Radar characteristics of the equatorial plains of Venus from Goldstone Observations: Implications for interpretation of Magellan data

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Abstract

Based on analyses of recent high resolution observations of the approximately 1000 km diameter Heng-0 ring structure by the Goldstone Solar System Radar, we predict that the structure is a large corona. Calibrated values of radar backscatter coefficient (σ°) indicate lateral variations of a factor of 4 in Fresnel reflectivity in the vicinity of Heng-0, as well as in other areas of the plains, at scales of tens of km. We predict that areas with very low reflectivity values, which occur in a variety of geological settings, are soil-dominated, with bulk densities as low as 1.5 g/cm3.

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