Latitudinal variations in Titan’s methane and haze from Cassini VIMS observations

We analyze observations taken with Cassini’s Visual and Infrared Mapping Spectrometer (VIMS), to determine the current methane and haze latitudinal distribution between 60°S and 40°N. The methane variation was measured primarily from its absorption band at 0.61 μm, which is optically thin enough to...

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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
Format:	Artikel
Sprache:	eng
Schlagworte:	Abundances, Atmospheres Astronomy Earth Sciences Earth, ocean, space Exact sciences and technology Radiative transfer Satellites, Atmospheres Sciences of the Universe Solar system Spectroscopy Titan
Online-Zugang:	Volltext
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