A reinterpretation of the convective heat transport concept is presented for the IRIS measurements as an essential energy transfer mechanism. Thermal convection in a radiatively heated ground atmosphere system is discussed along with CO2 sublimation and diffusion from the Martian polar ice cap. A systematic reappraisal of the existing model is also included.
Reinterpretation of Mariner 9 IRIS data on the basics of a simulation of radiative-conductive transfer in the dust-laden Martian atmosphere
01.07.1974
Report
Keine Angabe
Englisch
Water Vapour Abundance in Martian Atmosphere from Revised Mariner 9 IRIS Data
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|Martian winter atmosphere at north high latitudes: Mariner 9 IRIS data revisited
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