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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...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Springer Netherlands
2017
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| 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 |