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

Authors

232

  1. MP
    M. Perrut

    Separex (France), France

    3 publications · 1.2K citations

    3

    h-index

  2. AP
    Andrea Pucciarelli

    University of Pisa, Italy

    2 publications · 53 citations

    2

    h-index

  3. YD
    Yu. D. Fomin

    Institute for High Pressure Physics, Russia

    2 publications · 41 citations

    2

    h-index

  4. IM
    Ilmutdin M. Abdulagatov

    Dagestan Scientific Center of the Russian Academy of Sciences, Russia

    2 publications · 49 citations

    2

    h-index

  5. VN
    V. N. Ryzhov

    Institute for High Pressure Physics, Russia

    2 publications · 41 citations

    2

    h-index

1–5 of 232

Venues

  1. The Journal of Supercritical Fluids

    14 publications · 1.8K citations

    12

    h-index

  2. Nuclear Engineering and Design

    3 publications · 131 citations

    3

    h-index

  3. Lithos

    2 publications · 79 citations

    2

    h-index

  4. Fluid Phase Equilibria

    2 publications · 54 citations

    2

    h-index

  5. Journal of Chromatography A

    2 publications · 50 citations

    2

    h-index

1–5