Vol. 3, issue 11, article # 18

Galileiskii V. P., Morozov A. M., Oshlakov V. K. Color temperature of the atmosphere and the aerosol optical thickness. // Atmospheric and oceanic optics. 1990. V. 3. No. 11. P. 1116-1119.    PDF
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Abstract:

Analysis of the angular distributions of the color temperature and the pseudoemissivity, which were obtained from results of field measurements as well as simulations, showed that these parameters can be useful indicators for determining the optical state of the atmosphere, in particular, its optical thickness, as well as for selecting and identifying objects and phenomena observed in the atmosphere against the background formed by the scattered solar radiation.

References:

1. M.M. Gurevich, Photometry (Energoizdat., Leningrad, 1983), 272 pp.
2. A.S. Elizarenko, V.A. Solomatin, and Yu.G. Yakushenkov, Optoelectronic Systems for Studying Natural Resources (Nedra, Moscow, 1984), 215 pp.
3. V.P. Galileiskii and A.M. Morozov, Opt. Atm. 3, No. 8, 1005–1006 (1990).
4. A.I. Abramochkin, P.P. Vaulin, V.P. Galileĭskiĭ, et al., Stellar-solar phoelectric photometer, in: Laser Measurements of the Optical and Meteorological Parameters of the Atmosphere, Tomsk Affiliate of the Siberian Branch of the Academy of Sciences of the USSR, Tomsk (1981), pp. 14–19.
5. V.P. Galileiskii and A.M. Morozov, "Brightness of the atmosphere as observed from the surface of the planet", Moscow, VINITI, No. 1172–1387 (1987).
6. G.M. Krekov and R.F. Rakhimov, Lidar Model of the Continental Aerosol (Nauka, Novosibirsk, 1982), 199 pp.
7. V.N. Glushko, V.E. Pavlov, A.I. Ivanov, et al., Brightness and Polarization of the Cloud-Free Atmosphere (Nauka, Alma-Ata, 1979), 201 pp.