Determination of the radiation field in the chromosphere using the method of the observed line profile inversion

Details Determination of the radiation field in the chromosphere using the method of the observed line profile inversion Determination of the radiation field in the chromosphere using the method of the observed line profile inversion

Apr 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...67g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Mar.-Apr. 1986, p. 67-74. In Russian.

Computer Science

1

Chromosphere, Line Shape, Line Spectra, Solar Radiation, Solar Spectra, Spline Functions, Algorithms, Cubic Equations, Fredholm Equations, Polynomials, Solar Velocity

Scientific paper

The method of the observed profile inversion is modified by using local B-splines of second degree, polynomials, and cubic fundamental splines. The method is then extended to the case of an arbitrary nonthermal velocity field in the solar atmosphere. The algorithms proposed here are based on the assumption of a complete frequency redistribution in the core of a strong line.

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