B3 Non-refereed article in a conference publication
Consistency of the average flux of solar energetic particles over different timescales up to mega-years
Authors: Usoskin, Ilya; Koldobskiy, Sergey; Pouianov, Stepan; Raukunen, Osku; Vainio, Rami; Kovaltsov, Gennady
Editors: Saito, Takayuki; Okumura, Kimihiro
Conference name: International Cosmic Ray Conference
Publisher: Sissa Medialab Srl
Publication year: 2024
Journal: POS Proceedings of Science
Book title : Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)
Journal name in source: Proceedings of Science
Article number: 1244
Volume: 444
eISSN: 1824-8039
DOI: https://doi.org/10.22323/1.444.1244
Web address : https://pos.sissa.it/444/1244
Self-archived copy’s web address: https://research.utu.fi/converis/portal/detail/Publication/484557927
Fluxes of solar energetic particles (SEPs) produced during solar eruptive events such as flares or coronal mass ejections are directly measured by space-borne detectors over the past decades. However, rare (about once per millennium) extreme SEP events have been recently discovered as studied by terrestrial cosmogenic proxy data for the past ten millennia. In addition, isotopic analysis of lunar rocks can reveal the average SEP fluxes on the mega-year timescale. Until now, it was unclear whether the SEP fluxes averaged over different timescales are mutually consistent. These different datasets are analyzed here to study their mutual consistency. Using the data from directly measured SEPs and reconstructions of extreme SEP events, we built a joint probability distribution function of the occurrence of SEP annual integral fluxes in the energy range between 30 and 200 MeV on different timescales. Based on that, the expected long-time averaged SEP flux was computed and directly compared to the lunar data representing the mega-year SEP flux. The results imply that contrary to the earlier assumptions, the SEP fluxes directly measured during the recent decades are not representative of the long-term averaged SEP flux as they compose only 20 – 55 % of it. A major fraction of the mega-year averaged SEP flux is formed by rare but extremely strong SEP events. It is shown that the combined statistics of all three different datasets and timescales (decadal direct data, millennial cosmogenic proxy data and mega-year lunar data) are fully consistent, implying that our knowledge of the whole range of the SEP fluxes, from frequent weak events to rare extreme ones, is likely complete now.
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