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  • 1
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    In:  CASI
    Publication Date: 2019-06-27
    Description: A thermodynamic chart in which area represents energy per unit of mass is constructed for the Mars atmosphere. A surface pressure of 8 millibars and an atmospheric composition of approximately 100 percent carbon dioxide are assumed. Mixing-ratio and equivalent potential temperature lines are drawn to facilitate the study of water-vapor condensation. The region of sublimation of carbon dioxide is presented for the study of the formation of carbon dioxide clouds and surface frost.
    Keywords: SPACE SCIENCES
    Type: NASA-TM-X-58114 , JSC-08683
    Format: application/pdf
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