Spatial and Temporal Variations of Infrared Emissions in the Upper Atmosphere. 3. 5.3-μm Nitric Oxide Emission
- Authors: Semenov A.I.1, Medvedeva I.V.2, Perminov V.I.1
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Affiliations:
- Obukhov Institute of Atmospheric Physics
- Institute of Solar–Terrestrial Physics, Siberian Division
- Issue: Vol 58, No 2 (2018)
- Pages: 273-280
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156722
- DOI: https://doi.org/10.1134/S0016793218020172
- ID: 156722
Cite item
Abstract
The results of rocket and satellite measurements available in the literature of 5.3-μm nitric oxide emission in the upper atmosphere have been systematized and analyzed. Analytical dependences describing the height distribution of volumetric intensity of 5.3-μm emission of the NO molecule and its variations in a range of heights from 100 to 130 km as a function of the time of year, day, 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
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