The energy-dependent radiation transfer in a homogeneous finite sphere

Details The energy-dependent radiation transfer in a homogeneous finite sphere The energy-dependent radiation transfer in a homogeneous finite sphere

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.137..239e&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 137, no. 2, Oct. 1987, p. 239-250.

Statistics

Computation

Celestial Sphere, Heat Transfer, Mathematical Models, Radiant Flux Density, Computational Astrophysics, Kernel Functions, Laplace Transformation

Scientific paper

Radiation transfer problem in the slowing-down region is solved for a spherical geometry. Modelled kernels are used to represent the slowing-down kernel. Calculations are performed for the radiation flux at the boundary of the sphere for two cases: (1) in the presence of internal source, (2) if the radiation is incident on the sphere. Numerical results are obtained by using the Padé approximant technique.

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