Titan's surface mapping with VIMS/Cassini thanks to coupled atmospheric empirical correction and radiative transfer modeling

S. Rodriguez (1), S. Le Mouelic (2), P. Rannou (3,4), J.-P. Combe (5), L. Le Corre (2), G. Tobie (2), J. W. Barnes (6), C. Sotin (2,7), R. H. Brown (8), K. H. Baines (7), B. J. Buratti (7), R. N. Clark (9), Phil D. Nicholson (10) (1) Laboratoire AIM, Universite Paris 7, CNRS UMR-7158, CEA-Saclay/DSM/IRFU/SAp, France (sebastien.rodriguez@cea.fr, phone : +33 169088056). (2) Laboratoire de Planetologie et Geodynamique, Universite de Nantes, CNRS, UMR-6112, France. (3) Groupe de Spectrometrie Moleculaire et Atmospherique, CNRS UMR-6089, Universite de Reims Champagne-Ardenne, France. (4) LATMOS, CNRS UMR-7620, Universite Versailles-St-Quentin, 91371 Verrieres-le-Buisson, France. (5) The Bear Fight Center, 22, Fiddler's Road, Winthrop, WA 98862, USA. (6) NASA Ames Research Center M/S 244-30, Moffett Field, CA 94035, USA. (7) Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA. (8) Lunar and Planetary Lab., University of Arizona, Tucson, AZ, USA. (9) USGS, Denver Federal Center, Denver, CO, USA. (10) Cornell University, Astronomy Department, Ithaca, NY, USA.