Journal of the Optical Society of America · 1960 · 99 citations · 1 references
Natural SciencesAstronomyPhysicsInterstellar MediumOptical AstronomyOpticsOptical Transfer FunctionPath TracingRadial Distribution Functions
The two-path method (utilizing a mirror) is shown to provide sufficient information to solve for the true radial brightness distribution of a luminous medium in the presence of self-absorption. In the case where self-absorption is not large, an approximate solution to the problem is shown to be no more difficult than a solution for the “optically thin” approximation.
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