Surface Properties of Venus from Arecibo 12.6 cm Radar Observations

Details Surface Properties of Venus from Arecibo 12.6 cm Radar Observations Surface Properties of Venus from Arecibo 12.6 cm Radar Observations

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1855c&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1855

Physics

Scientific paper

We used the Arecibo radar system to create Stokes' parameter and degree
of linear polarization maps of Venus. Two prominent linearly polarized
features are near impact craters with associated parabolic deposits.
Maxwell Montes also shows some linear polarization.

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