Stratosphere-troposphere evolution during polar vortex intensification

被引:161
作者
Limpasuvan, V
Hartmann, DL
Thompson, DWJ
Jeev, K
Yung, YL
机构
[1] Coastal Carolina Univ, Dept Chem & Phys, Conway, SC 29528 USA
[2] Univ Washington, Dept Atmospher Sci, Seattle, WA 98195 USA
[3] Colorado State Univ, Dept Atmospher Sci, Ft Collins, CO 80523 USA
[4] Johns Hopkins Univ, Dept Earth & Planetary Sci, Baltimore, MD 21218 USA
[5] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
关键词
D O I
10.1029/2005JD006302
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
Stratosphere-troposphere evolution associated with polar vortex intensification (VI) events is examined during the Northern Hemisphere winter. The incipient stage of a VI event is marked by anomalously low wave activity and descending westerly anomalies over the depth of the polar stratosphere. Reduced poleward planetary wave heat flux occurs as the circumpolar wind becomes strongest and pressure anomalies penetrate toward the surface. Descending pressure patterns project strongly onto the positive state of the Northern Hemisphere Annular Mode (NAM). Concurrently, anomalous poleward momentum flux develops in the upper troposphere, and the related tropospheric mean meridional circulation maintains the attendant wind and temperature anomalies against surface drag. The gross behavior of the composite VI event is similar in shape but opposite in sign to that associated with sudden stratospheric warming events (SSWs). However, the descent of the wind and temperature anomalies over the VI life cycle is generally weaker and slower than its SSW counterpart preceding the maximum vortex anomaly. Similarly, after the maximum wind event, the weakening of the winds is faster than the strengthening of the winds after a SSW. This is because stratospheric wind reduction anomalies are produced by wave driving, which can be rapid, and increases in wind speed are associated with the radiative cooling of the polar cap, which happens more gradually. While the contributions of the anomalous momentum fluxes by the quasi-stationary and synoptic eddies are similar to SSWs, the much stronger anomalous momentum flux observed during VI can be attributed to the larger role of eddies with timescales between 15 and 40 days and of wave number 2 scale. Notable differences between VI and SSW appear in the tropical region. In particular, anomalous vortex intensification seems to occur preferentially during La Nina conditions.
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页码:1 / 15
页数:15
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