Energetic protons in Jupiter's magnetotail
Energetic protons (220 - 540 keV/nuc) observed by Galileo on orbits G8 and C9 in the Jovian magnetotail from DOY 150 to DOY 200 in 1997. The vertical lines denote the times when substorms occur.
See the related image in the right-hand menu for similar data of substorms in Earth's magnetotail, obtained wth the ESA Cluster mission.
Last Update: 1 September 2019