NASA NTRS · 19850049767
The anisotropic radiative transfer problem in optically thick, strongly magnetized plasma - A comparison of results
Abstract
The accuracy of four different methods for solving the coherent radiative transfer problem in a strongly magnetized plasma is compared. Specific attention is given to the case of a semi-infinite homogeneous plasma with a magnetic field perpendicular to the surface. The four approaches evaluated were: diffusion approximation schemes; the generalized H-function method of Silant'ev (1982) the Feautrier method of Nagel (1981) and the integral equation approach of Meszares and Bonazzola (1981). It is found that the coupled diffusion approximation schemes of Nagel (1981) and Kaminker et al. (1982) provided satisfactory results and were more efficient in many cases than direct numerical methods.
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Pavlov, G. G., Shibanov, Iu. A., Silantev, N. A., Nagel, W.. 1985-04-01. The anisotropic radiative transfer problem in optically thick, strongly magnetized plasma - A comparison of results. https://ntrs.nasa.gov/citations/19850049767
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