An asymptotic solution to the inverse problem of helioseismology for determining the internal differential rotation of the sun

Details An asymptotic solution to the inverse problem of helioseismology for determining the internal differential rotation of the sun An asymptotic solution to the inverse problem of helioseismology for determining the internal differential rotation of the sun

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..473k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, May 1988, p. 473-480. In Russian.

Statistics

Computation

1

Helioseismology, Solar Rotation, Asymptotic Methods, Computational Astrophysics

Scientific paper

The dependence of angular velocity versus radius and latitude in the
solar interior can be obtained from the frequency splitting of 5 minute
oscillations by solving two-dimensional integral Abels equation, if the
observational data are presented as a function of (l+1/2)/σ and
(l+1/2)/m.

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