Spatial and temporal variations in infrared emissions of the upper atmosphere. 2. 15-μm carbon dioxide emission


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Abstract

The results of rocket and satellite measurements of carbon dioxide emissions at a wavelength of 15 μm in the upper atmosphere have been systematized and analyzed. Analytical expressions describing the dependence of the altitude distribution of 15-μm CO2 emission intensity and its variation in the altitude range from 100 to 130 km on the season, latitude, and solar activity have been obtained.

About the authors

A. I. Semenov

Obukhov Institute of Atmospheric Physics

Author for correspondence.
Email: anasemenov@yandex.ru
Russian Federation, Moscow

I. V. Medvedeva

Institute of Solar–Terrestrial Physics, Siberian Division

Email: anasemenov@yandex.ru
Russian Federation, Irkutsk

V. I. Perminov

Obukhov Institute of Atmospheric Physics

Email: anasemenov@yandex.ru
Russian Federation, Moscow

Yu. A. Zheleznov

Institute of Electrophysics and Electroenergetics

Email: anasemenov@yandex.ru
Russian Federation, St. Petersburg

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