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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Detalles Bibliográficos
Autores principales: Huang, G.-H., Lin, C.-H., Lee, L. C.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2017
Materias:
Article
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

Internet

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

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