Radar studies of the moon
Dielectric constants, composition, and depths of layers of moon based on two-layer lunar model using radar echoes
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Dielectric constants, composition, and depths of layers of moon based on two-layer lunar model using radar echoes
Channel capacity, propagation times, echo suppressor problems, and associated problems in development of commercial communications satellite systems
Doppler characteristics of radar echoes reflected by solar corona
Radar echo measurements for determining lunar scattering properties
Performances of Echo II passive satellite, and passive satellite communications system
Radar echo data on motion, rotation, and surface scattering properties of Venus
Radar observations of Venus - echo data and planetary retrograde motion
X-band target simulator with spectral purity for long radar echo pulses
Radio echo technique applied to measurement of electron line density in ionization trains of intermediate type
Turbulence in upper atmosphere according to radio echo observations of meteor trains
Modulator transfer functions for fixed and ramp input waveforms, and nonlinear homomorphic system for echo removal
Radar echo measurements of increased meteor counts during middle months of 1963
Oblique echo presence during winter nights on auroral and subauroral latitudes ionograms, analyzing electron number density of nighttime F region in midlatitude trough vicinity
Radar experiments of sun at 38 mc/s, presenting results on echo variation with sunspot number, coronal irregularities, etc
Stratospheric aerosol concentrations observed by optical radar echoes compared with expected return from molecular atmosphere to obtain vertical profile
Planetary radar astronomy is the study of solar system entities (the moon, asteroids, and comets, as well as the major planets and their satellites and ring systems) by transmitting radio signals towards a target and receiving and analyzing the echoes.
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.