Intensification of preexisting auroral arc at substorm expansion phase onset:: Wave-like disruption during the first tens of seconds

被引:118
作者
Liang, Jun [1 ]
Donovan, E. F. [4 ]
Liu, W. W. [1 ]
Jackel, B. [4 ]
Syrjasuo, M. [5 ]
Mende, S. B. [2 ]
Frey, H. U. [2 ]
Angelopoulos, V. [2 ]
Connors, M. [3 ]
机构
[1] Canadian Space Agcy, Space Sci Branch, St Hubert, PQ J3Y 8Y9, Canada
[2] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[3] Athabasca Univ, Athabasca, AB T3G 2Z8, Canada
[4] Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada
[5] Finnish Meteorol Inst, FI-00101 Helsinki, Finland
关键词
D O I
10.1029/2008GL033666
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
With the deployment of the all-sky imager array of the THEMIS mission, we were able to construct a preliminary database of auroral substorm expansion phase onsets, from which we have established a number of common features characterizing the first tens of seconds of the substorm auroral intensification. We find that the intensification occurs within similar to 10 sec over an arc segment extending approximately 1 h MLT and featuring wave-like formations distributed in longitude. The longitudinal wave number ranges between 100 and 300 such that the wavelength is comparable to the ion gyroradius in the central plasma sheet. The scale the intensification is about 10-30 sec. This study casts important observational constraints on substorm onset theories.
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页数:6
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