EGU26-3730, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-3730
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 05 May, 08:30–10:15 (CEST), Display time Tuesday, 05 May, 08:30–12:30
 
Hall X4, X4.132
Simulations of Plasma Observatory's Energetic Particle Experiment
Hannes Ebeling1, Svea Jürgensen1, Christopher Liu2, Patrick Kühl1, Lars Berger1, Robert F. Wimmer-Schweingruber1, Vassilis Angelopoulos2, Ethan Tsai2, Ryan Caron2, Colin Wilkins2, Malcolm W. Dunlop3, Demet Ulusen Aksoy3, Mark Prydderch3, Alex Steven3, Rami Vainio4, and Jussi Lehti5
Hannes Ebeling et al.
  • 1Kiel University, Institute of Experimental and Applied Physics, Department for Extraterrestrial Physics, Kiel, Germany
  • 2University of California, Los Angeles, CA, USA
  • 3RAL Space, STFC (UKRI), Didcot, UK
  • 4University of Turku, Turku, Finland
  • 5ASRO, Turku, Finland

Plasma Observatory is a candidate for the European Space Agency's upcoming M7 science mission. It will investigate how particles are energized in space plasmas and how energy is transported across different scales and regions of the Earth’s magnetosphere. For this, the Energetic Particle Experiment (EPE) provides electron and ion measurements in the energy range from 30 to 600 keV, with an optional extension of measurements down to around 20 keV for electrons and ions and up to 1.5 MeV for ions. Both electron and ion measurements have an energy resolution of 20 % or better. The design of the EPE is based on the well-proven magnet-foil technique and features two geometrical factors for both electrons and ions in order to increase the dynamic range of observable fluxes.

To validate and demonstrate the EPE's capabilities, GEANT4 Monte Carlo simulations of the current instrument design were performed, which allowed to derive the geometrical factors and energy-dependent responses to electrons and protons. Based on these results, the instrument’s performance in the expected particle flux environments during the Plasma Observatory mission were investigated.

How to cite: Ebeling, H., Jürgensen, S., Liu, C., Kühl, P., Berger, L., Wimmer-Schweingruber, R. F., Angelopoulos, V., Tsai, E., Caron, R., Wilkins, C., Dunlop, M. W., Ulusen Aksoy, D., Prydderch, M., Steven, A., Vainio, R., and Lehti, J.: Simulations of Plasma Observatory's Energetic Particle Experiment, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3730, https://doi.org/10.5194/egusphere-egu26-3730, 2026.