Spectra from Cassini’s Visual and Infrared Mapping Spectrometer reveal the presence of a vast tropospheric cloud on Titan at latitudes 51- to 68- north and all longitudes observed (10- to 190- west). The derived characteristics indicate that this cloud is composed of ethane and forms as a result of...
Bibliographic Details
Published in: | Science |
Main Authors: |
Griffith, C. A.,
Penteado, P.,
Rannou, P.,
Brown, R.,
Boudon, V.,
Baines, K. H.,
Clark, R.,
Drossart, P.,
Buratti, B.,
Nicholson, P.,
McKay, C. P.,
Coustenis, A.,
Negrao, A.,
Jaumann, R. |
Format: | Other Non-Article Part of Journal/Newspaper
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Language: | unknown |
Published: |
2006
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Subjects: |
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Online Access: | http://elib.dlr.de/45050/
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