Twilight ray height determination

L. S. Shakun; V. D. Motritch

doi:10.1117/12.284778

3 September 1997 Twilight ray height determination

L. S. Shakun, V. D. Motritch

Proceedings Volume 3237, 23rd European Meeting on Atmospheric Studies by Optical Methods; (1997) https://doi.org/10.1117/12.284778
Event: Twenty-third European Meeting on Atmospheric Studies by Optical Methods, 1996, Kiev, Ukraine

Abstract

A new program that simulates the primary light dispersion in atmosphere during twilight is represented. Program uses the modified N. B. Divari model of light dispersion in the atmosphere. Optical depths, the twilight beam height and its half-width may be easily and with high speed obtained using this program. The flexible program construction may be used for the determination the twilight beam parameters by iteration. Obtained results coincide with those in literature.

Citation Download Citation

L. S. Shakun and V. D. Motritch "Twilight ray height determination", Proc. SPIE 3237, 23rd European Meeting on Atmospheric Studies by Optical Methods, (3 September 1997); https://doi.org/10.1117/12.284778

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