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Sources of solar wind over the solar activity cycle
Fast solar wind has been recognized, about 40 years ago, to originate in polar coronal holes (CHs), that, since then, have been identified with sources of recurrent high speed wind streams. As of today, however, there is no general consensus about whether there are, within CHs, preferential location...
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
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Elsevier
2013
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| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4295036/ https://www.ncbi.nlm.nih.gov/pubmed/25685421 http://dx.doi.org/10.1016/j.jare.2012.08.007 |