Contribution functions and the calculation of the mean optical depth of formation of Fraunhofer lines

Details Contribution functions and the calculation of the mean optical depth of formation of Fraunhofer lines Contribution functions and the calculation of the mean optical depth of formation of Fraunhofer lines

Aug 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58..825b&link_type=abstract

Astronomicheskii Zhurnal, vol. 58, July-Aug. 1981, p. 825-837. In Russian.

Astronomy and Astrophysics

Astronomy

6

Fraunhofer Lines, Optical Thickness, Solar Atmosphere, Solar Spectra, Atmospheric Models, Iron, Line Spectra, Oxygen

Scientific paper

Contribution functions for emission and depression are considered, as are the so-called response functions. On the basis of the physical conditions in the solar atmosphere, an attempt is made to formulate the requirements imposed on the contribution functions used in calculating the mean optical depth of formation of Fraunhofer lines. By way of example, calculations are made of the mean optical depth of formation of various segments of Fe I and O I Fraunhofer lines.

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