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Theoretical description of the temperature distribution in the Earth’s atmosphere


The temperature distribution in the Earth’s atmosphere is studied as a function of distance z counted from the Earth’s surface. Owing to the supposition about the interaction between the convective flow and solar radiation with regard to the coordinate dependence of the atmospheric density, meteorological measurements have been explained.

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Correspondence to S. O. Gladkov.

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Original Russian Text © S.O. Gladkov, 2009, published in Optika Atmosfery i Okeana.

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Gladkov, S.O. Theoretical description of the temperature distribution in the Earth’s atmosphere. Atmos Ocean Opt 22, 180–185 (2009).

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  • Oceanic Optic
  • Solar Surface
  • Blackbody Radiation
  • Dissipative Function
  • Convective Component