Spatial and temporal variations in infrared emissions of the upper atmosphere. 2. 15-μm carbon dioxide emission
- 作者: Semenov A.I.1, Medvedeva I.V.2, Perminov V.I.1, Zheleznov Y.A.3
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隶属关系:
- Obukhov Institute of Atmospheric Physics
- Institute of Solar–Terrestrial Physics, Siberian Division
- Institute of Electrophysics and Electroenergetics
- 期: 卷 57, 编号 5 (2017)
- 页面: 597-601
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156393
- DOI: https://doi.org/10.1134/S0016793217040168
- ID: 156393
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详细
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.
作者简介
A. Semenov
Obukhov Institute of Atmospheric Physics
编辑信件的主要联系方式.
Email: anasemenov@yandex.ru
俄罗斯联邦, Moscow
I. Medvedeva
Institute of Solar–Terrestrial Physics, Siberian Division
Email: anasemenov@yandex.ru
俄罗斯联邦, Irkutsk
V. Perminov
Obukhov Institute of Atmospheric Physics
Email: anasemenov@yandex.ru
俄罗斯联邦, Moscow
Yu. Zheleznov
Institute of Electrophysics and Electroenergetics
Email: anasemenov@yandex.ru
俄罗斯联邦, St. Petersburg
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