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Radar scattering from desert terrains, Pisgah/Lavic Region, California: Implications for MagellanA major component of the 1988 Mojave Field Experiment involved the simultaneous acquisition of quad-polarization multifrequency airborne Synthetic Aperture Radar (SAR) imaging radar data and ground measurements thought to be relevant to the radar scattering behavior of a variety of desert surfaces. In preparation for the Magellan mission to Venus, the experiment was designed to explore the ability of SAR to distinguish types of geological surfaces, and the effects of varying incidence angles on the appearance of such surfaces. The airborne SAR system acquired images at approx. 10 m resolution, at 3 incidence angles (30, 40, 50 degs) and at 3 wavelengths (P:68 cm, L:24 cm, C:5.6 cm). The polarimetric capabilities of the instrument allow the simulation of any combination of transmit and receive polarizations during data reduction. Calibrated trihedral corner reflectors were deployed within each scene to permit absolute radiometric calibration of the image data. Initial analyses of this comprehensive radar data set is reported, with emphasis on implications for interpretation of Magellan data.
Document ID
19900003127
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Plaut, J. J.
(Southern Methodist Univ. Dallas, TX., United States)
Arvidson, R. E.
(Washington Univ. Saint Louis, MO., United States)
Wall, S.
(Jet Propulsion Lab. California Inst. of Tech., Pasadena., United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Lunar and Planetary Inst., Abstracts for the Venus Geoscience Tutorial and Venus Geologic Mapping Workshop
Subject Category
Lunar And Planetary Exploration
Accession Number
90N12443
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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