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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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Kaydedildi:
Detaylı Bibliyografya
Yayımlandı:Living Rev Sol Phys
Yazar: Cranmer, Steven R.
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: Springer International Publishing 2009
Konular:
Online Erişim: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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