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Autor:
Eugene A. Maurchev, Nataly S. Shlyk, Alexey V. Dmitriev, Maria A. Abunina, Kseniia A. Didenko, Artem A. Abunin, Anatoly V. Belov
Publikováno v:
Atmosphere, Vol 15, Iss 2, p 151 (2024)
Numerical modeling of primary cosmic ray protons’ transport through the Earth’s atmosphere was performed for the energy spectra of solar energetic particle events (SEPs). Several events in the last three solar cycles were considered. A comparativ
Externí odkaz:
https://doaj.org/article/95792f8ecade44ed9803591c68c9d7bb
