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Relevant heating of the quiet solar corona by Alfvén waves: a result of adiabaticity breakdown
Ion heating by Alfvén waves has been considered for long as the mechanism explaining why the solar corona has a temperature several orders of magnitude higher than the photosphere. Unfortunately, as the measured wave frequencies are much smaller than the ion cyclotron frequency, particles were expec...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Nature Publishing Group UK
2019
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6776755/ https://www.ncbi.nlm.nih.gov/pubmed/31582798 http://dx.doi.org/10.1038/s41598-019-50820-x |