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https://doi.org/10.1023/a:1002081122641
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Cite Journal: Astrophysics and Space Science |  Publication Date: Jan 1, 1998 |
Affiliation: Queen Mary University of London
The inversion technique which we use is based on the ”quasi-asymptotic” description of solar p-modes developed by Roxburgh & Vorontsov (1996) which incorporates a Born approximation to permit a detailed treatment of the regions of rapid variation of seismic parameters with depth and strong influence of gravity perturbations.
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