The irregularities of the sunspot cycle and their theoretical modelling
arXiv:1312.3408 · doi:10.1007/s12648-014-0481-y
Abstract
The 11-year sunspot cycle has many irregularities, the most promi- nent amongst them being the grand minima when sunspots may not be seen for several cycles. After summarizing the relevant observational data about the irregularities, we introduce the flux transport dynamo model, the currently most successful theoretical model for explaining the 11-year sunspot cycle. Then we analyze the respective roles of nonlinearities and random fluctuations in creating the irregularities. We also discuss how it has recently been realized that the fluctuations in meridional circula- tion also can be a source of irregularities. We end by pointing out that fluctuations in the poloidal field generation and fluctuations in meridional circulation together can explain the occurrences of grand minima.
Invited paper for the C.V. Raman 125th birth anniversary issue of Indian Journal of Physics
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- A theoretical model of the variation of the meridional circulation with the solar cycle
- A Theoretical Model of the Near Surface Shear Layer of the Sun
- A Critical Assessment of the Flux Transport Dynamo
- Flux Transport Dynamo: From Modelling Irregularities to Making Predictions
- Surface Flux Transport Modeling using Physics Informed Neural Networks
- The Sun's polar magnetic field: datasets, proxies and theoretical issues
- Predicting a solar cycle before its onset using a flux transport dynamo model