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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...

Deskribapen osoa

Gorde:
Xehetasun bibliografikoak
Argitaratua izan da:Living Rev Sol Phys
Egile nagusia: Cranmer, Steven R.
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: Springer International Publishing 2009
Gaiak:
Sarrera elektronikoa: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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