Modeling the Earth’s Nightglow Intensity of the Chamberlain and Herzberg I Bands and Comparing the Calculation Results with the Experimental Data
The calculations of volume intensity profiles of the Earth’s nightglow of the Chamberlain and Herzberg I bands of molecular oxygen are given. The calculations of glow intensities of the Chamberlain and Herzberg I bands are compared with the experimental data obtained from the Discovery Space Shuttle...
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Published in | Geomagnetism and Aeronomy Vol. 62; no. 5; pp. 614 - 622 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
Moscow
Pleiades Publishing
01.10.2022
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
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Summary: | The calculations of volume intensity profiles of the Earth’s nightglow of the Chamberlain and Herzberg I bands of molecular oxygen are given. The calculations of glow intensities of the Chamberlain and Herzberg I bands are compared with the experimental data obtained from the Discovery Space Shuttle (STS-53) and from the EbertFastie spectrograph (Kitt Peak National Observatory, USA, Arizona). It is shown that the best agreement between the calculation results and experimental data is observed when correcting the quantum yields of the vibrational levels A'
3
Δ
u
and
of the molecular oxygen states under triple collisions. |
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ISSN: | 0016-7932 1555-645X 0016-7940 |
DOI: | 10.1134/S001679322204003X |