate significantly from the uniform -5/3 power law expected for the inverse energy-cascade regime of two-dimensional turbulence and also for inertial-range, three-dimensional turbulence. Instead, steeper spectra approximately consistent with a -3 power law are observed at horizontal scales smaller than 3 km for all velocity components as well as potential <span class="hlt">temperature</span>. Shallower spectra are observed at scales longer than 6 km. For horizontal velocity and potential <span class="hlt">temperature</span> the spectral indices at longer scales are between -1.5 and -2.0. For vertical velocity the spectrum at longer scales become flat. It is argued that the observed velocity and potential <span class="hlt">temperature</span> spectra are consistent with gravity waves. At smaller scales, the shapes are also superficially consistent with a Lumley-Shur-Weinstock buoyant subrange of turbulence and/or nonlinear gravity waves. Contemporaneous spectra of ozone and N(sub 2)O mixing ratio in the 100 to 1-km wavelength range do conform to an approximately uniform -5/3 power law. It is argued that this may reflect interactions between gravity wave <span class="hlt">air</span>-parcel displacements and laminar or filamentary structures in the trace gas mixing ratio field produced by enstropy-cascading two-dimensional turbulence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840062881&hterms=sass&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsass','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840062881&hterms=sass&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsass"><span>The effects of the variations in sea surface <span class="hlt">temperature</span> and atmospheric stability in the estimation of average <span class="hlt">wind</span> speed by SEASAT-SASS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liu, W. T.</p> <p>1984-01-01</p> <p>The average <span class="hlt">wind</span> speeds from the scatterometer (SASS) on the ocean observing satellite SEASAT are found to be generally higher than the average <span class="hlt">wind</span> speeds from ship reports. In this study, two factors, sea surface <span class="hlt">temperature</span> and atmospheric stability, are identified which affect microwave scatter and, therefore, wave development. The problem of relating satellite observations to a fictitious quantity, such as the neutral <span class="hlt">wind</span>, that has to be derived from in situ observations with models is examined. The study also demonstrates the dependence of SASS <span class="hlt">winds</span> on sea surface <span class="hlt">temperature</span> at low <span class="hlt">wind</span> speeds, possibly due to <span class="hlt">temperature</span>-dependent factors, such as water viscosity, which affect wave development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940015170','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940015170"><span>High <span class="hlt">temperature</span> co-axial <span class="hlt">winding</span> transformers</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Divan, Deepakraj M.; Novotny, Donald W.</p> <p>1993-01-01</p> <p>The analysis and design of co-axial <span class="hlt">winding</span> transformers is presented. The design equations are derived and the different design approaches are discussed. One of the most important features of co-axial <span class="hlt">winding</span> transformers is the fact that the leakage inductance is well controlled and can be made low. This is not the case in conventional <span class="hlt">winding</span> transformers. In addition, the power density of co-axial <span class="hlt">winding</span> transformers is higher than conventional ones. Hence, using co-axial <span class="hlt">winding</span> transformers in a certain converter topology improves the power density of the converter. The design methodology used in meeting the proposed specifications of the co-axial <span class="hlt">winding</span> transformer specifications are presented and discussed. The final transformer design was constructed in the lab. Co-axial <span class="hlt">winding</span> transformers proved to be a good choice for high power density and high frequency applications. They have a more predictable performance compared with conventional transformers. In addition, the leakage inductance of the transformer can be controlled easily to suit a specific application. For space applications, one major concern is the extraction of heat from power apparatus to prevent excessive heating and hence damaging of these units. Because of the vacuum environment, the only way to extract heat is by using a cold plate. One advantage of co-axial <span class="hlt">winding</span> transformers is that the surface area available to extract heat from is very large compared to conventional transformers. This stems from the unique structure of the co-axial transformer where the whole core surface area is exposed and can be utilized for cooling effectively. This is a crucial issue here since most of the losses are core losses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/49820','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/49820"><span>Can <span class="hlt">air</span> <span class="hlt">temperature</span> be used to project influences of climate change on stream <span class="hlt">temperature</span>?</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Ivan Arismendi; Mohammad Safeeq; Jason B Dunham; Sherri L Johnson</p> <p>2014-01-01</p> <p>Worldwide, lack of data on stream <span class="hlt">temperature</span> has motivated the use of regression-based statistical models to predict stream <span class="hlt">temperatures</span> based on more widely available data on <span class="hlt">air</span> <span class="hlt">temperatures</span>. Such models have been widely applied to project responses of stream <span class="hlt">temperatures</span> under climate change, but the performance of these models has not been fully evaluated. To...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790012416&hterms=microclimate&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmicroclimate','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790012416&hterms=microclimate&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmicroclimate"><span>Observations of the microclimate of a lake under cold <span class="hlt">air</span> advective conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bill, R. G., Jr.; Sutherland, R. A.; Bartholic, J. F.</p> <p>1977-01-01</p> <p>The moderating effects of Lake Apopka, Florida, on downwind surface <span class="hlt">temperatures</span> were evaluated under cold <span class="hlt">air</span> advective conditions. Point <span class="hlt">temperature</span> measurements north and south of the lake and data obtained from the NOAA satellite and a thermal scanner flown at 1.6 km, indicate that, under conditions of moderate <span class="hlt">winds</span> (approximately 4m/sec), surface <span class="hlt">temperatures</span> directly downwind may be higher than surrounding surface <span class="hlt">temperatures</span> by as much as 5 C. With surface <span class="hlt">wind</span> speed less than 1m/sec, no substantial <span class="hlt">temperature</span> effects were observed. Results of this study are being used in land use planning, lake level control and in agriculture for selecting planting sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DPPJ10054S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DPPJ10054S"><span><span class="hlt">Temperature</span> Dependence of Lithium Reactions with <span class="hlt">Air</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sherrod, Roman; Skinner, C. H.; Koel, Bruce</p> <p>2016-10-01</p> <p>Liquid lithium plasma facing components (PFCs) are being developed to handle long pulse, high heat loads in tokamaks. Wetting by lithium of its container is essential for this application, but can be hindered by lithium oxidation by residual gases or during tokamak maintenance. Lithium PFCs will experience elevated <span class="hlt">temperatures</span> due to plasma heat flux. This work presents measurements of lithium reactions at elevated <span class="hlt">temperatures</span> (298-373 K) when exposed to natural <span class="hlt">air</span>. Cylindrical TZM wells 300 microns deep with 1 cm2 surface area were filled with metallic lithium in a glovebox containing argon with less than 1.6 ppm H20, O2, and N2. The wells were transferred to a hot plate in <span class="hlt">air</span>, and then removed periodically for mass gain measurements. Changes in the surface topography were recorded with a microscope. The mass gain of the samples at elevated <span class="hlt">temperatures</span> followed a markedly different behavior to that at room <span class="hlt">temperature</span>. One sample at 373 K began turning red indicative of lithium nitride, while a second turned white indicative of lithium carbonate formation. Data on the mass gain vs. <span class="hlt">temperature</span> and associated topographic changes of the surface will be presented. Science Undergraduate Laboratory Internship funded by Department of Energy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4459207','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4459207"><span>Increases in plasma sheet <span class="hlt">temperature</span> with solar <span class="hlt">wind</span> driving during substorm growth phases</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Forsyth, C; Watt, C E J; Rae, I J; Fazakerley, A N; Kalmoni, N M E; Freeman, M P; Boakes, P D; Nakamura, R; Dandouras, I; Kistler, L M; Jackman, C M; Coxon, J C; Carr, C M</p> <p>2014-01-01</p> <p>During substorm growth phases, magnetic reconnection at the magnetopause extracts ∼1015 J from the solar <span class="hlt">wind</span> which is then stored in the magnetotail lobes. Plasma sheet pressure increases to balance magnetic flux density increases in the lobes. Here we examine plasma sheet pressure, density, and <span class="hlt">temperature</span> during substorm growth phases using 9 years of Cluster data (>316,000 data points). We show that plasma sheet pressure and <span class="hlt">temperature</span> are higher during growth phases with higher solar <span class="hlt">wind</span> driving, whereas the density is approximately constant. We also show a weak correlation between plasma sheet <span class="hlt">temperature</span> before onset and the minimum SuperMAG AL (SML) auroral index in the subsequent substorm. We discuss how energization of the plasma sheet before onset may result from thermodynamically adiabatic processes; how hotter plasma sheets may result in magnetotail instabilities, and how this relates to the onset and size of the subsequent substorm expansion phase. PMID:26074645</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26074645','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26074645"><span>Increases in plasma sheet <span class="hlt">temperature</span> with solar <span class="hlt">wind</span> driving during substorm growth phases.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Forsyth, C; Watt, C E J; Rae, I J; Fazakerley, A N; Kalmoni, N M E; Freeman, M P; Boakes, P D; Nakamura, R; Dandouras, I; Kistler, L M; Jackman, C M; Coxon, J C; Carr, C M</p> <p>2014-12-28</p> <p>During substorm growth phases, magnetic reconnection at the magnetopause extracts ∼10 15  J from the solar <span class="hlt">wind</span> which is then stored in the magnetotail lobes. Plasma sheet pressure increases to balance magnetic flux density increases in the lobes. Here we examine plasma sheet pressure, density, and <span class="hlt">temperature</span> during substorm growth phases using 9 years of Cluster data (>316,000 data points). We show that plasma sheet pressure and <span class="hlt">temperature</span> are higher during growth phases with higher solar <span class="hlt">wind</span> driving, whereas the density is approximately constant. We also show a weak correlation between plasma sheet <span class="hlt">temperature</span> before onset and the minimum SuperMAG AL (SML) auroral index in the subsequent substorm. We discuss how energization of the plasma sheet before onset may result from thermodynamically adiabatic processes; how hotter plasma sheets may result in magnetotail instabilities, and how this relates to the onset and size of the subsequent substorm expansion phase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMGC51D0449R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMGC51D0449R"><span>Trends in Surface <span class="hlt">Temperature</span> from <span class="hlt">AIRS</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ruzmaikin, A.; Aumann, H. H.</p> <p>2014-12-01</p> <p>To address possible causes of the current hiatus in the Earth's global <span class="hlt">temperature</span> we investigate the trends and variability in the surface <span class="hlt">temperature</span> using retrievals obtained from the measurements by the Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) and its companion instrument, the Advanced Microwave Sounding Unit (AMSU), onboard of Aqua spacecraft in 2002-2014. The data used are L3 monthly means on a 1x1degree spatial grid. We separate the land and ocean <span class="hlt">temperatures</span>, as well as <span class="hlt">temperatures</span> in Artic, Antarctic and desert regions. We find a monotonic positive trend for the land <span class="hlt">temperature</span> but not for the ocean <span class="hlt">temperature</span>. The difference in the regional trends can help to explain why the global surface <span class="hlt">temperature</span> remains almost unchanged but the frequency of occurrence of the extreme events increases under rising anthropogenic forcing. The results are compared with the model studies. This work was supported by the Jet Propulsion Laboratory of the California Institute of Technology, under a contract with the National Aeronautics and Space Administration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AMT....11..971I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AMT....11..971I"><span>Single-footprint retrievals of <span class="hlt">temperature</span>, water vapor and cloud properties from <span class="hlt">AIRS</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Irion, Fredrick W.; Kahn, Brian H.; Schreier, Mathias M.; Fetzer, Eric J.; Fishbein, Evan; Fu, Dejian; Kalmus, Peter; Wilson, R. Chris; Wong, Sun; Yue, Qing</p> <p>2018-02-01</p> <p>Single-footprint Atmospheric Infrared Sounder spectra are used in an optimal estimation-based algorithm (<span class="hlt">AIRS</span>-OE) for simultaneous retrieval of atmospheric <span class="hlt">temperature</span>, water vapor, surface <span class="hlt">temperature</span>, cloud-top <span class="hlt">temperature</span>, effective cloud optical depth and effective cloud particle radius. In a departure from currently operational <span class="hlt">AIRS</span> retrievals (<span class="hlt">AIRS</span> V6), cloud scattering and absorption are in the radiative transfer forward model and <span class="hlt">AIRS</span> single-footprint thermal infrared data are used directly rather than cloud-cleared spectra (which are calculated using nine adjacent <span class="hlt">AIRS</span> infrared footprints). Coincident MODIS cloud data are used for cloud a priori data. Using single-footprint spectra improves the horizontal resolution of the <span class="hlt">AIRS</span> retrieval from ˜ 45 to ˜ 13.5 km at nadir, but as microwave data are not used, the retrieval is not made at altitudes below thick clouds. An outline of the <span class="hlt">AIRS</span>-OE retrieval procedure and information content analysis is presented. Initial comparisons of <span class="hlt">AIRS</span>-OE to <span class="hlt">AIRS</span> V6 results show increased horizontal detail in the water vapor and relative humidity fields in the free troposphere above the clouds. Initial comparisons of <span class="hlt">temperature</span>, water vapor and relative humidity profiles with coincident radiosondes show good agreement. Future improvements to the retrieval algorithm, and to the forward model in particular, are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993PhDT........49J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993PhDT........49J"><span>Gap <span class="hlt">Winds</span> in a Fjord: Howe Sound, British Columbia.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jackson, Peter L.</p> <p>1993-01-01</p> <p> gradient and advection are the most important forces, followed by friction which becomes an important force in fast supercritical flow. The sensitivity of gap <span class="hlt">wind</span> speed to various parameters was found from sensitivity tests using the hydraulic model. Results indicated that gap <span class="hlt">wind</span> speed increases with increasing boundary layer height and speed at the head of channel, and increasing synoptic pressure gradient. Gap <span class="hlt">wind</span> speed decreases with increasing friction, and increasing boundary layer height at the seaward channel end. Increasing <span class="hlt">temperature</span> differences between the cold gap <span class="hlt">wind</span> <span class="hlt">air</span> and the warmer <span class="hlt">air</span> aloft was found to increase the variability of the flow--higher maximum but lower mean <span class="hlt">wind</span> speeds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS11B1654B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS11B1654B"><span>Skin <span class="hlt">Temperature</span> Processes in the Presence of Sea Ice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brumer, S. E.; Zappa, C. J.; Brown, S.; McGillis, W. R.; Loose, B.</p> <p>2013-12-01</p> <p>Monitoring the sea-ice margins of polar oceans and understanding the physical processes at play at the ice-ocean-<span class="hlt">air</span> interface is essential in the perspective of a changing climate in which we face an accelerated decline of ice caps and sea ice. Remote sensing and in particular InfraRed (IR) imaging offer a unique opportunity not only to observe physical processes at sea-ice margins, but also to measure <span class="hlt">air</span>-sea exchanges near ice. It permits monitoring ice and ocean <span class="hlt">temperature</span> variability, and can be used for derivation of surface flow field allowing investigating turbulence and shearing at the ice-ocean interface as well as ocean-atmosphere gas transfer. Here we present experiments conducted with the aim of gaining an insight on how the presence of sea ice affects the momentum exchange between the atmosphere and ocean and investigate turbulence production in the interplay of ice-water shear, convection, waves and <span class="hlt">wind</span>. A set of over 200 high resolution IR imagery records was taken at the US Army Cold Regions Research and Engineering Laboratory (CRREL, Hanover NH) under varying ice coverage, fan and pump settings. In situ instruments provided <span class="hlt">air</span> and water <span class="hlt">temperature</span>, salinity, subsurface currents and wave height. <span class="hlt">Air</span> side profiling provided environmental parameters such as <span class="hlt">wind</span> speed, humidity and heat fluxes. The study aims to investigate what can be gained from small-scale high-resolution IR imaging of the ice-ocean-<span class="hlt">air</span> interface; in particular how sea ice modulates local physics and gas transfer. The relationship between water and ice <span class="hlt">temperatures</span> with current and <span class="hlt">wind</span> will be addressed looking at the ocean and ice <span class="hlt">temperature</span> variance. Various skin <span class="hlt">temperature</span> and gas transfer parameterizations will be evaluated at ice margins under varying environmental conditions. Furthermore the accuracy of various techniques used to determine surface flow will be assessed from which turbulence statistics will be determined. This will give an insight on how ice presence</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/caa-permitting/comments-cape-wind-associates-llc-horseshoe-shoal-nantucket-sound-offshore-renewable','PESTICIDES'); return false;" href="https://www.epa.gov/caa-permitting/comments-cape-wind-associates-llc-horseshoe-shoal-nantucket-sound-offshore-renewable"><span>Comments for the Cape <span class="hlt">Wind</span> Associates, LLC, Horseshoe Shoal, Nantucket Sound (Offshore Renewable Energy Project/OCS <span class="hlt">Air</span> Permit)</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>List of comments for the Cape <span class="hlt">Wind</span> Associates, LLC, Horseshoe Shoal, Nantucket Sound (Offshore Renewable Energy Project/OCS <span class="hlt">Air</span> Permit: Massachusetts Plan Approval including nonattainment NSR Appendix A requirements).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080023251','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080023251"><span>Data Assimilation Experiments using Quality Controlled <span class="hlt">AIRS</span> Version 5 <span class="hlt">Temperature</span> Soundings</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>SUsskind, Joel</p> <p>2008-01-01</p> <p>The <span class="hlt">AIRS</span> Science Team Version 5 retrieval algorithm has been finalized and is now operational at the Goddard DAAC in the processing (and reprocessing) of all <span class="hlt">AIRS</span> data. The <span class="hlt">AIRS</span> Science Team Version 5 retrieval algorithm contains two significant improvements over Version 4: 1) Improved physics allows for use of <span class="hlt">AIRS</span> observations in the entire 4.3 pm C02 absorption band in the retrieval of <span class="hlt">temperature</span> profile T(p) during both day and night. Tropospheric sounding 15 pm C02 observations are now used primarily in the generation of cloud cleared radiances Ri. This approach allows for the generation of accurate values of Ri and T(p) under most cloud conditions. 2) Another very significant improvement in Version 5 is the ability to generate accurate case-by-case, level-by-level error estimates for the atmospheric <span class="hlt">temperature</span> profile, as well as for channel-by- channel error estimates for Ri. These error estimates are used for quality control of the retrieved products. We have conducted forecast impact experiments assimilating <span class="hlt">AIRS</span> <span class="hlt">temperature</span> profiles with different levels of quality control using the NASA GEOS-5 data assimilation system. Assimilation of quality controlled T(p) resulted in significantly improved forecast skill compared to that obtained from analyses obtained when all data used operationally by NCEP, except for <span class="hlt">AIRS</span> data, is assimilated. We also conducted an experiment assimilating <span class="hlt">AIRS</span> radiances uncontaminated by clouds, as done Operationally by ECMWF and NCEP. Forecasts resulting from assimilated <span class="hlt">AIRS</span> radiances were of poorer quality than those obtained assimilating <span class="hlt">AIRS</span> <span class="hlt">temperatures</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B21E0373D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B21E0373D"><span>The influence of <span class="hlt">air</span>-conditioning on street <span class="hlt">temperatures</span> in the city of Paris</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Munck, C. S.; Pigeon, G.; Masson, V.; Marchadier, C.; Meunier, F.; Tréméac, B.; Merchat, M.</p> <p>2010-12-01</p> <p>A consequence of urban heat islands in summer is the increased use of <span class="hlt">air</span>-conditioning during extreme heat events : the use of <span class="hlt">air</span>-conditioning systems, while cooling the inside of buildings releases waste heat (as latent and sensible heat) in the lower part of the urban atmosphere, hence potentially increasing <span class="hlt">air</span> street <span class="hlt">temperatures</span> where the heat is released. This may lead locally to a further increase in <span class="hlt">air</span> street <span class="hlt">temperatures</span>, therefore increasing the <span class="hlt">air</span> cooling demand, while at the same time lowering the efficiency of <span class="hlt">air</span>-conditioning units. A coupled model consisting of a meso-scale meteorological model (MESO-NH) and an urban energy balance model (TEB) has been implemented with an <span class="hlt">air</span>-conditioning module and used in combination to real spatialised datasets to understand and quantify potential increases in <span class="hlt">temperature</span> due to <span class="hlt">air</span>-conditioning heat releases for the city of Paris . In a first instance, the current types of <span class="hlt">air</span>-conditioning systems co-existing in the city were simulated (underground chilled water network, wet cooling towers and individual <span class="hlt">air</span>-conditioning units) to study the effects of latent and sensible heat releases on street <span class="hlt">temperatures</span>. In a third instance, 2 scenarios were tested to characterise the impacts of likely future trends in <span class="hlt">air</span>-conditioning equipment in the city : a first scenario for which current heat releases were converted to sensible heat, and a second based on 2030s projections of <span class="hlt">air</span>-conditioning equipment at the scale of the city. All the scenarios showed an increase in street <span class="hlt">temperature</span> which, as expected, was greater at night time than day time. For the first two scenarios, this increase in street <span class="hlt">temperatures</span> was localised at or near the sources of <span class="hlt">air</span>-conditioner heat releases, while the 2030s <span class="hlt">air</span>-conditioning scenario impacted wider zones in the city. The amplitude of the increase in <span class="hlt">temperature</span> varied from 0,25°C to 1°C for the <span class="hlt">air</span>-conditioning current state, between 0,25°C and 2°C for the sensible heat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/38101','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/38101"><span>Empirical downscaling of daily minimum <span class="hlt">air</span> <span class="hlt">temperature</span> at very fine resolutions in complex terrain</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Zachary A. Holden; John T. Abatzoglou; Charles H. Luce; L. Scott Baggett</p> <p>2011-01-01</p> <p>Available <span class="hlt">air</span> <span class="hlt">temperature</span> models do not adequately account for the influence of terrain on nocturnal <span class="hlt">air</span> <span class="hlt">temperatures</span>. An empirical model for night time <span class="hlt">air</span> <span class="hlt">temperatures</span> was developed using a network of one hundred and forty inexpensive <span class="hlt">temperature</span> sensors deployed across the Bitterroot National Forest, Montana. A principle component analysis (PCA) on minimum...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017hst..prop15234H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017hst..prop15234H"><span>Collecting the Missing Piece of the Puzzle: The <span class="hlt">Wind</span> <span class="hlt">Temperatures</span> of Arcturus (K2 III) and Aldeberan (K5 III)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harper, Graham</p> <p>2017-08-01</p> <p>Unravelling the poorly understood processes that drive mass loss from red giant stars requires that we empirically constrain the intimately coupled momentum and energy balance. Hubble high spectral resolution observations of <span class="hlt">wind</span> scattered line profiles, from neutral and singly ionized species, have provided measures of <span class="hlt">wind</span> acceleration, turbulence, terminal speeds, and mass-loss rates. These <span class="hlt">wind</span> properties inform us about the force-momentum balance, however, the spectra have not yielded measures of the much needed <span class="hlt">wind</span> <span class="hlt">temperatures</span>, which constrain the energy balance.We proposed to remedy this omission with STIS E140H observations of the Si III 1206 Ang. resonance emission line for two of the best studied red giants: Arcturus (alpha Boo: K2 III) and Aldebaran (alpha Tau: K5 III), both of which have detailed semi-empirical <span class="hlt">wind</span> velocity models. The relative optical depths of <span class="hlt">wind</span> scattered absorption in Si III 1206 Ang., O I 1303 Ang. triplet., C II 1335 Ang., and existing Mg II h & k and Fe II profiles give the <span class="hlt">wind</span> <span class="hlt">temperatures</span> through the thermally controlled ionization balance. The new <span class="hlt">temperature</span> constraints will be used to test existing semi-empirical models by comparision with multi-frequency JVLA radio fluxes, and also to constrain the flux-tube geometry and wave energy spectrum of magnetic wave-driven <span class="hlt">winds</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120014208','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120014208"><span>Assimilation of Quality Controlled <span class="hlt">AIRS</span> <span class="hlt">Temperature</span> Profiles using the NCEP GFS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Susskind, Joel; Reale, Oreste; Iredell, Lena; Rosenberg, Robert</p> <p>2013-01-01</p> <p>We have previously conducted a number of data assimilation experiments using <span class="hlt">AIRS</span> Version-5 quality controlled <span class="hlt">temperature</span> profiles as a step toward finding an optimum balance of spatial coverage and sounding accuracy with regard to improving forecast skill. The data assimilation and forecast system we used was the Goddard Earth Observing System Model , Version-5 (GEOS-5) Data Assimilation System (DAS), which represents a combination of the NASA GEOS-5 forecast model with the National Centers for Environmental Prediction (NCEP) operational Grid Point Statistical Interpolation (GSI) global analysis scheme. All analyses and forecasts were run at a 0.5deg x 0.625deg spatial resolution. Data assimilation experiments were conducted in four different seasons, each in a different year. Three different sets of data assimilation experiments were run during each time period: Control; <span class="hlt">AIRS</span> T(p); and <span class="hlt">AIRS</span> Radiance. In the "Control" analysis, all the data used operationally by NCEP was assimilated, but no <span class="hlt">AIRS</span> data was assimilated. Radiances from the Aqua AMSU-A instrument were also assimilated operationally by NCEP and are included in the "Control". The <span class="hlt">AIRS</span> Radiance assimilation adds <span class="hlt">AIRS</span> observed radiance observations for a select set of channels to the data set being assimilated, as done operationally by NCEP. In the <span class="hlt">AIRS</span> T(p) assimilation, all information used in the Control was assimilated as well as Quality Controlled <span class="hlt">AIRS</span> Version-5 <span class="hlt">temperature</span> profiles, i.e., <span class="hlt">AIRS</span> T(p) information was substituted for <span class="hlt">AIRS</span> radiance information. The <span class="hlt">AIRS</span> Version-5 <span class="hlt">temperature</span> profiles were presented to the GSI analysis as rawinsonde profiles, assimilated down to a case-by-case appropriate pressure level p(sub best) determined using the Quality Control procedure. Version-5 also determines case-by-case, level-by-level error estimates of the <span class="hlt">temperature</span> profiles, which were used as the uncertainty of each <span class="hlt">temperature</span> measurement. These experiments using GEOS-5 have shown that forecasts</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28495593','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28495593"><span>Enhanced <span class="hlt">air</span> dispersion modelling at a typical Chinese nuclear power plant site: Coupling RIMPUFF with two advanced diagnostic <span class="hlt">wind</span> models.