Mars radar scattering - Arecibo/Goldstone results at 12.6- and 3.5-cm wavelengths

Details Mars radar scattering - Arecibo/Goldstone results at 12.6- and 3.5-cm wavelengths Mars radar scattering - Arecibo/Goldstone results at 12.6- and 3.5-cm wavelengths

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar...98..240h&link_type=abstract

Icarus (ISSN 0019-1035), vol. 98, no. 2, Aug. 1992, p. 240-253. Research supported by NASA.

Physics

17

Continuous Wave Radar, Mars (Planet), Planetary Mapping, Radar Scattering, Doppler Radar, Polarized Radiation, Radar Echoes, Ultrahigh Frequencies

Scientific paper

A wide variety of aspects of Mars radar scattering are examined. The
spatial variations and wavelength dependence of the echo were
investigated from dual-polarization continuous-wave radar observations
of Mars from the 1988 and 1990 oppositions. The Arecibo S-band and
Goldstone X-band radars were used to make the observations.

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