The Interior of Venus: Inferred from Long Wavelength Geoid and Topography Data

Details The Interior of Venus: Inferred from Long Wavelength Geoid and Topography Data The Interior of Venus: Inferred from Long Wavelength Geoid and Topography Data

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1696n&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1696

Physics

Scientific paper

We constrain the flow pattern and upper- lower viscosity contrast in
Venusian mantle from the observed long wavelength admittance ( geoid
height / topographic height) data using a dynamic support model.

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