Geomagnetic activity signatures in wintertime stratosphere wind, temperature, and wave response

被引:93
作者
Seppala, A. [1 ]
Lu, H. [2 ]
Clilverd, M. A. [2 ]
Rodger, C. J. [3 ]
机构
[1] Finnish Meteorol Inst, FIN-00101 Helsinki, Finland
[2] British Antarctic Survey, NERC, Cambridge CB3 0ET, England
[3] Univ Otago, Dept Phys, Dunedin, New Zealand
基金
英国自然环境研究理事会; 芬兰科学院;
关键词
ENERGETIC PARTICLE-PRECIPITATION; QUASI-BIENNIAL OSCILLATION; UPPER-ATMOSPHERE; SOLAR-CYCLE; ENHANCEMENTS; TRANSPORT; ERA-40; IMPACT; OZONE; MODE;
D O I
10.1002/jgrd.50236
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
We analyzed ERA-40 and ERA Interim meteorological re-analysis data for signatures of geomagnetic activity in zonal mean zonal wind, temperature, and Eliassen-Palm flux in the Northern Hemisphere extended winter (November-March). We found that for high geomagnetic activity levels, the stratospheric polar vortex becomes stronger in late winter, with more planetary waves being refracted equatorward. The statistically significant signals first appear in December and continue until March, with poleward propagation of the signals with time, even though some uncertainty remains due to the limited amount of data available (similar to 50 years). Our results also indicated that the geomagnetic effect on planetary wave propagation has a tendency to take place when the stratosphere background flow is relatively stable or when the polar vortex is stronger and less disturbed in early winter. These conditions typically occur during high solar irradiance cycle conditions or westerly quasi-biennial oscillation conditions.
引用
收藏
页码:2169 / 2183
页数:15
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