6 October 1989 Determination Of Optical Properties And Composition Of Atmosphere From Measurements Of Optical Spectra
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Proceedings Volume 1129, Advanced Optical Instrumentation for Remote Sensing of the Earth's Surface from Space; (1989) https://doi.org/10.1117/12.961485
Event: 1989 International Congress on Optical Science and Engineering, 1989, Paris, France
Abstract
By means of automatic multichannel balloon-borne spectrometers the spectra of solar radiation have been measured at altitudes up to 30-32 km in the range of 0.4 to 12.0μm under different spectral resolutions. On the basis of the experimental data obtained using the procedure elaborated by the authors the profiles of ozone concentrations in atmosphere at altitudes of 15-25 km have been defined, as well as the concentrations of water vapour and methane at altitudes up to 30 km. Vertical and spectral dependencies are evaluated for total and aerosol attenuation of radiation within the range of 0.4 to 12.0μm at altitudes up to 30 km. The origin of the transparence properties of atmosphere is discussed.
© (1989) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Larisa A. Mirzoeva, Larisa A. Mirzoeva, Margaret S. Kiseleva, Margaret S. Kiseleva, } "Determination Of Optical Properties And Composition Of Atmosphere From Measurements Of Optical Spectra", Proc. SPIE 1129, Advanced Optical Instrumentation for Remote Sensing of the Earth's Surface from Space, (6 October 1989); doi: 10.1117/12.961485; https://doi.org/10.1117/12.961485
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