Rotation of the solar interior: compatibility of different helioseismic data sets
Accurate determination of the rotation rate in the inner radiative zone (0.2 r/Rsolar 0.5) of the sun from helioseismic observations requires rotational frequency splittings of exceptional quality. Indeed, only low degree modes are sensitive to the dynamics of the deep interior. Low and intermediate degree splittings have been estimated from a
Eff-Darwich, A. et al.
Fecha de publicación:
1
2001