The dynamics of the solar radiative zone |
| |
Authors: | Sylvaine Turck-Chièze Suzanne Talon |
| |
Institution: | 1. DAPNIA/CEA CE Saclay, UMR 7158 CEA-CNRS-University, Paris VII, FR 2707 ILP-Recherche, 91191 Gif-sur-Yvette cedex, France;2. Département de Physique, Université de Montréal, C.P. 6128, succ. centre-ville, Montréal, Que., Canada H3C 3J7 |
| |
Abstract: | The picture of the solar radiative zone is evolving quickly. This review is separated in two parts. We first recall how the two powerful probes of the solar interior, namely the neutrinos and helioseismology have scrutinized the microscopic properties of the solar radiative plasma. Recent observations stimulate today complementary activities beyond the standard stellar model through theoretical modeling of angular momentum transport by rotation, internal waves or (and) by magnetic fields to get access to the dynamical motions of this important region of the Sun. So in the second part, we summarize the first impact of such processes on the radiative zone. |
| |
Keywords: | Solar interior Helioseismology Neutrino Gravity waves |
本文献已被 ScienceDirect 等数据库收录! |
|