The FN method for solving radiative-transfer problems in plane geometry

Details The FN method for solving radiative-transfer problems in plane geometry The FN method for solving radiative-transfer problems in plane geometry

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ap%26ss..58..131s&link_type=abstract

Astrophysics and Space Science, vol. 58, no. 1, Sept. 1978, p. 131-137. Research supported by the Commissariat a l'Energie Atom

Astronomy and Astrophysics

Astrophysics

11

Albedo, Boundary Value Problems, Mathematical Models, Radiative Transfer, Scattering Functions, Chandrasekhar Equation, Legendre Functions, Optical Thickness, Radiant Flux Density, Spherical Harmonics

Scientific paper

The previously established FN method for isotropic scattering is extended to include a more realistic phase function. The full-range orthogonality theorem is used to develop 'exact' singular integral equations for the required exit distributions. It is noted that the FN method is considerably simpler and more efficient than the traditional method of spherical harmonics.

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