P029
Planetary Atmospheric, Surface, and Interior Science Using Radio and Laser Links

Session ID#: 74030

Session Description:
Solar system exploration has been advanced over the past five decades via Radio Science techniques to study planetary and solar phenomena as well as fundamental physics. The scope of this session includes investigations within the solar system as well as tests of fundamental physics to expand the frontiers of solar system exploration using radio and optical science to address the study of ocean worlds, planetary and small body interiors, the dynamics, composition, and thermal structure of planetary atmospheres, characterizing the scattering, electrical, and other properties of planetary surfaces, and research in fundamental physics and solar system dynamics. Relevant technology topics include the design of small spacecraft networks and constellations, advances in flight and ground instrumentation, advances in space clock technologies, novel communications architectures including optical links, advances in radio and laser technologies, and new techniques and instrumentation for entry probe radio science.
Index Terms:

6297 Instruments and techniques [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]
6964 Radio wave propagation [RADIO SCIENCE]
6979 Space and satellite communication [RADIO SCIENCE]
6994 Instruments and techniques [RADIO SCIENCE]


Primary Convener:  David H Atkinson, Jet Propulsion Laboratory, Pasadena, CA, United States
Conveners:  Sami Asmar, Jet Propulsion Laboratory, Pasadena, CA, United States, Luciano Iess, Univ. La Sapienza, Roma, Italy and Silvia Tellmann, University of Cologne, Cologne, Germany
Primary Liaison:  David H Atkinson, Jet Propulsion Laboratory, Pasadena, CA, United States
 
Measurements of atmospheric dynamics and composition from radiometric tracking of an ice giant entry probe (487815)
David H Atkinson1, Sami Asmar1 and Thomas R Spilker2, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Retired, JPL-Caltech, Pasadena, CA, United States
 
Impact of the Advanced Water Vapor Radiometer on the Juno Gravity Science Investigation (497152)
Dustin Buccino1, Marzia Parisi2, Daniel S Kahan3, Meegyeong Paik2, Yu-Ming Yang1, William M Folkner3 and Kamal Oudrhiri3, (1)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
 
Sensing small-scale structures in the lower Martian atmosphere with tomographic principles (510490)
Gregor Moeller, Chi O Ao and Anthony J Mannucci, NASA Jet Propulsion Laboratory, Pasadena, CA, United States
 
Pluto’s Surface Properties from the New Horizons Uplink Bistatic Radar Experiment (Invited) (510558)
Ivan Linscott1, Sami Asmar2, Michael Bird3, Chris DeBoy4, Rebecca Sepan4, Alan Stern5, Michael Vincent6, Kamal Oudrhiri7, Martin Paetzold8, Thomas Andert9, David P Hinson10, G Leonard Tyler1, Harold A Weaver Jr11, Leslie A Young12, William M Grundy13, Catherine Olkin6, Kimberly Ennico Smith14 and The New Horizons REX, GOMP, ATM and GGI Teams, (1)Stanford University, Stanford, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)University of Cologne, Cologne, Germany, (4)Applied Physics Laboratory Johns Hopkins, Laurel, United States, (5)Southwest Research Institute San Antonio, San Antonio, TX, United States, (6)Southwest Research Institute Boulder, Boulder, CO, United States, (7)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (8)University of Cologne; Rheinisches Institut fuer Umweltforschung (RIU), Department of Planetary Research, Cologne, Germany, (9)Universität der Bundeswehr München, Institute for Space Technology & Applications, Munich, Germany, (10)SETI Institute, Mountain View, CA, United States, (11)The Johns Hopkins University, Laurel, MD, United States, (12)Southwest Research Institute, Boulder, CO, United States, (13)Lowell Observatory, Flagstaff, AZ, United States, (14)NASA Ames Research Center, Moffett Field, CA, United States
 
Revisiting CONSERT results taking into account the exact lander position on the comet. (514517)
Wlodek W Kofman1,2, Sonia Zine2, Alain Herique2, Yves Rogez2 and Laurent Jorda3, (1)Space Research Centre, PAS, Warsaw, Poland, Warsaw, Poland, (2)University Grenoble Alpes, CNRS, IPAG, Grenoble, France, (3)Observatoire Astrophysique Marseille, Marseille, France
 
A combined analysis of planetary missions radio science experiments for precise determination of solar system dynamics (517780)
Gael Cascioli and Antonio Genova, Sapienza University of Rome, Rome, Italy
 