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Yun; Li, Hong; Sun, Sida; Fang, Sheng</p> <p>2017-09-01</p> <p>An enhanced <span class="hlt">air</span> dispersion modelling scheme is proposed to cope with the building layout and complex terrain of a typical Chinese nuclear power plant (NPP) site. In this modelling, the California Meteorological Model (CALMET) and the Stationary <span class="hlt">Wind</span> Fit and Turbulence (SWIFT) are coupled with the Risø Mesoscale PUFF model (RIMPUFF) for refined <span class="hlt">wind</span> field calculation. The near-field diffusion coefficient correction scheme of the Atmospheric Relative Concentrations in the Building Wakes Computer Code (ARCON96) is adopted to characterize dispersion in building arrays. The proposed method is evaluated by a <span class="hlt">wind</span> tunnel experiment that replicates the typical Chinese NPP site. For both <span class="hlt">wind</span> speed/direction and <span class="hlt">air</span> concentration, the enhanced modelling predictions agree well with the observations. The fraction of the predictions within a factor of 2 and 5 of observations exceeds 55% and 82% respectively in the building area and the complex terrain area. This demonstrates the feasibility of the new enhanced modelling for typical Chinese NPP sites. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130010684','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130010684"><span>Statistical Short-Range Guidance for Peak <span class="hlt">Wind</span> Speed Forecasts at Edwards <span class="hlt">Air</span> Force Base, CA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dreher, Joseph; Crawford, Winifred; Lafosse, Richard; Hoeth, Brian; Burns, Kerry</p> <p>2008-01-01</p> <p>The peak <span class="hlt">winds</span> near the surface are an important forecast element for Space Shuttle landings. As defined in the Shuttle Flight Rules (FRs), there are peak <span class="hlt">wind</span> thresholds that cannot be exceeded in order to ensure the safety of the shuttle during landing operations. The National Weather Service Spaceflight Meteorology Group (SMG) is responsible for weather forecasts for all shuttle landings. They indicate peak <span class="hlt">winds</span> are a challenging parameter to forecast. To alleviate the difficulty in making such <span class="hlt">wind</span> forecasts, the Applied Meteorology Unit (AMTJ) developed a personal computer based graphical user interface (GUI) for displaying peak <span class="hlt">wind</span> climatology and probabilities of exceeding peak-<span class="hlt">wind</span> thresholds for the Shuttle Landing Facility (SLF) at Kennedy Space Center. However, the shuttle must land at Edwards <span class="hlt">Air</span> Force Base (EAFB) in southern California when weather conditions at Kennedy Space Center in Florida are not acceptable, so SMG forecasters requested that a similar tool be developed for EAFB. Marshall Space Flight Center (MSFC) personnel archived and performed quality control of 2-minute average and 10-minute peak <span class="hlt">wind</span> speeds at each tower adjacent to the main runway at EAFB from 1997- 2004. They calculated <span class="hlt">wind</span> climatologies and probabilities of average peak <span class="hlt">wind</span> occurrence based on the average speed. The climatologies were calculated for each tower and month, and were stratified by hour, direction, and direction/hour. For the probabilities of peak <span class="hlt">wind</span> occurrence, MSFC calculated empirical and modeled probabilities of meeting or exceeding specific 10-minute peak <span class="hlt">wind</span> speeds using probability density functions. The AMU obtained and reformatted the data into Microsoft Excel PivotTables, which allows users to display different values with point-click-drag techniques. The GUT was then created from the PivotTables using Visual Basic for Applications code. The GUI is run through a macro within Microsoft Excel and allows forecasters to quickly display and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29037396','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29037396"><span>Maternal exposure to ambient <span class="hlt">air</span> <span class="hlt">temperature</span> during pregnancy and early childhood pneumonia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Miao, Yufeng; Shen, Yong-Ming; Lu, Chan; Zeng, Ji; Deng, Qihong</p> <p>2017-10-01</p> <p>Pneumonia has been widely recognized as the leading cause of death in children worldwide, but its etiology still remains unclear. We examined the association between maternal exposure to ambient <span class="hlt">air</span> <span class="hlt">temperature</span> during pregnancy and lifetime pneumonia in the offspring. We conducted a cohort study of 2598 preschool children aged 3-6 years in Changsha, China. The lifetime prevalence of pneumonia was assessed using questionnaire. We backwards estimated each child's exposure to <span class="hlt">air</span> <span class="hlt">temperature</span> during prenatal and postnatal periods. Multiple regression model was used to examine the association between childhood pneumonia and exposure to <span class="hlt">air</span> <span class="hlt">temperature</span> in terms of odd ratios (OR) and 95% confidence interval (CI). Prevalence of childhood pneumonia in Changsha was high up to 38.6%. We found that childhood pneumonia was significantly associated with prenatal exposure to <span class="hlt">air</span> <span class="hlt">temperature</span>, with adjusted OR (95% CI) = 1.77 (1.23-2.54) for an interquartile range (IQR) increase in <span class="hlt">temperature</span>, particularly during the second trimester with adjusted OR (95% CI) = 2.26 (1.32-3.89). Boys are more susceptible to the risk of pneumonia due to <span class="hlt">air</span> <span class="hlt">temperature</span> than girls. We further observed that maternal exposure to extreme heat days during pregnancy increased the risk of pneumonia in the offspring. Maternal exposure to <span class="hlt">air</span> <span class="hlt">temperature</span> during pregnancy, particularly the second trimester, was associated with pneumonia in the children, providing the evidence for fetal origins of pneumonia. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770010521','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770010521"><span>Recertification of the <span class="hlt">air</span> and methane storage vessels at the Langley 8-foot high-<span class="hlt">temperature</span> structures tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hudson, C. M.; Girouard, R. L.; Young, C. P., Jr.; Petley, D. H.; Hudson, J. L., Jr.; Hudgins, J. L.</p> <p>1977-01-01</p> <p>This center operates a number of sophisticated <span class="hlt">wind</span> tunnels in order to fulfill the needs of its researchers. Compressed <span class="hlt">air</span>, which is kept in steel storage vessels, is used to power many of these tunnels. Some of these vessels have been in use for many years, and Langley is currently recertifying these vessels to insure their continued structural integrity. One of the first facilities to be recertified under this program was the Langley 8-foot high-<span class="hlt">temperature</span> structures tunnel. This recertification involved (1) modification, hydrotesting, and inspection of the vessels; (2) repair of all relevant defects; (3) comparison of the original design of the vessel with the current design criteria of Section 8, Division 2, of the 1974 ASME Boiler and Pressure Vessel Code; (4) fracture-mechanics, thermal, and <span class="hlt">wind</span>-induced vibration analyses of the vessels; and (5) development of operating envelopes and a future inspection plan for the vessels. Following these modifications, analyses, and tests, the vessels were recertified for operation at full design pressure (41.4 MPa (6000 psi)) within the operating envelope developed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26683097','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26683097"><span>The Effects of <span class="hlt">Air</span> Pollution and <span class="hlt">Temperature</span> on COPD.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hansel, Nadia N; McCormack, Meredith C; Kim, Victor</p> <p>2016-06-01</p> <p>Chronic Obstructive Pulmonary Disease (COPD) affects 12-16 million people in the United States and is the third-leading cause of death. In developed countries, smoking is the greatest risk factor for the development of COPD, but other exposures also contribute to the development and progression of the disease. Several studies suggest, though are not definitive, that outdoor <span class="hlt">air</span> pollution exposure is linked to the prevalence and incidence of COPD. Among individuals with COPD, outdoor <span class="hlt">air</span> pollutants are associated with loss of lung function and increased respiratory symptoms. In addition, outdoor <span class="hlt">air</span> pollutants are also associated with COPD exacerbations and mortality. There is much less evidence for the impact of indoor <span class="hlt">air</span> on COPD, especially in developed countries in residences without biomass exposure. The limited existing data suggests that indoor particulate matter and nitrogen dioxide concentrations are linked to increased respiratory symptoms among patients with COPD. In addition, with the projected increases in <span class="hlt">temperature</span> and extreme weather events in the context of climate change there has been increased attention to the effects of heat exposure. Extremes of <span class="hlt">temperature</span>-both heat and cold-have been associated with increased respiratory morbidity in COPD. Some studies also suggest that <span class="hlt">temperature</span> may modify the effect of pollution exposure and though results are not conclusive, understanding factors that may modify susceptibility to <span class="hlt">air</span> pollution in patients with COPD is of utmost importance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100021378','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100021378"><span>Statistical Short-Range Guidance for Peak <span class="hlt">Wind</span> Forecasts on Kennedy Space Center/Cape Canaveral <span class="hlt">Air</span> Force Station, Phase III</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Crawford, Winifred</p> <p>2010-01-01</p> <p>This final report describes the development of a peak <span class="hlt">wind</span> forecast tool to assist forecasters in determining the probability of violating launch commit criteria (LCC) at Kennedy Space Center (KSC) and Cape Canaveral <span class="hlt">Air</span> Force Station (CCAFS). The peak <span class="hlt">winds</span> are an important forecast element for both the Space Shuttle and Expendable Launch Vehicle (ELV) programs. The LCC define specific peak <span class="hlt">wind</span> thresholds for each launch operation that cannot be exceeded in order to ensure the safety of the vehicle. The 45th Weather Squadron (45 WS) has found that peak <span class="hlt">winds</span> are a challenging parameter to forecast, particularly in the cool season months of October through April. Based on the importance of forecasting peak <span class="hlt">winds</span>, the 45 WS tasked the Applied Meteorology Unit (AMU) to develop a short-range peak-<span class="hlt">wind</span> forecast tool to assist in forecasting LCC violations.The tool includes climatologies of the 5-minute mean and peak <span class="hlt">winds</span> by month, hour, and direction, and probability distributions of the peak <span class="hlt">winds</span> as a function of the 5-minute mean <span class="hlt">wind</span> speeds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EPJP..131..410T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EPJP..131..410T"><span>Thermal performances of vertical hybrid PV/T <span class="hlt">air</span> collector</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tabet, I.; Touafek, K.; Bellel, N.; Khelifa, A.</p> <p>2016-11-01</p> <p>In this work, numerical analyses and the experimental validation of the thermal behavior of a vertical photovoltaic thermal <span class="hlt">air</span> collector are investigated. The thermal model is developed using the energy balance equations of the PV/T <span class="hlt">air</span> collector. Experimental tests are conducted to validate our mathematical model. The tests are performed in the southern Algerian region (Ghardaïa) under clear sky conditions. The prototype of the PV/T <span class="hlt">air</span> collector is vertically erected and south oriented. The absorber upper plate <span class="hlt">temperature</span>, glass cover <span class="hlt">temperature</span>, <span class="hlt">air</span> <span class="hlt">temperature</span> in the inlet and outlet of the collector, ambient <span class="hlt">temperature</span>, <span class="hlt">wind</span> speed, and solar radiation are measured. The efficiency of the collector increases with increase in mass flow of <span class="hlt">air</span>, but the increase in mass flow of <span class="hlt">air</span> reduces the <span class="hlt">temperature</span> of the system. The increase in efficiency of the PV/T <span class="hlt">air</span> collector is due to the increase in the number of fins added. In the experiments, the <span class="hlt">air</span> <span class="hlt">temperature</span> difference between the inlet and the outlet of the PV/T <span class="hlt">air</span> collector reaches 10 ° C on November 21, 2014, the interval time is between 10:00 and 14:00, and the <span class="hlt">temperature</span> of the upper plate reaches 45 ° C at noon. The mathematical model describing the dynamic behavior of the typical PV/T <span class="hlt">air</span> collector is evaluated by calculating the root mean square error and mean absolute percentage error. A good agreement between the experiment and the simulation results is obtained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040053577','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040053577"><span>Characteristics of Gaseous Diffusion Flames with High <span class="hlt">Temperature</span> Combustion <span class="hlt">Air</span> in Microgravity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ghaderi, M.; Gupta, A. K.</p> <p>2003-01-01</p> <p>The characteristics of gaseous diffusion flames have been obtained using high <span class="hlt">temperature</span> combustion <span class="hlt">air</span> under microgravity conditions. The time resolved flame images under free fall microgravity conditions were obtained from the video images obtained. The tests results reported here were conducted using propane as the fuel and about 1000 C combustion <span class="hlt">air</span>. The burner included a 0.686 mm diameter central fuel jet injected into the surrounding high <span class="hlt">temperature</span> combustion <span class="hlt">air</span>. The fuel jet exit Reynolds number was 63. Several measurements were taken at different <span class="hlt">air</span> preheats and fuel jet exit Reynolds number. The resulting hybrid color flame was found to be blue at the base of the flame followed by a yellow color flame. The length and width of flame during the entire free fall conditions has been examined. Also the relative flame length and width for blue and yellow portion of the flame has been examined under microgravity conditions. The results show that the flame length decreases and width increases with high <span class="hlt">air</span> preheats in microgravity condition. In microgravity conditions the flame length is larger with normal <span class="hlt">temperature</span> combustion <span class="hlt">air</span> than high <span class="hlt">temperature</span> <span class="hlt">air</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930091720','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930091720"><span>Correction of <span class="hlt">Temperatures</span> of <span class="hlt">Air</span>-Cooled Engine Cylinders for Variation in Engine and Cooling Conditions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schey, Oscar W; Pinkel, Benjamin; Ellerbrock, Herman H , Jr</p> <p>1939-01-01</p> <p>Factors are obtained from semiempirical equations for correcting engine-cylinder <span class="hlt">temperatures</span> for variation in important engine and cooling conditions. The variation of engine <span class="hlt">temperatures</span> with atmospheric <span class="hlt">temperature</span> is treated in detail, and correction factors are obtained for various flight and test conditions, such as climb at constant indicated <span class="hlt">air</span> speed, level flight, ground running, take-off, constant speed of cooling <span class="hlt">air</span>, and constant mass flow of cooling <span class="hlt">air</span>. Seven conventional <span class="hlt">air</span>-cooled engine cylinders enclosed in jackets and cooled by a blower were tested to determine the effect of cooling-<span class="hlt">air</span> <span class="hlt">temperature</span> and carburetor-<span class="hlt">air</span> <span class="hlt">temperature</span> on cylinder <span class="hlt">temperatures</span>. The cooling <span class="hlt">air</span> <span class="hlt">temperature</span> was varied from approximately 80 degrees F. to 230 degrees F. and the carburetor-<span class="hlt">air</span> <span class="hlt">temperature</span> from approximately 40 degrees F. to 160 degrees F. Tests were made over a large range of engine speeds, brake mean effective pressures, and pressure drops across the cylinder. The correction factors obtained experimentally are compared with those obtained from the semiempirical equations and a fair agreement is noted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1811274S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1811274S"><span><span class="hlt">Wind</span> slab formation in snow: experimental setup and first results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sommer, Christian; Lehning, Michael; Fierz, Charles</p> <p>2016-04-01</p> <p>The formation of <span class="hlt">wind</span>-hardened surface layers, also known as <span class="hlt">wind</span> slabs or <span class="hlt">wind</span> crusts, is studied. Better knowledge about which processes and parameters are important will lead to an improved understanding of the mass balances in polar and alpine areas. It will also improve snow-cover models (i.e. SNOWPACK) as well as the forecast of avalanche danger. A ring-shaped <span class="hlt">wind</span> tunnel has been built and instrumented. The facility is ring-shaped to simulate an infinitely long snow surface (infinite fetch). A SnowMicroPen (SMP) is used to measure the snow hardness. Other sensors measure environmental conditions such as <span class="hlt">wind</span> velocity, <span class="hlt">air</span> <span class="hlt">temperature</span>, <span class="hlt">air</span> humidity, the <span class="hlt">temperature</span> of the snow and of the snow surface. A camera is used to detect drifting particles and to measure the Specific Surface Area (SSA) at the snow surface via near-infrared photography. First experiments indicate that mechanical fragmentation followed by sintering is the most efficient process to harden the surface. The hardness increased rapidly during drifting snow events, but only slowly or not at all when the <span class="hlt">wind</span> speed was kept below the threshold for drifting snow. With drifting, the penetration resistance increased from the original 0.07 N to around 0.3 N in about an hour. Without drifting, a slow, further increase in resistance was observed. In about six hours, the hardness of the top 1-2 cm increased to 0.5 N. During this eight-hour experiment consisting of about two hours with intermittent drifting and six hours without drifting, the density at the surface increased from 66 kg/m3 to around 170 kg/m3. In the unaffected region close to the ground, the density increased from 100 kg/m3 to 110 kg/m3.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1412658-converting-wind-energy-ammonia-lower-pressure','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1412658-converting-wind-energy-ammonia-lower-pressure"><span>Converting <span class="hlt">Wind</span> Energy to Ammonia at Lower Pressure</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>Malmali, Mahdi; Reese, Michael; McCormick, Alon V.</p> <p></p> <p>Renewable <span class="hlt">wind</span> energy can be used to make ammonia. However, <span class="hlt">wind</span>-generated ammonia costs about twice that made from a traditional fossil-fuel driven process. To reduce the production cost, we replace the conventional ammonia condensation with a selective absorber containing metal halides, e.g., calcium chloride, operating at near synthesis <span class="hlt">temperatures</span>. With this reaction-absorption process, ammonia can be synthesized at 20 bar from <span class="hlt">air</span>, water, and <span class="hlt">wind</span>-generated electricity, with rates comparable to the conventional process running at 150–300 bar. In our reaction-absorption process, the rate of ammonia synthesis is now controlled not by the chemical reaction but largely by the pump usedmore » to recycle the unreacted gases. The results suggest an alternative route to distributed ammonia manufacture which can locally supply nitrogen fertilizer and also a method to capture stranded <span class="hlt">wind</span> energy as a carbon-neutral liquid fuel.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1412658-converting-wind-energy-ammonia-lower-pressure','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1412658-converting-wind-energy-ammonia-lower-pressure"><span>Converting <span class="hlt">Wind</span> Energy to Ammonia at Lower Pressure</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Malmali, Mahdi; Reese, Michael; McCormick, Alon V.; ...</p> <p>2017-11-07</p> <p>Renewable <span class="hlt">wind</span> energy can be used to make ammonia. However, <span class="hlt">wind</span>-generated ammonia costs about twice that made from a traditional fossil-fuel driven process. To reduce the production cost, we replace the conventional ammonia condensation with a selective absorber containing metal halides, e.g., calcium chloride, operating at near synthesis <span class="hlt">temperatures</span>. With this reaction-absorption process, ammonia can be synthesized at 20 bar from <span class="hlt">air</span>, water, and <span class="hlt">wind</span>-generated electricity, with rates comparable to the conventional process running at 150–300 bar. In our reaction-absorption process, the rate of ammonia synthesis is now controlled not by the chemical reaction but largely by the pump usedmore » to recycle the unreacted gases. The results suggest an alternative route to distributed ammonia manufacture which can locally supply nitrogen fertilizer and also a method to capture stranded <span class="hlt">wind</span> energy as a carbon-neutral liquid fuel.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050153817&hterms=1074&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D%2526%25231074','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050153817&hterms=1074&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3D%2526%25231074"><span>The mass and speed dependence of meteor <span class="hlt">air</span> plasma <span class="hlt">temperatures</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jenniskens, Peter; Laux, Christophe O.; Wilson, Michael A.; Schaller, Emily L.</p> <p>2004-01-01</p> <p>The speed and mass dependence of meteor <span class="hlt">air</span> plasma <span class="hlt">temperatures</span> is perhaps the most important data needed to understand how small meteoroids chemically change the ambient atmosphere in their path and enrich the ablated meteoric organic matter with oxygen. Such chemistry can play an important role in creating prebiotic compounds. The excitation conditions in various <span class="hlt">air</span> plasma emissions were measured from high-resolution optical spectra of Leonid storm meteors during NASA's Leonid Multi-Instrument Aircraft Campaign. This was the first time a sufficient number and range of <span class="hlt">temperature</span> measurements were obtained to search for meteoroid mass and speed dependencies. We found slight increases in <span class="hlt">temperature</span> with decreasing altitude, but otherwise nearly constant values for meteoroids with speeds between 35 and 72 km/s and masses between 10(-5) g and 1 g. We conclude that faster and more massive meteoroids produce a larger emission volume, but not a higher <span class="hlt">air</span> plasma <span class="hlt">temperature</span>. We speculate that the meteoric plasma may be in multiphase equilibrium with the ambient atmosphere, which could mean lower plasma <span class="hlt">temperatures</span> in a CO(2)-rich early Earth atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15104905','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15104905"><span>The mass and speed dependence of meteor <span class="hlt">air</span> plasma <span class="hlt">temperatures</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jenniskens, Peter; Laux, Christophe O; Wilson, Michael A; Schaller, Emily L</p> <p>2004-01-01</p> <p>The speed and mass dependence of meteor <span class="hlt">air</span> plasma <span class="hlt">temperatures</span> is perhaps the most important data needed to understand how small meteoroids chemically change the ambient atmosphere in their path and enrich the ablated meteoric organic matter with oxygen. Such chemistry can play an important role in creating prebiotic compounds. The excitation conditions in various <span class="hlt">air</span> plasma emissions were measured from high-resolution optical spectra of Leonid storm meteors during NASA's Leonid Multi-Instrument Aircraft Campaign. This was the first time a sufficient number and range of <span class="hlt">temperature</span> measurements were obtained to search for meteoroid mass and speed dependencies. We found slight increases in <span class="hlt">temperature</span> with decreasing altitude, but otherwise nearly constant values for meteoroids with speeds between 35 and 72 km/s and masses between 10(-5) g and 1 g. We conclude that faster and more massive meteoroids produce a larger emission volume, but not a higher <span class="hlt">air</span> plasma <span class="hlt">temperature</span>. We speculate that the meteoric plasma may be in multiphase equilibrium with the ambient atmosphere, which could mean lower plasma <span class="hlt">temperatures</span> in a CO(2)-rich early Earth atmosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28822259','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28822259"><span>Ambient <span class="hlt">air</span> pollution, <span class="hlt">temperature</span> and kawasaki disease in Shanghai, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lin, Zhijing; Meng, Xia; Chen, Renjie; Huang, Guoying; Ma, Xiaojing; Chen, Jingjing; Huang, Min; Huang, Meirong; Gui, Yonghao; Chu, Chen; Liu, Fang; Kan, Haidong</p> <p>2017-11-01</p> <p>Kawasaki disease (KD) is a kind of pediatric vasculitis of unknown etiology which mainly affects the development of coronary artery aneurysms. Few studies have explored the potential environmental risk factors on KD incidence. We performed a time-series analysis to investigate the associations between <span class="hlt">air</span> pollution and <span class="hlt">temperature</span> and KD in Shanghai, China. We collected daily-hospitalized KD patients that were admitted in major pediatric specialty hospitals located in the urban areas of Shanghai from 2001 to 2010. The over-dispersed generalized additive model was used to estimate the effects of <span class="hlt">air</span> pollutants on KD incidence on each day. Then, this model was combined with a distributed lag non-linear model to estimate the cumulative effects of <span class="hlt">temperature</span> over a week. There were positive but statistically insignificant associations between three major <span class="hlt">air</span> pollutants and KD incidence. The association between daily mean <span class="hlt">temperature</span> and KD was generally J-shaped with higher risks on hot days. The cumulative relative risk of KD at extreme hot <span class="hlt">temperature</span> (99th percentile, 32.4 °C) over a week was 1.91 [95% confidence interval (CI): 1.13, 3.23], compared with the referent <span class="hlt">temperature</span> (10.0 °C). This study suggested that a short-term exposure to high <span class="hlt">temperature</span> may significantly increase the incidence of KD, and the evidence linking <span class="hlt">air</span> pollution and KD incidence was limited. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AtmRe..80..263C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AtmRe..80..263C"><span><span class="hlt">Air</span> flow analysis in the upper Río Negro Valley (Argentina)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cogliati, M. G.; Mazzeo, N. A.</p> <p>2006-06-01</p> <p>The so called Upper Río Negro Valley in Argentina is one of the most important fruit and vegetable production regions of the country. It comprises the lower valleys of the Limay and Neuquén rivers and the upper Negro river valley. Out of the 41,671 cultivated hectares, 84.6% are cultivated with fruit trees, especially apple, pear and stone fruit trees. Late frosts occurring when trees are sensitive to low <span class="hlt">temperatures</span> have a significant impact on the regional production. This study presents an analysis of <span class="hlt">air</span> flow characteristics in the Upper Río Negro Valley and its relationship with ambient <span class="hlt">air</span> flow. To such effect, observations made when synoptic-scale weather patterns were favorable for radiative frosts (light <span class="hlt">wind</span> and clear sky) or nocturnal <span class="hlt">temperature</span> inversion in the lower layer were used. In the Negro river valley, both <span class="hlt">wind</span> channeling and downward horizontal momentum transport from ambient <span class="hlt">wind</span> were observed; in nighttime, very light <span class="hlt">wind</span> events occurred, possibly associated with drainage <span class="hlt">winds</span> from the nearby higher levels of the barda. In the Neuquén river valley, the prevailing effect appeared to be forced channeling, consistent with the results obtained in valleys where the synoptic scale <span class="hlt">wind</span> crossed the axis of the valley. In the Limay river valley, the flow was observed to blow parallel to the longitudinal valley axis, possibly influenced by pressure gradient and forced channeling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/865745','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/865745"><span><span class="hlt">Air</span> separation with <span class="hlt">temperature</span> and pressure swing</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Cassano, Anthony A.