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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...
| Autores principales: | , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2018
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| 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 |