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| | [No title] (Site not responding. Last check: 2007-10-13) |
 | | The Bouguer anomalies are derived from the 50th-degree and -order spherical harmonic gravity model, GMM-1, and the 8th-degree and -order topography model, M.TOPOGRAPHY.8X8.SPH.HARM.txt.done, referred to a geopotential surface, as described in Smith and Zuber, 'The shape of Mars and the topographic signature of the hemispheric dichotomy', Science, v. |
 | | The Bouguer correction to the gravitational potential is calculated, for spherical harmonic degree l=1,2,...,8 as: CB = 3*(rho/rhobar) / (2*l + 1) The topographic reduction density rho was 2900 kg/m3, and mean planetary density rhobar was 3340 kg/m3. |
 | | The resulting anomalies were then inverted for the topography of a moho (Mohorovicic Discontinuity) at a depth of 50 km, assuming a laterally constant density structure for the crust and mantle, and a density contrast between crust and mantle of 600 kg/m3. |
| wufs.wustl.edu /geodata/viking_mariner9/readme.txt (1284 words) |
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