The angle-dependent redistribution functions R(III) and R(IV) - Line absorption probability distribution functions and reemission coefficients

Details The angle-dependent redistribution functions R(III) and R(IV) - Line absorption probability distribution functions and reemission coefficients The angle-dependent redistribution functions R(III) and R(IV) - Line absorption probability distribution functions and reemission coefficients

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.106..299m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 106, no. 2, Nov. 1984, p. 299-307.

Mathematics

Probability

5

Angular Distribution, Line Spectra, Polarized Radiation, Probability Distribution Functions, Radiative Transfer, Scattering Functions, Absorption Spectra, Incoherent Scattering, Photons, Voigt Effect

Scientific paper

The line absorption probability distribution functions and the reemission coefficients are derived for the non-coherent scattering functions RIII and RIV. The appropriate line profile function for RIII is shown to be a simple Voigt function, while for RIV, the line absorption probability distribution function is more complex involving a linear combination of two Voigt functions and another more complex probability distribution. The structure of the reemission coefficients for RIII and RIV is then discussed.

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