A mechanism for the low nightside temperatures in the Venus thermosphere
A mechanism is proposed and discussed that may account for the extraordinarily low temperatures in the nightside upper atmosphere of Venus: cooling by the emission of infrared radiation in the rotational band of the H2O molecule, which represents a minor constituent of the atmosphere. A theoretical...
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| Veröffentlicht in: | Soviet astronomy letters 1984-09, Vol.10, p.291-293 |
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| Hauptverfasser: | , |
| Format: | Artikel |
| Sprache: | eng |
| Online-Zugang: | Volltext |
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