</p> <p>1986-01-01</p> <p>A chemical absorbent <span class="hlt">air</span> separation process is set forth which uses a <span class="hlt">temperature</span> swing absorption-desorption cycle in combination with a pressure swing wherein the pressure is elevated in the desorption stage of the process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.H53F1591O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.H53F1591O"><span>Geographical and Geomorphological Effects on <span class="hlt">Air</span> <span class="hlt">Temperatures</span> in the Columbia Basin's Signature Vineyards</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Olson, L.; Pogue, K. R.; Bader, N.</p> <p>2012-12-01</p> <p>The Columbia Basin of Washington and Oregon is one of the most productive grape-growing areas in the United States. Wines produced in this region are influenced by their terroir - the amalgamation of physical and cultural elements that influence grapes grown at a particular vineyard site. Of the physical factors, climate, and in particular <span class="hlt">air</span> <span class="hlt">temperature</span>, has been recognized as a primary influence on viticulture. <span class="hlt">Air</span> <span class="hlt">temperature</span> directly affects ripening in the grapes. Proper fruit ripening, which requires precise and balanced levels of acid and sugar, and the accumulation of pigment in the grape skin, directly correlates with the quality of wine produced. Many features control <span class="hlt">air</span> <span class="hlt">temperature</span> within a particular vineyard. Elevation, latitude, slope, and aspect all converge to form complex relationships with <span class="hlt">air</span> <span class="hlt">temperatures</span>; however, the relative degree to which these attributes affect <span class="hlt">temperatures</span> varies between regions and is not well understood. This study examines the influence of geography and geomorphology on <span class="hlt">air</span> <span class="hlt">temperatures</span> within the American Viticultural Areas (AVAs) of the Columbia Basin in eastern Washington and Oregon. The premier vineyards within each AVA, which have been recognized for producing high-quality wine, were equipped with <span class="hlt">air</span> <span class="hlt">temperature</span> monitoring stations that collected hourly <span class="hlt">temperature</span> measurements. A variety of <span class="hlt">temperature</span> statistics were calculated, including daily average, maximum, and minimum <span class="hlt">temperatures</span>. From these values, average diurnal variation and growing degree-days (10°C) were calculated. A variety of other statistics were computed, including date of first and last frost and time spent below a minimum <span class="hlt">temperature</span> threshold. These parameters were compared to the vineyard's elevation, latitude, slope, aspect, and local topography using GPS, ArcCatalog, and GIS in an attempt to determine their relative influences on <span class="hlt">air</span> <span class="hlt">temperatures</span>. From these statistics, it was possible to delineate two trends of <span class="hlt">temperature</span> variation</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA22362.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA22362.html"><span>Polar <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>2018-04-05</p> <p>This VIS image shows 'streamers' of clouds created by katabatic <span class="hlt">winds</span> at the north polar cap. Katabatic <span class="hlt">winds</span> are created by cold <span class="hlt">air</span> sinking at the pole and then speeding along the ice surface towards the edge of the polar cap. When the <span class="hlt">winds</span> enter troughs the <span class="hlt">wind</span> regime changes from laminar flow to choatic and clouds of ice particles and/or dust are visible. This <span class="hlt">wind</span> activity peaks at the start of northern hemisphere summer. Orbit Number: 53942 Latitude: 86.8433 Longitude: 99.3149 Instrument: VIS Captured: 2014-02-10 10:50 https://photojournal.jpl.nasa.gov/catalog/PIA22362</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ThApC.tmp...59P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ThApC.tmp...59P"><span><span class="hlt">Air</span> <span class="hlt">temperature</span> changes in Toruń (central Poland) from 1871 to 2010</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pospieszyńska, Aleksandra; Przybylak, Rajmund</p> <p>2018-02-01</p> <p>The article presents a detailed analysis of changes in <span class="hlt">air</span> <span class="hlt">temperature</span> in Toruń in the period 1871-2010 on the basis of homogenised monthly, seasonal and annual <span class="hlt">air</span> <span class="hlt">temperature</span> series which have been newly constructed (i.e. extended by the 50 years of 1871-1920). Over the 140-year study period, a sizeable and statistically significant increase of 0.1 °C per decade was found in the <span class="hlt">air</span> <span class="hlt">temperature</span> in Toruń. The greatest increases occurred for spring and winter, at 0.12 and 0.11 °C, respectively. A lesser warming, meanwhile, was recorded for autumn (0.10 °C/10 years), and particularly for summer (0.07 °C/10 years). The <span class="hlt">air</span> <span class="hlt">temperature</span> trends are statistically significant for all seasons. <span class="hlt">Air</span> <span class="hlt">temperature</span> differences between the monthly averages of three analysed subperiods (1871-1900, 1901-1950 and 1951-2010) and averages for the entire period under review rarely exceeded ± 0.5 °C. In all of these periods, the highest average <span class="hlt">air</span> <span class="hlt">temperatures</span> occurred in July and the lowest in January. The period of 1981-2010 had the highest frequency of occurrence of very and extremely warm seasons and years. Meanwhile, the highest frequency of very and extremely cool seasons and years was recorded in the 1940s and in the nineteenth century. In the period of 1871-2010, winters shortened markedly (by 7%) and summers lengthened by 3.8%. All of the presented aspects of <span class="hlt">air</span> <span class="hlt">temperature</span> in Toruń, which is representative of the climate of central Poland, are in close agreement with the findings of analogous studies of the same for other areas of Poland and Central Europe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26706765','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26706765"><span>A comparison of urban heat islands mapped using skin <span class="hlt">temperature</span>, <span class="hlt">air</span> <span class="hlt">temperature</span>, and apparent <span class="hlt">temperature</span> (Humidex), for the greater Vancouver area.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ho, Hung Chak; Knudby, Anders; Xu, Yongming; Hodul, Matus; Aminipouri, Mehdi</p> <p>2016-02-15</p> <p>Apparent <span class="hlt">temperature</span> is more closely related to mortality during extreme heat events than other <span class="hlt">temperature</span> variables, yet spatial epidemiology studies typically use skin <span class="hlt">temperature</span> (also known as land surface <span class="hlt">temperature</span>) to quantify heat exposure because it is relatively easy to map from satellite data. An empirical approach to map apparent <span class="hlt">temperature</span> at the neighborhood scale, which relies on publicly available weather station observations and spatial data layers combined in a random forest regression model, was demonstrated for greater Vancouver, Canada. Model errors were acceptable (cross-validated RMSE=2.04 °C) and the resulting map of apparent <span class="hlt">temperature</span>, calibrated for a typical hot summer day, corresponded well with past <span class="hlt">temperature</span> research in the area. A comparison with field measurements as well as similar maps of skin <span class="hlt">temperature</span> and <span class="hlt">air</span> <span class="hlt">temperature</span> revealed that skin <span class="hlt">temperature</span> was poorly correlated with both <span class="hlt">air</span> <span class="hlt">temperature</span> (R(2)=0.38) and apparent <span class="hlt">temperature</span> (R(2)=0.39). While the latter two were more similar (R(2)=0.87), apparent <span class="hlt">temperature</span> was predicted to exceed <span class="hlt">air</span> <span class="hlt">temperature</span> by more than 5 °C in several urban areas as well as around the confluence of the Pitt and Fraser rivers. We conclude that skin <span class="hlt">temperature</span> is not a suitable proxy for human heat exposure, and that spatial epidemiology studies could benefit from mapping apparent <span class="hlt">temperature</span>, using an approach similar to the one reported here, to better quantify differences in heat exposure that exist across an urban landscape. Copyright © 2015 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DPS....4921102S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DPS....4921102S"><span>Solar <span class="hlt">wind</span> control of stratospheric <span class="hlt">temperatures</span> in Jupiter's auroral regions?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sinclair, James Andrew; Orton, Glenn; Kasaba, Yasumasa; Sato, Takao M.; Tao, Chihiro; Waite, J. Hunter; Cravens, Thomas; Houston, Stephen; Fletcher, Leigh; Irwin, Patrick; Greathouse, Thomas K.</p> <p>2017-10-01</p> <p>Auroral emissions are the process through which the interaction of a planet’s atmosphere and its external magnetosphere can be studied. Jupiter exhibits auroral emission at a multitude of wavelengths including the X-ray, ultraviolet and near-infrared. Enhanced emission of CH4 and other stratospheric hydrocarbons is also observed coincident with Jupiter’s shorter-wavelength auroral emission (e.g. Caldwell et al., 1980, Icarus 44, 667-675, Kostiuk et al., 1993, JGR 98, 18823). This indicates that auroral processes modify the thermal structure and composition of the auroral stratosphere. The exact mechanism responsible for this auroral-related heating of the stratosphere has however remained elusive (Sinclair et al., 2017a, Icarus 292, 182-207, Sinclair et al., 2017b, GRL, 44, 5345-5354). We will present an analysis of 7.8-μm images of Jupiter measured by COMICS (Cooled Mid-Infrared Camera and Spectrograph, Kataza et al., 2000, Proc. SPIE(4008), 1144-1152) on the Subaru telescope. These images were acquired on January 11th, 12th, 13th, 14th, February 4, 5th and May 17th, 18th, 19th and 20th in 2017, allowing the daily variability of Jupiter’s auroral-related stratospheric heating to be tracked. Preliminary results suggest lower stratospheric <span class="hlt">temperatures</span> are directly forced by the solar <span class="hlt">wind</span> dynamical pressure. The southern auroral hotspot exhibited a significant increase in brightness <span class="hlt">temperature</span> over a 24-hour period. Over the same time period, a solar <span class="hlt">wind</span> propagation model (Tao et al. 2005, JGR 110, A11208) predicts a strong increase in the solar <span class="hlt">wind</span> dynamical pressure at Jupiter.</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 regional weather and climate. In this work, we present observational evidence of the impact of <span class="hlt">wind</span> farms on near-surface <span class="hlt">air</span> <span class="hlt">temperatures</span>. Data from perhaps the only meteorological field campaign in an operational <span class="hlt">wind</span> farm shows that downwind <span class="hlt">temperatures</span> are lower during the daytime and higher at night compared to the upwind environment. Corresponding radiosonde profiles at the nearby Edwards <span class="hlt">Air</span> 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 <span class="hlt">temperature</span> lapse rates. We conducted a set of 306 simulations with the Regional Atmospheric Modeling System (RAMS) to test if regional 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('https://ntrs.nasa.gov/search.jsp?R=19860062230&hterms=chemical+reactions&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dchemical%2Breactions','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860062230&hterms=chemical+reactions&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dchemical%2Breactions"><span>Rate constants for chemical reactions in high-<span class="hlt">temperature</span> nonequilibrium <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jaffe, R. L.</p> <p>1986-01-01</p> <p>In the nonequilibrium atmospheric chemistry regime that will be encountered by the proposed Aeroassisted Orbital Transfer Vehicle in the upper atmosphere, where <span class="hlt">air</span> density is too low for thermal and chemical equilibrium to be maintained, the detailed high <span class="hlt">temperature</span> <span class="hlt">air</span> chemistry plays a critical role in defining radiative and convective heating loads. Although vibrational and electronic <span class="hlt">temperatures</span> remain low (less than 15,000 K), rotational and translational <span class="hlt">temperatures</span> may reach 50,000 K. Attention is presently given to the effects of multiple <span class="hlt">temperatures</span> on the magnitudes of various chemical reaction rate constants, for the cases of both bimolecular exchange reactions and collisional excitation and dissociation reactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800016497','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800016497"><span>Effect of production microclimate on female thermal state with increased <span class="hlt">temperature</span> and <span class="hlt">air</span> humidity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Machablishvili, O. G.</p> <p>1980-01-01</p> <p>The thermal state of women during the effect of high <span class="hlt">air</span> <span class="hlt">temperature</span> and relative humidity with a varying degree of physical loads was studied. Parameters for <span class="hlt">air</span> <span class="hlt">temperature</span>, relative humidity, and <span class="hlt">air</span> movement were established. It was established that in women the thermo-regulatory stress occurs at lower <span class="hlt">air</span> <span class="hlt">temperatures</span> and with lower physical loads than in men. The accumulation of heat in women was revealed with lower <span class="hlt">air</span> <span class="hlt">temperature</span> than in men. It is concluded that to preserve the normal physiological state of the female organism it is necessary to create more favorable microclimate conditions and decrease the physical loads.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BoLMe.167..445L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BoLMe.167..445L"><span>Signatures of <span class="hlt">Air</span>-Wave Interactions Over a Large Lake</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Qi; Bou-Zeid, Elie; Vercauteren, Nikki; Parlange, Marc</p> <p>2018-06-01</p> <p>The <span class="hlt">air</span>-water exchange of momentum and scalars (<span class="hlt">temperature</span> and water vapour) is investigated using the Lake-Atmosphere Turbulent EXchange (LATEX) dataset. The <span class="hlt">wind</span> waves and swell are found to affect the coupling between the water surface and the <span class="hlt">air</span> differently. The surface-stress vector aligns with the <span class="hlt">wind</span> velocity in the presence of <span class="hlt">wind</span> waves, but a wide range of stress-<span class="hlt">wind</span> misalignment angles is observed during swell. The momentum transport efficiency decreases when significant stress-<span class="hlt">wind</span> misalignment is present, suggesting a strong influence of surface wave properties on surface drag. Based on this improved understanding of the role of wave-<span class="hlt">wind</span> misalignment, a new relative <span class="hlt">wind</span> speed for surface-layer similarity formulations is proposed and tested using the data. The new expression yields a value of the von Kármán constant (κ ) of 0.38, compared to 0.36 when using the absolute <span class="hlt">wind</span> speed, as well as reduced data fitting errors. Finally, the ratios of aerodynamic to scalar roughness lengths are computed and various existing models in the literature are tested using least-square fitting to the observed ratios. The tests are able to discriminate between the performance of various models; however, they also indicate that more investigations are required to understand the physics of scalar exchanges over waves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990071195','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990071195"><span>NASA Glenn 1-by 1-Foot Supersonic <span class="hlt">Wind</span> Tunnel User Manual</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Seablom, Kirk D.; Soeder, Ronald H.; Stark, David E.; Leone, John F. X.; Henry, Michael W.</p> <p>1999-01-01</p> <p>This manual describes the NASA Glenn Research Center's 1 - by 1 -Foot Supersonic <span class="hlt">Wind</span> Tunnel and provides information for customers who wish to conduct experiments in this facility. Tunnel performance envelopes of total pressure, total <span class="hlt">temperature</span>, and dynamic pressure as a function of test section Mach number are presented. For each Mach number, maps are presented of Reynolds number per foot as a function of the total <span class="hlt">air</span> <span class="hlt">temperature</span> at the test section inlet for constant total <span class="hlt">air</span> pressure at the inlet. General support systems-such as the service <span class="hlt">air</span>, combustion <span class="hlt">air</span>, altitude exhaust system, auxiliary bleed system, model hydraulic system, schlieren system, model pressure-sensitive paint, and laser sheet system are discussed. In addition, instrumentation and data processing, acquisition systems are described, pretest meeting formats and schedules are outlined, and customer responsibilities and personnel safety are addressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.8128K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.8128K"><span>Mesospheric <span class="hlt">Temperatures</span> and <span class="hlt">Winds</span> measured by a VHF Meteor Radar at King Sejong Station (62.2S, 58.8W), Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Yongha; Kim, Jeong-Han; Jee, Geonwha; Lee, Chang-Sup</p> <p>2010-05-01</p> <p>A VHF radar at King Sejong Station, Antarctica has been measuring meteor echoes since March 2007. <span class="hlt">Temperatures</span> near the mesopause are derived from meteor decay times with an improved method of selecting meteor echo samples, and compared with airglow <span class="hlt">temperatures</span> simultaneously observed by a spectral airglow <span class="hlt">temperature</span> imager (SATI). The <span class="hlt">temperatures</span> derived from meteor decay times are mostly consistent with the rotational <span class="hlt">temperatures</span> of SATI OH(6-2) and O2(0-1) emissions from March through October. During southern summer when SATI cannot be operated due to brief night time, the meteor radar observation shows cold mesospheric <span class="hlt">temperatures</span>, significantly lower than the CIRA86 model. The meteor radar observation also provides <span class="hlt">wind</span> field information between 80 and 100 km of altitude. The measured meridional <span class="hlt">winds</span> seem to follow the summer pole to winter pole circulation, and thus are correlated with the measured seasonal <span class="hlt">temperature</span> change. However, the correlation between meridional <span class="hlt">winds</span> and <span class="hlt">temperatures</span> is not found in day by day base, as a previous study reported. Tidal characteristics of both zonal and meridional <span class="hlt">winds</span> will also be compared with those of other Antarctic stations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AcO....77..201O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AcO....77..201O"><span>Seasonal patterns of body <span class="hlt">temperature</span> and microhabitat selection in a lacertid lizard</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortega, Zaida; Pérez-Mellado, Valentín</p> <p>2016-11-01</p> <p>In temperate areas, seasonal changes entail a source of environmental variation potentially important for organisms. Temperate ectotherms may be adapted to the seasonal fluctuations in environmental traits. For lizards, behavioural adaptations regarding microhabitat selection could arise to improve thermoregulation during the different seasons. However, little is still known about which traits influence microhabitat selection of lizards and their adaptation to seasonality. Here we used Podarcis guadarramae to study the role of potential intrinsic (body size, sex, age) and environmental traits (<span class="hlt">air</span> and substrate <span class="hlt">temperatures</span>, <span class="hlt">wind</span> speed, and sunlight) in the seasonal changes of body <span class="hlt">temperatures</span> and microhabitat selection of lizards. We measured body <span class="hlt">temperatures</span> of lizards in the same habitat during the four seasons and compared the climatic variables of the microhabitats selected by lizards with the mean climatic conditions available in their habitat. Body <span class="hlt">temperatures</span> were similar for adult males, adult females, and juveniles within each season, being significantly higher in summer than in the other seasons, and in spring than in winter. The same pattern was found regarding substrate and <span class="hlt">air</span> <span class="hlt">temperatures</span> of the selected microhabitats. <span class="hlt">Wind</span> speed and <span class="hlt">air</span> <span class="hlt">temperature</span> did not affect body <span class="hlt">temperatures</span>, while body length was marginally significant and substrate <span class="hlt">temperatures</span> and season did affect the body <span class="hlt">temperatures</span> of lizards. Our results during the whole year support the idea that the seasonality could be the most important factor affecting body <span class="hlt">temperatures</span> of these temperate species. Regarding microhabitat selection, environmental constraints, as environmental <span class="hlt">temperatures</span> and <span class="hlt">wind</span> speed, affected the seasonal changes on behavioural thermoregulation of lizards. This effect was similar between sexes and age classes, and was independent of body size. In addition, importance of sunlight exposure of the selected microhabitats (full sun, filtered sun, or shade) also</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720017686','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720017686"><span>Atmospheric pressure, density, <span class="hlt">temperature</span> and <span class="hlt">wind</span> variations between 50 and 200 km</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Justus, C. G.; Woodrum, A.</p> <p>1972-01-01</p> <p>Data on atmospheric pressure, density, <span class="hlt">temperature</span> and <span class="hlt">winds</span> between 50 and 200 km were collected from sources including Meteorological Rocket Network data, ROBIN falling sphere data, grenade release and pitot tube data, meteor <span class="hlt">winds</span>, chemical release <span class="hlt">winds</span>, satellite data, and others. These data were analyzed by a daily difference method and results on the distribution statistics, magnitude, and spatial structure of the irregular atmospheric variations are presented. Time structures of the irregular variations were determined by the analysis of residuals from harmonic analysis of time series data. The observed height variations of irregular <span class="hlt">winds</span> and densities are found to be in accord with a theoretical relation between these two quantities. The latitude variations (at 50 - 60 km height) show an increasing trend with latitude. A possible explanation of the unusually large irregular <span class="hlt">wind</span> magnitudes of the White Sands MRN data is given in terms of mountain wave generation by the Sierra Nevada range about 1000 km west of White Sands. An analytical method is developed which, based on an analogy of the irregular motion field with axisymmetric turbulence, allows measured or model correlation or structure functions to be used to evaluate the effective frequency spectra of scalar and vector quantities of a spacecraft moving at any speed and at any trajectory elevation angle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC53F1258R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC53F1258R"><span>Surface <span class="hlt">Temperature</span> variability from <span class="hlt">AIRS</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ruzmaikin, A.; Dang, V. T.; Aumann, H. H.</p> <p>2015-12-01</p> <p>To address the existence and possible causes of the climate hiatus in the Earth's global <span class="hlt">temperature</span> we investigate the trends and variability in the surface <span class="hlt">temperature</span> using retrievals obtained from the measurements by the Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) and its companion instrument, the Advanced Microwave Sounding Unit (AMSU), onboard of Aqua spacecraft in 2002-2014for the day and night conditions. The data used are L3 monthly means on a 1x1degree spatial grid. We separate the land and ocean <span class="hlt">temperatures</span>, as well as <span class="hlt">temperatures</span> in Artic, Antarctic and desert regions. We compare the satellite data with the new surface data produced by Karl et al. (2015) who denies the reality of the climate hiatus. The difference in the regional trends can help to explain why the global surface <span class="hlt">temperature</span> remains almost unchanged but the frequency of occurrence of the extreme events increases under rising anthropogenic forcing. The day-night difference is an indicator of the anthropogenic trend. This work was supported by the Jet Propulsion Laboratory of the California Institute of Technology, under a contract with the National Aeronautics and Space Administration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930081405','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930081405"><span>Compression-ignition Engine Performance at Altitudes and at Various <span class="hlt">Air</span> Pressures and <span class="hlt">Temperatures</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moore, Charles S; Collins, John H</p> <p>1937-01-01</p> <p>Engine test results are presented for simulated altitude conditions. A displaced-piston combustion chamber on a 5- by 7-inch single cylinder compression-ignition engine operating at 2,000 r.p.m. was used. Inlet <span class="hlt">air</span> <span class="hlt">temperature</span> equivalent to standard altitudes up to 14,000 feet were obtained. Comparison between performance at altitude of the unsupercharged compression-ignition engine compared favorably with the carburetor engine. Analysis of the results for which the inlet <span class="hlt">air</span> <span class="hlt">temperature</span>, inlet <span class="hlt">air</span> pressure, and inlet and exhaust pressure were varied indicates that engine performance cannot be reliably corrected on the basis of inlet <span class="hlt">air</span> density or weight of <span class="hlt">air</span> charge. Engine power increases with inlet <span class="hlt">air</span> pressure and decreases with inlet <span class="hlt">air</span> <span class="hlt">temperatures</span> very nearly as straight line relations over a wide range of <span class="hlt">air</span>-fuel ratios. Correction factors are given.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.2999A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.2999A"><span>Extraction of <span class="hlt">wind</span> and <span class="hlt">temperature</span> information from hybrid 4D-Var assimilation of stratospheric ozone using NAVGEM</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Allen, Douglas R.; Hoppel, Karl W.; Kuhl, David D.