Marc Crapeau

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The SMOS satellite mission, launched in 2009, allows global soil moisture estimations to be made using the L-band Microwave Emission of the Biosphere (L-MEB) model, which simulates the L-band microwave emissions produced by the soil–vegetation layer. This model was calibrated using various sources of in situ and airborne data. In the present study, we(More)
1 Université de Nantes, Laboratoire de Planétologie et Géodynamique, 2 rue Houssinière, 44322 Nantes Cedex 03, France 2 CNRS, UMR-6112, 2 rue Houssiniere, 44322 Nantes Cedex 03, France 3 Observatoire Aquitain des Sciences de l’Univers – UMR 5804, Floirac, France 20 4 Jet Propulsion Laboratory, M/S 183-501, 4800 Oak Grove Drive, Pasadena, CA 91109, USA 5(More)
Introduction: The SAR imaging mode of the Cassini Radar instrument allows to map the surface of Titan with a high-resolution [1]. The first Cassini close flyby Ta was acquired on 26 October 2004 and revealed a complex surface, with areas of low relief and dome-like volcanic constructs, flows and sinuous channels [1]. In particular, channels and fan-like(More)
Crapeau, S. Le Mouelic, Ph. Paillou, J.W. Barnes, R.H. Brown, C. Sotin, S. Wall, and the VIMS and RADAR science teams, 1 Laboratoire AIM, Centre d'étude de Saclay, IRFU/Sap, Centre de l'Orme des Merisiers, bât. 709, 91191 Gif/Yvette Cedex France, (email: sebastien.rodriguez@cea.fr), 2 Observatoire de Bordeaux, France, 3 Laboratoire de Planétologie et de(More)
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