Pluto’s Surface Properties from the New Horizons Uplink Bistatic Radar Experiment
Pluto’s Surface Properties from the New Horizons Uplink Bistatic Radar Experiment
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
