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Toroidal Magnetic Flux Budget in Mean-field Dynamo Model of Solar Cycles 23 and 24

We study the toroidal magnetic flux budget of the axisymmetric part of a data-driven 3D mean-field dynamo model of Solar Cycles 23 and 24. The model simulates the global solar dynamo that includes the effects of the formation and evolution of bipolar magnetic regions (BMRs) emerging on the solar sur...

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Bibliografische gegevens
Hoofdauteurs: Valery V. Pipin, Alexander G. Kosovichev
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: IOP Publishing 2024-01-01
Reeks:The Astrophysical Journal
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Online toegang:https://doi.org/10.3847/1538-4357/ad1590
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