Core Dynamos
Core Dynamo is a geophysical process model that generates planetary magnetic fields through the convective motion of electrically conducting fluids within a rotating planetary core, thereby distinguishing it from alternative magnetic field generation mechanisms by its reliance on rotational and magnetohydrodynamic effects.
291
Publications
19.6K
Citations
419
Authors
238
Institutions
Publications per year
2017–2026
47
Variants
Geodynamos
291
Geodynamo theory and simulations
Paul Roberts, Gary A. Glatzmaier · Reviews of Modern Physics · 2000 · 349 citations
1–5 of 291
419
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14
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Max Planck Institute for Solar System Research, Germany
13 publications · 1.3K citations
13
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Max Planck Institute for Solar System Research, Germany
12 publications · 835 citations
12
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12
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1–5 of 419
238

Centre National de la Recherche Scientifique
Paris, France
31 h-index
83 publications
5.5K citations
Planetary Science Institute
Tucson, United States
31 h-index
83 publications
7.7K citations

Institut de physique du globe de Paris
Paris, France
18 h-index
43 publications
2.5K citations

University of Leeds
Leeds, United Kingdom
17 h-index
30 publications
1.4K citations
University of California, Los Angeles
Los Angeles, United States
17 h-index
35 publications
3K citations

Johns Hopkins University
Baltimore, United States
17 h-index
31 publications
2.3K citations
Université Paris Cité
Paris, France
16 h-index
36 publications
2.4K citations
Massachusetts Institute of Technology
Cambridge, United States
15 h-index
51 publications
4.9K citations
1–8 of 238
GJI · 48 publications · 2.9K citations
32
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25 publications · 1.1K citations
21
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24 publications · 1.2K citations
19
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22 publications · 1.8K citations
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ApJ · 13 publications · 1K citations
13
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