词条 | Chandrasekhar's H-function |
释义 |
In atmospheric radiation, Chandrasekhar's H-function appears as the solutions of problems involving scattering, introduced by the Indian American astrophysicist Subrahmanyan Chandrasekhar.[1][2][3][4][5] The Chandrasekhar's H-function defined in the interval , satisfies the following nonlinear integral equation where the characteristic function is an even polynomial in satisfying the following condition . If the equality is satisfied in the above condition, it is called conservative case, otherwise non-conservative. Albedo is given by . An alternate form which would be more useful in calculating the H function numerically by iteration was derived by Chandrasekhar as, . In conservative case, the above equation reduces to . ApproximationThe H function can be approximated up to an order as where are the zeros of Legendre polynomials and are the positive, non vanishing roots of the associated characteristic equation where are the quadrature weights given by Explicit solution in the complex planeIn complex variable the H equation is then for , a unique solution is given by where the imaginary part of the function can vanish iff is real i.e., . Then we have The above solution is unique and bounded in the interval for conservative cases. In non-conservative cases, if the equation admits the roots , then there is a further solution given by Properties
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External links
References1. ^Chandrasekhar, Subrahmanyan. Radiative transfer. Courier Corporation, 2013. 2. ^Howell, John R., M. Pinar Menguc, and Robert Siegel. Thermal radiation heat transfer. CRC press, 2010. 3. ^Modest, Michael F. Radiative heat transfer. Academic press, 2013. 4. ^Hottel, Hoyt Clarke, and Adel F. Sarofim. Radiative transfer. McGraw-Hill, 1967. 5. ^Sparrow, Ephraim M., and Robert D. Cess. "Radiation heat transfer." Series in Thermal and Fluids Engineering, New York: McGraw-Hill, 1978, Augmented ed. (1978). 4 : Special functions|Integral equations|Scattering|Scattering, absorption and radiative transfer (optics) |
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