The depth of the convective boundary layer and implications for a Walker-like circulation on Mars

Details The depth of the convective boundary layer and implications for a Walker-like circulation on Mars The depth of the convective boundary layer and implications for a Walker-like circulation on Mars

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1197l&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1197

Physics

Scientific paper

Radio science observations indicate that the depth of the martian convective boundary layer varies strongly with surface height, although the surface temperature does not. We show that this effect is reproduced in martian limited area models and in global climate models. The implications for the global circulation when convective boundary layer depth varies with location are considered.

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