X-Band Scanning ARM Cloud Radar (XSACR) Cross-Wind RHI Scan Corrected (c1)
X-Band Scanning ARM Cloud Radar (XSACR) Cross-Wind RHI Scan Corrected
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X-Band Scanning ARM Cloud Radar (XSACR) Cross-Wind RHI Scan Corrected
X-Band Scanning ARM Cloud Radar (XSACR) Vertically Pointing Scan Corrected
X-Band Scanning ARM Cloud Radar (XSACR) Hemispherical Sky RHI Scans (6 horizon-to-horizon scans at 30-degree azimuth intervals) Corrected
X-Band Scanning ARM Cloud Radar (XSACR) Boundary Layer RHI Scan Corrected
The micropulse lidar (MPL) is a ground-based, optical, remote-sensing system designed primarily to determine the altitude of clouds; however, it is also used for detection of atmospheric aerosols. The physical principle is the same as for radar. Pulses of energy are transmitted into the atmosphere; the energy scattered back to the transceiver is collected and measured as a time-resolved signal, thereby detecting clouds and aerosols in real time. From the time delay between each outgoing pulse and the backscattered signal, the distance to the scatterer is inferred. Post-processing of the lidar return characterizes the extent and properties of aerosols or other particles in a region.
C-Band Scanning ARM Precipitation Radar, CF/Radial Formatted, Quality Controlled Tobac Tracking
C-Band Scanning ARM Precipitation Radar, CF/Radial Formatted, Quality Controlled Tobac Tracking Cloud Mask
Ka-Band ARM Zenith Radar, 2nd Generation, Precipitation Mode, Quality Control Corrections Applied
This data set contains multi-Doppler radar analysis from CSAPR-2, CSU-CHIVO, COW, and RMA-1 radars. These radars were collecting dual-polarization data during the CACTI/RELAMPAGO experiments in Argentina in 2018. Doppler analysis is systematically conducted for 31 days with convection. Three-dimensional wind fields are retrieved using the PyDDA algorithm. Dual-polarization information is also included in the data set.
C Scanning ARM Precipitation Radar 2nd generation (CSAPR2), Corrected Moments in Antenna Coordinates (CMAC)
Two major telecommunication activities were in process during the Venus encounter of 1962, the largest, activity involved the two-way communications and tracking of the Mariner spacecraft from the DSIF (Deep Space Instrumentation Facility) stations on the earth. The first, and by far the largest activity involved the two-way communications and tracking of the Mariner spacecraft from the DSIF stations on the earth. The DSIF includes stations at Goldstone, California; Woomera, Australia; and Johannesburg, South Africa. The second activity involved an earth-based radar which reflected signals off the planet Venus during the same month that the Mariner spacecraft was traveling toward the planet.
Electrical characteristics of the atmosphere and surface of venus from radar observation
Radar exploration of Venus - radiometer, spectral and polarization studies, automatic frequency tracking, frequency-time mapping, and amplitude modulated ranging
Antenna measurements at 35, 70 and 94 gc frequencies of Venus radiation characteristics, i.e., brightness temperature
Closed-loop range-locked radar system successful in range-tracking planet Venus
Estimates of permittivity and specular points on lunar surface
Planetary radar system at Venus site of NASA DEEP Space Instrumentation Facility for space communications, noting continuous-wave transmitters and receivers