Building reliable local models of the Venus gravity field from the cycles 5 and 6 of the Magellan LOS gravity data
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://www.agu.org/journals/gl/v024/i004/96GL04003/96GL04003.pdf
Reference10 articles.
1. The spectra of the topography of the Earth, Venus and Mars;Balmino;Geophys. Res. Lett.,1993
2. Estimation of local planetary gravity fields using line-of-sight gravity data and an integral operator;Barriot;Icarus,1992
3. Analysis of the LOS gravity data set from the Cycle 4 of the Magellan probe around Venus;Barriot;Icarus,1994
4. Analysis of the LOS gravity data sets from Cycles 5 and 6 of the Magellan probe around Venus (abstract);Barriot;EOS Trans. AGU,1995
5. A System of Subroutines for Iteratively Reweighted Least Squares Computations;Coleman;ACM Transactions on Mathematical Software,1980
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2. A method to determine regional lunar gravity fields from earth-based satellite tracking data;Planetary and Space Science;2005-11
3. Venus Gravity: 180th Degree and Order Model;Icarus;1999-05
4. A harmonic spline model for local estimation of planetary gravity fields from line-of-sight acceleration data;Journal of Geodesy;1999-04-28
5. A 180th degree and order model of the Venus gravity field from Magellan line of sight residual Doppler data;Geophysical Research Letters;1998-10-01
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