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

Authors

419

  1. PO
    Peter Olson

    Johns Hopkins University, United States

    20 publications · 1.1K citations

    17

    h-index

  2. DG
    David Gubbins

    University of Leeds, United Kingdom

    16 publications · 931 citations

    14

    h-index

  3. UR
    Ulrich R. Christensen

    Max Planck Institute for Solar System Research, Germany

    13 publications · 1.3K citations

    13

    h-index

  4. JW
    Johannes Wicht

    Max Planck Institute for Solar System Research, Germany

    12 publications · 835 citations

    12

    h-index

  5. PR
    Paul Roberts

    University of California, Los Angeles, United States

    12 publications · 1.8K citations

    12

    h-index

1–5 of 419

Venues

  1. Geophysical Journal International

    GJI · 48 publications · 2.9K citations

    32

    h-index

  2. Geophysical & Astrophysical Fluid Dynamics

    25 publications · 1.1K citations

    21

    h-index

  3. Geophysical Research Letters

    24 publications · 1.2K citations

    19

    h-index

  4. Physics of The Earth and Planetary Interiors

    22 publications · 1.8K citations

    16

    h-index

  5. The Astrophysical Journal

    ApJ · 13 publications · 1K citations

    13

    h-index

1–5