</p> <p>2018-03-01</p> <p>Extraction of <span class="hlt">wind</span> and <span class="hlt">temperature</span> information from stratospheric ozone assimilation is examined within the context of the Navy Global Environmental Model (NAVGEM) hybrid 4-D variational assimilation (4D-Var) data assimilation (DA) system. Ozone can improve the <span class="hlt">wind</span> and <span class="hlt">temperature</span> through two different DA mechanisms: (1) through the <q>flow-of-the-day</q> ensemble background error covariance that is blended together with the static background error covariance and (2) via the ozone continuity equation in the tangent linear model and adjoint used for minimizing the cost function. All experiments assimilate actual conventional data in order to maintain a similar realistic troposphere. In the stratosphere, the experiments assimilate simulated ozone and/or radiance observations in various combinations. The simulated observations are constructed for a case study based on a 16-day cycling truth experiment (TE), which is an analysis with no stratospheric observations. The impact of ozone on the analysis is evaluated by comparing the experiments to the TE for the last 6 days, allowing for a 10-day spin-up. Ozone assimilation benefits the <span class="hlt">wind</span> and <span class="hlt">temperature</span> when data are of sufficient quality and frequency. For example, assimilation of perfect (no applied error) global hourly ozone data constrains the stratospheric <span class="hlt">wind</span> and <span class="hlt">temperature</span> to within ˜ 2 m s-1 and ˜ 1 K. This demonstrates that there is dynamical information in the ozone distribution that can potentially be used to improve the stratosphere. This is particularly important for the tropics, where radiance observations have difficulty constraining <span class="hlt">wind</span> due to breakdown of geostrophic balance. Global ozone assimilation provides the largest benefit when the hybrid blending coefficient is an intermediate value (0.5 was used in this study), rather than 0.0 (no ensemble background error covariance) or 1.0 (no static background error covariance), which is consistent with other hybrid DA studies. When perfect global</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AdAtS..31.1127L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AdAtS..31.1127L"><span>Mapping near-surface <span class="hlt">air</span> <span class="hlt">temperature</span>, pressure, relative humidity and <span class="hlt">wind</span> speed over Mainland China with high spatiotemporal resolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Tao; Zheng, Xiaogu; Dai, Yongjiu; Yang, Chi; Chen, Zhuoqi; Zhang, Shupeng; Wu, Guocan; Wang, Zhonglei; Huang, Chengcheng; Shen, Yan; Liao, Rongwei</p> <p>2014-09-01</p> <p>As part of a joint effort to construct an atmospheric forcing dataset for mainland China with high spatiotemporal resolution, a new approach is proposed to construct gridded near-surface <span class="hlt">temperature</span>, relative humidity, <span class="hlt">wind</span> speed and surface pressure with a resolution of 1 km×1 km. The approach comprises two steps: (1) fit a partial thin-plate smoothing spline with orography and reanalysis data as explanatory variables to ground-based observations for estimating a trend surface; (2) apply a simple kriging procedure to the residual for trend surface correction. The proposed approach is applied to observations collected at approximately 700 stations over mainland China. The generated forcing fields are compared with the corresponding components of the National Centers for Environmental Prediction (NCEP) Climate Forecast System Reanalysis dataset and the Princeton meteorological forcing dataset. The comparison shows that, both within the station network and within the resolutions of the two gridded datasets, the interpolation errors of the proposed approach are markedly smaller than the two gridded datasets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25321553','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25321553"><span>Stratospheric <span class="hlt">temperature</span> measurement with scanning Fabry-Perot interferometer for <span class="hlt">wind</span> retrieval from mobile Rayleigh Doppler lidar.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xia, Haiyun; Dou, Xiankang; Shangguan, Mingjia; Zhao, Ruocan; Sun, Dongsong; Wang, Chong; Qiu, Jiawei; Shu, Zhifeng; Xue, Xianghui; Han, Yuli; Han, Yan</p> <p>2014-09-08</p> <p><span class="hlt">Temperature</span> detection remains challenging in the low stratosphere, where the Rayleigh integration lidar is perturbed by aerosol contamination and ozone absorption while the rotational Raman lidar is suffered from its low scattering cross section. To correct the impacts of <span class="hlt">temperature</span> on the Rayleigh Doppler lidar, a high spectral resolution lidar (HSRL) based on cavity scanning Fabry-Perot Interferometer (FPI) is developed. By considering the effect of the laser spectral width, Doppler broadening of the molecular backscatter, divergence of the light beam and mirror defects of the FPI, a well-behaved transmission function is proved to show the principle of HSRL in detail. Analysis of the statistical error of the HSRL is carried out in the data processing. A <span class="hlt">temperature</span> lidar using both HSRL and Rayleigh integration techniques is incorporated into the Rayleigh Doppler <span class="hlt">wind</span> lidar. Simultaneous <span class="hlt">wind</span> and <span class="hlt">temperature</span> detection is carried out based on the combined system at Delhi (37.371°N, 97.374°E; 2850 m above the sea level) in Qinghai province, China. Lower Stratosphere <span class="hlt">temperature</span> has been measured using HSRL between 18 and 50 km with temporal resolution of 2000 seconds. The statistical error of the derived <span class="hlt">temperatures</span> is between 0.2 and 9.2 K. The <span class="hlt">temperature</span> profile retrieved from the HSRL and <span class="hlt">wind</span> profile from the Rayleigh Doppler lidar show good agreement with the radiosonde data. Specifically, the max <span class="hlt">temperature</span> deviation between the HSRL and radiosonde is 4.7 K from 18 km to 36 km, and it is 2.7 K between the HSRL and Rayleigh integration lidar from 27 km to 34 km.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170002321&hterms=spectroscopy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dspectroscopy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170002321&hterms=spectroscopy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dspectroscopy"><span>Seasonal Variability of Saturn's Tropospheric <span class="hlt">Temperatures</span>, <span class="hlt">Winds</span> and Para-H2 from Cassini Far-IR Spectroscopy</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fletcher, Leigh N.; Irwin, P. G. J; Achterberg, R. K.; Orton, G. S.; Flasar, F. M.</p> <p>2015-01-01</p> <p>Far-IR 16-1000 micrometer spectra of Saturn's hydrogen-helium continuum measured by Cassini's Composite Infrared Spectrometer (CIRS) are inverted to construct a near-continuous record of upper tropospheric (70-700 mbar) <span class="hlt">temperatures</span> and para-H2 fraction as a function of latitude, pressure and time for a third of a saturnian year (2004-2014, from northern winter to northern spring). The thermal field reveals evidence of reversing summertime asymmetries superimposed onto the belt/zone structure. The <span class="hlt">temperature</span> structure is almost symmetric about the equator by 2014, with seasonal lag times that increase with depth and are qualitatively consistent with radiative climate models. Localised heating of the tropospheric hazes (100-250 mbar) create a distinct perturbation to the <span class="hlt">temperature</span> profile that shifts in magnitude and location, declining in the autumn hemisphere and growing in the spring. Changes in the para-H2 (f(sub p)) distribution are subtle, with a 0.02-0.03 rise over the spring hemisphere (200-500 mbar) perturbed by (i) low-f(sub p) <span class="hlt">air</span> advected by both the springtime storm of 2010 and equatorial upwelling; and (ii) subsidence of high-f(sub p) <span class="hlt">air</span> at northern high latitudes, responsible for a developing north-south asymmetry in f(sub p). Conversely, the shifting asymmetry in the para-H2 disequilibrium primarily reflects the changing <span class="hlt">temperature</span> structure (and hence the equilibrium distribution of f(sub p)), rather than actual changes in f(sub p) induced by chemical conversion or transport. CIRS results interpolated to the same point in the seasonal cycle as re-analysed Voyager-1 observations (early northern spring) show qualitative consistency from year to year (i.e., the same tropospheric asymmetries in <span class="hlt">temperature</span> and f(sub p)), with the exception of the tropical tropopause near the equatorial zones and belts, where downward propagation of a cool <span class="hlt">temperature</span> anomaly associated with Saturn's stratospheric oscillation could potentially perturb tropopause</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9789L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9789L"><span>Influence of <span class="hlt">air</span> <span class="hlt">temperature</span> on electric consumption in Moscow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lokoshchenko, Mikhail A.; Nikolayeva, Nataliya A.</p> <p>2017-04-01</p> <p>For the first time for mid latitudes and with the use of long-term data of Moscow State University Meteorological observatory a dependence of electric power consumption E on the <span class="hlt">air</span> <span class="hlt">temperature</span> T has been studied for each separate day for the period from 1990 to 2015 (totally - 9496 values). As a result, it is shown that the relation is in general decreasing in conditions of cold Moscow region: energy consumption as a rule reduces with a rise of the <span class="hlt">temperature</span>. However, in time of severe frosts the energy consumption increasing goes to nothing due to special measures for energy savings whereas during heat wave episodes of extremely hot weather (especially in summer of 2010) an opposite tendency appears to the energy consumption increase with the increase of the <span class="hlt">air</span> <span class="hlt">temperature</span> due to additional consumption for the <span class="hlt">air</span> conditioning. This relation between E and T is statistically significant with extremely high confidence probability (more than 0.999). The optimum <span class="hlt">temperature</span> for the energy saving is 18 ˚C. The <span class="hlt">air</span> <span class="hlt">temperature</span> limit values in Moscow during last decades have been discussed. Daily-averaged T varied from -28.0 ˚C in January of 2006 to +31.4 ˚C in August of 2010 so a range of this parameter is almost 60 ˚C. Catastrophic heat wave in 2010 appeared as a secondary summer maximum of the electric consumption annual course. The relation between E and T for separate years demonstrates strong weekly periodicity at the dynamics of E daily values. As a result statistical distribution of E daily values for separate years is bimodal. One its mode is connected with working-days and another one - with non-work days (Saturday, Sunday and holidays) when consumption is much less. In recent time weekly cycle at the electric consumption became weaker due to total fall of industry in Moscow. In recent years the dependence of energy consumption on the <span class="hlt">air</span> <span class="hlt">temperature</span> generally became stronger - probably due to changes of its structure (growth of non-industrial users</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApJS..236...41W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApJS..236...41W"><span>The Statistical Properties of Solar <span class="hlt">Wind</span> <span class="hlt">Temperature</span> Parameters Near 1 au</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, Lynn B., III; Stevens, Michael L.; Kasper, Justin C.; Klein, Kristopher G.; Maruca, Bennett A.; Bale, Stuart D.; Bowen, Trevor A.; Pulupa, Marc P.; Salem, Chadi S.</p> <p>2018-06-01</p> <p>We present a long-duration (∼10 yr) statistical analysis of the <span class="hlt">temperatures</span>, plasma betas, and <span class="hlt">temperature</span> ratios for the electron, proton, and alpha-particle populations observed by the <span class="hlt">Wind</span> spacecraft near 1 au. The mean(median) scalar <span class="hlt">temperatures</span> are T e,tot = 12.2(11.9) eV, T p,tot = 12.7(8.6) eV, and T α,tot = 23.9(10.8) eV. The mean(median) total plasma betas are β e,tot = 2.31(1.09), β p,tot = 1.79(1.05), and β α,tot = 0.17(0.05). The mean(median) <span class="hlt">temperature</span> ratios are (T e /T p )tot = 1.64(1.27), (T e /T α )tot = 1.24(0.82), and (T α /T p )tot = 2.50(1.94). We also examined these parameters during time intervals that exclude interplanetary (IP) shocks, times within the magnetic obstacles (MOs) of interplanetary coronal mass ejections (ICMEs), and times that exclude MOs. The only times that show significant alterations to any of the parameters examined are those during MOs. In fact, the only parameter that does not show a significant change during MOs is the electron <span class="hlt">temperature</span>. Although each parameter shows a broad range of values, the vast majority are near the median. We also compute particle–particle collision rates and compare to effective wave–particle collision rates. We find that, for reasonable assumptions of wave amplitude and occurrence rates, the effect of wave–particle interactions on the plasma is equal to or greater than the effect of Coulomb collisions. Thus, wave–particle interactions should not be neglected when modeling the solar <span class="hlt">wind</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_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.8034B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.8034B"><span><span class="hlt">Wind</span> Speed and Sea State Dependencies of <span class="hlt">Air</span>-Sea Gas Transfer: Results From the High <span class="hlt">Wind</span> Speed Gas Exchange Study (HiWinGS)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blomquist, B. W.; Brumer, S. E.; Fairall, C. W.; Huebert, B. J.; Zappa, C. J.; Brooks, I. M.; Yang, M.; Bariteau, L.; Prytherch, J.; Hare, J. E.; Czerski, H.; Matei, A.; Pascal, R. W.</p> <p>2017-10-01</p> <p>A variety of physical mechanisms are jointly responsible for facilitating <span class="hlt">air</span>-sea gas transfer through turbulent processes at the atmosphere-ocean interface. The nature and relative importance of these mechanisms evolves with increasing <span class="hlt">wind</span> speed. Theoretical and modeling approaches are advancing, but the limited quantity of observational data at high <span class="hlt">wind</span> speeds hinders the assessment of these efforts. The HiWinGS project successfully measured gas transfer coefficients (k660) with coincident wave statistics under conditions with hourly mean <span class="hlt">wind</span> speeds up to 24 m s-1 and significant wave heights to 8 m. Measurements of k660 for carbon dioxide (CO2) and dimethylsulfide (DMS) show an increasing trend with respect to 10 m neutral <span class="hlt">wind</span> speed (U10N), following a power law relationship of the form: k660 CO2˜U10N1.68 and k660 dms˜U10N1.33. Among seven high <span class="hlt">wind</span> speed events, CO2 transfer responded to the intensity of wave breaking, which depended on both <span class="hlt">wind</span> speed and sea state in a complex manner, with k660 CO2 increasing as the <span class="hlt">wind</span> sea approaches full development. A similar response is not observed for DMS. These results confirm the importance of breaking waves and bubble injection mechanisms in facilitating CO2 transfer. A modified version of the Coupled Ocean-Atmosphere Response Experiment Gas transfer algorithm (COAREG ver. 3.5), incorporating a sea state-dependent calculation of bubble-mediated transfer, successfully reproduces the mean trend in observed k660 with <span class="hlt">wind</span> speed for both gases. Significant suppression of gas transfer by large waves was not observed during HiWinGS, in contrast to results from two prior field programs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.6124F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.6124F"><span><span class="hlt">Air</span> and ground <span class="hlt">temperatures</span> along elevation and continentality gradients in Southern Norway</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farbrot, Herman; Hipp, Tobias; Etzelmüller, Bernd; Humlum, Ole; Isaksen, Ketil; Strand Ødegârd, Rune</p> <p>2010-05-01</p> <p>The modern southern boundary for Scandinavian permafrost is located in the mountains of Southern Norway. Permafrost and seasonal frost are considered key components of the cryosphere, and the climate-permafrost relation has acquired added importance with the increasing awareness and concern of rising <span class="hlt">air</span> <span class="hlt">temperatures</span>. The three-year research project CRYOLINK ("Permafrost and seasonal frost in southern Norway") aims at improving knowledge on past and present ground <span class="hlt">temperatures</span>, seasonal frost, and distribution of mountain permafrost in Southern Norway by addressing the fundamental problem of heat transfer between the atmosphere and the ground surface. Hence, several shallow boreholes have been drilled, and a monitoring program to measure <span class="hlt">air</span> and ground <span class="hlt">temperatures</span> was started August 2008. The borehole areas (Juvvass, Jetta and Tron) are situated along a west-east transect and, hence, a continentality gradient, and each area provides boreholes at different elevations. Here we present the first year of <span class="hlt">air</span> and ground <span class="hlt">temperatures</span> from these sites and discuss the influence of <span class="hlt">air</span> <span class="hlt">temperature</span> and ground surface charcteristics (snow conditions, sediments/bedrock, vegetation) on ground <span class="hlt">temperatures</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913259W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913259W"><span>Synoptic versus regional causes of icing on <span class="hlt">wind</span> turbines at an exposed <span class="hlt">wind</span> farm site in Germany</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weissinger, Maximilian; Strauss, Lukas; Serafin, Stefano; Dorninger, Manfred; Burchhart, Thomas; Fink, Martin</p> <p>2017-04-01</p> <p>Ice accretion on <span class="hlt">wind</span> turbine blades can lead to significant power production loss or even permanent structural damage on the turbine. With the ongoing construction of <span class="hlt">wind</span> 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 <span class="hlt">wind</span> turbine blades. The project focuses on a <span class="hlt">wind</span> 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 <span class="hlt">wind</span> turbines on top of the highest hills. The present study aims to investigate historical cases of <span class="hlt">wind</span> turbine icing and their meteorological causes at the Ellern <span class="hlt">wind</span> farm. The data available consists of a three-year period (2013-2016) of operational data from the Ellern <span class="hlt">wind</span> 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 <span class="hlt">air</span> 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 <span class="hlt">temperature</span> 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 <span class="hlt">air</span> masses to Central</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830046452&hterms=water+gas+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dwater%2Bgas%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830046452&hterms=water+gas+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dwater%2Bgas%2Bexchange"><span>Methane flux across the <span class="hlt">air</span>-water interface - <span class="hlt">Air</span> velocity effects</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sebacher, D. I.; Harriss, R. C.; Bartlett, K. B.</p> <p>1983-01-01</p> <p>Methane loss to the atmosphere from flooded wetlands is influenced by the degree of supersaturation and <span class="hlt">wind</span> stress at the water surface. Measurements in freshwater ponds in the St. Marks Wildlife Refuge, Florida, demonstrated that for the combined variability of CH4 concentrations in surface water and <span class="hlt">air</span> velocity over the water surface, CH4 flux varied from 0.01 to 1.22 g/sq m/day. The liquid exchange coefficient for a two-layer model of the gas-liquid interface was calculated as 1.7 cm/h for CH4 at <span class="hlt">air</span> velocity of zero and as 1.1 + 1.2 v to the 1.96th power cm/h for <span class="hlt">air</span> velocities from 1.4 to 3.5 m/s and water <span class="hlt">temperatures</span> of 20 C.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JMetR..32..288S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JMetR..32..288S"><span>Oscillation of Surface PM2.5 Concentration Resulting from an Alternation of Easterly and Southerly <span class="hlt">Winds</span> in Beijing: Mechanisms and Implications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, Zhaobin; Zhang, Xiaoling; Zhao, Xiujuan; Xia, Xiangao; Miao, Shiguang; Li, Ziming; Cheng, Zhigang; Wen, Wei; Tang, Yixi</p> <p>2018-04-01</p> <p>We used simultaneous measurements of surface PM2.5 concentration and vertical profiles of aerosol concentration, <span class="hlt">temperature</span>, and humidity, together with regional <span class="hlt">air</span> quality model simulations, to study an episode of aerosol pollution in Beijing from 15 to 19 November 2016. The potential effects of easterly and southerly <span class="hlt">winds</span> on the surface concentrations and vertical profiles of the PM2.5 pollution were investigated. Favorable easterly <span class="hlt">winds</span> produced strong upward motion and were able to transport the PM2.5 pollution at the surface to the upper levels of the atmosphere. The amount of surface PM2.5 pollution transported by the easterly <span class="hlt">winds</span> was determined by the strength and height of the upward motion produced by the easterly <span class="hlt">winds</span> and the initial height of the upward <span class="hlt">wind</span>. A greater amount of PM2.5 pollution was transported to upper levels of the atmosphere by upward <span class="hlt">winds</span> with a lower initial height. The pollutants were diluted by easterly <span class="hlt">winds</span> from clean ocean <span class="hlt">air</span> masses. The inversion layer was destroyed by the easterly <span class="hlt">winds</span> and the surface pollutants and warm <span class="hlt">air</span> masses were then lifted to the upper levels of the atmosphere, where they re-established a multi-layer inversion. This region of inversion was strengthened by the southerly <span class="hlt">winds</span>, increasing the severity of pollution. A vortex was produced by southerly <span class="hlt">winds</span> that led to the convergence of <span class="hlt">air</span> along the Taihang Mountains. Pollutants were transported from southern-central Hebei Province to Beijing in the boundary layer. Warm advection associated with the southerly <span class="hlt">winds</span> intensified the inversion produced by the easterly <span class="hlt">winds</span> and a more stable boundary layer was formed. The layer with high PM2.5 concentration became dee-per with persistent southerly <span class="hlt">winds</span> of a certain depth. The polluted <span class="hlt">air</span> masses then rose over the northern Taihang Mountains to the northern mountainous regions of Hebei Province.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp...41C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp...41C"><span>Mechanisms of the intensification of the upwelling-favorable <span class="hlt">winds</span> during El Niño 1997-1998 in the Peruvian upwelling system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chamorro, Adolfo; Echevin, Vincent; Colas, François; Oerder, Vera; Tam, Jorge; Quispe-Ccalluari, Carlos</p> <p>2018-01-01</p> <p>The physical processes driving the <span class="hlt">wind</span> intensification in a coastal band of 100 km off Peru during the intense 1997-1998 El Niño (EN) event were studied using a regional atmospheric model. A simulation performed for the period 1994-2000 reproduced the coastal <span class="hlt">wind</span> response to local sea surface <span class="hlt">temperature</span> (SST) forcing and large scale atmospheric conditions. The model, evaluated with satellite data, represented well the intensity, seasonal and interannual variability of alongshore (i.e. NW-SE) <span class="hlt">winds</span>. An alongshore momentum budget showed that the pressure gradient was the dominant force driving the surface <span class="hlt">wind</span> acceleration. The pressure gradient tended to accelerate the coastal <span class="hlt">wind</span>, while turbulent vertical mixing decelerated it. A quasi-linear relation between surface <span class="hlt">wind</span> and pressure gradient anomalies was found. Alongshore pressure gradient anomalies were caused by a greater increase in near-surface <span class="hlt">air</span> <span class="hlt">temperature</span> off the northern coast than off the southern coast, associated with the inhomogeneous SST warming. Vertical profiles of <span class="hlt">wind</span>, mixing coefficient, and momentum trends showed that the surface <span class="hlt">wind</span> intensification was not caused by the increase of turbulence in the planetary boundary layer. Moreover, the <span class="hlt">temperature</span> inversion in the vertical mitigated the development of pressure gradient due to <span class="hlt">air</span> convection during part of the event. Sensitivity experiments allowed to isolate the respective impacts of the local SST forcing and large scale condition on the coastal <span class="hlt">wind</span> intensification. It was primarily driven by the local SST forcing whereas large scale variability associated with the South Pacific Anticyclone modulated its effects. Examination of other EN events using reanalysis data confirmed that intensifications of alongshore <span class="hlt">wind</span> off Peru were associated with SST alongshore gradient anomalies, as during the 1997-1998 event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28147294','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28147294"><span>Identifying anthropogenic anomalies in <span class="hlt">air</span>, surface and groundwater <span class="hlt">temperatures</span> in Germany.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Benz, Susanne A; Bayer, Peter; Blum, Philipp</p> <p>2017-04-15</p> <p>Human activity directly influences ambient <span class="hlt">air</span>, surface and groundwater <span class="hlt">temperatures</span>. The most prominent phenomenon is the urban heat island effect, which has been investigated particularly in large and densely populated cities. This study explores the anthropogenic impact on the thermal regime not only in selected urban areas, but on a countrywide scale for mean annual <span class="hlt">temperature</span> datasets in Germany in three different compartments: measured surface <span class="hlt">air</span> <span class="hlt">temperature</span>, measured groundwater <span class="hlt">temperature</span>, and satellite-derived land surface <span class="hlt">temperature</span>. Taking nighttime lights as an indicator of rural areas, the anthropogenic heat intensity is introduced. It is applicable to each data set and provides the difference between measured local <span class="hlt">temperature</span> and median rural background <span class="hlt">temperature</span>. This concept is analogous to the well-established urban heat island intensity, but applicable to each measurement point or pixel of a large, even global, study area. For all three analyzed <span class="hlt">temperature</span> datasets, anthropogenic heat intensity grows with increasing nighttime lights and declines with increasing vegetation, whereas population density has only minor effects. While surface anthropogenic heat intensity cannot be linked to specific land cover types in the studied resolution (1km×1km) and classification system, both <span class="hlt">air</span> and groundwater show increased heat intensities for artificial surfaces. Overall, groundwater <span class="hlt">temperature</span> appears most vulnerable to human activity, albeit the different compartments are partially influenced through unrelated processes; unlike land surface <span class="hlt">temperature</span> and surface <span class="hlt">air</span> <span class="hlt">temperature</span>, groundwater <span class="hlt">temperatures</span> are elevated in cultivated areas as well. At the surface of Germany, the highest anthropogenic heat intensity with 4.5K is found at an open-pit lignite mine near Jülich, followed by three large cities (Munich, Düsseldorf and Nuremberg) with annual mean anthropogenic heat intensities >4K. Overall, surface anthropogenic heat intensities >0K and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020090258','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020090258"><span>The Breath of Planet Earth: Atmospheric Circulation. Assimilation of Surface <span class="hlt">Wind</span> Observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Atlas, Robert; Bloom, Stephen; Otterman, Joseph</p> <p>2000-01-01</p> <p>Differences in <span class="hlt">air</span> pressure are a major cause of atmospheric circulation. Because heat excites the movement of atoms, warm <span class="hlt">temperatures</span> cause, <span class="hlt">air</span> molecules to expand. Because those molecules now occupy a larger space, the pressure that their weight exerts is decreased. <span class="hlt">Air</span> from surrounding high-pressure areas is pushed toward the low-pressure areas, creating circulation. This process causes a major pattern of global atmosphere movement known as meridional circulation. In this form of convection, or vertical <span class="hlt">air</span> movement, heated equatorial <span class="hlt">air</span> rises and travels through the upper atmosphere toward higher latitudes. <span class="hlt">Air</span> just above the equator heads toward the North Pole, and <span class="hlt">air</span> just below the equator moves southward. This <span class="hlt">air</span> movement fills the gap created where increased <span class="hlt">air</span> pressure pushes down cold <span class="hlt">air</span>. The ,cold <span class="hlt">air</span> moves along the surface back toward the equator, replacing the <span class="hlt">air</span> masses that rise there. Another influence on atmospheric. circulation is the Coriolis force. Because of the Earth's rotation, large-scale <span class="hlt">wind</span> currents move in the direction of this axial spin around low-pressure areas. <span class="hlt">Wind</span> rotates counterclockwise in the Northern Hemisphere and clockwise in the Southern Hemisphere. just as the Earth's rotation affects airflow, so too does its surface. In the phenomenon of orographic lifting, elevated topographic features such as mountain ranges lift <span class="hlt">air</span> as it moves up their surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4568288','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4568288"><span>Reminiscences on the study of <span class="hlt">wind</span> waves</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>MITSUYASU, Hisashi</p> <p>2015-01-01</p> <p>The <span class="hlt">wind</span> blowing over sea surface generates tiny <span class="hlt">wind</span> waves. They develop with time and space absorbing <span class="hlt">wind</span> energy, and become huge <span class="hlt">wind</span> waves usually referred to ocean surface waves. The <span class="hlt">wind</span> waves cause not only serious sea disasters but also take important roles in the local and global climate changes by affecting the fluxes of momentum, heat and gases (e.g. CO2) through the <span class="hlt">air</span>-sea boundary. The present paper reviews the selected studies on <span class="hlt">wind</span> waves conducted by our group in the Research Institute for Applied Mechanics (RIAM), Kyushu University. The themes discussed are interactions between water waves and <span class="hlt">winds</span>, the energy spectrum of <span class="hlt">wind</span> waves, nonlinear properties of <span class="hlt">wind</span> waves, and the effects of surfactant on some <span class="hlt">air</span>-sea interaction phenomena. PMID:25864467</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25864467','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25864467"><span>Reminiscences on the study of <span class="hlt">wind</span> waves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mitsuyasu, Hisashi</p> <p>2015-01-01</p> <p>The <span class="hlt">wind</span> blowing over sea surface generates tiny <span class="hlt">wind</span> waves. They develop with time and space absorbing <span class="hlt">wind</span> energy, and become huge <span class="hlt">wind</span> waves usually referred to ocean surface waves. The <span class="hlt">wind</span> waves cause not only serious sea disasters but also take important roles in the local and global climate changes by affecting the fluxes of momentum, heat and gases (e.g. CO2) through the <span class="hlt">air</span>-sea boundary. The present paper reviews the selected studies on <span class="hlt">wind</span> waves conducted by our group in the Research Institute for Applied Mechanics (RIAM), Kyushu University. The themes discussed are interactions between water waves and <span class="hlt">winds</span>, the energy spectrum of <span class="hlt">wind</span> waves, nonlinear properties of <span class="hlt">wind</span> waves, and the effects of surfactant on some <span class="hlt">air</span>-sea interaction phenomena.