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Solar Open Flux Migration from Pole to Pole: Magnetic Field Reversal
Coronal holes are solar regions with low soft X-ray or low extreme ultraviolet intensities. The magnetic fields from coronal holes extend far away from the Sun, and thus they are identified as regions with open magnetic field lines. Coronal holes are concentrated in the polar regions during the suns...
| Autores principales: | , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Nature Publishing Group UK
2017
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5572711/ https://www.ncbi.nlm.nih.gov/pubmed/28842682 http://dx.doi.org/10.1038/s41598-017-09862-2 |