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Search for sources of solar cosmic rays in weak events
- Authors: Bazilevskaya G.A.1, Daibog E.I.2, Logachev Y.I.2
-
Affiliations:
- Lebedev Physical Institute of the Russian Academy of Sciences
- Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
- Issue: Vol 87, No 7 (2023)
- Pages: 1002-1004
- Section: Articles
- URL: https://journals.rcsi.science/0367-6765/article/view/135436
- DOI: https://doi.org/10.31857/S0367676523701764
- EDN: https://elibrary.ru/ORZTRP
- ID: 135436
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Abstract
Some of the weak solar proton events recorded by the Earth observer, in which protons with energy E > 10 MeV were observed, are really particles accelerated by a shock wave in interplanetary space. They can be associated with a flare and a coronal mass ejection ten of hours before the observed proton event, which ensure the injection of particles into the process of their subsequent acceleration in interplanetary space.
About the authors
G. A. Bazilevskaya
Lebedev Physical Institute of the Russian Academy of Sciences
Email: daibog@srd.sinp.msu.ru
Russia, 119991, Moscow
E. I. Daibog
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Author for correspondence.
Email: daibog@srd.sinp.msu.ru
Russia, 119991, Moscow
Yu. I. Logachev
Lomonosov Moscow State University, Skobeltsyn Institute of Nuclear Physics
Email: daibog@srd.sinp.msu.ru
Russia, 119991, Moscow
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