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Origins and properties of the quasi-stationary slow solar wind

โœ Scribed by M. V. Eselevich; V. G. Eselevich; K. Fujiki


Book ID
111436667
Publisher
Springer
Year
2008
Tongue
English
Weight
962 KB
Volume
52
Category
Article
ISSN
1063-7729

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๐Ÿ“œ SIMILAR VOLUMES


Relationships of quasi-stationary solar
โœ V. G. Eselevich ๐Ÿ“‚ Article ๐Ÿ“… 1992 ๐Ÿ› Springer ๐ŸŒ English โš– 1000 KB

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

The Long Slow Rise of Solar and Wind
โœ Smil, Vaclav ๐Ÿ“‚ Article ๐Ÿ“… 2013 ๐Ÿ› Nature Publishing Group ๐ŸŒ English โš– 519 KB