If Mars has permanent CO2 polar caps, atmospheric heat transport may cause the atmospheric pressure to be extremely sensitive to variations of solar heating at the poles. This could happen because atmospheric heating depends on density, which depends strongly on the polar temerature through the vapor pressure relation. A simple climatological model is used to stud the question.
CITATION STYLE
Gierasch, P. J., & Toon, O. B. (1973). Atmospheric Pressure Variation and the Climate of Mars. Journal of the Atmospheric Sciences, 30(8), 1502–1508. https://doi.org/10.1175/1520-0469(1973)030<1502:apvatc>2.0.co;2
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