P13C:
The Future of Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links II Posters
Submit an Abstract to this Session
Session ID#: 23453
Session Description:
Radio Science techniques have advanced solar system exploration for over five decades. In this session, ongoing and planned innovations that will significantly enhance the field will be presented. Session topics include planetary atmospheric, surface, and interior investigations that contribute to expanding the frontiers of solar system exploration in diverse areas such as determining the thickness of the ice sheets of ocean worlds, constraining the interior structures of the planets and small bodies, monitoring of planetary atmospheric dynamics and improvement of climate models, studying the scattering and other properties of planetary surfaces, and research in fundamental physics and solar system dynamics, among others. Technology topics include the design of small spacecraft networks and constellations, advances in flight and ground instrumentation, advancement in space clock technologies, novel communications architectures including optical links, and advances in radio and laser technologies, and new techniques and instrumentation for entry probe radio science.
Primary Convener: David H Atkinson, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Conveners: Sami Asmar, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, Luciano Iess, Sapienza University of Rome, Rome, Italy and Erwan Mazarico, NASA Goddard Space Flight Center, Greenbelt, MD, United States
Chairs: Luciano Iess1, Sami Asmar2, Erwan Mazarico3 and David H Atkinson2, (1)Sapienza University of Rome, Rome, Italy(2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States(3)NASA Goddard Space Flight Center, Greenbelt, MD, United States
OSPA Liaison: Luciano Iess, Sapienza University of Rome, Rome, Italy
Abstracts Submitted to this Session:
Hiroki Ando1, Tetsuya Fukuhara2, Masahiro Takagi1, Takeshi Imamura3, Norihiko Sugimoto4 and Hideo Sagawa1, (1)Kyoto Sangyo University, Kyoto, Japan, (2)Hokkaido Univ., Sapporo, Japan, (3)JAXA, Kanagawa, Japan, (4)Keio University, Department of Physics, Yokohama, Japan
Tatiana Bocanegra Bahamon1,2, Leonid Gurvits1,3, Guifre Molera Calves4, Giuseppe Cimo3,5, Dmitry Duev6, Sergei Pogrebenko3, Dominic Dirkx7 and Pascal Rosenblatt8, (1)Delft University of Technology, Delft, Netherlands, (2)Joint Institute for VLBI in Europe, Dwingeloo, Netherlands, (3)Joint Institute of VLBI in Europe (JIVE), Dwingeloo, Netherlands, (4)Finnish Geospatial Research Institute, Masala, Finland, (5)Netherlands Institute for Radio Astronomy, Dwingeloo, Netherlands, (6)California Institute of Technology, Pasadena, United States, (7)Delft University of Technology, Delft, 5612, Netherlands, (8)Géoazur - Université Nice Sophia Antipolis, Valbonne, France
Martin Paetzold1, Thomas Andert2, Michael Keith Bird3, Bernd Häusler4, David P Hinson5, Kerstin Peter1 and Silvia Tellmann1, (1)University of Cologne; Rheinisches Institut fuer Umweltforschung (RIU), Department of Planetary Research, Cologne, Germany, (2)Universität der Bundeswehr München, Institute for Space Technology & Applications, Munich, Germany, (3)RIU-Planetary Research, Cologne, Germany, (4)Universität der Bundeswehr, Institute for Space Technology & Applications, Munich, Germany, (5)SETI Institute, Mountain View, CA, United States
David H Atkinson1, Sami Asmar1, Joseph Lazio2 and Robert A Preston2, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
Emmanuel Decrossas, NASA Jet Propulsion Laboratory, Pasadena, CA, United States, David J Bell, NASA Jet Propulsion Laboratory, Flight Communications Systems, Pasadena, CA, United States, Curtis Jin, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, David Steinfeld, NASA Jet propulsion laboratory, Pasadena, United States and Jonathan Batres, NASA Jet Propulsion Laboratory, Pasadena, United States
Alessandra Babuscia1, David H Atkinson2, Joseph Lazio1 and Sami Asmar2, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States
Kuo-Hsin Tseng, National Central University, Center for Space and Remote Sensing Research, Kanagawa, Japan, Tzu-Pang Tseng, Cooperative Research Center for Spatial Information, Carlton, Australia, Yi-Shan Li, Chung Cheng Institute of Technology, National Defense University, Department of Environmental Information and Engineering, Taoyuan, Taiwan, Jing-Mei Wu, National Central University, GPS Science and Application Research Center, Taoyuan, Taiwan, Ta-Kang Yeh, National Taipei University, Department of Real Estate and Built Environment, New Taipei, Taiwan and Kun-Lin Chen, National Space Organization, Hsinchu, Taiwan
Dandan Mao1, Xiaoli Sun2, Gregory A Neumann2, Michael Kenneth Barker3, Erwan M Mazarico2, Evan Hoffman3, Thomas W Zagwodzki4, Mark H Torrence5, Jan Mcgarry3, David E Smith6 and Maria T Zuber7, (1)Sigma Space Corporation, Lanham, United States, (2)NASA Goddard Space Flight Center, Greenbelt, United States, (3)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (4)Cybioms Corporation, Rockville, MD, United States, (5)SGT Inc, Greenbelt, MD, United States, (6)Massachusetts Inst Tech, Cambridge, MA, United States, (7)Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, Cambridge, MA, United States
