Back to Volume
Paper: The Long-term Dynamics of the Solar Radiative Zone: New Results from the Solar and Heliospheric Observatory (SoHO) and Young Solar Analogs
Volume: 462, Progress in Solar/Stellar Physics with Helio- and Asteroseismology
Page: 366
Authors: Turck-Chièze, S.; Couvidat, S.; Eff-Darwich, A.; Duez, V.; García, R. A.; Mathis, S.; Mathur, S.; Piau, L.; Salabert, D.
Abstract: The Standard Solar Model (SSM) is no longer sufficient to interpret all the observations of the radiative zone obtained with the SoHO satellite. We recall our present knowledge of this internal region and compare recent results with models beyond the SSM assumptions. Then we discuss the missing processes and quantify some of them in using observations of young solar analogs to build a more realistic view of the Sun. This progress will be useful for understanding solar-like stars observed by CoRoT and Kepler.
Back to Volume