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

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...

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Bibliographic Details
Main Authors: Domeisen, Daniela I. V. (Author), Plumb, R. Alan (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: American Geophysical Union, 2014-03-27T15:55:55Z.
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100 1 0 |a Domeisen, Daniela I. V.  |e author 
100 1 0 |a Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences  |e contributor 
100 1 0 |a Plumb, R. Alan  |e contributor 
700 1 0 |a Plumb, R. Alan  |e author 
245 0 0 |a Traveling planetary-scale Rossby waves in the winter stratosphere: The role of tropospheric baroclinic instability 
260 |b American Geophysical Union,   |c 2014-03-27T15:55:55Z. 
856 |z Get fulltext  |u http://hdl.handle.net/1721.1/85926 
520 |a 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. 
520 |a National Science Foundation (U.S.) (grant 0808831) 
546 |a en_US 
655 7 |a Article 
773 |t Geophysical Research Letters