Determination of the hypothetical structure of the Martian crust by a free vibration method.

Details Determination of the hypothetical structure of the Martian crust by a free vibration method. Determination of the hypothetical structure of the Martian crust by a free vibration method.

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994sosyr..28...91g&link_type=abstract

Solar System Research, Vol. 28, No. 2, p. 91 - 97

Physics

Mars: Crust, Mars Surface: Methods Of Observation

Scientific paper

The diagnostic capabilities of the free vibration method are investigated for determining structural features of detailed models of the Martian crust. A set of models of Mars with different distributions of the density ρ and velocities VP and VS in the crust is used for this. Spheroidal and torsional vibrations for the numbers n = 20 to 10000 are calculated for these models. Dispersion curves for Rayleigh and Love waves are constructed, which identify the structure of the crust well.

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