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The birth of a coronal mass ejection

The Sun’s atmosphere is frequently disrupted by coronal mass ejections (CMEs), coupled with flares and energetic particles. The coupling is usually attributed to magnetic reconnection at a vertical current sheet connecting the flare and CME, with the latter embedding a helical magnetic structure kno...

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Detalles Bibliográficos
Autores principales: Gou, Tingyu, Liu, Rui, Kliem, Bernhard, Wang, Yuming, Veronig, Astrid M.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: American Association for the Advancement of Science 2019
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6428586/
https://www.ncbi.nlm.nih.gov/pubmed/30906858
http://dx.doi.org/10.1126/sciadv.aau7004