Link between premidnight second harmonic poloidal waves and auroral undulations: Conjugate observations with a Van Allen Probe spacecraft and a THEMIS all-sky imager

被引:14
|
作者
Motoba, T. [1 ]
Takahashi, K. [1 ]
Ukhorskiy, A. [1 ]
Gkioulidou, M. [1 ]
Mitchell, D. G. [1 ]
Lanzerotti, L. J. [2 ]
Korotova, G. I. [3 ,4 ]
Donovan, E. F. [5 ]
Wygant, J. R. [6 ]
Kletzing, C. A. [7 ]
Kurth, W. S. [7 ]
Blake, J. B. [8 ]
机构
[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[2] New Jersey Inst Technol, Newark, NJ 07102 USA
[3] IZMIRAN, Troitsk, Russia
[4] Univ Maryland, IPST, College Pk, MD 20742 USA
[5] Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada
[6] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA
[7] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[8] Aerosp Corp, Los Angeles, CA 90009 USA
基金
美国国家科学基金会;
关键词
auroral undulations; second harmonic waves; wave-particle interactions; LARGE-SCALE UNDULATIONS; GEOMAGNETIC-PULSATIONS; GIANT UNDULATIONS; DIFFUSE AURORA; MAGNETIC-FIELD; ALFVEN WAVES; EDGE; ASSOCIATION; INSTABILITY; BOUNDARY;
D O I
10.1002/2014JA020863
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report, for the first time, an auroral undulation event on 1 May 2013 observed by the Time History of Events and Macroscale Interactions During Substorms (THEMIS) all-sky imager (ASI) at Athabasca (L=4.6), Canada, for which in situ field and particle measurements in the conjugate magnetosphere were available from a Van Allen Probe spacecraft. The ASI observed a train of auroral undulation structures emerging spontaneously in the premidnight subauroral ionosphere during the growth phase of a substorm. The undulations had an azimuthal wavelength of similar to 180km and propagated westward at a speed of 3-4kms(-1). The successive passage over an observing point yielded quasiperiodic oscillations in diffuse auroral emissions with a period of similar to 40s. The azimuthal wave number m of the auroral luminosity oscillations was found to be m similar to-103. During the event, the spacecraftbeing on tailward stretched field lines similar to 0.5 R-E outside the plasmapause that mapped into the ionosphere conjugate to the auroral undulationsencountered intense poloidal ULF oscillations in the magnetic and electric fields. We identify the field oscillations to be the second harmonic mode along the magnetic field line through comparisons of the observed wave properties with theoretical predictions. The field oscillations were accompanied by oscillations in proton and electron fluxes. Most interestingly, both field and particle oscillations at the spacecraft had one-to-one association with the auroral luminosity oscillations around its footprint. Our findings strongly suggest that this auroral undulation event is closely linked to the generation of second harmonic poloidal waves.
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页码:1814 / 1831
页数:18
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