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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...
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| Publicado no: | Sci Rep |
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| Main Authors: | , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Nature Publishing Group UK
2017
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC5572711/ https://ncbi.nlm.nih.gov/pubmed/28842682 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/s41598-017-09862-2 |
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