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1211638S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1211638S"><span><span class="hlt">Winds</span> and <span class="hlt">Temperatures</span> in Venus Upper Atmosphere from High-Resolution Infrared Heterodyne Spectroscopy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sornig, Manuela; Sonnabend, Guido; Krötz, Peter; Stupar, Dusan</p> <p>2010-05-01</p> <p>Narrow non-LTE emission lines of CO2 at 10μm are induced by solar radiation in Venus upper atmosphere. Measurements of fully resolved emission lines can be used to probe the emitting regions of the atmosphere for <span class="hlt">winds</span> and tempertaures. Using infrared heterodyne spectroscopy kinetic <span class="hlt">temperatures</span> with a precision of 5 K can be calculated from the width of emission lines and <span class="hlt">wind</span> velocities can be determined from Doppler-shifts of emission lines with a precision up to 10 m/s. The non-LTE emission can only occur within a narrow pressure/altitude region around 110 km. At the I.Physikalisches Instiut of the University of Cologne we developed a Tunable Infrared Heterodyne Spectrometer (THIS) capable of accomplishing such ground-based measurements of planetary atmospheres. Beside high spectral resolution (R>107) infrared observations also provide high spatial resolution on the planet. Over the last two years we observed <span class="hlt">wind</span> velocities and <span class="hlt">temperatures</span> at several characteristic orbital positions of Venus using the McMath-Pierce-Solar Telescope on Kitt Peak, Arizona, USA. This telescope provides a field-of-view of 1.7 arcsec on an apparent diameter of Venus of approximately 20-60 arcsec. New observations close to inferior conjunction have been accomplished in March and in April 2009 An additional observing run took place in June 2009 at maximum western elongation. These observing geometries allow investigations of <span class="hlt">wind</span> velocities of different combinations of the superrotational component and the subsolar-antisolar (SS-AS) flow component. Due to the observing geometry during the March and April runs we focused on SS-AS flow. <span class="hlt">Wind</span> velocities around 140 m/s were found decreasing significantly at high latitudes. No significant superrotational component could be observed and the variability between these two runs was moderate. Data analysis for the run in June 2009 addressing mainly the superrotational component is still in progress. Retrieved <span class="hlt">temperatures</span> from all three</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/caa-permitting/application-documents-cape-wind-associates-llc-horseshoe-shoal-nantucket-sound','PESTICIDES'); return false;" href="https://www.epa.gov/caa-permitting/application-documents-cape-wind-associates-llc-horseshoe-shoal-nantucket-sound"><span>Application Documents for the Cape <span class="hlt">Wind</span> Associates, LLC, Horseshoe Shoal, Nantucket Sound (Offshore Renewable Energy Project/OCS <span class="hlt">Air</span> Permit)</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>List of application documents for the Cape <span class="hlt">Wind</span> Associates, LLC, Horseshoe Shoal, Nantucket Sound (Offshore Renewable Energy Project/OCS <span class="hlt">Air</span> Permit: Massachusetts Plan Approval including nonattainment NSR Appendix A requirements).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15484742','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15484742"><span>Evaluation of a novel <span class="hlt">wind</span> tunnel for the measurement of the kinetics of odour emissions from piggery effluent.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sohn, J H; Smith, R; Yoong, E; Hudson, N; Kim, T I</p> <p>2004-01-01</p> <p>A novel laboratory <span class="hlt">wind</span> tunnel, with the capability to control factors such as <span class="hlt">air</span> flow-rate, was developed to measure the kinetics of odour emissions from liquid effluent. The tunnel allows the emission of odours and other volatiles under an atmospheric transport system similar to ambient conditions. Sensors for <span class="hlt">wind</span> speed, <span class="hlt">temperature</span> and humidity were installed and calibrated. To calibrate the <span class="hlt">wind</span> tunnel, trials were performed to determine the gas recovery efficiency under different <span class="hlt">air</span> flow-rates (ranging from 0.001 to 0.028m3/s) and gas supply rates (ranging from 2.5 to 10.0 L/min) using a standard CO gas mixture. The results have shown gas recovery efficiencies ranging from 61.7 to 106.8%, while the average result from the trials was 81.14%. From statistical analysis, it was observed that the highest, most reliable gas recovery efficiency of the tunnel was 88.9%. The values of <span class="hlt">air</span> flow-rate and gas supply rate corresponding to the highest gas recovery efficiency were 0.028 m3/s and 10.0 L/min respectively. This study suggested that the <span class="hlt">wind</span> tunnel would provide precise estimates of odour emission rate. However, the <span class="hlt">wind</span> tunnel needs to be calibrated to compensate for errors caused by different <span class="hlt">air</span> flow-rates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/11533','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/11533"><span>Surface <span class="hlt">air</span> <span class="hlt">temperature</span> in a maritime metropolitan region</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>J. D. McTaggart-Cowen; J. W. S. Young</p> <p>1977-01-01</p> <p>In investigations of the micrometeorology of any area, one of the basic parameters required is the spatial and temporal distribution of the surface <span class="hlt">air</span> <span class="hlt">temperature</span>. A mobile instrument mounted on an automobile was used for measuring <span class="hlt">temperatures</span> within the surface mixed layer. Details are presented of a case study at Saint John, New Brunswick, in a summer period. The...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/34092','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/34092"><span><span class="hlt">Air</span> pollution removal and <span class="hlt">temperature</span> reduction by Gainesville's urban forest</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Francisco Escobedo; Jennifer A. Seitz; Wayne Zipperer</p> <p>2009-01-01</p> <p>Poor <span class="hlt">air</span> quality is a common problem in many urban areas. It can lead to human health problems and reduced visibility, and it can impair the health of plants and wildlife. The urban forest can help improve <span class="hlt">air</span> quality by removing pollutants and by reducing <span class="hlt">air</span> <span class="hlt">temperature</span> through shading and transpiration. Trees also emit volatile...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001JApMe..40.1413V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001JApMe..40.1413V"><span>Daily <span class="hlt">Air</span> <span class="hlt">Temperature</span> and Electricity Load in Spain.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Valor, Enric; Meneu, Vicente; Caselles, Vicente</p> <p>2001-08-01</p> <p>Weather has a significant impact on different sectors of the economy. One of the most sensitive is the electricity market, because power demand is linked to several weather variables, mainly the <span class="hlt">air</span> <span class="hlt">temperature</span>. This work analyzes the relationship between electricity load and daily <span class="hlt">air</span> <span class="hlt">temperature</span> in Spain, using a population-weighted <span class="hlt">temperature</span> index. The electricity demand shows a significant trend due to socioeconomic factors, in addition to daily and monthly seasonal effects that have been taken into account to isolate the weather influence on electricity load. The results indicate that the relationship is nonlinear, showing a `comfort interval' of ±3°C around 18°C and two saturation points beyond which the electricity load no longer increases. The analysis has also revealed that the sensitivity of electricity load to daily <span class="hlt">air</span> <span class="hlt">temperature</span> has increased along time, in a higher degree for summer than for winter, although the sensitivity in the cold season is always more significant than in the warm season. Two different <span class="hlt">temperature</span>-derived variables that allow a better characterization of the observed relationship have been used: the heating and cooling degree-days. The regression of electricity data on them defines the heating and cooling demand functions, which show correlation coefficients of 0.79 and 0.87, and predicts electricity load with standard errors of estimate of ±4% and ±2%, respectively. The maximum elasticity of electricity demand is observed at 7 cooling degree-days and 9 heating degree-days, and the saturation points are reached at 11 cooling degree-days and 13 heating degree-days, respectively. These results are helpful in modeling electricity load behavior for predictive purposes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011RScI...82i4704Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011RScI...82i4704Z"><span>Static voltage distribution between turns of secondary <span class="hlt">winding</span> of <span class="hlt">air</span>-core spiral strip transformer and its application</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Hong-bo; Liu, Jin-liang; Cheng, Xin-bing; Zhang, Yu</p> <p>2011-09-01</p> <p>The static voltage distribution between <span class="hlt">winding</span> turns has great impact on output characteristics and lifetime of the <span class="hlt">air</span>-core spiral strip pulse transformer (ACSSPT). In this paper, <span class="hlt">winding</span> inductance was calculated by electromagnetic theory, so that the static voltage distribution between turns of secondary <span class="hlt">winding</span> of ACSSPT was analyzed conveniently. According to theoretical analysis, a voltage gradient because of the turn-to-turn capacitance was clearly noticeable across the ground turns. Simulation results of Pspice and CST EM Studio codes showed that the voltage distribution between turns of secondary <span class="hlt">winding</span> had linear increments from the output turn to the ground turn. In experiment, the difference in increased voltage between the ground turns and the output turns of a 20-turns secondary <span class="hlt">winding</span> is almost 50%, which is believed to be responsible for premature breakdown of the insulation, particularly between the ground turns. The experimental results demonstrated the theoretical analysis and simulation results, which had important value for stable and long lifetime ACSSPT design. A new ACSSPT with improved structure has been used successfully in intense electron beam accelerators steadily.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770003810','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770003810"><span><span class="hlt">Wind</span> measurement system</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cliff, W. C.; Huffaker, R. M.; Dahm, W. K.; Thomson, J. A. L.; Lawrence, T. R.; Krause, M. C.; Wilson, D. J. (Inventor)</p> <p>1976-01-01</p> <p>A system for remotely measuring vertical and horizontal <span class="hlt">winds</span> present in discrete volumes of <span class="hlt">air</span> at selected locations above the ground is described. A laser beam is optically focused in range by a telescope, and the output beam is conically scanned at an angle about a vertical axis. The backscatter, or reflected light, from the ambient particulates in a volume of <span class="hlt">air</span>, the focal volume, is detected for shifts in wavelength, and from these, horizontal and vertical <span class="hlt">wind</span> components are computed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ThEng..64..201B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ThEng..64..201B"><span>Estimation of efficiency of the heat supply system based on a boiler house and a <span class="hlt">wind</span> turbine in the northern environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bezhan, A. V.; Minin, V. A.</p> <p>2017-03-01</p> <p>This article describes a methodological approach to defining indoor <span class="hlt">air</span> <span class="hlt">temperature</span> in buildings heated by a power supply unit consisting of a boiler house and a <span class="hlt">wind</span>-driven power plant (WDPP). We discuss a heating option for a residential building in the windy conditions of Murmansk city. We proved that, during the periods of strong <span class="hlt">wind</span>, a WDPP can partially or fully satisfy the heat demand and sometimes even create a surplus of energy. During low <span class="hlt">wind</span> weather, almost all loads are handled by the boiler house. We considered a possibility to accumulate the surplus energy obtained from a WDPP during strong <span class="hlt">wind</span> by increasing the <span class="hlt">temperature</span> in the whole building up to 25°C and further using the accumulated heat during the lowwind period when indoor <span class="hlt">air</span> <span class="hlt">temperature</span> may fall below 20°C. This allows saving organic fuel in the boiler house. We demonstrated how indoor <span class="hlt">air</span> <span class="hlt">temperature</span> in the building may change throughout the year when using the surplus energy from the WDPP due to thermal storage capacitance of the building. We also provided the results of study, showing favorable energy-related effects of using a WDPP along with the boiler house. It was determined that engaging a WDPP in fulfilling the diagram of heating loads promotes the decrease in the boiler house's contribution to heat supply by 30 to 50%, and using the surplus energy from the WDPP and thermal storage capacitance of the building allows reducing the contribution of the boiler house by 5-15% more in certain months.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1893c0088S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1893c0088S"><span>Multi-hole pressure probes to <span class="hlt">wind</span> tunnel experiments and <span class="hlt">air</span> data systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shevchenko, A. M.; Shmakov, A. S.</p> <p>2017-10-01</p> <p>The problems to develop a multihole pressure system to measure flow angularity, Mach number and dynamic head for <span class="hlt">wind</span> tunnel experiments or <span class="hlt">air</span> data systems are discussed. A simple analytical model with separation of variables is derived for the multihole spherical pressure probe. The proposed model is uniform for small subsonic and supersonic speeds. An error analysis was performed. The error functions are obtained, allowing to estimate the influence of the Mach number, the pitch angle, the location of the pressure ports on the uncertainty of determining the flow parameters.</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/2011AGUFM.A53D..04M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.A53D..04M"><span>Nocturnal <span class="hlt">Air</span> Seiches in the Arizona Meteor Crater</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muschinski, A.; Fritts, D. C.; Zhong, S.; Oncley, S. P.</p> <p>2011-12-01</p> <p>The Arizona Meteor Crater near Winslow, AZ is 170 m deep, has a diameter of 1.2 km, and it has a nearly circular shape. The motivation of the Meteor Crater Experiment (METCRAX), conducted in October 2006, was to use the Meteor Crater as a natural laboratory to study atmospheric phenomena that are typical for small basins. Among other observations, high-resolution <span class="hlt">wind</span>, <span class="hlt">temperature</span> and pressure measurements were collected with sonics and microbarometers, respectively, during the entire month. The sensors were mounted between 0.5 m and 8.5 m AGL on seven portable towers, five of which were located within the crater and two on the crater rim. Here we report observations of nocturnal <span class="hlt">air</span> seiches, that is, standing gravity waves associated with the time-harmonic sloshing of the cold-<span class="hlt">air</span> pool that forms at the bottom of the crater due to radiative cooling at night. We present time series, spectra, and spectrograms of <span class="hlt">temperature</span>, <span class="hlt">wind</span> and pressure fluctuations that characterize those <span class="hlt">air</span> seiches. Typical seiche periods were 15 min. We compare the observations with the time-harmonic solutions of the shallow-water equation and with numerical simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29730095','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29730095"><span>Body <span class="hlt">temperature</span> change and outcomes in patients undergoing long-distance <span class="hlt">air</span> medical transport.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nakajima, Mikio; Aso, Shotaro; Yasunaga, Hideo; Shirokawa, Masamitsu; Nakano, Tomotsugu; Miyakuni, Yasuhiko; Goto, Hideaki; Yamaguchi, Yoshihiro</p> <p>2018-04-30</p> <p>Short-distance <span class="hlt">air</span> medical transport for adult emergency patients does not significantly affect patients' body <span class="hlt">temperature</span> and outcomes. This study aimed to examine the influence of long-distance <span class="hlt">air</span> medical transport on patients' body <span class="hlt">temperatures</span> and the relationship between body <span class="hlt">temperature</span> change and mortality. We retrospectively enrolled consecutive patients transferred via helicopter or plane from isolated islands to an emergency medical center in Tokyo, Japan between April 2010 and December 2016. Patients' average body <span class="hlt">temperature</span> was compared before and after <span class="hlt">air</span> transport using a paired t-test, and corrections between body <span class="hlt">temperature</span> change and flight duration were calculated using Pearson's correlation coefficient. Multivariable logistic regression models were then used to examine the association between body <span class="hlt">temperature</span> change and in-hospital mortality. Of 1253 patients, the median age was 72 years (interquartile range, 60-82 years) and median flight duration was 71 min (interquartile range, 54-93 min). In-hospital mortality was 8.5%, and average body <span class="hlt">temperature</span> was significantly different before and after <span class="hlt">air</span> transport (36.7 °C versus 36.3 °C; difference: -0.36 °C; 95% confidence interval, -0.30 to -0.42; p < 0.001). There was no correlation between body <span class="hlt">temperature</span> change and flight duration (r = 0.025, p = 0.371). In-hospital death was significantly associated with (i) hyperthermia (>38.0 °C) or normothermia (36.0-37.9 °C) before <span class="hlt">air</span> transport and hypothermia after <span class="hlt">air</span> transport (odds ratio, 2.08; 95% confidence interval, 1.20-3.63; p = 0.009), and (ii) winter season (odds ratio, 2.15; 95% confidence interval, 1.08-4.27; p = 0.030). Physicians should consider body <span class="hlt">temperature</span> change during long-distance <span class="hlt">air</span> transport in patients with not only hypothermia but also normothermia or hyperthermia before <span class="hlt">air</span> transport, especially in winter. Copyright © 2018 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080015649&hterms=dehydration&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddehydration','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080015649&hterms=dehydration&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddehydration"><span>Using <span class="hlt">Wind</span> and <span class="hlt">Temperature</span> Fields to Study Dehydration Mechanisms in the Tropical Tropopause Layer</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pittman, Jasna; Miller, Timothy; Robertson, Franklin</p> <p>2008-01-01</p> <p>The tropics are the main region for troposphere-to-stratosphere transport (TST) of <span class="hlt">air</span>. One of the dominant mechanisms that control tropical TST of water vapor is freeze-drying by the cold tropical tropopause. This mechanism is supported by evidence from satellite observations of the "tape recorder", where seasonal changes in stratospheric water vapor are in phase with seasonal changes in tropopause <span class="hlt">temperatures</span> in the tropics. Over the last few years, however, the concept of the tropical tropopause has evolved from a single material surface to a layer called the Tropical Tropopause Layer (TTL). A recent hypothesis on dehydration mechanisms suggests that dehydration and entry point into the stratosphere are not always co-located (Holton and Gettelman, 2001). Instead, dehydration can occur during horizontal advection through Lagrangian 'cold pools', or coldest regions along a parcel's trajectory, as <span class="hlt">air</span> ascends within the TTL while the entry point into the stratosphere occurs at a different geographical location. In this study, we investigate the impact that these Lagrangian cold pools have on TTL moisture. For this purpose, we use in situ measurements of TTL water vapor obtained aboard NASA's WB-57 aircraft over the Eastern Tropical Pacific, and we compare these measurements to minimum saturation water vapor mixing ratios obtained from three-dimensional backward trajectory calculations. Aircraft measurements show frequent unsaturated conditions, which suggest that the entry value of stratospheric water vapor in this region was not set by local saturation conditions. Trajectory calculations, driven by both ECMWF operational analysis and reanalysis <span class="hlt">winds</span> and <span class="hlt">temperature</span> fields, are used to explore the impact (e.g., geographical location, timing, dehydration magnitude) of the Lagrangian cold pools intercepted by the parcels sampled by the aircraft. We find noteworthy differences in the location of the Lagrangian cold pools using the two ECMWF data sets, namely</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MS%26E..136a2056M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MS%26E..136a2056M"><span>Particulate Matter Levels in Ambient <span class="hlt">Air</span> Adjacent to Industrial Area</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mohamed, R. M. S. R.; Nizam, N. M. S.; Al-Gheethi, A. A.; Lajis, A.; Kassim, A. H. M.</p> <p>2016-07-01</p> <p><span class="hlt">Air</span> quality in the residential areas adjacent to the industrial regions is of great concern due to the association with human health risks. In this work, the concentrations of particulate matter (PM10) in the ambient <span class="hlt">air</span> of UTHM campus was investigated tostudy the <span class="hlt">air</span> qualityand their compliance to the Malaysian Ambient <span class="hlt">Air</span> Quality Guidelines (AAQG). The PM10 samples were taken over 24 hours from the most significant area at UTHM including Stadium, KolejKediamanTunDr. Ismail (KKTDI) and MakmalBahan. The meteorological parameters; <span class="hlt">temperature</span>, relative humidity, <span class="hlt">wind</span> speed and <span class="hlt">wind</span> direction as well as particulate matterwere estimated by using E-Sampler Particulate Matter (PM10) Collector. The highest concentrations of PM10 (55.56 µg/m3) was recorded at MakmalBahan during the working and weekend days. However, these concentrations are less than 150 pg/m3. It can be concluded that although UTHM is surrounded by the industrial area, the <span class="hlt">air</span> quality in the campus still within the standards limits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110011477','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110011477"><span>Weather Research and Forecasting Model <span class="hlt">Wind</span> Sensitivity Study at Edwards <span class="hlt">Air</span> Force Base, CA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Watson, Leela R.; Bauman, William H., III; Hoeth, Brian</p> <p>2009-01-01</p> <p>This abstract describes work that will be done by the Applied Meteorology Unit (AMU) in assessing the success of different model configurations in predicting "<span class="hlt">wind</span> cycling" cases at Edwards <span class="hlt">Air</span> Force Base, CA (EAFB), in which the <span class="hlt">wind</span> speeds and directions oscillate among towers near the EAFB runway. The Weather Research and Forecasting (WRF) model allows users to choose among two dynamical cores - the Advanced Research WRF (ARW) and the Non-hydrostatic Mesoscale Model (NMM). There are also data assimilation analysis packages available for the initialization of the WRF model - the Local Analysis and Prediction System (LAPS) and the Advanced Regional Prediction System (ARPS) Data Analysis System (ADAS). Having a series of initialization options and WRF cores, as well as many options within each core, creates challenges for local forecasters, such as determining which configuration options are best to address specific forecast concerns. The goal of this project is to assess the different configurations available and determine which configuration will best predict surface <span class="hlt">wind</span> speed and direction at EAFB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AtmEn.175...92L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AtmEn.175...92L"><span>Field evaluation of vegetation and noise barriers for mitigation of near-freeway <span class="hlt">air</span> pollution under variable <span class="hlt">wind</span> conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Eon S.; Ranasinghe, Dilhara R.; Ahangar, Faraz Enayati; Amini, Seyedmorteza; Mara, Steven; Choi, Wonsik; Paulson, Suzanne; Zhu, Yifang</p> <p>2018-02-01</p> <p>Traffic-related <span class="hlt">air</span> pollutants are a significant public health concern, particularly near freeways. Previous studies have suggested either soundwall or vegetation barriers might reduce the near-freeway <span class="hlt">air</span> pollution. This study aims to investigate the effectiveness of a combination of both soundwall and vegetation barrier for reducing ultrafine particles (UFPs, diameter ≤ 100 nm) and PM2.5 (diameter ≤ 2.5 μm) concentrations. Concurrent data collection was carried out at both upwind and downwind fixed locations approximately 10-15 m away from the edge of two major freeways in California. This study observed that the reduction of UFP and PM2.5 was generally greater with the combination barrier than with either soundwall or vegetation alone. Since there were no non-barrier sites at the study locations, the reductions reported here are all in relative terms. The soundwall barrier was more effective for reducing PM2.5 (25-53%) than UFPs (0-5%), and was most effective (51-53% for PM2.5) when the <span class="hlt">wind</span> speed ranged between 1 and 2 m/s. Under the same range of <span class="hlt">wind</span> speed, the vegetation barrier had little effect (0-5%) on reducing PM2.5; but was effective at reducing UFP (up to 50%). For both types of roadside barrier, decreasing <span class="hlt">wind</span> speed resulted in greater net reduction of UFPs (i.e., total number particle concentrations; inversely proportional). This trend was observed, however, only within specific particle size ranges (i.e., diameter < 20 nm for the soundwall barrier and 12-60 nm for the vegetation barrier). Out of these size ranges, the reduction of UFP concentration was proportional to increasing <span class="hlt">wind</span> speed. Overall findings of this study support positive effects of soundwall and vegetation barriers for near-freeway <span class="hlt">air</span> pollution mitigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150002872','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150002872"><span>Assimilation of <span class="hlt">Wind</span> Profiles from Multiple Doppler Radar <span class="hlt">Wind</span> Profilers for Space Launch Vehicle Applications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Decker, Ryan K.; Walker, John R.; Barbre, Robert E., Jr.; Leach, Richard D.</p> <p>2015-01-01</p> <p>Atmospheric <span class="hlt">wind</span> data are required by space launch vehicles in order to assess flight vehicle loads and performance on day-of-launch. Space launch ranges at NASA's Kennedy Space Center co-located with the United States <span class="hlt">Air</span> Force's (USAF) Eastern Range (ER) at Cape Canaveral <span class="hlt">Air</span> Force Station and USAF's Western Range (WR) at Vandenberg <span class="hlt">Air</span> Force Base have extensive networks of in-situ and remote sensing instrumentation to measure atmospheric <span class="hlt">winds</span>. Each instrument's technique to measure <span class="hlt">winds</span> has advantages and disadvantages in regards to use within vehicle trajectory analyses. Balloons measure <span class="hlt">wind</span> at all altitudes necessary for vehicle assessments, but two primary disadvantages exist when applying balloon output. First, balloons require approximately one hour to reach required altitudes. Second, balloons are steered by atmospheric <span class="hlt">winds</span> down range of the launch site that could significantly differ from those <span class="hlt">winds</span> along the vehicle ascent trajectory. These issues are mitigated by use of vertically pointing Doppler Radar <span class="hlt">Wind</span> Profilers (DRWPs). However, multiple DRWP instruments are required to provide <span class="hlt">wind</span> data over altitude ranges necessary for vehicle trajectory assessments. The various DRWP systems have different operating configurations resulting in different temporal and spatial sampling intervals. Therefore, software was developed to combine data from both DRWP-generated profiles into a single profile for use in vehicle trajectory analyses. This paper will present details of the splicing software algorithms and will provide sample output.