Cutoff rigidities, galactic cosmic ray flux, and heavy ion detections at Jupiter
- Martin Bødker Enghoff
, - Martin B Enghoff,
- Jacob Svensmark,
- Heidi N Becker,
- John L Jørgensen,
- Stavros Kotsiaros,
- Matija Herceg,
- James W Alexander,
- Meghan M Florence,
- John E P Connerney
Martin B Enghoff
National Space Institute, Technical University of Denmark, Kongens Lyngby
Jacob Svensmark
Niels Bohr Institute, University of Copenhagen, Department of Physics, Atmospheric, Oceanic and Planetary Physics, University of Oxford
Heidi N Becker
Jet Propulsion Laboratory, California Institute of Technology
John L Jørgensen
National Space Institute, Technical University of Denmark, Kongens Lyngby
Stavros Kotsiaros
National Space Institute, Technical University of Denmark, Kongens Lyngby
Matija Herceg
National Space Institute, Technical University of Denmark, Kongens Lyngby
James W Alexander
Jet Propulsion Laboratory, California Institute of Technology
Meghan M Florence
Jet Propulsion Laboratory, California Institute of Technology
John E P Connerney
Space Research Corporation
Abstract
• A galactic cosmic ray cutoff rigidity map for Jupiter was made using the JRM33 model and the Geomagnetic Cutoff Rigidity Computer Program • The flux of galactic cosmic ray protons into Jupiter's atmosphere was calculated based on BESS-Polar ii data • Detections of heavy ions by Juno's SRU were investigated and used to estimate their equatorial pitch angles22 Jan 2024Submitted to ESS Open Archive 22 Jan 2024Published in ESS Open Archive
