Abstract
INFRARED airglow emission is bright, patchy and erratic1,2. The primary source of this emission was identified by Meinel3 as rotation-vibration bands of the OH molecule. These and subsequent studies4–6 did not delineate the true morphology of the infrared night sky because large fields of view (∼20 deg2) were used and only point by point measurements taken. Accurate mapping of the night sky requires a small field of view to resolve the smallest structures and a rapid scanning rate to “freeze” any time variations in the luminosity.
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References
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PETERSON, A., KIEFFABER, L. Infrared Photography of OH Airglow Structures. Nature 242, 321–322 (1973). https://doi.org/10.1038/242321a0
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DOI: https://doi.org/10.1038/242321a0
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