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  4. Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability

Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability

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Author(s)
Domeisen, Daniela I. V.
•
Plumb, R. Alan
Date Issued
October 2012
Journal
Geophysical Research Letters
Publisher
American Geophysical Union
Citation
Domeisen, Daniela I. V., and R. Alan Plumb. “Traveling Planetary-Scale Rossby Waves in the Winter Stratosphere: The Role of Tropospheric Baroclinic Instability.” Geophys. Res. Lett. 39, no. 20 (October 28, 2012): n/a–n/a.
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Final published version
Abstract
The Southern Hemisphere winter stratosphere exhibits prominent traveling planetary-scale Rossby waves, which generally are not able to induce Stratospheric Sudden Warmings. A series of runs of a simplified general circulation model is presented, aimed at better understanding the generation of these waves. While the generation of planetary-scale traveling waves through the interaction of synoptic-scale waves is observed in a control run, when the model is truncated to permit only waves with zonal wave number 1 or 2, the long waves are found to increase in strength, leading to a considerably more active stratosphere including Sudden Warmings comparable in strength to Northern Hemisphere winter. This finding suggests that the role of tropospheric synoptic eddies is two-fold: while generating a weak planetary-scale wave flux into the stratosphere, their main effect is to suppress baroclinic instability of planetary-scale waves by stabilizing the tropospheric mean state.
MIT Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
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Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/85926
DOI of Published Version
https://doi.org/10.1029/2012GL053684
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