Dark Crater-related Deposits on Venus in Radar Cross-Section -- Emissivity Domain

Details Dark Crater-related Deposits on Venus in Radar Cross-Section -- Emissivity Domain Dark Crater-related Deposits on Venus in Radar Cross-Section -- Emissivity Domain

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1290b&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1290

Physics

Scientific paper

Diffuse features (parabolas and halos) associated with impact craters on
Venus are considered as deposits of loose material. A model of
electromagnetic wave reflection by such features is applied to the
observed emissivity and radar cross-section.

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