EGU24-6034, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-6034
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

A new scenario for widespread solar energetic particle events based on multi-spacecraft observations of the 13 March 2023 event

Nina Dresing1, Immanuel Jebaraj1, Erika Palmerio2, Christian Palmroos1, Christian Cohen3, Grant Mitchell4, Christina Lee5, Wenwen Wei5, Eleanna Asvestari6, Manon Jarry7, Gabriel Muro3, Laura Rodríguz-García8, and Nicola Wijsen9
Nina Dresing et al.
  • 1University of Turku, Finland (nina.dresing@utu.fi)
  • 2Predictive Science Inc., San Diego, CA, United States
  • 3Caltech, Pasadena, United States
  • 4NASA Goddard Space Flight Center, Greenbelt, MD, United States
  • 5Space Sciences Lab, UC Berkeley, United States
  • 6University of Helsinki, Finland
  • 7IRAP, CNRS, Université de Toulouse III-Paul Sabatier, Toulouse, France
  • 8Universidad de Alcalá, Department of Physics, Space Research Group, Alcalá de Henares, Spain
  • 9Department of Mathematics, KU Leuven, Leuven, Belgium

We report on multi-spacecraft measurements of a solar energetic particle (SEP) event that occurred on 13 March 2023. The Parker Solar Probe (PSP) mission was situated on the far side of the Sun as seen from Earth at a radial distance of only 49 solar radii and observed a very strong event including the associated CME and its shock passing over the spacecraft only four hours after the solar eruption. Solar Orbiter, BepiColombo, STEREO A, near-Earth spacecraft, and MAVEN at Mars were all situated within 50 degrees in longitude, and observed the event as well, proving its widespread character. Clear signatures of shock-driven energetic storm particle events were present at Solar Orbiter, STEREO A, and near-Earth spacecraft suggesting that the interplanetary CME-driven shock had a longitudinal extent of about 160 degrees. However, the solar event was accompanied by a series of pre-event CMEs and comparison with ENLIL simulation results suggest that the ESP events were associated with shocks driven by other CMEs. This scenario of particle re-acceleration at different pre-event-associated shocks, provides a new scenario for the generation of widespread SEP events. 

How to cite: Dresing, N., Jebaraj, I., Palmerio, E., Palmroos, C., Cohen, C., Mitchell, G., Lee, C., Wei, W., Asvestari, E., Jarry, M., Muro, G., Rodríguz-García, L., and Wijsen, N.: A new scenario for widespread solar energetic particle events based on multi-spacecraft observations of the 13 March 2023 event, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-6034, https://doi.org/10.5194/egusphere-egu24-6034, 2024.