Martian Atmospheric Induced Micro-Seismic Noise Generation: Large Eddy Simulations

Details Martian Atmospheric Induced Micro-Seismic Noise Generation: Large Eddy Simulations Martian Atmospheric Induced Micro-Seismic Noise Generation: Large Eddy Simulations

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1994l&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1994

Physics

Scientific paper

The surface of planets with an atmosphere or ocean has continuous
vibrations generated by the fluid envelop circulations and turbulences,
generating a microseismic noise. This is estimated for Mars by modeling
the interaction of large eddies.

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