First results from cruise tests of the Mercury Orbiter Radio science Experiment (MORE) of ESA’s BepiColombo mission (523810)
Paolo Cappuccio1, Virginia Notaro1, Luciano Iess1, Sami Asmar2, James Border2, Sabatino Ciarcia Sr.3, Andrea Di Ruscio1, Elsa Montagnon4, Javier De Vicente4, Mattia Mercolino5, Meegyeong Paik2, Lorenzo Simone3, Francesco Fiori6, Alessandra Palli6,7, Paolo Tortora6, Marco Zannoni6 and Josè Villalvilla4, (1)Sapienza University of Rome, Rome, Italy, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Thales Alenia Space Italy, Rome, Italy, (4)ESOC, Darmstadt, Germany, (5)ESTEC, Noordwjik, Netherlands, (6)University of Bologna, Department of Industrial Engineering, Bologna, Italy, (7)SITAEL S.P.A, Forlì, Italy
 
Ionospheric Electron Density Profile of Jupiter’s Moon Callisto and its Implication on Moon’s Interior Using Galileo’s Radio Occultation Observations. (546334)
Ashok Kumar Verma, University of California Los Angeles, Los Angeles, CA, United States, Raymond J Walker, University of California Los Angeles, Department of Earth, Planetary, and Space Sciences, Los Angeles, CA, United States and Krishan K Khurana, University of California at Los Angeles, Los Angeles, CA, United States
 
Enhanced Planetary Science with the Iris Radio for Smallsat Radio Science (546352)
Sami W Asmar1, David H Atkinson2, Kyle Botteon3, Robert Arthur Preston3 and Joseph Lazio3, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
 
Exploring the Interior of Venus with the VERITAS Gravity Science Investigation (Invited) (548346)
Erwan Mazarico1, Luciano Iess2, Doris Breuer3, Fabrizio De Marchi4, Alex S Konopliv5, Scott Hensley6 and Suzanne E Smrekar5, (1)NASA Goddard Space Flight Center, Greenbelt, MD, United States, (2)Univ. La Sapienza, Roma, Italy, (3)German Aerospace Center DLR Berlin, Berlin, Germany, (4)Sapienza University of Rome, Rome, Italy, (5)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (6)JPL-Radar Science & Engrg, Pasadena, CA, United States
 
MCMC-Based Model Parameter Estimation from Measurements of the Complex Electromagnetic Characteristics of Planetary Regolith Analog Materials (550477)
Alexandre Boivin1, Chun-An Tsai2, Dylan Christian Hickson3, Rebecca R Ghent1,4 and Michael G Daly5, (1)University of Toronto, Earth Sciences, Toronto, ON, Canada, (2)University of Toronto, Physics, Toronto, ON, Canada, (3)Arecibo Observatory, Arecibo, United States, (4)Planetary Science Institute Tucson, Tucson, United States, (5)York University, Centre for Research in Earth and Space Science, Toronto, ON, Canada
 
Radio-Holographic Methods for Inversion of Radio Occultation Experiments of Past Venus’ Spacecraft (558980)
Tatiana M Bocanegra-Bahamon1, Chi O Ao1, Kuo-Nung Wang2 and Sanjay S Limaye3, (1)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)University of Wisconsin Madison, Madison, WI, United States
 
Refined constraints on P9’s location through a new analysis of Cassini navigation data (560424)
Andrea Di Ruscio, Sapienza University of Rome, Rome, Italy, Agnès Fienga, Observatoire de la Côte d’Azur, Géoazur, Valbonne, France and Luciano Iess, Univ. La Sapienza, Roma, Italy
 
Sounding of Planetary Atmospheres and Ionospheres by Crosslink Occultations (573600)
Martin Paetzold1, Silvia Tellmann2, Bernd Häusler3, Tom Andert3, Michael Keith Bird4, Graciela Gonzalez Peytavi5 and Sami Asmar6, (1)University of Cologne; Rheinisches Institut fuer Umweltforschung (RIU), Department of Planetary Research, Cologne, Germany, (2)University of Cologne, Cologne, Germany, (3)Bundeswehr University Munich, Institute of Space Technology and Space Applications, Munich, Germany, (4)Univ Bonn, Bonn, Germany, (5)Universität der Bundeswehr München, Institute of Space Technology & Applications, Munich, Germany, (6)Jet Propulsion Laboratory, Pasadena, CA, United States
 
