Paper
13 December 2018 Empirical model of the nitric oxide emission 5.3 μm in the upper atmosphere
A. I. Semenov, I. V. Medvedeva, V. I. Perminov, V. Yu. Khomich, Yu. A. Zheleznov
Author Affiliations +
Proceedings Volume 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics; 10833A7 (2018) https://doi.org/10.1117/12.2504554
Event: XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, 2018, Tomsk, Russian Federation
Abstract
The systematization and the analysis of long-term data of satellite and rocket measurements of the 5.3-μm nitric oxide emission in the upper atmosphere were carried out. An analysis of photochemical processes leading to the producing of NO emission in the upper atmosphere is performed. Analytical relationships describing the seasonal and latitudinal variations in the intensity of the 5.3 μm NO emission, its altitude distribution, and the dependence on solar activity are obtained.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A. I. Semenov, I. V. Medvedeva, V. I. Perminov, V. Yu. Khomich, and Yu. A. Zheleznov "Empirical model of the nitric oxide emission 5.3 μm in the upper atmosphere", Proc. SPIE 10833, 24th International Symposium on Atmospheric and Ocean Optics: Atmospheric Physics, 10833A7 (13 December 2018); https://doi.org/10.1117/12.2504554
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KEYWORDS
Solar processes

Atmospheric modeling

NOx

Satellites

Molecules

Infrared radiation

Rockets

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