First steps toward data assimilation of Jupiter's radiation belts using Juno and radio observations and physics-based models
Daniel Santos-Costa1, Scott J Bolton2, George B Clark3, Peter Kollmann4, Barry Mauk4, Fran Bagenal5, Heidi N Becker6, Mike Janssen7, Steven Levin6, Fabiano A Oyafuso8, Virgil Adumitroaie9, Julien N Girard10, Philippe M Zarka11, Andrew P. Ingersoll12, William S Kurth13 and John E P Connerney14, (1)Southwest Research Institute, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, United States, (3)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (4)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (5)University of Colorado at Boulder, Boulder, CO, United States, (6)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (7)Jet Propulsion Laboratory, Pasadena, CA, United States, (8)Jet Propulsion Laboratory, Pasadena, United States, (9)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (10)CEA/SAp/Irfu, AIM, Saclay, France, (11)Observatoire de Paris, PSL, CNRS, LESIA, Meudon, France, (12)California Institute of Technology, Pasadena, CA, United States, (13)University of Iowa, Iowa City, IA, United States, (14)Space Research Corporation, Annapolis, United States
