
TL;DR
This paper reviews current understanding of the solar dynamo mechanism, highlights unresolved issues such as the alpha-effect and flux transport, and emphasizes the need for better constraints to develop reliable solar cycle models.
Contribution
It identifies key unresolved problems in solar dynamo theory and discusses how current observational and theoretical limitations hinder the development of a standard, predictive model.
Findings
Advances in magnetohydrodynamic dynamo theory improve understanding of the solar magnetic cycle.
Helioseismic observations help constrain some parameters in solar cycle models.
Significant uncertainties remain in processes like turbulent diffusion and flux pumping.
Abstract
The magnetic activity of the Sun, as manifested in the sunspot cycle, originates deep within its convection zone through a dynamo mechanism which involves non-trivial interactions between the plasma and magnetic field in the solar interior. Recent advances in magnetohydrodynamic dynamo theory have led us closer towards a better understanding of the physics of the solar magnetic cycle. In conjunction, helioseismic observations of large-scale flows in the solar interior has now made it possible to constrain some of the parameters used in models of the solar cycle. In the first part of this review, I briefly describe this current state of understanding of the solar cycle. In the second part, I highlight some of the outstanding issues in solar dynamo theory related to the the nature of the dynamo -effect, magnetic buoyancy and the origin of Maunder-like minima in activity. I also…
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