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Particle Acceleration Due to Coronal Non-null Magnetic Reconnection

Various topological features, for example magnetic null points and separators, have been inferred as likely sites of magnetic reconnection and particle acceleration in the solar atmosphere. In fact, magnetic reconnection is not constrained to solely take place at or near such topological features an...

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Detalles Bibliográficos
Autores principales: Threlfall, James, Neukirch, Thomas, Parnell, Clare Elizabeth
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2017
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7089664/
https://www.ncbi.nlm.nih.gov/pubmed/32226172
http://dx.doi.org/10.1007/s11207-017-1060-0