ARM: Spectra from 1290-MHz Beam-Steered Radar Wind Profiler (BSRWP) operating in low-low precipitation mode
Spectra from 1290-MHz Beam-Steered Radar Wind Profiler (BSRWP) operating in low-low precipitation mode
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Spectra from 1290-MHz Beam-Steered Radar Wind Profiler (BSRWP) operating in low-low precipitation mode
Spectra from 1290-MHz Beam-Steered Radar Wind Profiler (BSRWP) operating in low-low wind mode
Spectra from 1290-MHz Beam-Steered Radar Wind Profiler (BSRWP) operating in low precipitation mode
Spectra from 1290-MHz Beam-Steered Radar Wind Profiler (BSRWP) operating in low wind mode
1290-MHz Radar Wind Profiler, precipitation moments data
1290-MHz Radar Wind Profiler, precipitation consensus data
1290-MHz Radar Wind Profiler: Precipitation Averages, operating in high power mode
1290-MHz Radar Wind Profiler: Precipitation Averages, operating in low power mode
1290-MHz Radar Wind Profiler: Precipitation Moments, operating in high power mode
1290-MHz Radar Wind Profiler: Precipitation Moments, operating in low power mode
1290-MHz Radar Wind Profiler: Low Mode Wind Averages
1290-MHz Radar Wind Profiler: Wind Moments, operating in low power mode
915-MHz Radar Wind Profiler: Precipitation Averages, operating in high power mode
915-MHz Radar Wind Profiler: Precipitation Averages, operating in low power mode
915-MHz Radar Wind Profiler: Low Mode Wind Averages
The generation of the virtual heat flux in the convective MABL associated with the January 28, 1986 intense cold air airbreak offshore of the Carolinas is studied. A technique based on the joint frequency distribution of the virtual potential temperature and vertical motion (Mahrt and Paumier, 1984) is used. The results suggest that, if buoyancy is mainly driven by the temperature flux, the physical processes for generating buoyancy flux are about the same for boundary layers over land and ocean, even with different convective regimes.
A theoretical framework is developed to determine the so-called thermal state-of-charge (SOC) in solar heat receivers employing encapsulated phase change materials (PCMS) that undergo cyclic melting and freezing. The present problem is relevant to space solar dynamic power systems that would typically operate in low-Earth-orbit (LEO). The solar heat receiver is integrated into a closed-cycle Brayton engine that produces electric power during sunlight and eclipse periods of the orbit cycle. The concepts of available power and virtual source temperature, both on a finite-time basis, are used as the basis for determining the SOC. Analytic expressions for the available power crossing the aperture plane of the receiver, available power stored in the receiver, and available power delivered to the working fluid are derived, all of which are related to the SOC through measurable parameters. Lower and upper bounds on the SOC are proposed in order to delineate absolute limiting cases for a range of input parameters (orbital, geometric, etc.). SOC characterization is also performed in the subcooled, two-phase, and superheat regimes. Finally, a previously-developed physical and numerical model of the solar heat receiver component of NASA Lewis Research Center's Ground Test Demonstration (GTD) system is used in order to predict the SOC as a function of measurable parameters.
A theoretical framework is developed to determine the so-called thermal state-of-charge (SOC) in solar heat receivers employing encapsulated phase change materials (PCMS) that undergo cyclic melting and freezing. The present problem is relevant to space solar dynamic power systems that would typically operate in low-Earth-orbit (LEO). The solar heat receiver is integrated into a closed-cycle Brayton engine that produces electric power during sunlight and eclipse periods of the orbit cycle. The concepts of available power and virtual source temperature, both on a finite-time basis, are used as the basis for determining the SOC. Analytic expressions for the available power crossing the aperture plane of the receiver, available power stored in the receiver, and available power delivered to the working fluid are derived, all of which are related to the SOC through measurable parameters. Lower and upper bounds on the SOC are proposed in order to delineate absolute limiting cases for a range of input parameters (orbital, geometric, etc.). SOC characterization is also performed in the subcooled, two-phase, and superheat regimes. Finally, a previously-developed physical and numerical model of the solar heat receiver component of NASA Lewis Research Center's Ground Test Demonstration (GTD) system is used in order to predict the SOC as a function of measurable parameters.