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A change in the relationship between chromospheric activity and the large-scale magnetic field for G stars on the main sequence

E L Brown,S. V. Jeffers,S. C. Marsden,J. Morin,S. Boro Saikia, P. Petit,M. Jardine,Victor See,A. A. Vidotto,M. W. Mengel,Merten Nikolay Dahlkemper

HAL (Le Centre pour la Communication Scientifique Directe)（2022）

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Key words
chromospheric activity,magnetic field,stars,large-scale
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