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 |
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Sprache: | eng |
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