A radar investigation of the solar corona
Radar measurements of solar corona, and average radar cross section of sun
SEARCH · Engineering Papers
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
Radar measurements of solar corona, and average radar cross section of sun
Radar tracking parameters and contact time errors from graphic estimation of radar tracking coverage of near earth orbits
An optimum method for determining satellite orbits from radar data is presented in this report. Offering a good combination of speed and accuracy, the method makes use of orbit inclination and orbit elements in the plane, and proceeds with a differential correction of the orbit elements. Rapid, accurate methods of computing orbit elements are required to predict satellite positions for acquisition by other radars at points later along the orbit. In some cases the data are limited to a single pass over the observing station. The dynamical method is described in detail, and its accuracy is compared with those of two other methods: the purely geometrical, and the least-squares geometrical. By this optimum method the computing time, including the differential correction time, is 1 minute. Without differential correction, the rough determination takes from 10 to 20 seconds with approximately 5 miles positional uncertainty.
Understanding the spatial heterogeneity beneath Thwaites Glacier, West Antarctica, is vital to projecting its impact on future sea levels. Radar-echo sounding (RES) is commonly used to infer subglacial conditions, but these data can be challenging to interpret. We assess basal heterogeneity across Thwaites Glacier by comparing RES returns to a radar backscattering simulator for over 400 km of RES data. The modeled variations in bed returned power exhibited a strong correlation with actual RES data in 40% of our simulated flight segments, which we consider evidence for a relatively homogeneous glacier bed. Other sites (40%) demonstrated improved fit quality when hydrology or substrate transitions were introduced in the bed material model. The remaining simulated segments (20%) were diagnosed as having more complex basal heterogeneity. The spatial distribution of complex heterogeneity appears to coincide with asymmetric patterns in the RES specularity content, which has been interpreted in previous studies as a signature for channelized hydrology. Conversely, the homogeneous substrate locations coincide with areas of fast-moving ice in western Thwaites. Our simulation method can isolate power variations induced by material heterogeneity vs topography, which is an important limitation of existing RES analysis methods.
Pulse and cw radar techniques for measurement and detection of echo power and their application to planets
Pulse and CW radar techniques for measurement and detection of echo power and their application to planets
Radar ranging of venus, the doppler effect and the determination of the astronomical unit
Theoretical expression for the terminal velocity of cylindrical radar chaff under model atmosphere conditions
Electrical characteristics of the atmosphere and surface of venus from radar observation
Description of two antennas, one with a cw transmitter and the other with a maser receiver, used in the jpl venus radar experiment in 1961
High power continuous wave radar transmitter - Space communications
Closed-loop range-locked radar system successful in range-tracking planet Venus
Cislunar medium property determinations by Doppler-frequency and Faraday-polarization lunar radar measurements
Radar observations of Venus - reflectivity, angular scattering, surface markings, and rotation measurements
Planetary radar system at Venus site of NASA DEEP Space Instrumentation Facility for space communications, noting continuous-wave transmitters and receivers
Spectrum and range spectrum analysis of Venus radar echoes obtained from experiments
1964 results of high resolution CW radar spectral studies of Venus at NASA/JPL Deep Space Instrumentation Facility at Goldstone, California
Pulsed microwave radar backscattering used in model tests of clear air turbulence detection