Convective Dynamo Action
Convective Dynamo Action is a physical mechanism within the broader class of dynamo processes that generates and sustains large-scale magnetic fields in stellar interiors through the combined effects of turbulent convection and rotational shear, distinguishing it from purely laminar or induction-driven dynamos by its reliance on convective fluid motions to amplify and organize magnetic flux.
218
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17.2K
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314
Authors
220
Institutions
Publications per year
2017–2026
39
Parents
218
Large-scale magnetic topologies of late M dwarfs★
J. Morin, J.‐F. Donati, P. Petit et al. · Monthly Notices of the Royal Astronomical Society · 2010 · 459 citations · Full text
Natural Sciences, Astronomy, Physics +13
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Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France
9 publications · 1.5K citations
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Joint Institute for Laboratory Astrophysics, United States
8 publications · 1.3K citations
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8
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8
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Centre National de la Recherche Scientifique
Paris, France
21 h-index
73 publications
10.2K citations
Max Planck Institute for Solar System Research
Göttingen, Germany
15 h-index
26 publications
2.8K citations

University of Leeds
Leeds, United Kingdom
14 h-index
26 publications
1.4K citations

University of Exeter
Exeter, United Kingdom
13 h-index
24 publications
1.1K citations
Université Paris Cité
Paris, France
13 h-index
22 publications
2.8K citations
NSF NCAR High Altitude Observatory
Boulder, United States
12 h-index
15 publications
1.7K citations
University of Cambridge
Cambridge, United Kingdom
12 h-index
15 publications
878 citations
University of Colorado Boulder
Boulder, United States
12 h-index
20 publications
1.6K citations
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ApJ · 35 publications · 4.7K citations
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17 publications · 938 citations
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19 publications · 713 citations
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11 publications · 982 citations
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10 publications · 437 citations
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