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Beam electrons as a source of Hα flare ribbons

The observations of solar flare onsets show rapid increase of hard and soft X-rays, ultra-violet emission with large Doppler blue shifts associated with plasma upflows, and Hα hydrogen emission with red shifts up to 1–4 Å. Modern radiative hydrodynamic models account well for blue-shifted emission,...

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Detalles Bibliográficos
Autores principales: Druett, Malcolm, Scullion, Eamon, Zharkova, Valentina, Matthews, Sarah, Zharkov, Sergei, Rouppe Van der Voort, Luc
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group 2017
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5490266/
https://www.ncbi.nlm.nih.gov/pubmed/28653670
http://dx.doi.org/10.1038/ncomms15905