The dynamics of electron-ion coupling in the shock transition region

被引:20
作者
Shimada, N
Hoshino, M
机构
[1] JSPS, Tokyo 1848795, Japan
[2] Commun Res Labs, Tokyo 1848795, Japan
[3] Univ Tokyo, Dept Earth & Planetary Sci, Bunkyo Ku, Tokyo 1130033, Japan
关键词
D O I
10.1063/1.1557911
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
In the shock transition region the process of electron-ion coupling under Buneman instability between inflow electrons and reflected ions is investigated. Buneman instability often evolves into a highly nonlinear state with strong wave-particle interaction like velocity phase hole (vortex) dynamics. Previous studies have shown that these electron holes contribute to the strong electron heating and acceleration. In this study, how electron holes affect the ions and interact with them is examined. Under the condition of Buneman instability dominant, the electron holes preserve their coherent large-amplitude structure for a sufficiently long period of time to modify the ion population electrostatically. Electron holes resonate with the ion population through the ion-acoustic branch, and then some of the inflow ions are rapidly decelerated and reflected by the electric field at the electron holes. As a result of gaining additional energy from the inflow ion population, the amplitude of the electric field of the hole becomes 40% larger than what was estimated in some previous studies, which did not take the coupling ions into account. Although the electron hole-ion coupling state is seen in such a small scale as electron inertia length (c/omega(pe)), this large electric field of the electron hole leads to a strong disturbance and heating of the plasma. This study may provide a first indication of what regulates strong electron heating in the shock transition region through the coupling process between the electrons and ions. (C) 2003 American Institute of Physics.
引用
收藏
页码:1113 / 1119
页数:7
相关论文
共 20 条
[1]   Bipolar electrostatic structures in the shock transition region: Evidence of electron phase space holes [J].
Bale, SD ;
Kellogg, PJ ;
Larson, DE ;
Lin, RP ;
Goetz, K ;
Lepping, RP .
GEOPHYSICAL RESEARCH LETTERS, 1998, 25 (15) :2929-2932
[2]   Electrostatic turbulence and Debye-Scale structures associated with electron thermalization at collisionless shocks [J].
Bale, SD ;
Hull, A ;
Larson, DE ;
Lin, RP ;
Muschietti, L ;
Kellogg, PJ ;
Goetz, K ;
Monson, SJ .
ASTROPHYSICAL JOURNAL, 2002, 575 (01) :L25-L28
[3]  
Dieckmann ME, 2000, ASTRON ASTROPHYS, V356, P377
[4]   Large-scale numerical simulations of ion beam instabilities in unmagnetized astrophysical plasmas [J].
Dieckmann, ME ;
Ljung, P ;
Ynnerman, A ;
McClements, KG .
PHYSICS OF PLASMAS, 2000, 7 (12) :5171-5181
[5]   RELATIVISTIC MAGNETOSONIC SHOCK-WAVES IN SYNCHROTRON SOURCES - SHOCK STRUCTURE AND NONTHERMAL ACCELERATION OF POSITRONS [J].
HOSHINO, M ;
ARONS, J ;
GALLANT, YA ;
LANGDON, AB .
ASTROPHYSICAL JOURNAL, 1992, 390 (02) :454-479
[6]   Nonthermal electrons at high Mach number shocks: Electron shock surfing acceleration [J].
Hoshino, M ;
Shimada, N .
ASTROPHYSICAL JOURNAL, 2002, 572 (02) :880-887
[7]  
Hoshino M, 2001, PROG THEOR PHYS SUPP, P149, DOI 10.1143/PTPS.143.149
[8]  
Kojima H., 1999, Advances in Space Research, V23, P1689, DOI 10.1016/S0273-1177(99)00377-4
[9]   EVIDENCE FOR SHOCK ACCELERATION OF HIGH-ENERGY ELECTRONS IN THE SUPERNOVA REMNANT SN1006 [J].
KOYAMA, K ;
PETRE, R ;
GOTTHELF, EV ;
HWANG, U ;
MATSUURA, M ;
OZAKI, M ;
HOLT, SS .
NATURE, 1995, 378 (6554) :255-258
[10]   THE STRUCTURE OF PERPENDICULAR BOW SHOCKS [J].
LEROY, MM ;
WINSKE, D ;
GOODRICH, CC ;
WU, CS ;
PAPADOPOULOS, K .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1982, 87 (NA7) :5081-5094