NDLI: Geographic control of Titan's mid-latitude clouds.

Content Provider	Semantic Scholar
Author	Roe, Henry G. Brown, Michael E. Schaller, Emily L. Bouchez, Antonin H. Trujillo, Chadwick A.
Copyright Year	2005
Abstract	Observations of Titan's mid-latitude clouds from the W. M. Keck and Gemini Observatories show that they cluster near 350 degrees W longitude, 40 degrees S latitude. These clouds cannot be explained by a seasonal shift in global circulation and thus presumably reflect a mechanism on Titan such as geysering or cryovolcanism in this region. The rate of volatile release necessary to trigger cloud formation could easily supply enough methane to balance the loss to photolysis in the upper atmosphere.
Starting Page	97
Ending Page	101
Page Count	5
File Format	PDF HTM / HTML
Alternate Webpage(s)	http://www.gps.caltech.edu/~mbrown/papers/ps/geographic.pdf
Alternate Webpage(s)	http://web.gps.caltech.edu/~mbrown/papers/ps/geographic.pdf
Alternate Webpage(s)	http://authors.library.caltech.edu/34408/2/Roe.SOM.pdf
PubMed reference number	16239473v1
Volume Number	310
Issue Number	5747
Journal	Science
Language	English
Access Restriction	Open
Subject Keyword	Latitude:Angle:Point in time:Cancer.To be specified in another part of the message:Quantitative photolysis
Content Type	Text
Resource Type	Article

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Geographic control of Titan's mid-latitude clouds.