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Continuous high-precision photometry of stars provided by space missions such as CoRoT, Kepler, and K2 represents a unique way to study stellar rotation and magnetism. The coupling of these studies of the surface dynamics with asteroseismology is changing our view to surface and internal dynamics. In this proceedings I will provide the latest developments in the understanding of surface and internal rotation and magnetic fields. I will also discuss the possible discovery of strong internaldoi:10.1051/eas/1982020 fatcat:losrczpbwjd5fn5fn2jm2xbg4q