An exact solution of the equation of transfer with three-term scattering indicatrix in an exponential atmosphere

Details An exact solution of the equation of transfer with three-term scattering indicatrix in an exponential atmosphere An exact solution of the equation of transfer with three-term scattering indicatrix in an exponential atmosphere

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.179...89k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 179, no. 1, May 1991, p. 89-96.

Astronomy and Astrophysics

Astrophysics

1

Radiative Transfer, Scattering Functions, Stellar Atmospheres, Absorptivity, Boundary Conditions, Exponential Functions, Laplace Transformation, Thermal Emission

Scientific paper

The general equation for radiative transfer in the Milne-Eddington model is considered here. The scattering function is assumed to be quadratically anisotropic in the cosine of the scattering angle and Planck's intensity function is assumed for thermal emission. Here, Planck's function is taken as a nonlinear function of optical depth. The exact solution for emergent intensity from the bounding face is obtained by the method of the Laplace transform in combination with the Wiener-Hopf technique.

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