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Coronal Holes
Coronal holes are the darkest and least active regions of the Sun, as observed both on the solar disk and above the solar limb. Coronal holes are associated with rapidly expanding open magnetic fields and the acceleration of the high-speed solar wind. This paper reviews measurements of the plasma pr...
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| Gepubliceerd in: | Living Rev Sol Phys |
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| Hoofdauteur: | |
| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Springer International Publishing
2009
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| Onderwerpen: | |
| Online toegang: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4841186/ https://ncbi.nlm.nih.gov/pubmed/27194961 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.12942/lrsp-2009-3 |
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