Lunar Internal Structure Estimated from Local Admittance between Gravity and Topography

Details Lunar Internal Structure Estimated from Local Admittance between Gravity and Topography Lunar Internal Structure Estimated from Local Admittance between Gravity and Topography

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1277n&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1277

Physics

Scientific paper

The admittance curves between localized gravity disturbance and
topography of lunar basins support classification of the Type I, II, and
primary mascon basins.

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