Slow Solar Wind
Slow Solar Wind is a type of solar wind characterized by lower velocities typically below 400 km/s, originating from the Sun's equatorial regions and distinguished from the fast solar wind by its higher density, lower speed, and association with closed magnetic field lines in the corona.
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16.7K
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648
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273
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2017–2026
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289
Highly structured slow solar wind emerging from an equatorial coronal hole
S. D. Bale, Samuel T. Badman, J. W. Bonnell et al. · Nature · 2019 · 582 citations · Full text
A MODEL FOR THE SOURCES OF THE SLOW SOLAR WIND
S. K. Antiochos, Z. Mikić, V. S. Titov et al. · The Astrophysical Journal · 2011 · 318 citations · Full text
Natural Sciences, Astronomy, Physics +17
J. T. Gosling, J. R. Asbridge, S. J. Bame et al. · Journal of Geophysical Research Atmospheres · 1978 · 306 citations
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University of Michigan
Ann Arbor, United States
30 h-index
84 publications
6.1K citations

Centre National de la Recherche Scientifique
Paris, France
29 h-index
123 publications
8.7K citations
Goddard Space Flight Center
Greenbelt, United States
28 h-index
65 publications
6.4K citations

United States Naval Research Laboratory
Washington, United States
24 h-index
56 publications
4.6K citations

University of New Hampshire
Durham, United States
18 h-index
37 publications
2.1K citations
University of California, Berkeley
Berkeley, United States
18 h-index
101 publications
12.8K citations
National Institute for Astrophysics
Rome, Italy
18 h-index
55 publications
1.7K citations

Sorbonne Université
Paris, France
17 h-index
43 publications
4.3K citations
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ApJ · 76 publications · 4.2K citations
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JGR · 44 publications · 3.9K citations
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22 publications · 1K citations
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23 publications · 2.2K citations
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20 publications · 543 citations
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