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- W4322004587 abstract "<p>The Emirates Mars Mission (EMM) Hope Probe observes at diurnal and subseasonal timescales, while having a vertical coverage that allows it to couple the lower atmosphere to the upper atmosphere. EMM observes lower atmosphere conditions through its two instruments EXI and EMIRS, and the upper atmosphere with the EMUS instrument. This work uses outputs from the Mars Planetary Climate Model (MPCM) to understand the effects of dust storms on water vapor in the Martian atmosphere and the resulting escape of hydrogen. We compare our model results to what is observed in the Martian atmosphere through the Hope Probe instruments and use our understanding of the model to evaluate regions that are not covered vertically by EMM instrumentation in order to understand dust storm effects on the water vapor&#8217;s circulation and eventual rise in altitude to the middle atmosphere leading to hydrogen escape.</p>" @default.
- W4322004587 created "2023-02-26" @default.
- W4322004587 creator A5083542611 @default.
- W4322004587 date "2023-02-26" @default.
- W4322004587 modified "2023-09-29" @default.
- W4322004587 title "Dust Storm Effects on Water Vapor and Hydrogen on Mars in the MPCM and as seen by EMM" @default.
- W4322004587 doi "https://doi.org/10.5194/egusphere-egu23-13004" @default.
- W4322004587 hasPublicationYear "2023" @default.
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