The Rotation of the Solar Core: Compatibility of the Different Data Sets Available
A combination of inverse and forward analysis techniques has been applied to p-modes rotational splittings in order to infer the solar rotation rate in the deeper radiative regions (r 0.45Rodot). In this analysis, we first infer the rotation distribution down to 0.45Rodot using a 2D inversion method. We then use that rotation rate to discuss the
Eff-Darwich, A. et al.
Fecha de publicación:
0
1998