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Chromospheric structure and activity in solar analogues
2004
Proceedings of the International Astronomical Union
Preserved Fulltext
We computed chromospheric models of the Sun as a star and of nine solar analogues. The stars have a wide variety of magnetic activity levels, which allows us to study the differences in atmospheric structures induced by activity.
doi:10.1017/s1743921304007355
fatcat:377jenpsobblth2pvmazf4s4ay