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Continuous high-precision photometry of stars, provided by space missionssuch as CoRoT, Kepler, and K2, represents a unique way to study stellarrotation and magnetism. The coupling of these studies of the surface dynamicswith asteroseismology is changing our view to surface and internal dynamics. Inthis proceedings I will provide the latest developments in the understanding ofsurface and internal rotation and magnetic fields. I will also discuss thepossible discovery of strong internal magnetic fields of dynamo origin in theconvective cores of stars above 1.2-1.4 solar masses. I will finish byproviding constraints on gyrochronology laws for low-mass stars and put the Suninto context of its magnetism when compared to other solar-analog stars.

Stellar dynamics of low mass stars from the surface to the interior measured by CoRoT and Kepler