Pc1 pearl waves with magnetosonic dispersion

被引:8
|
作者
Feygin, F. Z.
Nekrasov, A. K.
Pikkarainen, T.
Raita, T.
Prikner, K.
机构
[1] Russian Acad Sci, Inst Phys Earth, Moscow 123995, Russia
[2] Univ Oulu, Dept Phys Sci, FIN-90014 Oulu, Finland
[3] Univ Oulu, Sodankyla Geophys Observ, FIN-99600 Sodankyla, Finland
[4] Acad Sci Czech Republic, Inst Geophys, Prague 14131 4, Sporilov, Czech Republic
基金
俄罗斯基础研究基金会;
关键词
magnetosphere; geomagnetic pulsations; Alfven waves; magnetosonic waves;
D O I
10.1016/j.jastp.2007.01.019
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Results of the analysis of 15 unusual Pc1 pearl wave events with inverse dispersion in comparison with the dispersion of well-known electromagnetic ion-cyclotron (EMIC) waves in the form of classic pearl pulsations are presented. Pulsations with the dynamical spectrum consisting of both falling tones only (first type) and events with structures, which start with the falling tones and then develop into rising tones (second type), have been discovered. The first type corresponds to the frequency dispersion of magnetosonic waves (R-waves), and the second type corresponds to the mixed frequency dispersion of R-waves and EMIC waves (L-waves). All events were observed during quiet geomagnetic periods. The duration of the events is about 20-30min. For the interpretation of these phenomena, the cyclotron instability driven by energetic proton beams with relative mean velocity v(0) directed along the background magnetic field and corresponding to an energy similar to 10-100 keV is considered. The interaction of such proton beams with waves having frequencies omega<omega(i) (omega(i) is the ion gyrofrequency) leads to the instability, which allows the fastest growth of electromagnetic oscillations with the dispersion of R-wave type. When the velocity of the proton beam decreases (v(0)similar to 0), R-waves attenuate and L-waves (for the proton temperature T-perpendicular to > T-parallel to) will be amplified. This instability is the reason for the generation of classic Pet pearl pulsations with the usual dispersion and allows explaining the transition of the dispersion from R- to L-waves. (C) 2007 Elsevier Ltd. All rights reserved.
引用
收藏
页码:1644 / 1650
页数:7
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