Articles | Volume 19, issue 4
Technical note
28 Feb 2019
Technical note |  | 28 Feb 2019

Technical note: Bimodality in mesospheric OH rotational population distributions and implications for temperature measurements

Konstantinos S. Kalogerakis


Interactive discussion

Status: closed
Status: closed
AC: Author comment | RC: Referee comment | SC: Short comment | EC: Editor comment
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Peer-review completion

AR: Author's response | RR: Referee report | ED: Editor decision
AR by Konstantinos Kalogerakis on behalf of the Authors (05 Feb 2019)  Author's response
ED: Publish as is (12 Feb 2019) by Franz-Josef Lübken
Short summary
Light emission from energetic hydroxyl radical, OH*, is a prominent feature in spectra of the night sky. It is routinely used to determine the temperature of the atmosphere near 90 km. This note shows that the common practice of using only a few emission features from low rotational excitation to determine rotational temperatures does not account for the bimodality of the OH population distributions and can lead to large systematic errors.
Final-revised paper