Supercritical Core Fluids
Supercritical Core Fluids is a theoretical construct in planetary core dynamics denoting a state of fluid matter within a planetary core that exists beyond its critical point, where distinct liquid and gas phases cease to exist, enabling unique regimes of density, compressibility, and heat transfer that govern core convection and magnetic field generation.
74
Publications
5.2K
Citations
232
Authors
117
Institutions
Publications per year
2017–2026
19
Parents
74
1–5 of 74
232
3
h-index
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Dagestan Scientific Center of the Russian Academy of Sciences, Russia
2 publications · 49 citations
2
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2
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1–5 of 232
117

Centre National de la Recherche Scientifique
Paris, France
4 h-index
15 publications
578 citations
Queen Mary University of London
London, United Kingdom
2 h-index
5 publications
122 citations
Dagestan State University
Makhachkala, Russia
2 h-index
2 publications
49 citations

University of Rochester
Rochester, United States
2 h-index
6 publications
165 citations
Institut de Chimie de la Matière Condensée de Bordeaux
Pessac, France
2 h-index
8 publications
352 citations
Virginia Tech
Blacksburg, United States
2 h-index
2 publications
185 citations

University of Pisa
Pisa, Italy
2 h-index
5 publications
128 citations
GFZ Helmholtz Centre for Geosciences
Potsdam, Germany
2 h-index
4 publications
83 citations
1–8 of 117
14 publications · 1.8K citations
12
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3 publications · 131 citations
3
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2 publications · 79 citations
2
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2 publications · 54 citations
2
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2 publications · 50 citations
2
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1–5