The Martian geomorphology as mapped by the Mars Express High Resolution Stereo Camera (HRSC): Implications for Geological Processes and Climate Conditions.
Thomas Roatsch1, Ralf Jaumann1, Gerhard Neukum2, Daniela Tirsch1, Ernst Hauber3, Harald Hoffmann1, Klaus Gwinner1, Frank Scholten1, Gaetano Di Achille4, Thomas C Duxbury5, Gino Erkeling6, Stefan vanGasselt2, Sanjeev Gupta7, James W Head III8, Harald Hiesinger9, Wing-Huen Ip10, Horst Uwe Keller11, Maarten G Kleinhans12, Thomas Kneisl2, Thomas B McCord13, Peter Muller14, John Murray15, Monica Pondrelli16, Thomas Platz2, Patrick Claude Pinet17, Dennis Reiss9, Angelo Pio Rossi18, Lutz Wendt2, David A Williams19, Nicolas Mangold20 and Tilman Spohn1, (1)German Aerospace Center DLR Berlin, Berlin, Germany, (2)Free University of Berlin, Berlin, Germany, (3)German Aerospace Centre (DLR), Berlin, Germany, (4)CNR National Institute for Astrophysics, Rome, Italy, (5)George Mason University, Fairfax, VA, United States, (6)Uni Muenster, Muenster, Germany, (7)Imperial College London, London, United Kingdom, (8)Brown University, Providence, RI, United States, (9)University of Münster, Münster, Germany, (10)NCU National Central University of Taiwan, Jhongli, Taiwan, (11)Technical University of Braunschweig, Braunschweig, Germany, (12)Utrecht University, Utrecht, Netherlands, (13)Bear Fight Institute, Winthrop, WA, United States, (14)Mullard Space Science Laboratory, Dorking, United Kingdom, (15)Open University, Milton Keynes, United Kingdom, (16)University of Chieti-Pescara, Pescara, Italy, (17)IRAP, Toulouse, Italy, (18)Jacobs University Bremen, Bremen, Germany, (19)Arizona State University, Tempe, AZ, United States, (20)LPGN Laboratoire de Planétologie et Géodynamique de Nantes, Nantes Cedex 03, France