Balmer decrement in a medium illuminated by powerful radiation

Details Balmer decrement in a medium illuminated by powerful radiation Balmer decrement in a medium illuminated by powerful radiation

Aug 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975afz....11..421k&link_type=abstract

Astrofizika, vol. 11, Aug. 1975, p. 421-437. In Russian.

Astronomy and Astrophysics

Astrophysics

1

Astronomical Spectroscopy, Balmer Series, H Lines, Radiation Sources, Radiative Transfer, Astrophysics, Lyman Spectra, Optical Thickness, Paschen Series

Scientific paper

The paper investigates the nonlinear transfer of radiation in the hydrogen lines in a medium illuminated by high-energy radiation. An analytical solution to the steady-state problem is obtained for the case where the illumination is so great that the optical thickness in the hydrogen lines is less than unity. Emission and absorption decrements are calculated numerically for the Lyman, Balmer, Paschen, and Brackett series. An algorithm is proposed for the solution of the more general unsteady-state problem.

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