EGU24-8445, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-8445
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Measurements of ultra-relativistic electrons during solar energetic particle events - Results from the Ulysses Kiel Electron Telescope

Marlon Köberle, Bernd Heber, and Carlotta Jöhnk
Marlon Köberle et al.
  • Kiel University, Kiel, Germany (koeberle@physik.uni-kiel.de)

Solar energetic particle (SEP) events are increases of ions and electrons caused
by solar activity namely flares and coronal mass ejections. While the most
energetic ion population is well studied, SEP events accelerating electrons above
20 MeV have only been reported from measurements by ISEE III in the 1980’s
and the Kiel Electron Telescope (KET).
The KET aboard Ulysses launched in 1990 and measured the electron flux in
the energy range from 4 MeV to above 6 GeV. Here we report on observations
of ultra-relativistic electrons and show spectra of electron events during solar
cycle 22 and 23 until the end of 2008. The maximum electron energy exceeded
100 MeV during the August 16, 2001 SEP event.
This study has received funding from the European Union’s Horizon 2020
research and innovation programme under grant agreement No. 101004159
(SPEARHEAD).

How to cite: Köberle, M., Heber, B., and Jöhnk, C.: Measurements of ultra-relativistic electrons during solar energetic particle events - Results from the Ulysses Kiel Electron Telescope, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-8445, https://doi.org/10.5194/egusphere-egu24-8445, 2024.