On a possible control mechanism for solar wind outflow velocity from coronal holes
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/BF00680448.pdf
Reference20 articles.
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3. Eselevich, V. G. and Fainshtein, V. G.: 1992,Planetary Space Sci. 40, 105.
4. Eselevich, V. G. and Filippov, M. A.: 1986,Planetary Space Sci. 34, 1119.
5. Eselevich, V. G., Kaigorodov, A. P., and Fainshtein, V. G.: 1990,Planetary Space Sci. 38, 459.
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2. Characteristics of Low-latitude Coronal Holes near the Maximum of Solar Cycle 24;The Astrophysical Journal;2017-02-01
3. Propagation of the 12 May 1997 interplanetary coronal mass ejection in evolving solar wind structures;Journal of Geophysical Research;2005
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