Abstract
The intensities of the Atmospheric bands of molecular oxygen Ivʹvʺ (cm–2s–1) in the nightglow of the Earth’s atmosphere are calculated for different latitudes and seasons. The calculations were performed using experimental data on the profiles of atomic oxygen concentrations for different seasons. The calculated integral intensities of Atmospheric bands are compared with experimental data obtained from the space shuttle (STS transport system), as well as from the Keck I telescope. It is shown that there is good agreement between theoretical calculations and experimental data for the considered latitudes, but better agreement is received with data obtained from Keck I telescope.
Published Version
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