In this paper, by considering an example of four Carrington rotations ( 167 l, 1672, 1681, and 1682), it is shown that there generally exists an exhaustive correspondence between quasi-stationary flows of'fast' and 'slow' solar wind (SW), on the one hand, and their sources on the Sun: coronal holes
β¦ LIBER β¦
Concerning sources of eruptive flows on the sun
β Scribed by V.G. Eselevich
- Book ID
- 107844823
- Publisher
- Elsevier Science
- Year
- 1991
- Tongue
- English
- Weight
- 739 KB
- Volume
- 39
- Category
- Article
- ISSN
- 0032-0633
No coin nor oath required. For personal study only.
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