Nonthermal electrons at high Mach number shocks: Electron shock surfing acceleration

被引:151
作者
Hoshino, M [1 ]
Shimada, N [1 ]
机构
[1] Univ Tokyo, Dept Earth & Planetary Phys, Bunkyo Ku, Tokyo 1130033, Japan
关键词
acceleration of particles; cosmic rays; plasmas; shock waves;
D O I
10.1086/340454
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the suprathermal electron acceleration mechanism in a perpendicular magnetosonic shock wave in a high Mach number regime by using a particle-in-cell simulation. We find that shock surfing/surfatron acceleration producing suprathermal electrons occurs in the shock transition region, where a series of large-amplitude electrostatic solitary waves ( ESWs) are excited by Buneman instability under the interaction between the reflected ions and the incoming electrons. It is shown that the electrons are likely to be trapped by ESWs, and during the trapping phase they can be effectively accelerated by the shock motional/convection electric field. We discuss that suprathermal electrons can be accelerated up to m(i)c(2) (v(0)/c), where m(i)c(2) is the ion rest mass energy and v(0) is the shock upstream flow velocity. Furthermore, some of these suprathermal electrons may be effectively trapped for an infinitely long time when the Alfven Mach number M-A exceeds several tens, and they are accelerated up to the shock potential energy determined by the global shock size.
引用
收藏
页码:880 / 887
页数:8
相关论文
共 44 条
[1]  
Axford W. I., 1977, INT COSMIC RAY C, P132
[2]   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
[3]   ACCELERATION OF COSMIC-RAYS IN SHOCK FRONTS .1. [J].
BELL, AR .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1978, 182 (01) :147-156
[4]   Electron acceleration to ultrarelativistic energies in a collisionless oblique shock wave [J].
Bessho, N ;
Ohsawa, Y .
PHYSICS OF PLASMAS, 1999, 6 (08) :3076-3085
[5]  
BLANDFORD RD, 1978, APJ, V179, P573
[6]   INSTABILITY, TURBULENCE, AND CONDUCTIVITY IN CURRENT-CARRYING PLASMA [J].
BUNEMAN, O .
PHYSICAL REVIEW LETTERS, 1958, 1 (01) :8-9
[7]   A MECHANISM FOR STRONG SHOCK ELECTRON HEATING IN SUPERNOVA-REMNANTS [J].
CARGILL, PJ ;
PAPADOPOULOS, K .
ASTROPHYSICAL JOURNAL, 1988, 329 (01) :L29-L32
[8]   Cygnus A [J].
Carilli, CL ;
Barthel, PD .
ASTRONOMY AND ASTROPHYSICS REVIEW, 1996, 7 (01) :1-54
[9]   ELECTRON HEATING BY ELECTRON-ION BEAM INSTABILITIES [J].
DAVIDSON, RC ;
KRALL, NA ;
PAPADOPOULOS, K ;
SHANNY, R .
PHYSICAL REVIEW LETTERS, 1970, 24 (11) :579-+
[10]  
Dieckmann ME, 2000, ASTRON ASTROPHYS, V356, P377