Fast Solar Wind
Fast Solar Wind is a type of solar wind characterized by high velocity streams, typically exceeding 500 km/s, that originate from coronal holes and exhibit lower density and temperature compared to the slow solar wind.
270
Publications
15.4K
Citations
658
Authors
276
Institutions
Publications per year
2017–2026
49
Parents
270
Alfvénic waves with sufficient energy to power the quiet solar corona and fast solar wind
Scott W. McIntosh, Bart De Pontieu, M. Carlsson et al. · Nature · 2011 · 599 citations
Natural Sciences, Astronomy, Physics +17
1–5 of 270
658
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Center for Astrophysics Harvard & Smithsonian, United States
11 publications · 449 citations
11
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1–5 of 658
276

Imperial College London
London, United Kingdom
23 h-index
52 publications
4.8K citations
University of Michigan
Ann Arbor, United States
20 h-index
64 publications
3.2K citations
Laboratoire d’études spatiales et d’instrumentation en astrophysique
Meudon, France
20 h-index
43 publications
4.6K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
18 h-index
36 publications
2.1K citations

Centre National de la Recherche Scientifique
Paris, France
18 h-index
43 publications
4.7K citations

Observatoire de Paris
Paris, France
17 h-index
37 publications
4.4K citations

Southwest Research Institute
San Antonio, United States
17 h-index
31 publications
2.4K citations
Jet Propulsion Laboratory
Pasadena, United States
17 h-index
27 publications
2.1K citations
1–8 of 276
ApJ · 74 publications · 4.4K citations
37
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JGR · 56 publications · 3.7K citations
35
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20 publications · 1.5K citations
18
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15 publications · 771 citations
14
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17 publications · 519 citations
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