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Cassini imaging of Titan's high-latitude lakes, clouds, and south-polar surface changes

  • Published:2009-01 Issue:2 Volume:36 Page:n/a-n/a
  • ISSN:0094-8276
  • Container-title:Geophysical Research Letters
  • language:en
  • Short-container-title:Geophys. Res. Lett.

Author:

Turtle E. P.1,Perry J. E.2,McEwen A. S.2,DelGenio A. D.3,Barbara J.3,West R. A.4,Dawson D. D.2,Porco C. C.5

Affiliation:

1. Applied Physics Laboratory; Johns Hopkins University; Laurel; Maryland; USA

2. Lunar and Planetary Laboratory; University of Arizona; Tucson; Arizona; USA

3. NASA Goddard Institute for Space Studies; New York; New York; USA

4. Jet Propulsion Laboratory; California Institute of Technology; Pasadena; California; USA

5. Space Science Institute; Boulder; Colorado; USA

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Reference31 articles.

1. TRAMS: A new dynamic cloud model for Titan's methane clouds;Barth;Geophys. Res. Lett.,2007

2. The identification of liquid ethane in Titan's Ontario Lacus;Brown;Nature,2008

3. Fussner , S. 2006 Search for 938 nm specular enhancement on Titan Univ. of Ariz. Tucson

4. The evolution of Titan's mid-latitude clouds;Griffith;Science,2005

5. Evidence for a polar ethane cloud on Titan;Griffith;Science,2006

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