Nonlinear electron acceleration by oblique whistler waves: Landau resonance vs. cyclotron resonance

被引:55
作者
Artemyev, A. V. [1 ,2 ]
Vasiliev, A. A. [2 ,4 ,5 ]
Mourenas, D. [3 ]
Agapitov, O. V. [1 ,6 ]
Krasnoselskikh, V. V. [1 ]
机构
[1] LPC2E CNRS Univ Orleans, Orleans, France
[2] RAS, Space Res Inst, Moscow 117901, Russia
[3] CEA, DAM, DIF, Arpajon, France
[4] Aix Marseille Univ, CNRS, CPT, UMR 7332, F-13288 Marseille, France
[5] Univ Toulon & Var, CNRS, CPT, UMR 7332, F-83957 La Garde, France
[6] Natl Taras Shevchenko Univ Kiev, Kiev, Ukraine
基金
俄罗斯基础研究基金会;
关键词
ENERGY DIFFUSION-COEFFICIENTS; RADIATION BELT ELECTRONS; PITCH-ANGLE SCATTERING; MODE WAVES; MAGNETIC-FIELD; RELATIVISTIC ELECTRONS; SURFATRON ACCELERATION; PARTICLE INTERACTION; VLF WAVES; MAGNETOSPHERE;
D O I
10.1063/1.4836595
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
This paper is devoted to the study of the nonlinear interaction of relativistic electrons and high amplitude strongly oblique whistler waves in the Earth's radiation belts. We consider electron trapping into Landau and fundamental cyclotron resonances in a simplified model of dipolar magnetic field. Trapping into the Landau resonance corresponds to a decrease of electron equatorial pitch-angles, while trapping into the first cyclotron resonance increases electron equatorial pitch-angles. For 100 keV electrons, the energy gained due to trapping is similar for both resonances. For electrons with smaller energy, acceleration is more effective when considering the Landau resonance. Moreover, trapping into the Landau resonance is accessible for a wider range of initial pitch-angles and initial energies in comparison with the fundamental resonance. Thus, we can conclude that for intense and strongly oblique waves propagating in the quasi-electrostatic mode, the Landau resonance is generally more important than the fundamental one. (C) 2013 AIP Publishing LLC.
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页数:15
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