Planetary and Earth seismology with space geodesy: seismic requirements on performances for Earth, Europa, the Moon and Jupiter. (575431)
Philippe Henri Lognonné1, Douglas G Currie2, William M Folkner3, Patrick Gaulme4, Tristan Guillot5, Hubert Halloin6, Sharon Kedar7, David Mimoun8, Clive Robert Neal9, Mark P Panning10, Sebastien De Raucourt1, David J Stevenson11 and Renee C Weber12, (1)Université de Paris, Institut de physique du globe de Paris, CNRS, Paris, France, (2)University of Maryland College Park, College Park, MD, United States, (3)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (4)Max Planck Institute for Solar System Research, Goettingen, Germany, (5)Observatoire de la Côte d’Azur, Nice, France, (6)University Denis Diderot Paris VII, Paris Cedex 13, France, (7)JPL, Pasadena, CA, United States, (8)ISAE, INSTITUT SUPERIEUR DE L'AERONAUTIQUE ET DE L'ESPACE, Toulouse, OCCITANIE, France, (9)Univ Notre Dame, Notre Dame, IN, United States, (10)Univ of FL-Geological Sciences, Gainesville, FL, United States, (11)California Institute of Technology, Pasadena, CA, United States, (12)NASA/NSSTC, Huntsville, AL, United States
 
Planetary radio science measurement scheme based on the downlink signals of China's first Mars probe (578658)
Deqing Kong, Chunlai Li, Hongbo Zhang, Weibin Wen and Qin Zhou, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
 
Juno Radio Science Observations and Gravity Science Calibrations of Io Plasma Torus: IPT Impacts to Europa Gravity Science (580598)
Yu-Ming Yang1, Dustin Buccino2, Marzia Parisi1, William M Folkner2, Phillip H Phipps3, Daniel S Kahan2, Paul Withers3 and Kamal Oudrhiri2, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States, (3)Boston University, Boston, MA, United States
 
High-resolution Gravity Field and Tides of Callisto from the MAGIC Gravity Investigation (580623)
Antonio Genova1, Erwan Mazarico2, Sander J Goossens3, Gael Cascioli1, Maria T Zuber4 and David E. Smith5, (1)Sapienza University of Rome, Rome, Italy, (2)NASA Goddard Space Flight Center, Code 698, Greenbelt, MD, United States, (3)NASA GSFC / UMBC CRESST, Greenbelt, MD, United States, (4)Massachusetts Inst Tech, Cambridge, MA, United States, (5)Massachusetts Institute of Technology, Cambridge, United States
 
Investigating the Venusian surface-atmosphere dynamic coupling (598034)
Panagiotis Vergados1, Attila Komjathy2, Quentin Brissaud3, Chi O Ao4, Tatiana M Bocanegra-Bahamon4, Siddharth Krishnamoorthy4, Robert Arthur Preston4, Joseph Lazio4, Sami W Asmar1 and David H Atkinson1, (1)Jet Propulsion Laboratory, Pasadena, CA, United States, (2)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (3)California Institute of Technology, Seismological Laboratory, Pasadena, CA, United States, (4)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
 
Suborbital Spaceflight Communication with a Tube-Deployed Reentry Vehicle (604104)
Feng Li1, Avery Brock1, Timothy White1, Hunter Kannianinen1, Daniel Cordon1 and Marcus S. Murbach2, (1)University of Idaho, Moscow, ID, United States, (2)NASA Ames Research Center, Moffett Field, CA, United States
 
The Potential for Ka-Band Radio Occultation Measurements in the Study of the Venus Atmosphere (604402)
Paul G Steffes, Georgia Institute of Technology Main Campus, Atlanta, GA, United States and Alexander B. Akins, Georgia Institute of Technology Main Campus, Atlanta, United States
 
Developing a User Interface for the Processing and Analysis of Planetary Radio Science Data: Implications for Orbital Forward-Scatter Bistatic Radar Observations of Planetary Surfaces (618522)
Paul Sirri1, Elizabeth M Palmer2 and Essam Heggy2,3, (1)Occidental College, Computer Science, Los Angeles, CA, United States, (2)University of Southern California, Electrical Engineering - Electrophysics, Los Angeles, CA, United States, (3)NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, United States
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