Water vapor in the middle atmosphere of Mars during the 2007 global dust storm

•Vertical distributions of H2O have been measured during the MY28 global dust storm.•Strong increase of the H2O density at 60–80 km was observed at Ls = 268°–285° in both hemispheres.•In high northern latitudes the large water content was not correlated with the dust loading and was not repeated in...

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Veröffentlicht in:	Icarus (New York, N.Y. 1962) N.Y. 1962), 2018-01, Vol.300, p.440-457
Hauptverfasser:	Fedorova, Anna, Bertaux, Jean-Loup, Betsis, Daria, Montmessin, Franck, Korablev, Oleg, Maltagliati, Luca, Clarke, John
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Atmosphere Earth and Planetary Astrophysics Mars Sciences of the Universe Solar and Stellar Astrophysics Solar occultations Water vapor
Online-Zugang:	Volltext
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