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Observations of gravity waves in the OH airglow layer above Rothera (68S, 68W) using a three-dimensional S-Transform analysis
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  • Shaun Martin Dempsey,
  • Neil P Hindley,
  • Corwin James Wright,
  • Nicholas Mitchell,
  • Tracy Moffat-Griffin,
  • Pierre-Dominique Pautet,
  • Michael J. Taylor
Shaun Martin Dempsey
University of Bath
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Neil P Hindley
University of Bath
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Corwin James Wright
University of Bath

Corresponding Author:[email protected]

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Nicholas Mitchell
University of Bath
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Tracy Moffat-Griffin
British Antarctic Survey
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Pierre-Dominique Pautet
Utah State Uiversity
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Michael J. Taylor
Utah State University
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Abstract

In this study, we apply the three-dimensional Stockwell Transform (3DST) to a novel dataset, namely airglow imager data from Rothera (68S, 68W). We use this approach to investigate small-scale high-frequency gravity waves (GWs) in the hydroxyl (OH) airglow layer, at a height $\sim$87 km in the mesosphere and lower thermosphere (MLT). MLT GWs are often underrepresented in models, being parameterised due to their small scale size and as such, the significant quantities of momentum and energy transferred by these small waves are missed. Better quantification of these waves is thus needed to support future model development. We find that the 3DST can identify waves and extract wave properties and their locations. Horizontal wavelengths are observed ranging from 10 to 40 km and vertical wavelengths of 15 to 40 km, with wave periods of 5 to 9 minutes, peaking at 7.5 minutes. These values are consistent with previous studies. Group speeds are found to be non-zero and large, implying that these GWs travel horizontally and fast. This case study demonstrates that the 3DST can be applied to airglow imager data and can successfully extract GW parameters. This is an important step in automating GW analysis in airglow.
10 Jan 2023Submitted to ESS Open Archive
17 Jan 2023Published in ESS Open Archive