Large-scale planetary disturbances in stratospheric temperature at high-latitudes in the southern summer hemisphere

The global structure and propagation of large-scale (periods >5 days) waves in the Southern Hemisphere summer (December 2006–February 2007) at 60° S–75° S latitude are examined using temperature data from GPS radio occultation measurements by COSMIC/FORMOSAT 3 satellite constellation at 20 km and...

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Bibliographic Details
Published in:Atmospheric Chemistry and Physics
Main Authors: Shepherd, M. G., Tsuda, T.
Format: Article in Journal/Newspaper
Language:English
Published: Copernicus Publications 2008
Subjects:
Online Access:https://doi.org/10.5194/acp-8-7557-2008
https://noa.gwlb.de/receive/cop_mods_00047944
https://noa.gwlb.de/servlets/MCRFileNodeServlet/cop_derivate_00047564/acp-8-7557-2008.pdf
https://acp.copernicus.org/articles/8/7557/2008/acp-8-7557-2008.pdf
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Summary:The global structure and propagation of large-scale (periods >5 days) waves in the Southern Hemisphere summer (December 2006–February 2007) at 60° S–75° S latitude are examined using temperature data from GPS radio occultation measurements by COSMIC/FORMOSAT 3 satellite constellation at 20 km and 30 km altitude. Spectral analysis has revealed eastward propagating planetary scale perturbations with wavenumbers 1 and 2 and periods of 10, 16 and 23 days, and stationary waves with wavenumbers 1 and 2. The results obtained show a very dynamically active Antarctic summer stratosphere. The novel aspect of the work is in the use of the GPS COSMIC data providing multiple local times each day, thus allowing large-scale wave analysis at high Southern latitudes and revealing planetary wave activity not normally observed in summer, but more consistent with late winter and spring conditions in the stratosphere.