Accelerated Flows at Jupiter’s Magnetopause: Evidence for Magnetic Reconnection Along the Dawn Flank
Robert W Ebert1, Frederic Allegrini2,3, Scott J Bolton3, Fran Bagenal4, John E P Connerney5, George B Clark6, William S Kurth7, Steven Levin8, Philippe Louarn9, Barry Mauk10, David J McComas1,11, Michelle L Reno1,12, Michelle F Thomsen13, Philip W Valek1,14, Scott Weidner15 and Robert J Wilson16, (1)Southwest Research Institute, San Antonio, TX, United States, (2)University of Texas at San Antonio, Department of Physics & Astronomy, San Antonio, TX, United States, (3)Southwest Research Institute, San Antonio, United States, (4)University of Colorado at Boulder, Boulder, CO, United States, (5)Space Research Corporation, Annapolis, United States, (6)The Johns Hopkins University Applied Physics Laboratory, Laurel, United States, (7)University of Iowa, Iowa City, IA, United States, (8)Jet Propulsion Laboratory, Pasadena, United States, (9)IRAP, Toulouse, France, (10)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (11)Princeton University, Department of Astrophysical Sciences and Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (12)Austin Mission Consulting, Austin, TX, United States, (13)Planetary Science Institute Tucson, Tucson, AZ, United States, (14)University of Texas at San Antonio, Department of Physics and Astronomy, San Antonio, TX, United States, (15)Princeton University, Princeton, NJ, United States, (16)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
