A two-Martian years survey of the water vapor saturation state on Mars based on ACS NIR/TGO occultations
On Mars, condensation is the major factor constraining the vertical distribution of water vapor. Recent measurements of water and temperature profiles showed that water can be strongly supersaturated at and above the level where clouds form during the aphelion and perihelion seasons. Since 2018, the...
| Príomhchruthaitheoirí: | , , , , , , , , , , , |
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| Formáid: | Journal article |
| Teanga: | English |
| Foilsithe / Cruthaithe: |
American Geophysical Union
2022
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