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Heating mechanisms of the solar corona
The solar corona is a tenuous outer atmosphere of the Sun. Its million-degree temperature was discovered spectroscopically in the 1940s, but its origin has been debated since then without complete convergence. Currently there are two classes of models; the wave theory and the microflare/nanoflare th...
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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The Japan Academy
2017
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5422629/ https://www.ncbi.nlm.nih.gov/pubmed/28190871 http://dx.doi.org/10.2183/pjab.93.006 |