Monitoring the Optical Stability of the Atmosphere for Small and Large Optical Thicknesses

  • V. E. Pavlov

Abstract

The brightness of the sky on the solar almucantar is chiefly determined by the following parameters [1, 2]: the solar zenith distance z, the optical thickness of the atmosphere τ 1 and the albedo of the underlying surface q, and it is greatly dependent upon the form of the scattering indicatrix.

Keywords

Turbidity Kazakhstan 

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Literature Cited

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© Consultants Bureau, New York 1970

Authors and Affiliations

  • V. E. Pavlov

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