T. Corbard(1), M.P.
Di Mauro(2), T. Sekii(3),
and the GOLF
team
(1)Laboratoire
G.-D Cassini, Observatoire de la
Côte d'Azur, BP 4229, 06304 Nice Cedex 4
(2)Istituto di Astronomia dell'Università di Catania, Viale A.Doria,
6 I-95125 Catania, Italy
(3)Institute of Astronomy, Madingley
Rd., Cambridge, CB3 0HA, U.K.
The low degree splittings obtained from one year of GOLF data analysis
are combined with the MDI medium-l 144-day splittings in order to infer
the solar internal rotation as a function of the radius down to 
.
Several inverse methods are applied to the same data and the uncertainties
on the solution as well as the resolution reachable are discussed. The
results are compared with the one obtained from the low degree splittings
estimated from GONG network.
Key words: solar core rotation; inversion.
