Unusual enhancement of ~ 30 MeV proton flux in an ICME sheath region

In gradual Solar Energetic Particle (SEP) events, shock waves driven by coronal mass ejections (CMEs) play a major role in accelerating particles, and the energetic particle flux enhances substantially when the shock front passes by the observer. Such enhancements are historically referred to as Ene...

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Detalles Bibliográficos
Autores principales: Oka, Mitsuo, Obara, Takahiro, Nitta, Nariaki V., Yashiro, Seiji, Shiota, Daikou, Ichimoto, Kiyoshi
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2021
Materias:
Express Letter
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7846546/
https://www.ncbi.nlm.nih.gov/pubmed/33584116
http://dx.doi.org/10.1186/s40623-021-01362-y

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7846546/
https://www.ncbi.nlm.nih.gov/pubmed/33584116
http://dx.doi.org/10.1186/s40623-021-01362-y

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