Formation of Novae and Coronae on Venus. Tectonophysical Modeling Using Gravity Models

Details Formation of Novae and Coronae on Venus. Tectonophysical Modeling Using Gravity Models Formation of Novae and Coronae on Venus. Tectonophysical Modeling Using Gravity Models

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1531k&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1531

Physics

1

Scientific paper

Novae and coronae formation was simulated using caoutchouc as a model of
lower ductile part of lithosphere and dry flour as a model of upper
brittle part of it. Distribution and character of the deformational
structures is described.

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