Morphology of Four Flow Fields on Titan: Implications for Modes of Origin

E. R. Stofan (1) , T. Farr (2) , R. L. Kirk (3) , R. M. Lopes (2) , R. Lorenz (4) , J.I. Lunine (5) , K. L. Mitchell (2) , Philippe Paillou (6, 7, 8) , J. Radebaugh (5) , S. W. Wall (2) , C. A. Wood (9) , Cassini Radar Team

1 Proxemy Research Inc
2 JPL - Jet Propulsion Laboratory
3 US Geological Survey [Flagstaff]
4 APL - Johns Hopkins University Applied Physics Laboratory [Laurel, MD]
5 LPL - Lunar and Planetary Laboratory [Tucson]
6 L3AB - Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux
7 OASU - Observatoire aquitain des sciences de l'univers
8 LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac]
9 Wheeling Jesuit University

We describe four flow fields associated with channels that have been observed in Cassini Radar data of Titan.

Domaines: Planétologie et astrophysique de la terre [astro-ph.EP]; Planétologie et astrophysique de la terre [astro-ph.EP]

E. R. Stofan, T. Farr, R. L. Kirk, R. M. Lopes, R. Lorenz, et al.. Morphology of Four Flow Fields on Titan: Implications for Modes of Origin. 2009LPI..40.1043S - 40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, id.1043, 2009, the Woodlands, United States. ⟨hal-00405363⟩