The b and h functions for integral equations with displacement kernels: a computational method and an application to radiative transfer (Q580946)
From MaRDI portal
 | This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: The b and h functions for integral equations with displacement kernels: a computational method and an application to radiative transfer |
scientific article; zbMATH DE number 4018339
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | The b and h functions for integral equations with displacement kernels: a computational method and an application to radiative transfer |
scientific article; zbMATH DE number 4018339 |
Statements
The b and h functions for integral equations with displacement kernels: a computational method and an application to radiative transfer (English)
0 references
1987
0 references
The solutions of Fredholm integral equations as well as certain functionals on the solutions are discussed. The basic functions b and h which occur as solutions of a linear two-point boundary value problem pose a problem of stability. It is shown that the problem can be solved by using a Gram-Schmidt orthogonalization scheme.
0 references
displacement kernels
0 references
reflection coefficient
0 references
radiative transfer
0 references
transmission coefficients
0 references
numerical stability
0 references
Gram-Schmidt orthogonalization
0 references
0 references
0 references
0 references
