P51C:
Radar Investigations of Planetary Surfaces and Subsurfaces I Posters
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Session ID#: 12855
Session Description:
Proposed and existing radar instruments are enabling an unprecedented range of radio geophysical observations of the surfaces and subsurfaces of solar system bodies. This has spurred the development and application of new instrumentation, processing, modeling, analysis, and interpretation approaches to planetary radar science and engineering. We invite abstracts on any topic involving the use of radar data to understand planetary bodies. These may describe (but are not limited to) new results from existing radar observations, the development and application of new observation or data processing techniques, numerical modeling of existing or future observations, and/or the analysis of airborne or orbital radar data from terrestrial analog studies for solar system observation.
Primary Convener: Gerald Patterson, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Conveners: Dustin M Schroeder, Stanford University, Department of Electrical Engineering, Stanford, United States, Lynn M Carter, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Cyril Grima, Institute for Geophysics, Austin, TX, United States
Chairs: Gerald Patterson, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Lynn M Carter, NASA Goddard Space Flight Center, Greenbelt, MD, United States
OSPA Liaison: Cyril Grima, Institute for Geophysics, Austin, TX, United States
Abstracts Submitted to this Session:
Alexandre Boivin1, Dylan Christian Hickson2, Alister Cunje1, Chun-An Tsai3, Rebecca R Ghent1,4 and Michael G Daly5, (1)University of Toronto, Earth Sciences, Toronto, ON, Canada, (2)Colorado School of Mines, Golden, CO, United States, (3)University of Toronto, Physics, Toronto, ON, Canada, (4)Planetary Science Institute, Tucson, United States, (5)York University, Centre for Research in Earth and Space Science, Toronto, ON, Canada
Chun-An Tsai1, Rebecca R Ghent2 and Alexandre Boivin2, (1)University of Toronto, Physics, Toronto, ON, Canada, (2)University of Toronto, Earth Sciences, Toronto, ON, Canada
Mark Haynes1, Dustin M Schroeder2, Xueyang Duan1, Darmin Arumugam3, Joseph G McMichael4, Scott Hensley5 and Thomas A Cwik6, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)Stanford University, Department of Electrical Engineering, Stanford, United States, (3)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (4)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (5)Jet Propulsion Laboratory, Pasadena, United States, (6)Jet Propulsion Laboratory, Pasadena, CA, United States
Allan H Treiman1, Elise Michelle Harrington2 and Virgil L Sharpton1, (1)Lunar and Planetary Institute, Houston, TX, United States, (2)University of Western Ontario, London, Canada
Ken Ishiyama, Japan Aerospace Exploration Agency, Kanagawa, Japan, Atsushi Kumamoto, Tohoku University, Sendai, Japan and Jianqing Feng, Chinese Academy of Sciences, Beijing, China
Gerald Patterson, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Anne Virkki, Arecibo Observatory, Arecibo, United States and Patrick A Taylor, Arecibo Observatory, Arecibo, PR, United States
Graziella Caprarelli1,2, Roberto Orosei3, Angelo Pio Rossi4, Federico Cantini5, Lynn M Carter6, Irene Papiano7, Marco Cartacci8, Andrea Cicchetti8 and Raffaella Noschese9, (1)University of South Australia, Division of IT, Engineering and the Environment, Adelaide, SA, Australia, (2)International Research School of Planetary Sciences, Chieti, Italy, (3)Istituto di Radioastronomia, Istituto Nazionale di Astrofisica, Bologna, Italy, (4)Earthgraph GmbH, Bremen, Germany, (5)Ecole Normale Polytechnique Federale de Lausanne, Space Engineering Center, EPFL ESC, Lausanne, Switzerland, (6)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (7)Liceo Scientifico Augusto Righi, Bologna, Italy, (8)IAPS-INAF, Rome, Italy, (9)INAF-IAPS, Rome, Italy
Hyun-Seob Baik, Korea Institute of Geoscience & Mineral Research, Geophysical Exploration, Daejeon, Korea, Republic of (South); University of Science and technology, South Korea, Geophysical Exploration, Daejeon, Korea, Republic of (South) and Jungrack Kim, University of Seoul, Seoul, Korea, Republic of (South)
Dirk Plettemeier1, Christoph Statz1, Ronny Hahnel1, Wolf-Stefan Benedix1, Svein-Erik Hamran2 and Valerie Ciarletti3, (1)Dresden University of Technology, Dresden, Germany, (2)FFI, Kjeller, Norway, (3)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France
Flora Paganelli, American Public University System Charles Town, Space Studies, Charles Town, WV, United States, Gerald Schubert, University of California Los Angeles, Los Angeles, CA, United States, Rosaly M C Lopes, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, Michael Malaska, NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, Alice Anne Le Gall, LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France, Randolph L Kirk, USGS Astrogeology Science Center, Flagstaff, AZ, United States and The Cassini RADAR Science Team
