A. R. G. Santos, M. S. Cunha, P. P. Avelino
As a result of the magnetic cycle, the properties of the solar oscillations vary periodically. With the recent discovery of manifestations of activity cycles in the seismic data of other stars, the understanding of the different contributions to such variations becomes even more important. With this in mind, we built an empirical parameterised model able to reproduce the properties of the sunspot cycle. The resulting simulations can be used to estimate the magnetic-induced frequency shifts.
The Space Photometry Revolution - CoRoT Symposium 3, Kepler KASC-7 Joint Meeting
Volume 101, Number 0605