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Infrared Photography of OH Airglow Structures

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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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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