Constraining magnetic-activity modulations in three solar-like stars observed by CoRoT and NARVAL
Context. Stellar activity cycles are the manifestation of dynamo process running in the stellar interiors. They have been observed from years to decades thanks to the measurement of stellar magnetic proxies on the surface of the stars, such as the chromospheric and X-ray emissions, and to the measurement of the magnetic field with
Mathur, S. et al.
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2013