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920024974','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920024974"><span>Relationship between <span class="hlt">wind</span>, waves and radar backscatter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Katsaros, Kristina B.; Ataktuerk, Serhad S.</p> <p>1991-01-01</p> <p>The aim of the research was to investigate the relationship between <span class="hlt">wind</span>, waves, and radar backscatter from water surface. To this end, three field experiments with periods of 2 to 4 weeks were carried out during summer months in 1988, 1989 and 1990. For these periods, the University of Washington group provided (1) environmental parameters such as <span class="hlt">wind</span> speed, <span class="hlt">wind</span> stress, and atmospheric stratification through measurements of surface fluxes (of momentum, sensible heat and latent heat) and of <span class="hlt">air</span> and water <span class="hlt">temperatures</span>; and (2) wave height spectra including both the dominant waves and the short gravity-capillary waves. Surface flux measurements were performed by using our well tested instruments: a K-Gill twin propeller-vane anemometer and a fast response thermocouple psychrometer. Wave heights were measured by a resistance wire wave gauge. The University of Kansas group was responsible for the operation of the microwave radars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.A13I0402G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.A13I0402G"><span>Examination Of A Strong Downslope Warming <span class="hlt">Wind</span> Event Over The Larsen Ice Shelf In Antarctica Through Modeling And Aircraft Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grosvenor, D. P.; Choularton, T. W.; Gallagher, M. W.; Lachlan-Cope, T. A.; King, J. C.</p> <p>2009-12-01</p> <p>The high mountains of the Antarctic Peninsula (AP) provide a climatic barrier between the west and east. The east side is generally blocked from the warmer oceanic <span class="hlt">air</span> of the west and is consequently usually under the influence of colder continental <span class="hlt">air</span>. On occasion, however, <span class="hlt">air</span> from the west can cross the barrier in the form of strong <span class="hlt">winds</span> travelling down the eastern slopes, which are also very warm and dry due to adiabatic descent. They penetrate onto the Larsen ice shelves where they lead to above zero surface <span class="hlt">temperatures</span> and are therefore likely to encourage surface melting. Crevasse propagation due to the weight of accumulated meltwater is currently thought to have been the major factor in causing the near total disintegration of the Larsen B ice shelf in 2002. In January 2006 the British Antarctic Survey performed an aircraft flight over the Larsen C ice shelf on the east side of the AP, which sampled a strong downslope <span class="hlt">wind</span> event. Surface flux measurements over the ice shelf suggest that the sensible heat provided by the warm jets would be likely to be negated by latent heat losses from ice ablation. The main cause of any ice melting was likely to be due to shortwave radiation input. However, the warming from the jets is still likely to be important by acting as an on/off control for melting by keeping <span class="hlt">air</span> <span class="hlt">temperatures</span> above zero. In addition, the dryness of the <span class="hlt">winds</span> is likely to prevent cloud cover and thus maximize exposure of the ice shelf to solar energy input. This case study has been modeled using the WRF mesoscale model. The model reproduces the strong downslope <span class="hlt">winds</span> seen by the aircraft with good comparisons of <span class="hlt">wind</span> speed and <span class="hlt">temperature</span> profiles through the <span class="hlt">wind</span> jets. Further comparisons to surface station data have allowed progress towards achieving the best set up of the model for this case. The modeling agrees with the results of the aircraft study in suggesting that solar radiation input is likely to provide the largest amount of energy for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160003581','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160003581"><span>Validation of <span class="hlt">AIRS</span> V6 Surface <span class="hlt">Temperature</span> over Greenland with GCN and NOAA Stations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lee, Jae N.; Hearty, Thomas; Cullather, Richard; Nowicki, Sophie; Susskind, Joel</p> <p>2016-01-01</p> <p>This work compares the temporal and spatial characteristics of the AIRSAMSU (Atmospheric Infrared Sounder Advanced Microwave Sounding Unit A) Version 6 and MODIS (Moderate resolution Imaging Spectroradiometer) Collection 5 derived surface <span class="hlt">temperatures</span> over Greenland. To estimate uncertainties in space-based surface <span class="hlt">temperature</span> measurements, we re-projected the MODIS Ice Surface <span class="hlt">Temperature</span> (IST) to 0.5 by 0.5 degree spatial resolution. We also re-gridded <span class="hlt">AIRS</span> Skin <span class="hlt">Temperature</span> (Ts) into the same grid but classified with different cloud conditions and surface types. These co-located data sets make intercomparison between the two instruments relatively straightforward. Using this approach, the spatial comparison between the monthly mean <span class="hlt">AIRS</span> Ts and MODIS IST is in good agreement with RMS 2K for May 2012. This approach also allows the detection of any long-term calibration drift and the careful examination of calibration consistency in the MODIS and <span class="hlt">AIRS</span> <span class="hlt">temperature</span> data record. The temporal correlations between <span class="hlt">temperature</span> data are also compared with those from in-situ measurements from GC-Net (GCN) and NOAA stations. The coherent time series of surface <span class="hlt">temperature</span> evident in the correlation between <span class="hlt">AIRS</span> Ts and GCN <span class="hlt">temperatures</span> suggest that at monthly time scales both observations capture the same climate signal over Greenland. It is also suggested that <span class="hlt">AIRS</span> surface <span class="hlt">air</span> <span class="hlt">temperature</span> (Ta) can be used to estimate the boundary layer inversion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DPS....4821615K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DPS....4821615K"><span><span class="hlt">Temperature</span> and <span class="hlt">Wind</span> Measurements in Venus Lower Thermosphere between 2007 and 2015</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krause, Pia; Sornig, Manuela; Wischnewski, Carolin; Sonnabend, Guido; Stangier, Tobias; Herrmann, Maren; Kostiuk, Theodor; Livengood, Timothy A.; Pätzold, Martin</p> <p>2016-10-01</p> <p>The structure of Venus atmosphere and its thermal and dynamical behavior was intensely studied during the past decade by groundbased and the space mission Venus Express. A comprehensive understanding of the atmosphere, however, is still missing. Direct measurements of atmospheric parameters on various time scales and at different locations across the planet are essential for better understanding and to validate global circulation models. Line-resolved spectroscopy of infrared CO2 transitions provides a powerful tool to accomplish measurements of <span class="hlt">temperature</span> and <span class="hlt">wind</span> speed within the neutral atmosphere, using Doppler line-broadening and Doppler shift. <span class="hlt">Temperature</span> is the motor to drive circulation, and <span class="hlt">wind</span> speed is the result. Measuring both provides both the basis and an empirical test for circulation models. Non-LTE emission lines at 10 µm that originate from a pressure level of 1μbar, ~110 km altitude, probe the lower thermosphere and are measurable at high spectral resolution using the infrared heterodyne spectrometers THIS (University of Cologne), HIPWAC (NASA GSFC) and MILAHI (Tohoku University).Thermal and dynamical structures on the Venus day side are retrieved using a newly developed method that considers the influence of the spectrometer field-of-view (FoV) and the dispersion of spectral properties across the FoV. New conclusions from the ground-based observing campaigns between 2007 and 2015 will be presented based on this retrieval methodology. The spatial resolution on the planetary disk is different for each campaign, depending on the apparent diameter of the planet and the diffraction-limited FoV of the telescope. Previously, a comparison of the observing campaigns was limited due to the difference in spatial resolution. The new retrieval method enables comparing observations with different observing geometry. The observations yield a large quantity of <span class="hlt">temperature</span> and <span class="hlt">wind</span> measurements at different positions on the planetary disk, which supports</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E3SWC..3201020H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E3SWC..3201020H"><span><span class="hlt">Wind</span> tunnel study of natural ventilation of building integrated photovoltaics double skin façade</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hudişteanu, Sebastian Valeriu; Popovici, Cătălin George; Cherecheş, Nelu-Cristian</p> <p>2018-02-01</p> <p>The paper presents a <span class="hlt">wind</span> tunnel experimental analysis of a small-scale building model (1:30). The objective of the study is to determine the <span class="hlt">wind</span> influence on the ventilation of a double skin façade channel (DSF) and the cooling effect over integrated photovoltaic panels. The tests were achieved by conceiving and implementation of an experimental program using a <span class="hlt">wind</span> tunnel with atmospheric boundary layer. The effect of the <span class="hlt">wind</span> over the ventilation of the horizontal channels of double skin façades is evaluated for different incident velocities. The results are generalized for the average steady state values of the velocities analysed. The experimental results put in evidence the correlation between the reference <span class="hlt">wind</span> velocity and the dynamics of the <span class="hlt">air</span> movement inside the double skin façade. These values are used to determine the convective heat transfer and the cooling effect of the <span class="hlt">air</span> streams inside the channel upon the integrated photovoltaic panels. The decrease of the photovoltaic panels <span class="hlt">temperature</span> determines a raise of 11% in efficiency and power generated.</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 regions of increased and decreased surface heat flux on either side of turbine columns. The regions are correlated with coherent wake rotation in the turbine-array. On the upwelling side there is decreased flux, while on the downwelling side cool <span class="hlt">air</span> 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 <span class="hlt">temperature</span> 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/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 <span class="hlt">temperature</span></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 regional 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 region 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 regions. 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> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JPhCS.524a2074S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JPhCS.524a2074S"><span>Offshore Floating <span class="hlt">Wind</span> Turbine-driven Deep Sea Water Pumping for Combined Electrical Power and District Cooling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sant, T.; Buhagiar, D.; Farrugia, R. N.</p> <p>2014-06-01</p> <p>A new concept utilising floating <span class="hlt">wind</span> turbines to exploit the low <span class="hlt">temperatures</span> of deep sea water for space cooling in buildings is presented. The approach is based on offshore hydraulic <span class="hlt">wind</span> turbines pumping pressurised deep sea water to a centralised plant consisting of a hydro-electric power system coupled to a large-scale sea water-cooled <span class="hlt">air</span> conditioning (AC) unit of an urban district cooling network. In order to investigate the potential advantages of this new concept over conventional technologies, a simplified model for performance simulation of a vapour compression AC unit was applied independently to three different systems, with the AC unit operating with (1) a constant flow of sea surface water, (2) a constant flow of sea water consisting of a mixture of surface sea water and deep sea water delivered by a single offshore hydraulic <span class="hlt">wind</span> turbine and (3) an intermittent flow of deep sea water pumped by a single offshore hydraulic <span class="hlt">wind</span> turbine. The analysis was based on one year of <span class="hlt">wind</span> and ambient <span class="hlt">temperature</span> data for the Central Mediterranean that is known for its deep waters, warm climate and relatively low <span class="hlt">wind</span> speeds. The study confirmed that while the present concept is less efficient than conventional turbines utilising grid-connected electrical generators, a significant portion of the losses associated with the hydraulic transmission through the pipeline are offset by the extraction of cool deep sea water which reduces the electricity consumption of urban <span class="hlt">air</span>-conditioning units.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170006569','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170006569"><span><span class="hlt">Temperature</span> Mapping of <span class="hlt">Air</span> Film-Cooled Thermal Barrier Coated Surfaces Using Phosphor Thermometry</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Eldridge, Jeffrey I.</p> <p>2016-01-01</p> <p>While the effects of thermal barrier coating (TBC) thermal protection and <span class="hlt">air</span> film cooling effectiveness for jet engine components are usually studied separately, their contributions to combined cooling effectiveness are interdependent and are not simply additive. Therefore, combined cooling effectiveness must be measured to achieve an optimum balance between TBC thermal protection and <span class="hlt">air</span> film cooling. Phosphor thermometry offers several advantages for mapping <span class="hlt">temperatures</span> of <span class="hlt">air</span> film cooled surfaces. While infrared thermography has been typically applied to study <span class="hlt">air</span> film cooling effectiveness, <span class="hlt">temperature</span> accuracy depends on knowing surface emissivity (which may change) and correcting for effects of reflected radiation. Because decay time-based full-field phosphor thermometry is relatively immune to these effects, it can be applied advantageously to <span class="hlt">temperature</span> mapping of <span class="hlt">air</span> film-cooled TBC-coated surfaces. In this presentation, an overview will be given of efforts at NASA Glenn Research Center to perform <span class="hlt">temperature</span> mapping of <span class="hlt">air</span> film-cooled TBC-coated surfaces in a burner rig test environment. The effects of thermal background radiation and flame chemiluminescence on the measurements are investigated, and the strengths and limitations of this method for studying <span class="hlt">air</span> film cooling effectiveness are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRC..117.5035A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRC..117.5035A"><span>Statistics of surface divergence and their relation to <span class="hlt">air</span>-water gas transfer velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Asher, William E.; Liang, Hanzhuang; Zappa, Christopher J.; Loewen, Mark R.; Mukto, Moniz A.; Litchendorf, Trina M.; Jessup, Andrew T.</p> <p>2012-05-01</p> <p><span class="hlt">Air</span>-sea gas fluxes are generally defined in terms of the <span class="hlt">air</span>/water concentration difference of the gas and the gas transfer velocity,kL. Because it is difficult to measure kLin the ocean, it is often parameterized using more easily measured physical properties. Surface divergence theory suggests that infrared (IR) images of the water surface, which contain information concerning the movement of water very near the <span class="hlt">air</span>-water interface, might be used to estimatekL. Therefore, a series of experiments testing whether IR imagery could provide a convenient means for estimating the surface divergence applicable to <span class="hlt">air</span>-sea exchange were conducted in a synthetic jet array tank embedded in a <span class="hlt">wind</span> tunnel. Gas transfer velocities were measured as a function of <span class="hlt">wind</span> stress and mechanically generated turbulence; laser-induced fluorescence was used to measure the concentration of carbon dioxide in the top 300 μm of the water surface; IR imagery was used to measure the spatial and temporal distribution of the aqueous skin <span class="hlt">temperature</span>; and particle image velocimetry was used to measure turbulence at a depth of 1 cm below the <span class="hlt">air</span>-water interface. It is shown that an estimate of the surface divergence for both <span class="hlt">wind</span>-shear driven turbulence and mechanically generated turbulence can be derived from the surface skin <span class="hlt">temperature</span>. The estimates derived from the IR images are compared to velocity field divergences measured by the PIV and to independent estimates of the divergence made using the laser-induced fluorescence data. Divergence is shown to scale withkLvalues measured using gaseous tracers as predicted by conceptual models for both <span class="hlt">wind</span>-driven and mechanically generated turbulence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..170a2035C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..170a2035C"><span>Oxidation characteristics of MgF2 in <span class="hlt">air</span> at high <span class="hlt">temperature</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, H. K.; Jie, Y. Y.; Chang, L.</p> <p>2017-02-01</p> <p>High <span class="hlt">temperature</span> oxidation properties of MgF2 in <span class="hlt">air</span> were studied. The changes of phase composition, macro surface morphology, weight and elemental composition of MgF2 samples with <span class="hlt">temperature</span> were investigated by using XRD, EDS and gravimetric analyses. The results show that the oxidation reaction of MgF2 converted to MgO occurred at high <span class="hlt">temperature</span>, and the reaction was accelerated by the increase of <span class="hlt">temperature</span> and the presence of impurities. This result clarifies the understanding of the high <span class="hlt">temperature</span> oxidation behavior of MgF2 in <span class="hlt">air</span>, and provides a theoretical basis for the reasonable application of MgF2 in optical coating materials, electronic ceramic materials and magnesium melt protection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC51D1188J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC51D1188J"><span>Globally-Gridded Interpolated Night-Time Marine <span class="hlt">Air</span> <span class="hlt">Temperatures</span> 1900-2014</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Junod, R.; Christy, J. R.</p> <p>2016-12-01</p> <p>Over the past century, climate records have pointed to an increase in global near-surface average <span class="hlt">temperature</span>. Near-surface <span class="hlt">air</span> <span class="hlt">temperature</span> over the oceans is a relatively unused parameter in understanding the current state of climate, but is useful as an independent <span class="hlt">temperature</span> metric over the oceans and serves as a geographical and physical complement to near-surface <span class="hlt">air</span> <span class="hlt">temperature</span> over land. Though versions of this dataset exist (i.e. HadMAT1 and HadNMAT2), it has been strongly recommended that various groups generate climate records independently. This University of Alabama in Huntsville (UAH) study began with the construction of monthly night-time marine <span class="hlt">air</span> <span class="hlt">temperature</span> (UAHNMAT) values from the early-twentieth century through to the present era. Data from the International Comprehensive Ocean and Atmosphere Data Set (ICOADS) were used to compile a time series of gridded UAHNMAT, (20S-70N). This time series was homogenized to correct for the many biases such as increasing ship height, solar deck heating, etc. The time series of UAHNMAT, once adjusted to a standard reference height, is gridded to 1.25° pentad grid boxes and interpolated using the kriging interpolation technique. This study will present results which quantify the variability and trends and compare to current trends of other related datasets that include HadNMAT2 and sea-surface <span class="hlt">temperatures</span> (HadISST & ERSSTv4).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1346740-room-temperature-air-crystallized-perovskite-film-high-performance-solar-cells','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1346740-room-temperature-air-crystallized-perovskite-film-high-performance-solar-cells"><span>Room <span class="hlt">temperature</span>, <span class="hlt">air</span> crystallized perovskite film for high performance solar cells</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Dubey, Ashish; Kantack, Nicholas; Adhikari, Nirmal; ...</p> <p>2016-05-31</p> <p>For the first time, room <span class="hlt">temperature</span> heating free growth and crystallization of perovskite films in ambient <span class="hlt">air</span> without the use of thermal annealing is reported. Highly efficient perovskite nanorod-based solar cells were made using ITO/PEDOT:PSS/CH 3NH 3PbI 3 nanorods/PC 60BM/rhodamine/Ag. All the layers except PEDOT:PSS were processed at room <span class="hlt">temperature</span> thereby eliminating the need for thermal treatment. Perovskite films were spin coated inside a N-2 filled glovebox and immediately were taken outside in <span class="hlt">air</span> having 40% relative humidity (RH). Exposure to humid <span class="hlt">air</span> was observed to promote the crystallization process in perovskite films even at room <span class="hlt">temperature</span>. Perovskite films keptmore » for 5 hours in ambient <span class="hlt">air</span> showed nanorod-like morphology having high crystallinity, with devices exhibiting the highest PCE of 16.83%, which is much higher than the PCE of 11.94% for traditional thermally annealed perovskite film based devices. Finally, it was concluded that moisture plays an important role in room <span class="hlt">temperature</span> crystallization of pure perovskite nanorods, showing improved optical and charge transport properties, which resulted in high performance solar cells.« 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_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/2015EGUGA..17.4718T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.4718T"><span>Experimental investigation of effect of surface gravity waves and spray on heat and momentum flux at strong <span class="hlt">wind</span> conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Troitskaya, Yuliya; Sergeev, Daniil; Vdovin, Maxim; Kandaurov, Alexander; Ermakova, Olga; Kazakov, Vassily</p> <p>2015-04-01</p> <p>The most important characteristics that determine the interaction between atmosphere and ocean are fluxes of momentum, heat and moisture. For their parameterization the dimensionless exchange coefficients (the surface drag coefficient CD and the heat transfer coefficient or the Stanton number CT) are used. Numerous field and laboratory experiments show that CD increases with increasing <span class="hlt">wind</span> speed at moderate and strong <span class="hlt">wind</span>, and as it was shows recently CD decreases at hurricane <span class="hlt">wind</span> speed. Waves are known to increase the sea surface resistance due to enhanced form drag, the sea spray is considered as a possible mechanism of the 'drag reduction' at hurricane conditions. The dependence of heat transfer coefficient CD on the <span class="hlt">wind</span> speed is not so certain and the role of the mechanism associated with the wave disturbances in the mass transfer is not completely understood. Observations and laboratory data show that this dependence is weaker than for the CD, and there are differences in the character of the dependence in different data sets. The purpose of this paper is investigation of the effect of surface waves on the turbulent exchange of momentum and heat within the laboratory experiment, when <span class="hlt">wind</span> and wave parameters are maintained and controlled. The effect of spray on turbulent exchange at strong <span class="hlt">winds</span> is also estimated. A series of experiments to study the processes of turbulent exchange of momentum and heat in a stably stratified <span class="hlt">temperature</span> turbulent boundary layer <span class="hlt">air</span> flow over waved water surface were carried out at the <span class="hlt">Wind</span> - wave stratified flume of IAP RAS, the peculiarity of this experiment was the option to change the surface wave parameters regardless of the speed of the <span class="hlt">wind</span> flow in the channel. For this purpose a polyethylene net with the variable depth (0.25 mm thick and a cell of 1.6 mm × 1.6mm) has been stretched along the channel. The waves were absent when the net was located at the level of the undisturbed water surface, and had maximum</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813552E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813552E"><span>Immersion and contact freezing experiments in the Mainz <span class="hlt">wind</span> tunnel laboratory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eppers, Oliver; Mayer, Amelie; Diehl, Karoline; Mitra, Subir; Borrmann, Stephan; Szakáll, Miklós</p> <p>2016-04-01</p> <p>Immersion and contact freezing are of outmost important ice nucleation processes in mixed phase clouds. Experimental studies are carried out in the Mainz vertical <span class="hlt">wind</span> tunnel laboratory in order to characterize these nucleation processes for different ice nucleating particles (INP), such as for mineral dust or biological particles. Immersion freezing is investigated in our laboratory with two different experimental techniques, both attaining contact-free levitation of liquid droplets and cooling of the surrounding <span class="hlt">air</span> down to about -25 °C. In an acoustic levitator placed in the cold room of our laboratory, drops with diameters of 2 mm are investigated. In the vertical <span class="hlt">air</span> stream of the <span class="hlt">wind</span> tunnel droplets with diameter of 700 micron are freely floated at their terminal velocities, simulating the flow conditions of the free atmosphere. Furthermore, the <span class="hlt">wind</span> tunnel offers a unique platform for contact freezing experiments. Supercooled water droplets are floated in the vertical <span class="hlt">air</span> stream at their terminal velocities and INP are injected into the tunnel <span class="hlt">air</span> stream upstream of them. As soon as INP collides with the supercooled droplet the contact freezing is initiated. The first results of immersion and contact freezing experiments with cellulose particles both in the acoustic levitator and in the <span class="hlt">wind</span> tunnel will be presented. Cellulose is considered as typical INP of biological origin and a macrotracer for plant debris. Nucleating properties of cellulose will be provided, mainly focusing on the <span class="hlt">temperature</span>, INP concentration, and specific surface area dependences of the freezing processes. Direct comparison between the different experimental techniques (acoustic levitator and <span class="hlt">wind</span> tunnel), as well as between nucleation modes (immersion and contact freezing) will be presented. The work is carried out within the framework of the German research unit INUIT.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170000893','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170000893"><span>Using C-Band Dual-Polarization Radar Signatures to Improve Convective <span class="hlt">Wind</span> Forecasting at Cape Canaveral <span class="hlt">Air</span> Force Station and NASA Kennedy Space Center</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Amiot, Corey G.; Carey, Lawrence D.; Roeder, William P.; McNamara, Todd M.; Blakeslee, Richard J.</p> <p>2017-01-01</p> <p>The United States <span class="hlt">Air</span> Force's 45th Weather Squadron (45WS) is the organization responsible for monitoring atmospheric conditions at Cape Canaveral <span class="hlt">Air</span> Force Station and NASA Kennedy Space Center (CCAFS/KSC) and issuing warnings for hazardous weather conditions when the need arises. One such warning is issued for convective <span class="hlt">wind</span> events, for which lead times of 30 and 60 minutes are desired for events with peak <span class="hlt">wind</span> gusts of 35 knots or greater (i.e., Threshold-1) and 50 knots or greater (i.e., Threshold-2), respectively (Roeder et al. 2014).