EGU25-7322, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-7322
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under the Creative Commons Attribution 4.0 License.
Characteristic Properties of 30 eV to 30 keV Electrons at Low-Altitude Over Jupiter’s Northern Polar Aurora
1,2,1,2,6,7,8,1,- 1Southwest Research Institute, Department of Space Research, San Antonio, Texas, United States of America (rebert@swri.edu)
- 2Department of Physics and Astronomy, University of Texas at San Antonio, San Antonio, Texas, USA
- 3Johns Hopkins University Applied Physics Lab, Laurel, Maryland, USA
- 4School of Physics and Astronomy, College of Science and Engineering, University of Minnesota, Minneapolis, Minnesota, USA
- 5Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, Colorado, USA
- 6Space Research Corporation, Annapolis, Maryland, USA
- 7NASA Goddard Space Flight Center, Greenbelt, Maryland, USA
- 8Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey, USA
How to cite: Ebert, R., Clark, G., Elliott, S., Allegrini, F., Bagenal, F., Bolton, S., Connerney, J., Szalay, J., Valek, P., and Wilson, R.: Characteristic Properties of 30 eV to 30 keV Electrons at Low-Altitude Over Jupiter’s Northern Polar Aurora, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7322, https://doi.org/10.5194/egusphere-egu25-7322, 2025.