Abstract
The diagnostic possibilities of body waves for refining the models of the Martian interior structure are explored. The MATLAB-based software is developed for calculating the theoretical travel time curves and estimating the amplitudes of P- and S-waves for the predicted values of seismic moments of the marsquakes. The traveltimes of the P- and S-waves, as well as the reflected phases and the phases that passed through the core as the functions of epicentral distance, are compared for different test models of the interior of Mars.
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