The b and h functions for integral equations with displacement kernels: a computational method and an application to radiative transfer
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Publication:580946
DOI10.1016/0096-3003(87)90032-4zbMath0626.65140OpenAlexW2091566257MaRDI QIDQ580946
Melvin R. Scott, Robert E. Kalaba, Harriet H. Kagiwada
Publication date: 1987
Published in: Applied Mathematics and Computation (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/0096-3003(87)90032-4
Gram-Schmidt orthogonalizationnumerical stabilityradiative transferreflection coefficienttransmission coefficientsdisplacement kernels
Numerical methods for integral equations (65R20) Fredholm integral equations (45B05) Radiative transfer in astronomy and astrophysics (85A25)
Uses Software
Cites Work
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- Imbedding methods for the integral equations for the optimal control of time-lag systems. I: Parameter dependence
- Numerical solution of unstable two-point boundary-value problems by quasilinearization and orthonormalization
- Initial-value methods for the basic boundary-value problem and integral equation of radiative transfer
- Computational Solution of Linear Two-Point Boundary Value Problems via Orthonormalization