Latitudinal variations in Titana[tm]s methane and haze from Cassini VIMS observations

We analyze observations taken with Cassinia[tm]s Visual and Infrared Mapping Spectrometer (VIMS), to determine the current methane and haze latitudinal distribution between 60A degree S and 40A degree N. The methane variation was measured primarily from its absorption band at 0.61I14m, which is opti...

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Veröffentlicht in:Icarus (New York, N.Y. 1962) N.Y. 1962), 2010-03, Vol.206 (1), p.352-365
Hauptverfasser: Penteado, Paulo F, Griffith, Caitlin A, Tomasko, Martin G, Engel, Steffi, See, Charles, Doose, Lyn, Baines, Kevin H, Brown, Robert H, Buratti, Bonnie J, Clark, Roger, Nicholson, Phillip, Sotin, Christophe
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Sprache:eng
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