An \(L^1\) refined projection approximate solution of the radiation transfer equation in stellar atmospheres
DOI10.1016/S0377-0427(01)00403-4zbMath1005.65144OpenAlexW1994978427MaRDI QIDQ1602762
Mario Ahues, Olivier Titaud, Alain Largillier, Paulo B. Vasconcelos, Filomena D. d'Almeida
Publication date: 24 June 2002
Published in: Journal of Computational and Applied Mathematics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/s0377-0427(01)00403-4
convergenceGalerkin methodnumerical examplesastrophysicsparallelizationweakly singular kerneliterative refinementsecond kind Fredholm integral equationstellar atmospheresradiation transfer equation
Numerical methods for integral equations (65R20) Integral equations of the convolution type (Abel, Picard, Toeplitz and Wiener-Hopf type) (45E10) Radiative transfer in astronomy and astrophysics (85A25)
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