Field-aligned acceleration of ions by the Alfven waves in the polar regions

被引:3
|
作者
Guglielmi, A.
Lundin, R.
Potapov, A.
Tsegmed, B.
Petrunin, A.
机构
[1] Inst Solar Terr Phys SB RAS, Irkutsk 664033, Russia
[2] Inst Phys Earth RAS, Moscow, Russia
[3] Swedish Inst Space Phys, S-98128 Kiruna, Sweden
[4] Res Ctr Astron & Geophys, Ulaanbaatar, Mongolia
关键词
ponderomotive forces; magnetosphere; Alfven waves;
D O I
10.1016/j.asr.2005.03.006
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Ponderomotive field-aligned acceleration of ions by Alfven waves is a fundamental process in terrestrial and celestial plasmas. Ponderomotive forcing may transfer wave energy and momentum to plasmas on small scales as well as on large scales. The process is expected to play an important role in energizing ionospheric ions over the polar region, leading to outflow of ions into the outer magnetosphere. We discuss the acceleration of upward moving heavy ions like O+ and how they behave while approaching the resonant altitude, i.e., where the gyrofrequency equals the wave frequency. In the vicinity of the resonant altitude the so-called magnetic moment pumping (NIMP) process dominates [Lundin, R., Hultqvist, B. Ionospheric plasma escape by high-amplitude electric fields: magnetic moment "pumping". J. Geophys. Res. 94, 6665-6680, 1989; Guglielmil A., Lundin, R. Ponderomotive upward acceleration of ions by ion cyclotron and Alfven waves over the polar regions. J. Geophys. Res. 106, 13,219-13,236, 2001]. The problem is to remove the singularity, the pole, of the MMP ponderomotive potential at the resonance altitude where the solution, the heavy ion energy goes to infinity. To eliminate this singularity we present three different modifications to remove the pole of the MMP force equation: (a) assuming a finite transverse size of the wave field, (b) introducing an effective collision frequency, and (c) assuming a finite ion-transit time. We check the validity of these modifications by test particle simulation in the framework of a 2D model of the electromagnetic wave field by comparing the numerical solutions of the exact equation of motion with the solutions of the MMP equation. (C) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:617 / 621
页数:5
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