Dynamical processes in the solar radiative interior
Astrophysics
2007-05-23 v1
Abstract
Recent seismic observations coming from acoustic and gravity modes clearly show that the solar standard model has reached its limits and can no longer be used to interpret satisfactorily seismic observations. In this paper, we present a review of the non-standard processes that may be added to the solar models in order to improve our understanding of the helioseismic data. We also present some results obtained when applying ``non-standard'' stellar evolution to the modelling of the Sun.
Keywords
Cite
@article{arxiv.astro-ph/0609381,
title = {Dynamical processes in the solar radiative interior},
author = {A. Palacios and S. Talon and S. Turck-Chieze and C. Charbonnel},
journal= {arXiv preprint arXiv:astro-ph/0609381},
year = {2007}
}
Comments
8 pages, 6 figures, to appear in the volume ESA-SP 624 of ESA Special Publications - Proceedings of the SOHO18 / GONG 2006 / HELAS I meeting, held in Sheffield (UK) in August 2006