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Full-Sun observations for identifying the source of the slow solar wind
Fast (>700 km s(−1)) and slow (~400 km s(−1)) winds stream from the Sun, permeate the heliosphere and influence the near-Earth environment. While the fast wind is known to emanate primarily from polar coronal holes, the source of the slow wind remains unknown. Here we identify possible sites of o...
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| Pubblicato in: | Nat Commun |
|---|---|
| Autori principali: | , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Nature Pub. Group
2015
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| Soggetti: | |
| Accesso online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC4354106/ https://ncbi.nlm.nih.gov/pubmed/25562705 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1038/ncomms6947 |
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