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ThApC.108..591N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ThApC.108..591N"><span>The effect of <span class="hlt">air</span> <span class="hlt">temperature</span> and human thermal indices on mortality in Athens, Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nastos, Panagiotis T.; Matzarakis, Andreas</p> <p>2012-05-01</p> <p>This paper investigates whether there is any association between the daily mortality for the wider region of Athens, Greece and the thermal conditions, for the 10-year period 1992-2001. The daily mortality datasets were acquired from the Hellenic Statistical Service and the daily meteorological datasets, concerning daily maximum and minimum <span class="hlt">air</span> <span class="hlt">temperature</span>, from the Hellinikon/Athens meteorological station, established at the headquarters of the Greek Meteorological Service. Besides, the daily values of the thermal indices Physiologically Equivalent <span class="hlt">Temperature</span> (PET) and Universal Thermal Climate Index (UTCI) were evaluated in order to interpret the grade of physiological stress. The first step was the application of Pearson's χ 2 test to the compiled contingency tables, resulting in that the probability of independence is zero ( p = 0.000); namely, mortality is in close relation to the <span class="hlt">air</span> <span class="hlt">temperature</span> and PET/UTCI. Furthermore, the findings extracted by the generalized linear models showed that, statistically significant relationships ( p < 0.01) between <span class="hlt">air</span> <span class="hlt">temperature</span>, PET, UTCI and mortality exist on the same day. More concretely, on one hand during the cold period (October-March), a 10°C decrease in daily maximum <span class="hlt">air</span> <span class="hlt">temperature</span>, minimum <span class="hlt">air</span> <span class="hlt">temperature</span>, <span class="hlt">temperature</span> range, PET and UTCI is related with an increase 13%, 15%, 2%, 7% and 6% of the probability having a death, respectively. On the other hand, during the warm period (April-September), a 10°C increase in daily maximum <span class="hlt">air</span> <span class="hlt">temperature</span>, minimum <span class="hlt">air</span> <span class="hlt">temperature</span>, <span class="hlt">temperature</span> range, PET and UTCI is related with an increase 3%, 1%, 10%, 3% and 5% of the probability having a death, respectively. Taking into consideration the time lag effect of the examined parameters on mortality, it was found that significant effects of 3-day lag during the cold period appears against 1-day lag during the warm period. In spite of the general aspect that cold conditions seem to be favourable factors for daily mortality</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013MeScT..24i5302P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013MeScT..24i5302P"><span>Measurement of <span class="hlt">temperature</span> and pressure on the surface of a blunt cone using FBG sensor in hypersonic <span class="hlt">wind</span> tunnel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prasad, A. S. Guru; Sharath, U.; Nagarjun, V.; Hegde, G. M.; Asokan, S.</p> <p>2013-09-01</p> <p>Measurement of <span class="hlt">temperature</span> and pressure exerted on the leeward surface of a blunt cone specimen has been demonstrated in the present work in a hypersonic <span class="hlt">wind</span> tunnel using fiber Bragg grating (FBG) sensors. The experiments were conducted on a 30° apex-angle blunt cone with 51 mm base diameter at <span class="hlt">wind</span> flow speeds of Mach 6.5 and 8.35 in a 300 mm hypersonic <span class="hlt">wind</span> tunnel of Indian Institute of Science, Bangalore. A special pressure insensitive <span class="hlt">temperature</span> sensor probe along with the conventional bare FBG sensors was used for explicit <span class="hlt">temperature</span> and aerodynamic pressure measurement respectively on the leeward surface of the specimen. computational fluid dynamics (CFD) simulation of the flow field around the blunt cone specimen has also been carried out to obtain the <span class="hlt">temperature</span> and pressure at conditions analogous to experiments. The results obtained from FBG sensors and the CFD simulations are found to be in good agreement with each other.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050188550','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050188550"><span><span class="hlt">WIND</span> Flow Solver Released</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Towne, Charles E.</p> <p>1999-01-01</p> <p>The <span class="hlt">WIND</span> code is a general-purpose, structured, multizone, compressible flow solver that can be used to analyze steady or unsteady flow for a wide range of geometric configurations and over a wide range of flow conditions. <span class="hlt">WIND</span> is the latest product of the NPARC Alliance, a formal partnership between the NASA Lewis Research Center and the <span class="hlt">Air</span> Force Arnold Engineering Development Center (AEDC). <span class="hlt">WIND</span> Version 1.0 was released in February 1998, and Version 2.0 will be released in February 1999. The <span class="hlt">WIND</span> code represents a merger of the capabilities of three existing computational fluid dynamics codes--NPARC (the original NPARC Alliance flow solver), NXAIR (an <span class="hlt">Air</span> Force code used primarily for unsteady store separation problems), and NASTD (the primary flow solver at McDonnell Douglas, now part of Boeing).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/984517','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/984517"><span><span class="hlt">Wind</span> turbine generators having <span class="hlt">wind</span> assisted cooling systems and cooling methods</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bagepalli, Bharat [Niskayuna, NY; Barnes, Gary R [Delanson, NY; Gadre, Aniruddha D [Rexford, NY; Jansen, Patrick L [Scotia, NY; Bouchard, Jr., Charles G.; Jarczynski, Emil D [Scotia, NY; Garg, Jivtesh [Cambridge, MA</p> <p>2008-09-23</p> <p>A <span class="hlt">wind</span> generator includes: a nacelle; a hub carried by the nacelle and including at least a pair of <span class="hlt">wind</span> turbine blades; and an electricity producing generator including a stator and a rotor carried by the nacelle. The rotor is connected to the hub and rotatable in response to <span class="hlt">wind</span> acting on the blades to rotate the rotor relative to the stator to generate electricity. A cooling system is carried by the nacelle and includes at least one ambient <span class="hlt">air</span> inlet port opening through a surface of the nacelle downstream of the hub and blades, and a duct for flowing <span class="hlt">air</span> from the inlet port in a generally upstream direction toward the hub and in cooling relation to the stator.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26214379','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26214379"><span>Skin sites to predict deep-body <span class="hlt">temperature</span> while wearing firefighters' personal protective equipment during periodical changes in <span class="hlt">air</span> <span class="hlt">temperature</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, Siyeon; Lee, Joo-Young</p> <p>2016-04-01</p> <p>The aim of this study was to investigate stable and valid measurement sites of skin <span class="hlt">temperatures</span> as a non-invasive variable to predict deep-body <span class="hlt">temperature</span> while wearing firefighters' personal protective equipment (PPE) during <span class="hlt">air</span> <span class="hlt">temperature</span> changes. Eight male firefighters participated in an experiment which consisted of 60-min exercise and 10-min recovery while wearing PPE without self-contained breathing apparatus (7.75 kg in total PPE mass). <span class="hlt">Air</span> <span class="hlt">temperature</span> was periodically fluctuated from 29.5 to 35.5 °C with an amplitude of 6 °C. Rectal <span class="hlt">temperature</span> was chosen as a deep-body <span class="hlt">temperature</span>, and 12 skin <span class="hlt">temperatures</span> were recorded. The results showed that the forehead and chest were identified as the most valid sites to predict rectal <span class="hlt">temperature</span> (R(2) = 0.826 and 0.824, respectively) in an environment with periodically fluctuated <span class="hlt">air</span> <span class="hlt">temperatures</span>. This study suggests that particular skin <span class="hlt">temperatures</span> are valid as a non-invasive variable when predicting rectal <span class="hlt">temperature</span> of an individual wearing PPE in changing ambient <span class="hlt">temperatures</span>. Practitioner Summary: This study should offer assistance for developing a more reliable indirect indicating system of individual heat strain for firefighters in real time, which can be used practically as a precaution of firefighters' heat-related illness and utilised along with physiological monitoring.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..126a2028M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..126a2028M"><span>Relative <span class="hlt">air</span> <span class="hlt">temperature</span> analysis external building on Gowa Campus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mustamin, Tayeb; Rahim, Ramli; Baharuddin; Jamala, Nurul; Kusno, Asniawaty</p> <p>2018-03-01</p> <p>This study aims to data analyze the relative <span class="hlt">temperature</span> and humidity of the <span class="hlt">air</span> outside the building. Data retrieval taken from weather monitoring device (monitoring) Vaisala, RTU (Remote Terminal Unit), Which is part of the AWS (Automatic Weather Stations) Then Processing data processed and analyzed by using Microsoft Excel program in the form of graph / picture fluctuation Which shows the average value, standard deviation, maximum value, and minimum value. Results of data processing then grouped in the form: Daily, and monthly, based on time intervals every 30 minutes. The results showed Outside <span class="hlt">air</span> <span class="hlt">temperatures</span> in March, April, May and September 2016 Which entered in the thermal comfort zone according to SNI standard (Indonesian National Standard) only at 06.00-10.00. In late March to early April Thermal comfort zone also occurs at 15.30-18.00. The highest maximum <span class="hlt">air</span> <span class="hlt">temperature</span> occurred in September 2016 at 11.01-11.30 And the lowest minimum value in September 2016, time 6:00 to 6:30. The result of the next analysis shows the level of data conformity with thermal comfort zone based on SNI (Indonesian National Standard) every month.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ThApC.126..575K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ThApC.126..575K"><span>Local <span class="hlt">air</span> <span class="hlt">temperature</span> tolerance: a sensible basis for estimating climate variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kärner, Olavi; Post, Piia</p> <p>2016-11-01</p> <p>The customary representation of climate using sample moments is generally biased due to the noticeably nonstationary behaviour of many climate series. In this study, we introduce a moment-free climate representation based on a statistical model fitted to a long-term daily <span class="hlt">air</span> <span class="hlt">temperature</span> anomaly series. This model allows us to separate the climate and weather scale variability in the series. As a result, the climate scale can be characterized using the mean annual cycle of series and local <span class="hlt">air</span> <span class="hlt">temperature</span> tolerance, where the latter is computed using the fitted model. The representation of weather scale variability is specified using the frequency and the range of outliers based on the tolerance. The scheme is illustrated using five long-term <span class="hlt">air</span> <span class="hlt">temperature</span> records observed by different European meteorological stations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21665190','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21665190"><span><span class="hlt">Air</span> conditioner operation behaviour based on students' skin <span class="hlt">temperature</span> in a classroom.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Song, Gook-Sup; Lim, Jae-Han; Ahn, Tae-Kyung</p> <p>2012-01-01</p> <p>A total of 25 college students participated in a study to determine when they would use an <span class="hlt">air</span> conditioner during a lecture in a university classroom. The ambient <span class="hlt">temperature</span> and relative humidity were measured 75 cm above the floor every minute. Skin <span class="hlt">temperatures</span> were measured every minute at seven points, according to the recommendation of Hardy and Dubois. The average clothing insulation value (CLO) of subjects was 0.53 ± 0.07 CLO. The mean <span class="hlt">air</span> velocity in the classroom was 0.13 ± 0.028 m/s. When the subjects turned the <span class="hlt">air</span> conditioner both on and off, the average ambient <span class="hlt">temperatures</span>, relative humidity and mean skin <span class="hlt">temperatures</span> were 27.4 and 23.7 °C (p = 0.000), 40.9 and 40.0% (p = 0.528) and 32.7 and 32.2 °C (p = 0.024), respectively. When the status of the <span class="hlt">air</span> conditioner was changed, the differences of skin <span class="hlt">temperatures</span> in core body parts (head, abdomen and thigh) were not statistically significant. However, in the extremities (mid-lower arm, hand, shin and instep), the differences were statistically significant. Subjects preferred a fluctuating environment to a constant <span class="hlt">temperature</span> condition. We found that a changing environment does not affect classroom study. Copyright © 2011 Elsevier Ltd and The Ergonomics Society. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70187762','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70187762"><span>Evaluation of the Global Land Data Assimilation System (GLDAS) <span class="hlt">air</span> <span class="hlt">temperature</span> data products</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ji, Lei; Senay, Gabriel B.; Verdin, James P.</p> <p>2015-01-01</p> <p>There is a high demand for agrohydrologic models to use gridded near-surface <span class="hlt">air</span> <span class="hlt">temperature</span> data as the model input for estimating regional and global water budgets and cycles. The Global Land Data Assimilation System (GLDAS) developed by combining simulation models with observations provides a long-term gridded meteorological dataset at the global scale. However, the GLDAS <span class="hlt">air</span> <span class="hlt">temperature</span> products have not been comprehensively evaluated, although the accuracy of the products was assessed in limited areas. In this study, the daily 0.25° resolution GLDAS <span class="hlt">air</span> <span class="hlt">temperature</span> data are compared with two reference datasets: 1) 1-km-resolution gridded Daymet data (2002 and 2010) for the conterminous United States and 2) global meteorological observations (2000–11) archived from the Global Historical Climatology Network (GHCN). The comparison of the GLDAS datasets with the GHCN datasets, including 13 511 weather stations, indicates a fairly high accuracy of the GLDAS data for daily <span class="hlt">temperature</span>. The quality of the GLDAS <span class="hlt">air</span> <span class="hlt">temperature</span> data, however, is not always consistent in different regions of the world; for example, some areas in Africa and South America show relatively low accuracy. Spatial and temporal analyses reveal a high agreement between GLDAS and Daymet daily <span class="hlt">air</span> <span class="hlt">temperature</span> datasets, although spatial details in high mountainous areas are not sufficiently estimated by the GLDAS data. The evaluation of the GLDAS data demonstrates that the <span class="hlt">air</span> <span class="hlt">temperature</span> estimates are generally accurate, but caution should be taken when the data are used in mountainous areas or places with sparse weather stations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611318W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611318W"><span>The Impacts of a 2-Degree Rise in Global <span class="hlt">Temperatures</span> upon Gas-Phase <span class="hlt">Air</span> Pollutants in Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watson, Laura; Josse, Béatrice; Marecal, Virginie; Lacressonnière, Gwendoline; Vautard, Robert; Gauss, Michael; Engardt, Magnuz; Nyiri, Agnes; Siour, Guillaume</p> <p>2014-05-01</p> <p>The 15th session of the Conference of Parties (COP 15) in 2009 ratified the Copenhagen Accord, which "recognises the scientific view that" global <span class="hlt">temperature</span> rise should be held below 2 degrees C above pre-industrial levels in order to limit the impacts of climate change. Due to the fact that a 2-degree limit has been frequently referred to by policy makers in the context of the Copenhagen Accord and many other high-level policy statements, it is important that the impacts of this 2-degree increase in <span class="hlt">temperature</span> are adequately analysed. To this end, the European Union sponsored the project IMPACT2C, which uses a multi-disciplinary international team to assess a wide variety of impacts of a 2-degree rise in global <span class="hlt">temperatures</span>. For example, this future increase in <span class="hlt">temperature</span> is expected to have a significant influence upon meteorological conditions such as <span class="hlt">temperature</span>, precipitation, and <span class="hlt">wind</span> direction and intensity; which will in turn affect the production, deposition, and distribution of <span class="hlt">air</span> pollutants. For the first part of the <span class="hlt">air</span> quality analysis within the IMPACT2C project, the impact of meteorological forcings on gas phase <span class="hlt">air</span> pollutants over Europe was studied using four offline atmospheric chemistry transport models. Two sets of meteorological forcings were used for each model: reanalysis of past observation data and global climate model output. Anthropogenic emissions of ozone precursors for the year 2005 were used for all simulations in order to isolate the impact of meteorology and assess the robustness of the results across the different models. The differences between the simulations that use reanalysis of past observation data and the simulations that use global climate model output show how global climate models modify climate hindcasts by boundary conditions inputs: information that is necessary in order to interpret simulations of future climate. The baseline results were assessed by comparison with <span class="hlt">Air</span>Base (Version 7) measurement data, and were</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=342843','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=342843"><span><span class="hlt">Wind</span> erosion processes and control</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><span class="hlt">Wind</span> erosion continues to threaten the sustainability of our nations' soil, <span class="hlt">air</span>, and water resources. To effectively apply conservation systems to prevent <span class="hlt">wind</span> driven soil loss, an understanding of the fundamental processes of <span class="hlt">wind</span> erosion is necessary so that land managers can better recognize the ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA578419','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA578419"><span>Predicting the Turbulent <span class="hlt">Air</span>-Sea Surface Fluxes, Including Spray Effects, from Weak to Strong <span class="hlt">Winds</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-09-30</p> <p>almost complete decoupling of the <span class="hlt">wind</span> field from the sea surface . As a result of the weak surface stress, the flow becomes almost free from the...shore flow . In turn, wave growth and the associated surface roughness (z0) are limited. Consequently, the stability increases further in a...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Predicting the Turbulent <span class="hlt">Air</span>-Sea Surface Fluxes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110010194','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110010194"><span>Lessons Learned from <span class="hlt">AIRS</span>: Improved Determination of Surface and Atmospheric <span class="hlt">Temperatures</span> Using Only Shortwave <span class="hlt">AIRS</span> Channels</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Susskind, Joel</p> <p>2011-01-01</p> <p>This slide presentation reviews the use of shortwave channels available to the Atmospheric Infrared Sounder (<span class="hlt">AIRS</span>) to improve the determination of surface and atmospheric <span class="hlt">temperatures</span>. The <span class="hlt">AIRS</span> instrument is compared with the Infrared Atmospheric Sounding Interferometer (IASI) on-board the MetOp-A satellite. The objectives of the <span class="hlt">AIRS</span>/AMSU were to (1) provide real time observations to improve numerical weather prediction via data assimilation, (2) Provide observations to measure and explain interannual variability and trends and (3) Use of <span class="hlt">AIRS</span> product error estimates allows for QC optimized for each application. Successive versions in the <span class="hlt">AIRS</span> retrieval methodology have shown significant improvement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25875162','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25875162"><span>Ambient <span class="hlt">air</span> pollution, <span class="hlt">temperature</span> and out-of-hospital coronary deaths in Shanghai, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dai, Jinping; Chen, Renjie; Meng, Xia; Yang, Changyuan; Zhao, Zhuohui; Kan, Haidong</p> <p>2015-08-01</p> <p>Few studies have evaluated the effects of ambient <span class="hlt">air</span> pollution and <span class="hlt">temperature</span> in triggering out-of-hospital coronary deaths (OHCDs) in China. We evaluated the associations of <span class="hlt">air</span> pollution and <span class="hlt">temperature</span> with daily OHCDs in Shanghai, China from 2006 to 2011. We applied an over-dispersed generalized additive model and a distributed lag nonlinear model to analyze the effects of <span class="hlt">air</span> pollution and <span class="hlt">temperature</span>, respectively. A 10 μg/m(3) increase in the present-day PM10, PM2.5, SO2, NO2 and CO were associated with increases in OHCD mortality of 0.49%, 0.68%, 0.88%, 1.60% and 0.08%, respectively. A 1 °C decrease below the minimum-mortality <span class="hlt">temperature</span> corresponded to a 3.81% increase in OHCD mortality on lags days 0-21, and a 1 °C increase above minimum-mortality <span class="hlt">temperature</span> corresponded to a 4.61% increase over lag days 0-3. No effects were found for in-hospital coronary deaths. This analysis suggests that <span class="hlt">air</span> pollution, low <span class="hlt">temperature</span> and high <span class="hlt">temperature</span> may increase the risk of OHCDs. Copyright © 2015 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GRC-1944-C-05818.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GRC-1944-C-05818.html"><span>Altitude <span class="hlt">Wind</span> Tunnel Control Room at the Aircraft Engine Research Laboratory</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1944-07-21</p> <p>Operators in the control room for the Altitude <span class="hlt">Wind</span> Tunnel at the National Advisory Committee for Aeronautics (NACA) Aircraft Engine Research Laboratory remotely operate a Wright R–3350 engine in the tunnel’s test section. Four of the engines were used to power the B–29 Superfortress, a critical weapon in the Pacific theater during World War II. The <span class="hlt">wind</span> tunnel, which had been in operation for approximately six months, was the nation’s only <span class="hlt">wind</span> tunnel capable of testing full-scale engines in simulated altitude conditions. The soundproof control room was used to operate the <span class="hlt">wind</span> tunnel and control the engine being run in the test section. The operators worked with assistants in the adjacent Exhauster Building and Refrigeration Building to manage the large altitude simulation systems. The operator at the center console controlled the tunnel’s drive fan and operated the engine in the test section. Two sets of pneumatic levers near his right forearm controlled engine fuel flow, speed, and cooling. Panels on the opposite wall, out of view to the left, were used to manage the combustion <span class="hlt">air</span>, refrigeration, and exhauster systems. The control panel also displayed the master <span class="hlt">air</span> speed, altitude, and <span class="hlt">temperature</span> gauges, as well as a plethora of pressure, <span class="hlt">temperature</span>, and airflow readings from different locations on the engine. The operator to the right monitored the manometer tubes to determine the pressure levels. Despite just being a few feet away from the roaring engine, the control room remained quiet during the tests.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AtmRe.196...62S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AtmRe.196...62S"><span>Intense <span class="hlt">air</span>-sea exchanges and heavy orographic precipitation over Italy: The role of Adriatic sea surface <span class="hlt">temperature</span> uncertainty</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stocchi, Paolo; Davolio, Silvio</p> <p>2017-11-01</p> <p>Strong and persistent low-level <span class="hlt">winds</span> blowing over the Adriatic basin are often associated with intense precipitation events over Italy. Typically, in case of moist southeasterly <span class="hlt">wind</span> (Sirocco), rainfall affects northeastern Italy and the Alpine chain, while with cold northeasterly currents (Bora) precipitations are localized along the eastern slopes of the Apennines and central Italy coastal areas. These events are favoured by intense <span class="hlt">air</span>-sea interactions and it is reasonable to hypothesize that the Adriatic sea surface <span class="hlt">temperature</span> (SST) can affect the amount and location of precipitation. High-resolution simulations of different Bora and Sirocco events leading to severe precipitation are performed using a convection-permitting model (MOLOCH). Sensitivity experiments varying the SST initialization field are performed with the aim of evaluating the impact of SST uncertainty on precipitation forecasts, which is a relevant topic for operational weather predictions, especially at local scales. Moreover, diagnostic tools to compute water vapour fluxes across the Italian coast and atmospheric water budget over the Adriatic Sea have been developed and applied in order to characterize the <span class="hlt">air</span> mass that feeds the precipitating systems. Finally, the investigation of the processes through which the SST influences location and intensity of heavy precipitation allows to gain a better understanding on mechanisms conducive to severe weather in the Mediterranean area and in the Adriatic basin in particular. Results show that the effect of the Adriatic SST (uncertainty) on precipitation is complex and can vary considerably among different events. For both Bora and Sirocco events, SST does not influence markedly the atmospheric water budget or the degree of moistening of <span class="hlt">air</span> that flows over the Adriatic Sea. SST mainly affects the stability of the atmospheric boundary layer, thus influencing the flow dynamics and the orographic flow regime, and in turn, the precipitation pattern.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22022361','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22022361"><span>Perceiving nasal patency through mucosal cooling rather than <span class="hlt">air</span> <span class="hlt">temperature</span> or nasal resistance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhao, Kai; Blacker, Kara; Luo, Yuehao; Bryant, Bruce; Jiang, Jianbo</p> <p>2011-01-01</p> <p>Adequate perception of nasal airflow (i.e., nasal patency) is an important consideration for patients with nasal sinus diseases. The perception of a lack of nasal patency becomes the primary symptom that drives these patients to seek medical treatment. However, clinical assessment of nasal patency remains a challenge because we lack objective measurements that correlate well with what patients perceive. The current study examined factors that may influence perceived patency, including <span class="hlt">air</span> <span class="hlt">temperature</span>, humidity, mucosal cooling, nasal resistance, and trigeminal sensitivity. Forty-four healthy subjects rated nasal patency while sampling <span class="hlt">air</span> from three facial exposure boxes that were ventilated with untreated room <span class="hlt">air</span>, cold <span class="hlt">air</span>, and dry <span class="hlt">air</span>, respectively. In all conditions, <span class="hlt">air</span> <span class="hlt">temperature</span> and relative humidity inside each box were recorded with sensors connected to a computer. Nasal resistance and minimum airway cross-sectional area (MCA) were measured using rhinomanometry and acoustic rhinometry, respectively. General trigeminal sensitivity was assessed through lateralization thresholds to butanol. No significant correlation was found between perceived patency and nasal resistance or MCA. In contrast, <span class="hlt">air</span> <span class="hlt">temperature</span>, humidity, and butanol threshold combined significantly contributed to the ratings of patency, with mucosal cooling (heat loss) being the most heavily weighted predictor. <span class="hlt">Air</span> humidity significantly influences perceived patency, suggesting that mucosal cooling rather than <span class="hlt">air</span> <span class="hlt">temperature</span> alone provides the trigeminal sensation that results in perception of patency. The dynamic cooling between the airstream and the mucosal wall may be quantified experimentally or computationally and could potentially lead to a new clinical evaluation tool.</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('https://ntrs.nasa.gov/search.jsp?R=20040171661&hterms=saber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsaber','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040171661&hterms=saber&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsaber"><span>Analysis of <span class="hlt">Temperature</span> and <span class="hlt">Wind</span> Measurements from the TIMED Mission: Comparison with UARS Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Huang, Frank; Mayr, Hans; Killeen, Tim; Russell, Jim; Reber, Skip</p> <p>2004-01-01</p> <p>We report on an analysis of <span class="hlt">temperature</span> and <span class="hlt">wind</span> data based respectively on measurements with the SABER (Sounding of the Atmosphere using Broadband Emission Radiometry) and TIDI (TIMED Doppler Interferometer) instruments on the TIMED (Thermosphere-Ionosphere-Mesosphere-Energetics and Dynamics) mission. Comparisons are made with corresponding results obtained from the HRDI (High Resolution Doppler Imager), MLS (Microwave Limb Sounder) and CLAES (Cryogenic Limb Array Etalon Spectrometer) instruments on the UARS (Upper Atmosphere Research Satellite) spacecraft. The TIMED and UARS instruments have important common and uncommon properties in their sampling of the data as a function local solar time. For comparison between the data from the two satellite missions, we present the derived diurnal tidal and zonal-mean variations of <span class="hlt">temperature</span> and <span class="hlt">winds</span>, obtained as functions of season, latitude, and altitude. The observations are also compared with results from the Numerical Spectral Model (NSM).