Stellar Dynamo Theory

Stellar Dynamo Theory is a physical theory that explains the generation and maintenance of stellar magnetic fields through the conversion of kinetic energy from convective motions and differential rotation within a star’s interior into magnetic energy via magnetohydrodynamic processes.

267

Publications

17.9K

Citations

405

Authors

258

Institutions

Publications per year

2017–2026

44

Authors

405

  1. DM
    D. Moss

    University of Manchester, United Kingdom

    15 publications · 436 citations

    12

    h-index

  2. LL
    L. L. Kitchatinov

    Institute of Solar-Terrestrial Physics, Russia

    10 publications · 471 citations

    10

    h-index

  3. DD
    D. D. Sokoloff

    Lomonosov Moscow State University, Russia

    10 publications · 305 citations

    10

    h-index

  4. AB
    Axel Brandenburg

    Stockholm University, Sweden

    9 publications · 357 citations

    9

    h-index

  5. GM
    G. Meynet

    University of Geneva, Switzerland

    8 publications · 892 citations

    8

    h-index

1–5 of 405

Venues

  1. Astronomy and Astrophysics

    47 publications · 4.3K citations

    28

    h-index

  2. The Astrophysical Journal

    ApJ · 46 publications · 4.5K citations

    28

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    48 publications · 2.5K citations

    27

    h-index

  4. Geophysical & Astrophysical Fluid Dynamics

    16 publications · 669 citations

    13

    h-index

  5. Astronomische Nachrichten

    11 publications · 366 citations

    10

    h-index

1–5