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Exploring sources of gravity waves in the southern winter stratosphere through ray-tracing 3-D satellite observations
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  • Phoebe E Noble,
  • Sebastian Rhode,
  • Neil P Hindley,
  • Peter Berthelemy,
  • Tracy Moffat-Griffin,
  • Peter Preusse,
  • Lars Hoffmann,
  • Corwin James Wright
Phoebe E Noble
University of Bath

Corresponding Author:[email protected]

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Sebastian Rhode
Forschungszentrum Jülich
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Neil P Hindley
University of Bath
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Peter Berthelemy
University of Bath
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Tracy Moffat-Griffin
British Antarctic Survey
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Peter Preusse
Institute of Energy and Climate Research (IEK-7: Stratosphere), Forschungszentrum Jülich
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Lars Hoffmann
Forschungszentrum Jülich
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Corwin James Wright
University of Bath
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Abstract

During winter, the latitude belt at 60S is one of the most intense hotspots of stratospheric gravity wave (GW) activity. However, producing accurate representations of GW dynamics in this region in numerical models has proved exceptionally challenging. One reason for this is that questions remain regarding the relative contributions of different orographic and non-orographic sources of GWs here.
We use 3-D satellite GW observations from the Atmospheric InfraRed Sounder (AIRS) from winter 2012 in combination with the Gravity-wave Regional Or Global Ray Tracer (GROGRAT) to backwards ray trace GWs to their sources. We trace over 14.2 million rays, which allows us to investigate GW propagation and to produce systematic estimates of the relative contribution of orographic and non-orographic sources to the total observed stratospheric GW momentum flux in this region.
We find that in winter 56% of momentum flux (MF) traces back to the ocean and 44% to land, despite land representing less than a quarter of the region’s area. This demonstrates that, while orographic sources contribute much more momentum flux per unit area, the large spatial extent of non-orographic sources leads to a higher overall contribution. The small islands of Kerguelen and South Georgia specifically contribute up to 1.6% and 0.7% of average monthly stratospheric MF, and the intermittency of these sources suggests that their short-timescale contribution is even higher. These results provide the important insights needed to significantly advance our knowledge of the atmospheric momentum budget in the Southern polar region.
04 Apr 2024Submitted to ESS Open Archive
16 Apr 2024Published in ESS Open Archive