The relation between stellar magnetic field geometry and chromospheric activity cycles I: The highly variable field of Epsilon Eridani at activity minimum

25 Oct 2017 Jeffers S. V. Saikia S. Boro Barnes J. R. Petit P. Marsden S. C. Jardine M. M. Vidotto A. A.

The young and magnetically active K dwarf Epsilon Eridani exhibits a chromospheric activity cycle of about 3 years. Previous reconstructions of its large-scale magnetic field show strong variations at yearly epochs... (read more)

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  • SOLAR AND STELLAR ASTROPHYSICS