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The mechanisms that produce solar energetic particles (SEPs) are still highly debated but coronal shock waves have been proposed as efficient particle accelerators that may be implicated in the production of SEPs.An analysis of 32 Coronal Mass Ejecti
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::df942107766aafd16fe7c98a76e7f149
https://doi.org/10.5194/egusphere-egu23-6946
https://doi.org/10.5194/egusphere-egu23-6946
Autor:
Manon Jarry, Alexis P. Rouillard, Illya Plotnikov, Athanasios Kouloumvakos, Alexander Warmuth
Publikováno v:
Astronomy & Astrophysics. 672:A127
Coronal and interplanetary shock waves produced by coronal mass ejections (CMEs) are major drivers of space-weather phenomena, inducing major changes in the heliospheric radiation environment and directly perturbing the near-Earth environment, includ