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Group-theoretical description of radiative transfer in one-dimensional media

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Group theory is used to describe a procedure for adding inhomogeneous absorbing and scattering atmospheres in a one-dimensional approximation. The inhomogeneity originates in the variation of the scattering coefficient with depth. Group representations are derived for the composition of media in three different cases: inhomogeneous atmospheres in which the scattering coefficient varies continuously with depth, composite or multicomponent atmospheres, and the special case of homogeneous atmospheres. We extend an earlier proposal to solve problems in radiative transfer theory by first finding global characteristics of a medium (reflection and transmission coefficients) and then determining the internal radiation field for an entire family of media without solving any new equations. Semi-infinite atmospheres are examined separately. For some special depth dependences of the scattering coefficients it is possible to obtain simple analytic solutions expressed in terms of elementary functions. An algorithm for numerical solution of radiative transfer problems in inhomogeneous atmospheres is described.

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Authors and Affiliations

  1. V. A. Ambartsumyan Byurakan Astrophysical Observatory, Byurakan, Armenia

    A. G. Nikoghossian

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  1. A. G. Nikoghossian
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Correspondence to A. G. Nikoghossian.

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Translated from Astrofizika, Vol. 54, No. 1, pp. 149–162 (February 2011).

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Nikoghossian, A.G. Group-theoretical description of radiative transfer in one-dimensional media. Astrophysics 54, 126–138 (2011). https://doi.org/10.1007/s10511-011-9164-y

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  • DOI: https://doi.org/10.1007/s10511-011-9164-y

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