EGU21-9953, updated on 04 Mar 2021
https://doi.org/10.5194/egusphere-egu21-9953
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Multi-energy analysis of SPREAdFAST proton events

Rositsa Miteva, Kamen Kozarev, and Mohamed Nedal
Rositsa Miteva et al.
  • Institute of Astronomy with National Astronomical Observatory - Bulgarian Academy of Sciences, Sofia, Bulgaria (rmiteva@nao-rozhen.org)

We present the procedure of event selection, data analysis and interpretation of solar energetic protons during the last solar cycle 24 for the needs of the SPREAdFAST project. Data from SOHO/ERNE and ACE/EPAM instruments have been analysed for nearly 100 proton events in the available energy bands. The energy dependence of the proton peak intensities and background spectra is completed. The energy range from a few to 130 MeV has been covered. Protons from the SPREAdFAST historical event list have been selected for a detailed comparative analysis. The validation between the observed and simulated proton events is presented and discussed.

How to cite: Miteva, R., Kozarev, K., and Nedal, M.: Multi-energy analysis of SPREAdFAST proton events, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-9953, https://doi.org/10.5194/egusphere-egu21-9953, 2021.

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