Paper
3 September 1997 Height scattering indicatrices and the earth's atmosphere scattering coefficient
Yu. I. Zaginailo, Yu. M. Gorbanev, V. D. Motrich
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Proceedings Volume 3237, 23rd European Meeting on Atmospheric Studies by Optical Methods; (1997) https://doi.org/10.1117/12.284761
Event: Twenty-third European Meeting on Atmospheric Studies by Optical Methods, 1996, Kiev, Ukraine
Abstract
Observation material of 1993 - 1995 seasons is reduced and optical characteristics of upper atmosphere of the Earth are obtained, and namely: height indicatrices of terrestrial atmosphere scattering and volume coefficient of scattering. For wavelengths 754 nm and 585 nm indicatrices of scattering are obtained for height 10, 20, . . ., 80, 100 km above the ground level whereas for 356 nm indicatrices for height 30, 40, . . . 80, 100 km are obtained. Indicatrices are typically most extended at small height (10 - 40 km) and more sloping at heights 90 km and more at small height antropogeneous and heterogeneous dust is accumulated. This dust concentration diminishes with height and at those of 50 - 80 km a relative purification of the Earth's atmosphere from the dust constituent takes place. At heights over 80 km a considerable contribution is made to scattering by the cosmic dust influx.
© (1997) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Yu. I. Zaginailo, Yu. M. Gorbanev, and V. D. Motrich "Height scattering indicatrices and the earth's atmosphere scattering coefficient", Proc. SPIE 3237, 23rd European Meeting on Atmospheric Studies by Optical Methods, (3 September 1997); https://doi.org/10.1117/12.284761
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