Dynamo-related Core Evolution

Dynamo-Related Core Evolution is a theoretical framework within planetary science that describes the temporal development of a planet's metallic core through convective and compositional changes driven by magnetic dynamo activity, distinguishing it from non-dynamo thermal or chemical evolution models.

40

Publications

2.8K

Citations

97

Authors

75

Institutions

Publications per year

2017–2026

9

Authors

97

  1. BP
    B. P. Weiss

    Massachusetts Institute of Technology, United States

    9 publications · 1.1K citations

    9

    h-index

  2. SM
    Sonia M. Tikoo-Schantz

    Planetary Science Institute, United States

    6 publications · 744 citations

    6

    h-index

  3. DL
    David L. Shuster

    University of California, Berkeley, United States

    5 publications · 637 citations

    5

    h-index

  4. TL
    T. L. Grove

    Massachusetts Institute of Technology, United States

    5 publications · 574 citations

    5

    h-index

  5. JG
    J. Gattacceca

    Centre de Recherche et d’Enseignement de Géosciences de l’Environnement, France

    4 publications · 446 citations

    4

    h-index

1–5 of 97

Venues

  1. Icarus

    6 publications · 254 citations

    6

    h-index

  2. Journal of Geophysical Research Planets

    6 publications · 201 citations

    6

    h-index

  3. Science

    6 publications · 754 citations

    6

    h-index

  4. Physics of The Earth and Planetary Interiors

    3 publications · 278 citations

    3

    h-index

  5. Earth and Planetary Science Letters

    3 publications · 136 citations

    3

    h-index

1–5