Numerical evaluation of Chandrasekhar's H-function, its first and second differential coefficients, its pole and moments from the new form for plane parallel scattering atmosphere in radiative transfer

dc.creatorDas, Rabindra Nath
dc.creatorBera, Rasajit
dc.date2007-11-21
dc.date.accessioned2026-07-07T08:44:13Z
dc.date.available2026-07-07T08:44:13Z
dc.descriptionIn this paper, the new forms obtained for Chandrasekhar's H- function in Radiative Transfer by one of the authors both for non-conservative and conservative cases for isotropic scattering in a semi-infinite plane parallel atmosphere are used to obtain exclusively new forms for the first and second derivatives of H-function . The numerics for evaluation of zero of dispersion function, for evaluation of H-function and its derivatives and its zeroth, the first and second moments are outlined. Those are used to get ready and accurate extensive tables of H-function and its derivatives, pole and moments for different albedo for scattering by iteration and Simpson's one third rule . The schemes for interpolation of H-function for any arbitrary value of the direction parameter for a given albedo are also outlined. Good agreement has been observed in checks with the available results within one unit of ninth decimal
dc.description39 pages
dc.identifierhttps://arxiv.org/abs/0711.3336
dc.identifierhttp://arxiv.org/abs/0711.3336
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/142582
dc.subjectAstrophysics
dc.titleNumerical evaluation of Chandrasekhar's H-function, its first and second differential coefficients, its pole and moments from the new form for plane parallel scattering atmosphere in radiative transfer
dc.typetext

Files

Collections