Magnetically Controlled Stellar Winds
Magnetically Controlled Stellar Winds is a theoretical construct in astrophysics that models stellar winds as outflows of ionized particles whose dynamics, geometry, and mass-loss rates are dominantly regulated by the large-scale magnetic field of the host star.
50
Publications
3K
Citations
101
Authors
72
Institutions
Publications per year
2017–2026
11
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1–5 of 50
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Center for Astrophysics Harvard & Smithsonian, United States
3 publications · 163 citations
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3
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1–5 of 101
72
University of Delaware
Newark, United States
4 h-index
6 publications
924 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
4 h-index
6 publications
198 citations
Institute of Astronomy
Moscow, Russia
3 h-index
5 publications
91 citations
Institut de Planétologie et d'Astrophysique de Grenoble
Grenoble, France
2 h-index
2 publications
115 citations
University of Washington
Seattle, United States
2 h-index
2 publications
66 citations
Centre de Recherche Astrophysique de Lyon
Lyon, France
2 h-index
3 publications
151 citations
University of California, Santa Barbara
Santa Barbara, United States
2 h-index
3 publications
600 citations
Goddard Space Flight Center
Greenbelt, United States
2 h-index
4 publications
321 citations
1–8 of 72
ApJ · 17 publications · 1.2K citations
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10 publications · 543 citations
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AJ · 3 publications · 128 citations
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2 publications · 77 citations
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2 publications · 143 citations
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