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A Synchronized Two-Dimensional [Formula: see text] –[Formula: see text] Model of the Solar Dynamo
We consider a conventional [Formula: see text] –[Formula: see text] -dynamo model with meridional circulation that exhibits typical features of the solar dynamo, including a Hale-cycle period of around 20 years and a reasonable shape of the butterfly diagram. With regard to recent ideas of a tidal s...
Autores principales: | , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Netherlands
2023
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10352445/ https://www.ncbi.nlm.nih.gov/pubmed/37469612 http://dx.doi.org/10.1007/s11207-023-02173-y |
Sumario: | We consider a conventional [Formula: see text] –[Formula: see text] -dynamo model with meridional circulation that exhibits typical features of the solar dynamo, including a Hale-cycle period of around 20 years and a reasonable shape of the butterfly diagram. With regard to recent ideas of a tidal synchronization of the solar cycle, we complement this model by an additional time-periodic [Formula: see text] -term that is localized in the tachocline region. It is shown that amplitudes of some decimeters per second are sufficient for this [Formula: see text] -term to become capable of entraining the underlying dynamo. We argue that such amplitudes of [Formula: see text] may indeed be realistic, since velocities in the range of m s(−1) are reachable, e.g., for tidally excited magneto–Rossby waves. SUPPLEMENTARY INFORMATION: The online version contains supplementary material available at 10.1007/s11207-023-02173-y. |
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