From high-latitude auroral beams to equatorial radiation belts: Results from the JEDI instrument at Jupiter


Peter Kollmann1, George B Clark1, Barry Mauk1, Chris Paranicas1, Dennis K Haggerty2, Abigail M Rymer1, Joachim Saur3, John E P Connerney4, Steven Levin5 and Scott J Bolton6, (1)Johns Hopkins University Applied Physics Laboratory, Laurel, MD, United States, (2)Johns Hopkins Univ, Laurel, MD, United States, (3)University of Cologne, Cologne, Germany, (4)Space Research Corporation, Annapolis, United States, (5)Jet Propulsion Laboratory, Pasadena, United States, (6)Southwest Research Institute, San Antonio, United States
Back to: Our Evolving Understanding of Auroral Processes and Magnetosphere Dynamics at Jupiter Through Juno and Earth-Based Observations I