The Deep Structure of Coronae on Venus: The Beta-Atla-Themis Region

Details The Deep Structure of Coronae on Venus: The Beta-Atla-Themis Region The Deep Structure of Coronae on Venus: The Beta-Atla-Themis Region

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1430p&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1430

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Scientific paper

Gravity modeling indicates the presence of hot diapirs under some large
coronae in the BAT region of Venus. Other coronae are located over
regions of average mantle temperature, indicating a significant period
of thermal cooling since those coronae formed.

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