Spatial and temporal variations in infrared emissions of the upper atmosphere. 2. 15-μm carbon dioxide emission
- Authors: Semenov A.I.1, Medvedeva I.V.2, Perminov V.I.1, Zheleznov Y.A.3
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Affiliations:
- Obukhov Institute of Atmospheric Physics
- Institute of Solar–Terrestrial Physics, Siberian Division
- Institute of Electrophysics and Electroenergetics
- Issue: Vol 57, No 5 (2017)
- Pages: 597-601
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156393
- DOI: https://doi.org/10.1134/S0016793217040168
- ID: 156393
Cite item
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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