Titan’s mid-latitude surface regions with Cassini VIMS and SAR
Titan’s mid-latitude surface regions with Cassini VIMS and SAR
Anezina Solomonidou1, Rosaly M C Lopes1, Athena Coustenis2, Michael Malaska3, Sebastien Rodriguez4, Pierre Drossart5, Michael A Janssen6, Alice Anne Le Gall7, Bernard Schmitt8, Mathieu Hirtzig9, Luca Maltagliati10, Frank Sohl11, Katrin Stephan12, Ralf Jaumann11, Robert Hamilton Brown13, Edward Villanueva1, Christos Matsoukas14 and Emmanuel Bratsolis15, (1)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)LESIA, Paris Observatory, CNRS, UPMC Univ. Paris 06, Univ. Paris-Diderot, Meudon, France, (3)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (4)AIM - CEA/CNRS/Uni. P7, Gif/Yvette, France, (5)LESIA Observatoire de Paris, Meudon, France, (6)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (7)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France, (8)Univ. Grenoble Alpes, CNRS, CNES, IPAG, 38000 Grenoble, France, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), Grenoble, France, (9)Fondation “La main à la pâte”, Montrouge, France, (10)Paris Observatory Meudon, Meudon, France, (11)German Aerospace Center DLR Berlin, Berlin, Germany, (12)German Aerospace Center, Berlin, Germany, (13)University of Arizona, Tucson, AZ, United States, (14)National and Kapodistrian University of Athens, Athens, Greece, (15)National and Kapodistrian University of Athens, Department of Physics, Athens, Greece