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900033104&hterms=evapotranspiration&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Devapotranspiration','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900033104&hterms=evapotranspiration&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Devapotranspiration"><span>On estimating total daily evapotranspiration from remote surface <span class="hlt">temperature</span> measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carlson, Toby N.; Buffum, Martha J.</p> <p>1989-01-01</p> <p>A method for calculating daily evapotranspiration from the daily surface energy budget using remotely sensed surface <span class="hlt">temperature</span> and several meteorological variables is presented. Vaules of the coefficients are determined from simulations with a one-dimensional boundary layer model with vegetation cover. Model constants are obtained for vegetation and bare soil at two <span class="hlt">air</span> <span class="hlt">temperature</span> and <span class="hlt">wind</span> speed levels over a range of surface roughness and <span class="hlt">wind</span> speeds. A different means of estimating the daily evapotranspiration based on the time rate of increase of surface <span class="hlt">temperature</span> during the morning is also considered. Both the equations using our model-derived constants and field measurements are evaluated, and a discussion of sources of error in the use of the formulation is given.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29696842','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29696842"><span>[Effects of <span class="hlt">wind</span> speed on drying processes of fuelbeds composed of Mongolian oak broad-leaves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Li Bin; Sun, Ping; Jin, Sen</p> <p>2016-11-18</p> <p>Water desorption processes of fuel beds with Mongolian oak broad-leaves were observed under conditions with various <span class="hlt">wind</span> speeds but nearly constant <span class="hlt">air</span> <span class="hlt">temperature</span> and humidity. The effects of <span class="hlt">wind</span> speed on drying coefficients of fuel beds with various moisture contents were analyzed. Three phases of drying process, namely high initial moisture content (>75%) of phase 1, transition state of phase 2, and equilibrium phase III could be identified. During phase 1, water loss rate under higher <span class="hlt">wind</span> speed was higher than that under lower <span class="hlt">wind</span> speed. Water loss rate under higher <span class="hlt">wind</span> speed was lower than that under lower <span class="hlt">wind</span> speed during phase 2. During phase 3, water loss rates under different <span class="hlt">wind</span> speeds were similar. The <span class="hlt">wind</span> effects decreased with the decrease of fuel moisture. The drying coefficient of the Mongolian oak broad-leaves fuel beds was affected by <span class="hlt">wind</span> speed and fuel bed compactness, and the interaction between these two factors. The coefficient increased with <span class="hlt">wind</span> speed roughly in a monotonic cubic polynomial form.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23192299','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23192299"><span>Numerical modeling on <span class="hlt">air</span> quality in an urban environment with changes of the aspect ratio and <span class="hlt">wind</span> direction.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yassin, Mohamed F</p> <p>2013-06-01</p> <p>Due to heavy traffic emissions within an urban environment, <span class="hlt">air</span> quality during the last decade becomes worse year by year and hazard to public health. In the present work, numerical modeling of flow and dispersion of gaseous emissions from vehicle exhaust in a street canyon were investigated under changes of the aspect ratio and <span class="hlt">wind</span> direction. The three-dimensional flow and dispersion of gaseous pollutants were modeled using a computational fluid dynamics (CFD) model which was numerically solved using Reynolds-averaged Navier-Stokes (RANS) equations. The diffusion flow field in the atmospheric boundary layer within the street canyon was studied for different aspect ratios (W/H=1/2, 3/4, and 1) and <span class="hlt">wind</span> directions (θ=90°, 112.5°, 135°, and 157.5°). The numerical models were validated against <span class="hlt">wind</span> tunnel results to optimize the turbulence model. The numerical results agreed well with the <span class="hlt">wind</span> tunnel results. The simulation demonstrated that the minimum concentration at the human respiration height within the street canyon was on the windward side for aspect ratios W/H=1/2 and 1 and <span class="hlt">wind</span> directions θ=112.5°, 135°, and 157.5°. The pollutant concentration level decreases as the <span class="hlt">wind</span> direction and aspect ratio increase. The <span class="hlt">wind</span> velocity and turbulence intensity increase as the aspect ratio and <span class="hlt">wind</span> direction increase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790046097&hterms=moderating&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmoderating','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790046097&hterms=moderating&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dmoderating"><span>Simulating the moderating effect of a lake on downwind <span class="hlt">temperatures</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bill, R. G., Jr.; Chen, E.; Sutherland, R. A.; Bartholic, J. F.</p> <p>1979-01-01</p> <p>A steady-state, two-dimensional numerical model is used to simulate <span class="hlt">air</span> <span class="hlt">temperatures</span> and humidity downwind of a lake at night. Thermal effects of the lake were modelled for the case of moderate and low surface <span class="hlt">winds</span> under the cold-<span class="hlt">air</span> advective conditions that occur following the passage of a cold front. Surface <span class="hlt">temperatures</span> were found to be in good agreement with observations. A comparison of model results with thermal imagery indicated the model successfully predicts the downwind distance for which thermal effects due to the lake are significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/caa-permitting/final-permit-documents-cape-wind-associates-llc-horseshoe-shoal-nantucket-sound','PESTICIDES'); return false;" href="https://www.epa.gov/caa-permitting/final-permit-documents-cape-wind-associates-llc-horseshoe-shoal-nantucket-sound"><span>Final Permit Documents for the Cape <span class="hlt">Wind</span> Associates, LLC, Horseshoe Shoal, Nantucket Sound (Offshore Renewable Energy Project/OCS <span class="hlt">Air</span> Permit)</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>List of finla permit documents for the Cape <span class="hlt">Wind</span> Associates, LLC, Horseshoe Shoal, Nantucket Sound (Offshore Renewable Energy Project/OCS <span class="hlt">Air</span> Permit: Massachusetts Plan Approval including nonattainment NSR Appendix A requirements).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51A2008K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51A2008K"><span>Comparison of <span class="hlt">Wind</span> Speeds and <span class="hlt">Temperatures</span> Simulated by the Local Data Assimilation and Prediction System with Those observed at AWSs in Korea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>KIM, D. J.; Kim, J.</p> <p>2017-12-01</p> <p>In this study, the characteristics of 10-m <span class="hlt">wind</span> speeds and 2-m <span class="hlt">temperatures</span> predicted by the local data assimilation and prediction system (LDAPS) in Korea meteorological administration (KMA) were analyzed by comparing those observed at automatic weather stations (AWSs). The LDAPS is a currently operating meteorology prediction system with the horizontal resolution of about 1.5 km. We classified the AWSs into four categories (urban, rural, coastal, and mountainous areas) based on the surrounding land-use types and locations of the AWSs and selected 30 AWSs for each category. For each category, we investigated how well the LDAPS predicted 10-m <span class="hlt">wind</span> speeds and 2-m <span class="hlt">temperatures</span> at the AWSs and statistically analyzed the LDAPS characteristics in predicting the meteorological variables. In the mountainous area, the LDAPS underestimated 2-m <span class="hlt">temperatures</span> due to the resolution and coordinate system of the LDAPS. In the urban area, the LDAPS overestimated the 10-m <span class="hlt">wind</span> speeds and underestimated the 2-m <span class="hlt">temperatures</span>, implying that the LDAPS should consider the physical process to reflect the urban effects on <span class="hlt">wind</span> speeds and <span class="hlt">temperatures</span> in urban areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..254r2012T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..254r2012T"><span>Effect of <span class="hlt">air</span> gap on apparent <span class="hlt">temperature</span> of body wearing various sizes of T-shirt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takatera, M.; Uchiyama, E.; Zhu, C.; Kim, KO; Ishizawa, H.</p> <p>2017-10-01</p> <p>We investigated the effect of <span class="hlt">air</span> gap on the apparent <span class="hlt">temperature</span>. Using the developed thermocouple fabric and a thermal manikin, we measured <span class="hlt">temperature</span> distribution of the measuring garments due to the change of T-shirt sizes. We were able to measure the apparent <span class="hlt">temperature</span> distribution at points near a body while wearing different sizes of T-shirts. It was observed that the <span class="hlt">temperature</span> distribution depending on different <span class="hlt">air</span> gap between clothing and body. The apparent <span class="hlt">temperature</span> depends on garment size and place. The effect of <span class="hlt">air</span> gap on apparent <span class="hlt">temperature</span> of body was experimentally confirmed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH11B2447J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH11B2447J"><span>High Time-Resolved Kinetic <span class="hlt">Temperatures</span> of Solar <span class="hlt">Wind</span> Minor Ions Measured with SOHO/CELIAS/CTOF</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Janitzek, N. P.; Berger, L.; Drews, C.; Wimmer-Schweingruber, R. F.</p> <p>2017-12-01</p> <p>Solar <span class="hlt">wind</span> heavy ions with an atomic number Z > 2 are referred to as minor ions since they represent a fraction of less than one percent of all solar <span class="hlt">wind</span> ions. They can be therefore regarded as test particles, only reacting to but not driving the dynamics of the solar <span class="hlt">wind</span> plasma, which makes them a unique diagnostic tool for plasma wave phenomena both in the solar atmosphere and the extended heliosphere. In the past, several studies have investigated the kinetic <span class="hlt">temperatures</span> of minor ions, but due to low counting statistics these studies are based on ion velocity distribution functions (VDFs) recorded over time periods of several hours. The Charge Time-Of-Flight (CTOF) mass spectrometer as part of the Charge, ELement and Isotope Analysis System (CELIAS) onboard the SOlar and Heliospheric Observatory (SOHO) provides solar <span class="hlt">wind</span> heavy ion 1D radial VDFs with excellent charge state separation, an unprecedented cadence of 5 minutes and very high counting statistics, exceeding similar state-of-the-art instruments by a factor of ten. In our study, based on CTOF measurements at Langrangian point L1 between DOY 150 and DOY 220 in 1996, we investigate systematically the influence of the VDF time resolution on the derived kinetic <span class="hlt">temperatures</span> for solar <span class="hlt">wind</span> silicon and iron ions. The selected ion set spans a wide range of mass-per-charge from 3 amu/e < m/q < 8 amu/e. Therefore, it is suitable for the search of signatures of gyrofrequency-dependent heating processes resulting from the resonant interaction of heavy ions with ion-cyclotron waves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28163877','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28163877"><span><span class="hlt">Wind</span> and water tunnel testing of a morphing aquatic micro <span class="hlt">air</span> vehicle.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Siddall, Robert; Ortega Ancel, Alejandro; Kovač, Mirko</p> <p>2017-02-06</p> <p>Aerial robots capable of locomotion in both <span class="hlt">air</span> and water would enable novel mission profiles in complex environments, such as water sampling after floods or underwater structural inspections. The design of such a vehicle is challenging because it implies significant propulsive and structural design trade-offs for operation in both fluids. In this paper, we present a unique Aquatic Micro <span class="hlt">Air</span> Vehicle (AquaMAV), which uses a reconfigurable wing to dive into the water from flight, inspired by the plunge diving strategy of water diving birds in the family Sulidae . The vehicle's performance is investigated in <span class="hlt">wind</span> and water tunnel experiments, from which we develop a planar trajectory model. This model is used to predict the dive behaviour of the AquaMAV, and investigate the efficacy of passive dives initiated by wing folding as a means of water entry. The paper also includes first field tests of the AquaMAV prototype where the folding wings are used to initiate a plunge dive.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5206604','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5206604"><span><span class="hlt">Wind</span> and water tunnel testing of a morphing aquatic micro <span class="hlt">air</span> vehicle</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ortega Ancel, Alejandro; Kovač, Mirko</p> <p>2017-01-01</p> <p>Aerial robots capable of locomotion in both <span class="hlt">air</span> and water would enable novel mission profiles in complex environments, such as water sampling after floods or underwater structural inspections. The design of such a vehicle is challenging because it implies significant propulsive and structural design trade-offs for operation in both fluids. In this paper, we present a unique Aquatic Micro <span class="hlt">Air</span> Vehicle (AquaMAV), which uses a reconfigurable wing to dive into the water from flight, inspired by the plunge diving strategy of water diving birds in the family Sulidae. The vehicle's performance is investigated in <span class="hlt">wind</span> and water tunnel experiments, from which we develop a planar trajectory model. This model is used to predict the dive behaviour of the AquaMAV, and investigate the efficacy of passive dives initiated by wing folding as a means of water entry. The paper also includes first field tests of the AquaMAV prototype where the folding wings are used to initiate a plunge dive. PMID:28163877</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29931637','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29931637"><span>The contribution of <span class="hlt">wind</span> wave changes on diminishing ice period in Lake Pyhäjärvi during the last half-century.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wu, Tingfeng; Qin, Boqiang; Zhu, Guangwei; Huttula, Timo; Lindfors, Antti; Ventelä, Anne-Mari; Sheng, Yongwei; Ambrose, Richard F</p> <p>2018-06-21</p> <p>To address the contribution of long-term <span class="hlt">wind</span> wave changes on diminishing ice period in Northern European lakes, an in situ observation of <span class="hlt">wind</span> waves was conducted to calibrate a <span class="hlt">wind</span>-wave numerical model for Lake Pyhäjärvi, which is the largest lake in southwest Finland. Using station-measured hydrometeorological data from 1963 to 2013 and model-simulated <span class="hlt">wind</span> waves, correlation and regression analyses were conducted to assess the changing trend and main influences on ice period. Ice period in Lake Pyhäjärvi decreased significantly over 51 years (r = 0.47, P < 0.01). The analysis of main hydrometeorological factors to ice period showed that the significant <span class="hlt">air</span> <span class="hlt">temperature</span> rise is the main contributor for the diminishing of ice period in the lake. Besides <span class="hlt">air</span> <span class="hlt">temperature</span>, <span class="hlt">wind</span>-induced waves can also weaken lake ice by increasing water mixing and lake ice breakage. The regression indicated that mean significant wave height in December and April was negatively related to ice period (r = - 0.48, P < 0.01). These results imply that long-term changes of <span class="hlt">wind</span> waves related to climate change should be considered to fully understand the reduction of aquatic ice at high latitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JASTP..71..841K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JASTP..71..841K"><span>ARIMA representation for daily solar irradiance and surface <span class="hlt">air</span> <span class="hlt">temperature</span> time series</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kärner, Olavi</p> <p>2009-06-01</p> <p>Autoregressive integrated moving average (ARIMA) models are used to compare long-range temporal variability of the total solar irradiance (TSI) at the top of the atmosphere (TOA) and surface <span class="hlt">air</span> <span class="hlt">temperature</span> series. The comparison shows that one and the same type of the model is applicable to represent the TSI and <span class="hlt">air</span> <span class="hlt">temperature</span> series. In terms of the model type surface <span class="hlt">air</span> <span class="hlt">temperature</span> imitates closely that for the TSI. This may mean that currently no other forcing to the climate system is capable to change the random walk type variability established by the varying activity of the rotating Sun. The result should inspire more detailed examination of the dependence of various climate series on short-range fluctuations of TSI.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AIPC.1699f0006D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AIPC.1699f0006D"><span>The effect of <span class="hlt">air</span> <span class="hlt">temperature</span> on the sappan wood extract drying</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Djaeni, M.; Triyastuti, M. S.; Asiah, N.; Annisa, A. N.; Novita, D. A.</p> <p>2015-12-01</p> <p>The sappan wood extract contain natural colour called brazilin that can be used as a food colouring and antioxidant. The product is commonly found as a dry extract powder for consummer convenience. The spray dryer with <span class="hlt">air</span> dehumidification can be an option to retain the colour and antioxidant agent. This paper discusses the effect of <span class="hlt">air</span> <span class="hlt">temperature</span> on sappan wood extract drying that was mixed with maltodextrin. As responses, the particle size, final moisture content, and extract solubility degradation were observed. In all cases, the process conducted in <span class="hlt">temperature</span> ranging 90 - 110°C can retain the brazilin quality as seen in solubility and particle size. In addition, the sappan wood extract can be fully dried with moisture content below 2%. Moreover, with the increase of <span class="hlt">air</span> <span class="hlt">temperature</span>, the particle size of dry extract can be smaller.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004MeScT..15..413L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004MeScT..15..413L"><span>A new ultrasonic <span class="hlt">temperature</span> measurement system for <span class="hlt">air</span> conditioners in automobiles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liao, Teh-Lu; Tsai, Wen-Yuan; Huang, Chih-Feng</p> <p>2004-02-01</p> <p>This paper presents a microcomputer-based ultrasonic <span class="hlt">temperature</span> sensor system to measure the <span class="hlt">temperature</span> of an <span class="hlt">air</span> conditioner (AC) in an automobile. It uses the ultrasonic measurement of the changes in the speed of sound in the <span class="hlt">air</span> to determine the <span class="hlt">temperature</span> of the environmental <span class="hlt">air</span>. The changes in the speed of sound are calculated by combining time-of-flight (TOF) and phase shift techniques. This method can work in a wider range than using phase shift alone and is more accurate than the TOF scheme. In the proposed system, we use 40 ± 2 kHz ultrasonic transducers and adopt a single-pass operation. An 89c51 single-chip microcomputer-based binary frequency shift-keyed (BFSK) signal generator and phase detector are designed to record and calculate the TOF, phase shift of the two frequencies and <span class="hlt">temperature</span>. These data are then sent to either an LCD display or to a PC for calibration and examination. Experimental results show that the proposed measurement system has a high accuracy of ± 0.4 °C from 0 to 80 °C and can reflect the <span class="hlt">temperature</span> change within 100 ms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012MAP...117..181Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012MAP...117..181Z"><span>Hourly predictive Levenberg-Marquardt ANN and multi linear regression models for predicting of dew point <span class="hlt">temperature</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zounemat-Kermani, Mohammad</p> <p>2012-08-01</p> <p>In this study, the ability of two models of multi linear regression (MLR) and Levenberg-Marquardt (LM) feed-forward neural network was examined to estimate the hourly dew point <span class="hlt">temperature</span>. Dew point <span class="hlt">temperature</span> is the <span class="hlt">temperature</span> at which water vapor in the <span class="hlt">air</span> condenses into liquid. This <span class="hlt">temperature</span> can be useful in estimating meteorological variables such as fog, rain, snow, dew, and evapotranspiration and in investigating agronomical issues as stomatal closure in plants. The availability of hourly records of climatic data (<span class="hlt">air</span> <span class="hlt">temperature</span>, relative humidity and pressure) which could be used to predict dew point <span class="hlt">temperature</span> initiated the practice of modeling. Additionally, the <span class="hlt">wind</span> vector (<span class="hlt">wind</span> speed magnitude and direction) and conceptual input of weather condition were employed as other input variables. The three quantitative standard statistical performance evaluation measures, i.e. the root mean squared error, mean absolute error, and absolute logarithmic Nash-Sutcliffe efficiency coefficient ( {| {{{Log}}({{NS}})} |} ) were employed to evaluate the performances of the developed models. The results showed that applying <span class="hlt">wind</span> vector and weather condition as input vectors along with meteorological variables could slightly increase the ANN and MLR predictive accuracy. The results also revealed that LM-NN was superior to MLR model and the best performance was obtained by considering all potential input variables in terms of different evaluation criteria.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010055268','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010055268"><span>Apparatus and Method for Measuring <span class="hlt">Air</span> <span class="hlt">Temperature</span> Ahead of an Aircraft for Controlling a Variable Inlet/Engine Assembly</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gary, Bruce L. (Inventor)</p> <p>2001-01-01</p> <p>The apparatus and method employ remote sensing to measure the <span class="hlt">air</span> <span class="hlt">temperature</span> a sufficient distance ahead of the aircraft to allow time for a variable inlet/engine assembly to be reconfigured in response to the measured <span class="hlt">temperature</span>, to avoid inlet unstart and/or engine compressor stall. In one embodiment, the apparatus of the invention has a remote sensor for measuring at least one <span class="hlt">air</span> <span class="hlt">temperature</span> ahead of the vehicle and an inlet control system for varying the inlet. The remote sensor determines a change in <span class="hlt">temperature</span> value using at least one <span class="hlt">temperature</span> measurement and prior <span class="hlt">temperature</span> measurements corresponding to the location of the aircraft. The control system uses the change in <span class="hlt">air</span> <span class="hlt">temperature</span> value to vary the inlet configuration to maintain the position of the shock wave during the arrival of the measured <span class="hlt">air</span> in the inlet. In one embodiment, the method of the invention includes measuring at least one <span class="hlt">air</span> <span class="hlt">temperature</span> ahead of the vehicle, determining an <span class="hlt">air</span> <span class="hlt">temperature</span> at the vehicle from prior <span class="hlt">air</span> <span class="hlt">temperature</span> measurements, determining a change in <span class="hlt">temperature</span> value using the <span class="hlt">air</span> <span class="hlt">temperature</span> at the vehicle and the at least one <span class="hlt">air</span> <span class="hlt">temperature</span> measurement ahead of the vehicle, and using the change in <span class="hlt">temperature</span> value to-reposition the airflow inlet, to cause the shock wave to maintain substantially the same position within the inlet as the airflow <span class="hlt">temperature</span> changes within the inlet.</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 <span class="hlt">temperature</span> gradients and vertical <span class="hlt">wind</span> shear on MLT region 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 <span class="hlt">temperature</span> measurements were taken successfully from 2007 to 2009 in the mesopause region over São José dos Campos (23.1°S, 45.9°W). Strong gradients on these vertical <span class="hlt">temperature</span> profiles are often observed. A simple theoretical study has shown that <span class="hlt">temperature</span> 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 region. 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 <span class="hlt">temperature</span>, 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 region 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('http://adsabs.harvard.edu/abs/1998APS..DFD..DI02L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998APS..DFD..DI02L"><span>Natural ventilation of buildings: opposing <span class="hlt">wind</span> and buoyancy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Linden, Paul; Hunt, Gary</p> <p>1998-11-01</p> <p>The use of natural ventilation in buildings is an attractive way to reduce energy usage thereby reducing costs and CO2 emissions. Generally, it is necessary to remove excess heat from a building and the designer can use the buoyancy forces associated with the above ambient <span class="hlt">temperatures</span> within the building to drive a flow - 'stack' ventilation. The most efficient mode is displacement ventilation where warm <span class="hlt">air</span> accumulates near the top of the building and flows out through upper level vents and cooler <span class="hlt">air</span> flows in at lower levels. Ventilation will also be driven between these lower and upper openings by the <span class="hlt">wind</span>. We report on laboratory modeling and theory which investigates the effects of an opposing <span class="hlt">wind</span> on stack ventilation driven by a constant source of heat within a space under displacement ventilation. We show that there is a critical <span class="hlt">wind</span> speed, expressed in dimensionless terms as a critical Froude number, above which displacement ventilation is replaced by (less efficient) mixing ventilation with reversed flow. Below this critical speed, displacement ventilation, in which the interior has a two-layer stratification, is maintained. The criterion for the change in ventilation mode is derived from general considerations of mixing efficiencies in stratified flows. We conclude that even when <span class="hlt">wind</span> effects might appear to be dominant, the inhibition of mixing by the stable stratification within the space ensures that stack ventilation can operate over a wide range of apparently adverse conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3192719','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3192719"><span>Perceiving Nasal Patency through Mucosal Cooling Rather than <span class="hlt">Air</span> <span class="hlt">Temperature</span> or Nasal Resistance</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhao, Kai; Blacker, Kara; Luo, Yuehao; Bryant, Bruce; Jiang, Jianbo</p> <p>2011-01-01</p> <p>Adequate perception of nasal airflow (i.e., nasal patency) is an important consideration for patients with nasal sinus diseases. The perception of a lack of nasal patency becomes the primary symptom that drives these patients to seek medical treatment. However, clinical assessment of nasal patency remains a challenge because we lack objective measurements that correlate well with what patients perceive.The current study examined factors that may influence perceived patency, including <span class="hlt">air</span> <span class="hlt">temperature</span>, humidity, mucosal cooling, nasal resistance, and trigeminal sensitivity. Forty-four healthy subjects rated nasal patency while sampling <span class="hlt">air</span> from three facial exposure boxes that were ventilated with untreated room <span class="hlt">air</span>, cold <span class="hlt">air</span>, and dry <span class="hlt">air</span>, respectively. In all conditions, <span class="hlt">air</span> <span class="hlt">temperature</span> and relative humidity inside each box were recorded with sensors connected to a computer. Nasal resistance and minimum airway cross-sectional area (MCA) were measured using rhinomanometry and acoustic rhinometry, respectively. General trigeminal sensitivity was assessed through lateralization thresholds to butanol. No significant correlation was found between perceived patency and nasal resistance or MCA. In contrast, <span class="hlt">air</span> <span class="hlt">temperature</span>, humidity, and butanol threshold combined significantly contributed to the ratings of patency, with mucosal cooling (heat loss) being the most heavily weighted predictor. <span class="hlt">Air</span> humidity significantly influences perceived patency, suggesting that mucosal cooling rather than <span class="hlt">air</span> <span class="hlt">temperature</span> alone provides the trigeminal sensation that results in perception of patency. The dynamic cooling between the airstream and the mucosal wall may be quantified experimentally or computationally and could potentially lead to a new clinical evaluation tool. PMID:22022361</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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