Chromospheric structure and activity in solar analogues

M. C. Vieytes, P. J. D. Mauas, C. C. Cincunegui
2004 Proceedings of the International Astronomical Union  
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