Bibcode
Mathur, S.; García, R. A.; Eff-Darwich, A.
Referencia bibliográfica
Magnetic Coupling between the Interior and Atmosphere of the Sun, edited by S.S. Hasan and R.J. Rutten; Astrophysics and Space Science Proceedings. ISSN 1570-6591 (Print) 1570-6605 (Online) Published by Springer Berlin Heidelberg; ISBN 978-3-642-02858-8 (Print) 978-3-642-02859-5 (Online), pp.364-367
Advertised on:
2010
Número de citas
0
Número de citas referidas
0
Descripción
Solar gravity (g) modes propagate within the radiative part of the solar
interior and are highly sensitive to the physical conditions of the
solar core. They would represent the best tool to infer the structure
and the dynamics of the radiative interior, in particular the core, if
they were properly detected and characterized. Although individual
rotational splittings for g modes have not yet been calculated, we have
to understand the effect of these modes, and also low-degree
high-frequency p modes, on the inversion of the solar rotation rate
between 0.1 and 0.2R&sun;. In this work, we follow the
methodology developed in Mathur et al. [2008, A&A, 484, 517] and
García et al. [2008a, A.N., 329, 476], adding g modes and
low-degree high-frequency p modes to artificial inversion data sets, in
order to study how they convey information on the solar core rotation.