P51G:
Radar Investigations of Planetary Surfaces and Subsurfaces I Posters
Submit an Abstract to this Session
Session ID#: 44356
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, Department of Electrical Engineering, Stanford, United States
Conveners: Cyril Grima, University of Texas, Institute for Geophysics, Austin, TX, United States, Gerald Patterson, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States and Lynn M Carter, NASA Goddard Space Flight Cent, Greenbelt, United States
Primary Liaison: Lynn M Carter, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Chairs: Dustin M Schroeder, Stanford University, Department of Geophysics, Stanford, United States and Gerald Patterson, Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States
OSPA Liaison: Lynn M Carter, NASA Goddard Space Flight Cent, Greenbelt, United States
Abstracts Submitted to this Session:
Xiao Tang1, Lei Zhang2 and Xiaoli Ding1, (1)Hong Kong Polytechnic University, Hong Kong, Hong Kong, (2)Hong Kong Polytechnic University, The Department of Land Surveying and Geo-Informatics, Hong Kong, Hong Kong
Lynn M Carter, University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, Noah E Petro, NASA GSFC, Greenbelt, United States, Bruce A Campbell, Smithsonian Center for Earth and Planetary Studies, Washington, United States, David M. H. Baker, NASA Goddard Space Flight Center, Greenbelt, MD, United States and Gareth A Morgan, Planetary Science Institute, Washington DC, United States
Gerald Patterson1, Lynn M Carter2, Angela M Stickle1, Joshua T Cahill1, Michael C Nolan3, Gareth A Morgan4, Dustin M Schroeder5, Bruce A Campbell6 and the Mini-RF team, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)NASA Goddard Space Flight Cent, Greenbelt, United States, (3)Arecibo Observatory, Arecibo, PR, United States, (4)Planetary Science Institute, Tucson, United States, (5)Stanford University, Department of Geophysics, Stanford, United States, (6)Smithsonian Center for Earth and Planetary Studies, Washington, United States
Graciela Gonzalez Peytavi, Universität der Bundeswehr München, Institute of Space Technology & Applications, Munich, Germany, Tom Andert, Bundeswehr University Munich, Institute of Space Technology and Space Applications, Munich, Germany, Martin Paetzold, University of Cologne; Rheinisches Institut fuer Umweltforschung (RIU), Department of Planetary Research, Cologne, Germany, Bernd Häusler, Universität der Bundeswehr München, Institute of Space Technology & Applications, München, Germany, Stefan Remus, Telespazio VEGA UK LTD, SRE-OO, ESTEC, Noordwijk, Netherlands, Silvia Tellmann, RIU, Cologne, Planetary Research, Cologne, Germany, Michael Keith Bird, RIU-Planetary Research, Cologne, Germany and Sami W Asmar, Jet Propulsion Laboratory, Pasadena, United States
Donald D Blankenship, University of Texas, Institute for Geophysics, Austin, United States, Duncan A Young, Institute for Geophysics, Austin, TX, United States and REASON Team
Duncan A Young, University of Texas at Austin, University of Texas Institute for Geophysics, Austin, TX, United States, Cyril Grima, University of Texas, Institute for Geophysics, Austin, TX, United States, Gregor Steinbrügge, German Aerospace Center DLR Berlin, Berlin, Germany, Kirk Michael Scanlan, University of Alberta, Civil and Environmental Engineering, Edmonton, AB, Canada, Scott D Kempf, University of Texas Institute for Geophysics, Austin, United States, Donald D Blankenship, University of Texas, Institute for Geophysics, Austin, United States and REASON team
Isabella Alexandra Pena1, Dustin M Schroeder2 and Davide Castelletti2, (1)University of California Berkeley, Berkeley, CA, United States, (2)Stanford University, Department of Geophysics, Stanford, United States
Sean Thomas Peters1, Dustin M Schroeder2, Davide Castelletti3, Mark Haynes4 and Andrew Romero-Wolf4, (1)MIT Lincoln Laboratory, Department of Electrical Engineering, Lexington, United States, (2)Stanford University, Department of Electrical Engineering, Stanford, United States, (3)Stanford University, Department of Geophysics, Stanford, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, United States
Gregor Steinbrügge, Institute for Geophysics, University of Texas at Austin, Austin, United States and the PRIME Team
Bruce A Campbell, Smithsonian Center for Earth and Planetary Studies, Washington, United States, Jennifer L Whitten, Smithsonian National Air and Space Museum, Center for Earth and Planetary Studies, Washington, United States, Gareth A Morgan, Planetary Science Institute, Tucson, United States and Clara L Meier, College of Charleston, Charleston, United States
Gareth A Morgan, Planetary Science Institute, Tucson, United States and Bruce A Campbell, Smithsonian Center for Earth and Planetary Studies, Washington, United States
Jennifer L Whitten, Smithsonian National Air and Space Museum, Center for Earth and Planetary Studies, Washington, United States, Bruce A Campbell, Smithsonian Center for Earth and Planetary Studies, Washington, United States and Jeffrey J Plaut, JPL, Pasadena, CA, United States
Dirk Plettemeier1, Christoph Statz1, Yun Lu1, Wolf-Stefan Benedix1, Svein-Erik Hamran2, Yann Hervé3, Alice Anne Le Gall3 and Valerie Ciarletti4, (1)Dresden University of Technology, Dresden, Germany, (2)University of Oslo, Oslo, Norway, (3)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France, (4)LATMOS/CNRS, Guyancourt, France
Jian Deng, China University of Geosciences Wuhan, Wuhan, China
Dylan Christian Hickson, Colorado School of Mines, Golden, CO, United States, Alexandre Boivin, University of Toronto, Toronto, ON, Canada, Michael G Daly, York University, Centre for Research in Earth and Space Science, Toronto, ON, Canada, Rebecca R Ghent, Planetary Science Intitute, Tuscon, United States and Chun-An Tsai, University of Toronto, Physics, Toronto, ON, Canada
