Abstract
AbstractThis paper presents and discusses the vertical profiles of the potential temperature in the Martian boundary layer. The profiles were remotely sensed from on‐board the Spirit Mars Exploration Rover during the first 702 sols of its operation in 2004–2005. The rover carried the Miniature Thermal Emission Spectrometer (Mini‐TES), which allowed it to retrieve temperature profiles up to a level 2 km above the ground surface. The data analysed here permit a reconstruction of the diurnal and seasonal structure of the lower part of the Martian convective boundary layer, an evaluation of the boundary layer depth, and a computation of the temperature heat flux. Copyright © 2009 Royal Meteorological Society
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