Core Dynamo Models

Core Dynamo Models is a computational or mathematical framework that simulates the generation and evolution of the Earth's magnetic field by modeling the fluid dynamo processes within the planet's outer core, distinguished by its incorporation of magnetohydrodynamics, rotational effects, and thermal convection to explain geomagnetic phenomena including reversals.

167

Publications

11.2K

Citations

287

Authors

175

Institutions

Publications per year

2017–2026

24

Variants

Geodynamo Models

Authors

287

  1. JA
    Julien Aubert

    Institut de physique du globe de Paris, France

    13 publications · 875 citations

    13

    h-index

  2. PO
    Peter Olson

    Johns Hopkins University, United States

    11 publications · 382 citations

    11

    h-index

  3. PR
    Paul Roberts

    University of California, Los Angeles, United States

    8 publications · 1.5K citations

    8

    h-index

  4. UR
    Ulrich R. Christensen

    Max Planck Institute for Solar System Research, Germany

    7 publications · 511 citations

    7

    h-index

  5. HA
    Hagay Amit

    Centre National de la Recherche Scientifique, France

    6 publications · 251 citations

    6

    h-index

1–5 of 287

Venues

  1. Geophysical Journal International

    GJI · 33 publications · 1.8K citations

    25

    h-index

  2. Geophysical Research Letters

    13 publications · 559 citations

    12

    h-index

  3. Geophysical & Astrophysical Fluid Dynamics

    11 publications · 545 citations

    11

    h-index

  4. Icarus

    9 publications · 413 citations

    9

    h-index

  5. Journal of Geophysical Research Atmospheres

    JGR · 9 publications · 353 citations

    9

    h-index

1–5