The long term dynamics of the solar radiative zone associated to new results from SoHO and young solar analogs

Details The long term dynamics of the solar radiative zone associated to new results from SoHO and young solar analogs The long term dynamics of the solar radiative zone associated to new results from SoHO and young solar analogs

2011-09-19

arxiv.org/abs/1109.4125v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

8 pages, 5 figures, 61st Fujihara seminar proceedings on Progress in solar/stellar physics with helio- and asteroseismology ed

Scientific paper

The Standard Solar Model (SSM) is no more 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 the recent results to models beyond the SSM assumptions. Then we discuss the missing processes and quantify some of them in using young analog observations to build a more realistic view of our star. This progress will be useful for solar-like stars observed by COROT and KEPLER.

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