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• W2022144092 abstract "Observations of the seasonal cycle of water vapor in the Mars atmosphere imply that there is a seasonal exchange of water with a reservoir of ice in the polar regions and of adsorbed water in the global near-surface regolith. The equilibrium between water vapor and adsorbed water is sufficiently temperature-dependent that seasonal surface temperature variations are capable of driving a large exchange of water between the atmosphere and subsurface. A one-dimensional model of this process is presented, and calculations are done of the amount of water exchanged seasonally at each latitude. For the likely range of regolith properties, this exchange is found to be from 10 to 150% of the observed variation; atmospheric transport and supply from the polar regions must make up the difference between the predicted and observed variation. These values can be further constrained using models of atmospheric transport processes. Due to the latitudinal gradient of atmospheric vapor, there will also be a gradient of subsurface adsorbed water, with the largest abundance in the north and the least in the south; this gradient occurs independent of the regolith diffusivity." @default.
• W2022144092 created "2016-06-24" @default.
• W2022144092 creator A5072674162 @default.
• W2022144092 date "1983-07-01" @default.
• W2022144092 modified "2023-09-24" @default.
• W2022144092 title "The role of seasonal reservoirs in the Mars water cycle" @default.
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• W2022144092 doi "https://doi.org/10.1016/0019-1035(83)90046-5" @default.
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