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Large gradual solar energetic particle events
Solar energetic particles, or SEPs, from suprathermal (few keV) up to relativistic ([Formula: see text] few GeV) energies are accelerated near the Sun in at least two ways: (1) by magnetic reconnection-driven processes during solar flares resulting in impulsive SEPs, and (2) at fast coronal-mass-eje...
Autores principales: | , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer International Publishing
2016
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7175685/ https://www.ncbi.nlm.nih.gov/pubmed/32355890 http://dx.doi.org/10.1007/s41116-016-0002-5 |