Dynamo Bistability

Dynamo Bistability is a theoretical construct in solar dynamo theory that describes the coexistence of two distinct stable dynamo states under identical boundary conditions, distinguished by their differing magnetic field configurations and temporal behaviors.

16

Publications

2.5K

Citations

37

Authors

33

Institutions

Publications per year

2017–2026

2

Authors

37

  1. LP
    Ludovic Petitdemange

    École Normale Supérieure - PSL, France

    2 publications · 149 citations

    2

    h-index

  2. MB
    Michaël Berhanu

    Centre National de la Recherche Scientifique, France

    1 publications · 30 citations

    1

    h-index

  3. DA
    David Acheson

    University of Oxford, United Kingdom

    1 publications · 61 citations

    1

    h-index

  4. PH
    P. Hoyng

    Space Research Organisation Netherlands, Netherlands

    1 publications · 41 citations

    1

    h-index

  5. FH
    F. H. Busse

    University of Bayreuth, Germany

    1 publications · 10 citations

    1

    h-index

1–5 of 37

Venues

  1. The Astrophysical Journal

    ApJ · 2 publications · 145 citations

    2

    h-index

  2. 2

    h-index

  3. Astronomy and Astrophysics

    1 publications · 92 citations

    1

    h-index

  4. Journal of Fluid Mechanics

    1 publications · 30 citations

    1

    h-index

  5. Geophysical & Astrophysical Fluid Dynamics

    1 publications · 41 citations

    1

    h-index

1–5