Dynamo Wave Propagation

Dynamo Wave Propagation is a theoretical construct in solar dynamo theory that describes the spatial and temporal evolution of magnetic field generation due to the interaction between turbulent convective flows and differential rotation in the Sun’s interior, distinguished by its wave-like behavior in latitude and depth arising from the combined effects of the α-effect and meridional circulation.

141

Publications

10.8K

Citations

232

Authors

143

Institutions

Publications per year

2017–2026

10

Authors

232

  1. DD
    D. D. Sokoloff

    Lomonosov Moscow State University, Russia

    12 publications · 347 citations

    12

    h-index

  2. KM
    K. M. Kuzanyan

    Institute of Terrestrial Magnetism Ionosphere and Radio Wave Propagation, Russia

    8 publications · 225 citations

    8

    h-index

  3. AB
    Axel Brandenburg

    Stockholm University, Sweden

    8 publications · 2.1K citations

    7

    h-index

  4. HY
    Hirokazu Yoshimura

    The University of Tokyo, Japan

    6 publications · 496 citations

    6

    h-index

  5. JW
    J. Warnecke

    Max Planck Institute for Solar System Research, Germany

    5 publications · 336 citations

    5

    h-index

1–5 of 232

Venues

  1. The Astrophysical Journal

    ApJ · 25 publications · 4.1K citations

    18

    h-index

  2. Geophysical & Astrophysical Fluid Dynamics

    13 publications · 430 citations

    12

    h-index

  3. 9

    h-index

  4. Astronomy and Astrophysics

    7 publications · 289 citations

    7

    h-index

  5. Geophysical Research Letters

    6 publications · 227 citations

    6

    h-index

1–5