Estimates of the harmonic coefficients of the topography of Venus using data from the Pioneer-Venus orbiter spacecraft

Details Estimates of the harmonic coefficients of the topography of Venus using data from the Pioneer-Venus orbiter spacecraft Estimates of the harmonic coefficients of the topography of Venus using data from the Pioneer-Venus orbiter spacecraft

Jun 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989avest..23..150g&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 23, Apr.-June 1989, p. 150-156. In Russian.

Astronomy and Astrophysics

Astronomy

Harmonic Analysis, Pioneer Venus Spacecraft, Topography, Venus Surface, Autocorrelation, Planetary Gravitation

Scientific paper

A model of the Venusian global topography is obtained by fitting a 27
deg harmonic series based on data from the Pioneer-Venus orbiter
spacecraft. The mean radius of Venus in this model is 6051.88 km. It is
shown that a correlation between gravity and topography is a
characteristic feature of Venus.

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