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Exact solution of a radiative transfer problem by the Laplace Transform and Wiener-Hopf Technique

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Abstract

The transfer equation for the case of grey scattering according to Rayleigh's phase function in a semi-infinite axially symmetric atmosphere is considered. The emergent intensity and the intensity at any optical depth have been determined by the Laplace Transform and Wiener-Hopf Technique.

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Authors and Affiliations

  1. Department of Mathematics, University of North Bengal, West Bengal, India

    S. Karanjai

  2. Department of Mathematics, Malda College, Malda, West Bengal, India

    Z. Islam

Authors
  1. S. Karanjai
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  2. Z. Islam
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Karanjai, S., Islam, Z. Exact solution of a radiative transfer problem by the Laplace Transform and Wiener-Hopf Technique. Astrophys Space Sci 208, 113–123 (1993). https://doi.org/10.1007/BF00658138

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  • DOI: https://doi.org/10.1007/BF00658138

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