Method to observe O+ and S2+ by the JADE-I instrument on NASA’s Juno mission to Jupiter
Thomas K Kim1,2, Philip W Valek2, David J McComas3, Scott J Bolton4, Frederic Allegrini4, Nigel G Angold5, Fran Bagenal6, Kyung Chae2, John E P Connerney7, Robert W Ebert2, Steven Levin8, Chad E Loeffler2, Philippe Louarn9, Craig J Pollock10, Drake A Ranquist11, Michelle L Reno2, Jamey Szalay2, Michelle F Thomsen12, Scott Weidner13, Robert J Wilson14 and Jenna Lynn Zink1, (1)University of Texas at San Antonio, San Antonio, TX, United States, (2)Southwest Research Institute, San Antonio, TX, United States, (3)Princeton University, Department of Astrophysical Sciences and Office of the Vice President for the Princeton Plasma Physics Laboratory, Princeton, NJ, United States, (4)Southwest Research Institute, San Antonio, United States, (5)Angold Consulting for SwRI, La Cañada, CA, United States, (6)University of Colorado at Boulder, Boulder, CO, United States, (7)Space Research Corporation, Annapolis, United States, (8)Jet Propulsion Laboratory, Pasadena, CA, United States, (9)IRAP, Toulouse, France, (10)University of Alaska Fairbanks, Geophysical Institute, Fairbanks, AK, United States, (11)Laboratory for Atmospheric and Space Physics, Boulder, CO, United States, (12)Planetary Science Institute Tucson, Tucson, AZ, United States, (13)Princeton University, Princeton, NJ, United States, (14)University of Colorado Boulder, Laboratory for Atmospheric and Space Physics, Boulder, United States
Scientific Team Name: Juno JADE Team
