P036:
Radar Investigations of Planetary Surface and Subsurfaces





Session ID#: 23083

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:  Dustin M Schroeder, Stanford University, Geophysics and Electrical Engineering, Stanford, CA, United States
Conveners:  G Wesley Patterson, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, Cyril Grima, Institute for Geophysics, Austin, TX, United States and Lynn M Carter, University of Arizona, Tucson, AZ, United States
Index Terms:

0794 Instruments and techniques [CRYOSPHERE]
6218 Jovian satellites [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
6949 Radar astronomy [RADIO SCIENCE]
6969 Remote sensing [RADIO SCIENCE]

Abstracts Submitted to this Session:

Sean Thomas Peters1, Dustin M Schroeder1, Andrew Romero-Wolf2 and Mark Haynes3, (1)Stanford University, Geophysics and Electrical Engineering, Stanford, CA, United States, (2)Jet Propulsion Laboratory, Altadena, CA, United States, (3)Jet Propulsion Laboratory, Pasadena, CA, United States
Paul K Byrne1, Richard Ghail2, A M Celal Sengor3, Christian Klimczak4 and Sean C Solomon4, (1)North Carolina State University, Department of Marine, Earth, and Atmospheric Sciences, Raleigh, NC, United States, (2)Imperial College London, London, United Kingdom, (3)Istanbul Technical Univ, Istanbul, Turkey, (4)Carnegie Inst Washington, Department of Terrestrial Magnetism, Washington, DC, United States
Dylan Christian Hickson, York University, Centre for Research in Earth and Space Science, Toronto, ON, Canada, Alexandre Boivin, University of Toronto, Toronto, ON, Canada, Michael G Daly, York University, Toronto, ON, Canada, Rebecca R Ghent, Planetary Science Institute Tucson, Tucson, AZ, United States, Michael C Nolan, Arecibo Observatory, Arecibo, PR, United States, Kimbery Tait, The Royal Ontario Museum, Department of Natural History, Mineralogy, Toronto, ON, Canada, Alister Cunje, University of Toronto, Earth Sciences, Toronto, ON, Canada and Chun-An Tsai, University of Toronto, Physics, Toronto, ON, Canada
Michael C Nolan1, Lance Benner2, Jon D Giorgini2, Ellen S Howell1, Robert Kerr3, Dante S Lauretta1, Christopher Magri4, Jean-Luc Margot5 and Daniel Jay Scheeres6, (1)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (2)JPL, Pasadena, CA, United States, (3)Computational Physics Inc., Chelmsford, N. Chelmsford, MA, United States, (4)University of Maine at Farmington, Farmington, ME, United States, (5)UCLA, Los Angeles, CA, United States, (6)University of Colorado Boulder, Boulder, CO, United States
Sanchari Thakur and Lorenzo Bruzzone, University of Trento, Trento, Italy
Alexandre Boivin1, Dylan Christian Hickson2, Alister Cunje1, Chun-An Tsai3, Rebecca R Ghent1,4 and Michael G Daly2, (1)University of Toronto, Earth Sciences, Toronto, ON, Canada, (2)York University, Centre for Research in Earth and Space Science, Toronto, ON, Canada, (3)University of Toronto, Physics, Toronto, ON, Canada, (4)Planetary Science Institute Tucson, Tucson, AZ, United States
Alice Anne Le Gall1, Richard West2, Michael A Janssen2, Cedric Leyrat3, Lea Bonnefoy4 and Emmanuel Lellouch5, (1)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)LESIA Observatoire de Paris, Meudon, France, (4)LESIA-LATMOS, Paris, France, (5)Observatoire de Paris, LERMA, Paris, France
Maria Carmela Raguso, Marco Mastrogiuseppe, Roberto Seu and Lorenzo Piazzo, Sapienza University of Rome, DIET, Rome, Italy
Svein-Erik Hamran1, Hans E. F. Amundsen2, Tor Berger1, Lynn M Carter3, Henning Dypvik4, Rebecca R Ghent5, Jack Kohler6, Michael T Mellon7, Daniel Cahn Nunes8, David A Paige9, Dirk Plettemeier10 and Patrick Russell9, (1)FFI, Kjeller, Norway, (2)Vestfonna Geophysical, Trondheim, Norway, (3)NASA Goddard Space Flight Cent, Greenbelt, MD, United States, (4)University of Oslo, Oslo, Norway, (5)Planetary Science Institute Tucson, Tucson, AZ, United States, (6)Norwegian Polar Institute, Tromsø, Norway, (7)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (8)Jet Propulsion Laboratory, Pasadena, CA, United States, (9)University of California Los Angeles, Los Angeles, CA, United States, (10)Dresden University of Technology, Dresden, Germany
Yann Hervé1, Valerie Ciarletti1, Alice Anne Le Gall1, Nicolas Oudart1, Damien Loizeau2, Christophe Guiffaut3, Sophie Dorizon1 and the WISDOM team, (1)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (2)Laboratoire de Géologie de Lyon, Villeurbanne, France, (3)Xlim, Limoges, France
Graziella Caprarelli, University of South Australia, Division of IT, Engineering and the Environment, Adelaide, SA, Australia, Roberto Orosei, Istituto di Radioastronomia, Istituto Nazionale di Astrofisica, Bologna, Italy, Marco Mastrogiuseppe, Sapienza University of Rome, DIET, Rome, Italy and Marco Cartacci, IAPS-INAF, Rome, Italy
Parvathy Prem, G Wesley Patterson and Michael I Zimmerman, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
Angela M Stickle1, G Wesley Patterson1, Joshua T Cahill2 and The Mini-RF Team, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)JHU/APL, Laurel, MD, United States
Matthew Robert Perry1, Nathaniel E Putzig1, Isaac B Smith1, Frederick J Foss II2 and Bruce A Campbell3, (1)Planetary Science Institute, Lakewood, CO, United States, (2)Freestyle Analytic & Quantitative Services, LLC, Longmont, CO, United States, (3)Smithsonian National Air and Space Museum, Washington, DC, United States
Gerald Patterson1, Angela M Stickle2, Joshua T Cahill3, F. Scott Turner4, J. Robert Jensen1 and the Mini-RF team, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (3)JHU/APL, Laurel, MD, United States, (4)Johns Hopkins University, Balitmore, MD, United States
Lynn M Carter, University of Arizona, Tucson, AZ, United States, Gareth Morgan, Smithsonian National Air and Space Museum, Washington, DC, United States and Nathaniel E Putzig, Planetary Science Institute, Lakewood, CO, United States
Omkar Pradhan, University of Colorado at Boulder, Electrical, Computer and Energy Engineering, Boulder, CO, United States, Albin John Gasiewski, Univ of Colorado, Boulder, CO, United States and William Stone, Organization Not Listed, Washington, DC, United States
Joshua T Cahill1, Gerald Patterson2, F. S. Turner1, Gareth Morgan3, Angela M Stickle4, Emerson J Speyerer5, Raymond C Espiritu6, B. J. Thomson7 and Mini-RF Team, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Applied Physics Laboratory, Laurel, MD, United States, (3)Smithsonian National Air and Space Museum, Washington, DC, United States, (4)Applied Physics Laboratory Johns Hopkins, Laurel, MD, United States, (5)Arizona State University, School of Earth and Space Exploration, Tempe, AZ, United States, (6)Johns Hopkins Applied Physics Laboratory, Laurel, MD, United States, (7)University of Tenessee, Knoxville, TN, United States
Juha Vierinen, Univrsity of Tromsø, Tromso, Norway

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