Solar Rotation from 2d Inversion
Résumé
A 2-D regularized least square inversion code for solar rotation has been constructed which approximates the rotation rate by piecewise polynomials projected on B-splines. It is applied to the rotational splitting data of BBSO (Ref. 1). A discussion of the in uence of the number and order of the spline basis on the results is given. Preliminary results of inversion with LOI data (Ref. 2) are presented.
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