Abstract
In this work, we first establish a simple procedure to obtain with 11-figure accuracy the values of Chandrasekhar’s H-function for isotropic scattering using a closed-form integral representation and the Gauss-Legendre quadrature. Based on the numerical values of the function produced by this method for various combinations of ϖ 0, the single scattering albedo, and μ, the cosine of the zenith angle θ of the direction of radiation emergent from or incident upon a semi-infinite scattering-absorbing medium, we propose a rational approximation formula with μ 1/4 and \(\sqrt{1-\varpi_{0}}\) as the independent variables. This allows us to reproduce the correct values of H(ϖ 0,μ) within a relative error of 2.1×10−5 without recourse to any iterative procedure or root-finding process.
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An erratum to this article can be found online at http://dx.doi.org/10.1007/s10509-013-1589-9.
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Kawabata, K., Limaye, S.S. Rational approximation formula for Chandrasekhar’s H-function for isotropic scattering. Astrophys Space Sci 332, 365–371 (2011). https://doi.org/10.1007/s10509-010-0512-x
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DOI: https://doi.org/10.1007/s10509-010-0512-x