Convective Dynamo Action

Convective Dynamo Action is a physical mechanism within the broader class of dynamo processes that generates and sustains large-scale magnetic fields in stellar interiors through the combined effects of turbulent convection and rotational shear, distinguishing it from purely laminar or induction-driven dynamos by its reliance on convective fluid motions to amplify and organize magnetic flux.

218

Publications

17.2K

Citations

314

Authors

220

Institutions

Publications per year

2017–2026

39

Authors

314

  1. AB
    Axel Brandenburg

    Stockholm University, Sweden

    12 publications · 1K citations

    11

    h-index

  2. AS
    A. S. Brun

    Commissariat à l'Énergie Atomique et aux Énergies Alternatives, France

    9 publications · 1.5K citations

    9

    h-index

  3. JT
    Juri Toomre

    Joint Institute for Laboratory Astrophysics, United States

    8 publications · 1.3K citations

    8

    h-index

  4. MR
    M. R. E. Proctor

    University of Cambridge, United Kingdom

    8 publications · 229 citations

    8

    h-index

  5. CA
    C. A. Jones

    University of Exeter, United Kingdom

    8 publications · 610 citations

    8

    h-index

1–5 of 314

Venues

  1. The Astrophysical Journal

    ApJ · 35 publications · 4.7K citations

    28

    h-index

  2. Astronomy and Astrophysics

    17 publications · 938 citations

    16

    h-index

  3. Geophysical & Astrophysical Fluid Dynamics

    19 publications · 713 citations

    15

    h-index

  4. Physics of The Earth and Planetary Interiors

    11 publications · 982 citations

    11

    h-index

  5. Geophysical Research Letters

    10 publications · 437 citations

    10

    h-index

1–5