First steps toward data assimilation of Jupiter's radiation belts using Juno and radio observations and physics-based models

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ADS bibcode: 2016AGUFM.P33C2161S
year: 2016
Listed Authors: Santos-Costa, D.; Bolton, S. J.; Clark, G. B.; Kollmann, P.; Mauk, B.; Bagenal, F.; Becker, H. N.; Janssen, M.; Levin, S.; Oyafuso, F. A.; Adumitroaie, V.; Girard, J. N.; Zarka, P. M.; Ingersoll, A. P.; Kurth, W. S.; Connerney, J. E. P.
Listed Institutions: Southwest Research Institute, San Antonio, TX, United States; Southwest Research Institute, San Antonio, TX, United States; Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States; Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States; Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States; University of Colorado at Boulder, Boulder, CO, United States; Jet Propulsion Laboratory, Pasadena, CA, United States; Jet Propulsion Laboratory, Pasadena, CA, United States; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States; Jet Propulsion Laboratory, Pasadena, CA, United States; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States; AIM, CEA/SAp/Irfu, Saclay, France; LESIA, Observatoire de Paris, Meudon, France; California Institute of Technology, Pasadena, CA, United States; University of Iowa, Iowa City, IA, United States; NASA Goddard Space Flight Center, Greenbelt, MD, United States

First steps toward data assimilation of Jupiter's radiation belts using Juno and radio observations and physics-based models

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