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
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2.5K
Citations
37
Authors
33
Institutions
Publications per year
2017–2026
2
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Astrophysical magnetic fields and nonlinear dynamo theory
Axel Brandenburg, Kandaswamy Subramanian · Physics Reports · 2005 · 1.7K citations · Full text
Chaos in the Rikitake two-disc dynamo system
Keisuke Ito · Earth and Planetary Science Letters · 1980 · 113 citations
What controls the magnetic geometry of M dwarfs?
Astronomy and Astrophysics · 2012 · 92 citations · Full text
Natural Sciences, Astronomy, Physics +14
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Max Planck Institute for Solar System Research
Göttingen, Germany
2 h-index
5 publications
409 citations
École Normale Supérieure - PSL
Paris, France
2 h-index
3 publications
279 citations

Centre National de la Recherche Scientifique
Paris, France
2 h-index
17 publications
499 citations

Pulkovo Observatory
Saint Petersburg, Russia
1 h-index
1 publications
33 citations
Laboratoire des Écoulements Géophysiques et Industriels
Grenoble, France
1 h-index
1 publications
30 citations

University of Manchester
Manchester, United Kingdom
1 h-index
1 publications
33 citations
University of Oxford
Oxford, United Kingdom
1 h-index
1 publications
61 citations

École Normale Supérieure de Lyon
Lyon, France
1 h-index
5 publications
150 citations
1–8 of 33
ApJ · 2 publications · 145 citations
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2 publications · 97 citations
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1 publications · 92 citations
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1 publications · 30 citations
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1 publications · 41 citations
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