Abstract

A Monte Carlo model has been developed which simulates the multiple-scattering of middle-uv radiation in the lower atmosphere. The source of radiation is assumed to be monochromatic and located at a point. The physical effects taken into account in the model are Rayleigh and Mie scattering, pure absorption by particulates and trace atmospheric gases, and ground albedo. The model output consists of the multiply scattered radiance as a function of look-angle of a detector located within the atmosphere. Several examples are discussed, and comparisons are made with direct-source and single-scattered contributions to the signal received by the detector.

© 1978 Optical Society of America

Experimental and theoretical studies of the aureole about a point source that is due to atmospheric scattering in the middle ultraviolet

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Backscattered UV radiation: effects of multiple scattering and the lower boundary of the atmosphere

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Ultraviolet aureole around a source at a finite distance

Fred Riewe and Alex E. S. Green
Appl. Opt. 17(12) 1923-1929 (1978)

Backward Monte Carlo Calculations of the Polarization Characteristics of the Radiation Emerging from Spherical-Shell Atmospheres

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Aureole radiance field about a source in a scattering–absorbing medium

Alexander S. Zachor
Appl. Opt. 17(12) 1911-1922 (1978)