Observational evidence of the generation mechanism for rising-tone chorus

被引:62
|
作者
Cully, C. M. [1 ]
Angelopoulos, V. [2 ]
Auster, U. [3 ]
Bonnell, J. [4 ]
Le Contel, O. [5 ]
机构
[1] Swedish Inst Space Phys, SE-75121 Uppsala, Sweden
[2] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA
[3] Inst Geophys & Extraterr Phys, D-38106 Braunschweig, Germany
[4] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[5] CNRS Ecole Polytech UPMC, Lab Phys Plasmas, F-78140 Velizy Villacoublay, France
基金
瑞典研究理事会;
关键词
WHISTLER-MODE CHORUS; STORM-TIME CHORUS; THEMIS; EMISSIONS; MAGNETOMETER; INSTRUMENT; DIFFUSION;
D O I
10.1029/2010GL045793
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Chorus emissions are a striking feature of the electromagnetic wave environment in the Earth's magnetosphere. These bursts of whistler-mode waves exhibit characteristic frequency sweeps (chirps) believed to result from wave-particle trapping of cyclotron-resonant particles. Based on the theory of Omura et al. (2008), we predict the sweep rates of chorus elements observed by the THEMIS satellites. The predictions use independent observations of the electron distribution functions and have no free parameters. The predicted chirp rates are a function of wave amplitude, and this relation is clearly observed. The predictive success of the theory lends strong support to its underlying physical mechanism: cyclotron-resonant wave-particle trapping. Citation: Cully, C. M., V. Angelopoulos, U. Auster, J. Bonnell, and O. Le Contel (2011), Observational evidence of the generation mechanism for rising-tone chorus, Geophys. Res. Lett., 38, L01106, doi:10.1029/2010GL045793.
引用
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页数:5
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