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Effects of Emerging Bipolar Magnetic Regions in Mean-field Dynamo Model of Solar Cycles 23 and 24

We model the physical parameters of Solar Cycles 23 and 24 using a nonlinear dynamical mean-field dynamo model that includes the formation and evolution of bipolar magnetic regions (BMRs). The Parker-type dynamo model consists of a complete MHD system in the mean-field formulation: the 3D magnetic i...

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Auteurs principaux: V. V. Pipin, A. G. Kosovichev, V. E. Tomin
Format: Artigo
Langue:Inglês
Publié: IOP Publishing 2023-01-01
Collection:The Astrophysical Journal
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Accès en ligne:https://doi.org/10.3847/1538-4357/acaf69
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