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Observationally quantified reconnection providing a viable mechanism for active region coronal heating

The heating of the Sun’s corona has been explained by several different mechanisms including wave dissipation and magnetic reconnection. While both have been shown capable of supplying the requisite power, neither has been used in a quantitative model of observations fed by measured inputs. Here we...

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Detalles Bibliográficos
Autores principales: Yang, Kai E., Longcope, Dana W., Ding, M. D., Guo, Yang
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2018
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5814417/
https://www.ncbi.nlm.nih.gov/pubmed/29449655
http://dx.doi.org/10.1038/s41467-018-03056-8