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Proceedings Paper

Statistical modeling of radiative heat transfer in circumstellar medium
Author(s): S. A. Brednikhin; B. A. Kargin
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Paper Abstract

The present paper is devoted to modeling radiative heat transfer in forming planetary systems. A solution of the transfer equation with multiple sources for dusty media of spherical polydispersive particles is considered. An algorithm for computation of the temperature distribution in circumstellar disks is proposed. Coincidence of numerical results and known analytical cases is shown. The spatial distributions of optical characteristics and matter temperature of β - Pictoris debris disk are obtained for a low spatial resolution.

Paper Details

Date Published: 11 February 2009
PDF: 10 pages
Proc. SPIE 7296, Fifteenth International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics, 72960F (11 February 2009); doi: 10.1117/12.823810
Show Author Affiliations
S. A. Brednikhin, Novosibirsk State Univ. (Russian Federation)
B. A. Kargin, Institute of Computational Mathematics and Mathematical Geophysics (Russian Federation)


Published in SPIE Proceedings Vol. 7296:
Fifteenth International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics
Gennadii G. Matvienko; Yurii N. Ponomarev, Editor(s)

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