Substorm onset timing via traveltime magnetoseismology

被引:19
作者
Chi, P. J. [1 ]
Russell, C. T. [1 ]
Ohtani, S. [2 ]
机构
[1] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA
[2] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
关键词
PI2; PULSATIONS; CURRENT WEDGE; MAGNETOSPHERE; SHEET; MODEL; FLOW;
D O I
10.1029/2008GL036574
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
This letter introduces a traveltime magnetoseismic technique that can estimate the substorm onset time in the magnetotail from multi-point observations of Pi 2 pulsations. The arrival time of Pi 2, which is defined as the first peak in Pi 2 amplitude, observed by ground magnetometers presents a strong function of latitude. Using the Tamao traveltime as the forward model, the magnetoseismic inversion from the observed Pi 2 arrival time infers that the onset of the 22 July 1998 substorm in the magnetotail started at X similar to -20 RE at 6: 53: 10 UT, or 1-3 minutes earlier than the Pi 2 onset time conventionally identified in ground records. The magnetoseismic result is further compared with the observations of auroral brightening, revealing a clear sequence of events during this substorm. Citation: Chi, P. J., C. T. Russell, and S. Ohtani (2009), Substorm onset timing via traveltime magnetoseismology, Geophys. Res. Lett., 36, L08107, doi: 10.1029/2008GL036574.
引用
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页数:5
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