Articles | Volume 16, issue 9
https://doi.org/10.5194/acp-16-5611-2016
https://doi.org/10.5194/acp-16-5611-2016
Research article
 | 
04 May 2016
Research article |  | 04 May 2016

Response of OH airglow emissions to mesospheric gravity waves and comparisons with full-wave model simulation at a low-latitude Indian station

Rupesh N. Ghodpage, Michael P. Hickey, Alok K. Taori, Devendraa Siingh, and Parashram T. Patil

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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 Alok Taori on behalf of the Authors (15 Mar 2016)  Author's response    Manuscript
ED: Referee Nomination & Report Request started (23 Mar 2016) by Jayanarayanan Kuttippurath
RR by Anonymous Referee #2 (24 Mar 2016)
RR by Anonymous Referee #1 (04 Apr 2016)
ED: Reconsider after minor revisions (Editor review) (04 Apr 2016) by Jayanarayanan Kuttippurath
AR by Alok Taori on behalf of the Authors (05 Apr 2016)  Author's response    Manuscript
ED: Publish subject to technical corrections (17 Apr 2016) by Jayanarayanan Kuttippurath
AR by Alok Taori on behalf of the Authors (19 Apr 2016)  Author's response    Manuscript
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Short summary
Gravity-wave-induced oscillations have been characterized over Kolhapur (16.8°N and 74.2°E), India, using the adiabatic variations in OH airglow intensity and temperature data. The results show that there exist large deviations from one investigation to the other. We also use a full-wave model to simulate the response of OH emission to the wave motion and compare the results with observed values. This report discusses the observed wave characteristics and cause of the noted difference.
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