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arXiv · 1612.02544

Starspots, Stellar Cycles and Stellar Flares: Lessons from Solar Dynamo Models

Arnab Rai Choudhuri
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Abstract

In this review, we discuss whether the present solar dynamo models can be extrapolated to explain various aspects of stellar activity. We begin with a summary of the following kinds of data for solar-like stars: (i) data pertaining to stellar cycles from Ca H/K emission over many years; (ii) X-ray data indicating hot coronal activity; (iii) starspot data (especially about giant polar spots); and (iv) data pertaining to stellar superflares. Then we describe the current status of solar dynamo modelling---giving an introduction to the flux transport dynamo model, the currently favoured model for the solar cycle. While an extrapolation of this model to solar-like stars can explain some aspects of observational data, some other aspects of the data still remain to be theoretically explained. It is not clear right now whether we need a different kind of dynamo mechanism for stars having giant starspots or producing very strong superflares.

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Arnab Rai Choudhuri. 2016-12-08. Starspots, Stellar Cycles and Stellar Flares: Lessons from Solar Dynamo Models. https://doi.org/10.1007/s11433-016-0413-7

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