On the numerical calculation of the solar rotational splitting coefficients

Details On the numerical calculation of the solar rotational splitting coefficients On the numerical calculation of the solar rotational splitting coefficients

Mar 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...351..682d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 351, March 10, 1990, p. 682-686.

Statistics

Computation

1

Computational Astrophysics, Solar Interior, Solar Magnetic Field, Solar Oscillations, Solar Rotation, Angular Velocity, Convection Currents, Dynamo Theory, Least Squares Method, Legendre Functions, P Waves

Scientific paper

An alternative method for numerically calculating the solar rotational
splitting coefficient is developed. The efficacy of the method is
illustrated using South Pole data. The robustness of a(2i+1) is shown to
be excellent for i = 0 and to decrease with increasing i, whereas the
values of b(2i+1) appear to be sensitive to the method of calculation.

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