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Method for Studying Twilight Phenomena

  • V. G. Fesenkov

Abstract

Many papers have been devoted to the investigation of twilight phenomena, but they have been mainly of a descriptive nature. Conclusions about the optical properties of the upper atmosphere, which, it would seem, should be the principal goal of twilight research, are usually drawn in a highly elementary manner, on the basis of rather arbitrary simplifying assumptions. The optical properties of twilight are incomparably more complex than those of the daytime sky.

Keywords

Solar Disk Symmetric Point Atmospheric Ozone Noctilucent Cloud Zenith Distance 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Literature Cited

  1. 1.
    V. G. Fesenkov, “On the earth’s atmospheric shadow,” Astron. zh., Vol. 26, No. 4 (1949).Google Scholar
  2. 2.
    V. G. Fesenkov, Trudy Astrofiz. inst., Alma-Ata, Vol. 3, p. 214 (1962).Google Scholar
  3. 3.
    V. G. Fesenkov, “On sounding the optical properties of the atmosphere with artificial satellites,” Astron. zh., Vol. 43, No. 6 (1966).Google Scholar

Copyright information

© Consultants Bureau, New York 1970

Authors and Affiliations

  • V. G. Fesenkov

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