Statistical modeling of radiative heat transfer in circumstellar medium

Details Statistical modeling of radiative heat transfer in circumstellar medium Statistical modeling of radiative heat transfer in circumstellar medium

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spie.7296e..14b&link_type=abstract

Fifteenth International Symposium on Atmospheric and Ocean Optics/Atmospheric Physics. Edited by Brednikhin, S. A.; Kargin, B.

Physics

Optics

Scientific paper

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.

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