ELECTRON ACCELERATION AT A LOW MACH NUMBER PERPENDICULAR COLLISIONLESS SHOCK

被引:37
作者
Umeda, Takayuki [1 ]
Yamao, Masahiro [1 ]
Yamazaki, Ryo [2 ]
机构
[1] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan
[2] Hiroshima Univ, Dept Phys Sci, Higashihiroshima 7398526, Japan
关键词
acceleration of particles; plasmas; shock waves; FULL PARTICLE SIMULATION; REST-FRAME MODEL; SUPERNOVA-REMNANTS; SURFING ACCELERATION; MAGNETIC-FIELD; NONTHERMAL EMISSION; BOW SHOCK; GALAXY; FLUCTUATIONS; INJECTION;
D O I
10.1088/0004-637X/695/1/574
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A full particle simulation study is carried out on the electron acceleration at a collisionless, relatively low Alfven Mach number (M-A = 5), perpendicular shock. Recent self-consistent hybrid shock simulations have demonstrated that the shock front of perpendicular shocks has a dynamic rippled character along the shock surface of low Mach number perpendicular shocks. In this paper, the effect of the rippling of perpendicular shocks on the electron acceleration is examined by means of large-scale (ion-scale) two-dimensional full particle simulations. It has been shown that a large-amplitude electric field is excited at the shock front in association with the ion-scale rippling, and that reflected ions are accelerated upstream at a localized region where the shock-normal electric field of the rippled structure is polarized upstream. The current-driven instability caused by the highly accelerated reflected ions has a high growth rate of up to large-amplitude electrostatic waves. Energetic electrons are then generated by the large-amplitude electrostatic waves via electron surfing acceleration at the leading edge of the shock-transition region. The present result suggests that the electron surfing acceleration is also a common feature at low Mach number perpendicular collisionless shocks.
引用
收藏
页码:574 / 579
页数:6
相关论文
共 40 条
[1]   Electron injection at high Mach number quasi-perpendicular shocks: Surfing and drift acceleration [J].
Amano, T. ;
Hoshino, M. .
ASTROPHYSICAL JOURNAL, 2007, 661 (01) :190-202
[2]   ELECTRON SHOCK SURFING ACCELERATION IN MULTIDIMENSIONS: TWO-DIMENSIONAL PARTICLE-IN-CELL SIMULATION OF COLLISIONLESS PERPENDICULAR SHOCK [J].
Amano, Takanobu ;
Hoshino, Masahiro .
ASTROPHYSICAL JOURNAL, 2009, 690 (01) :244-251
[3]   A spatial and spectral study of nonthermal filaments in historical supernova remnants:: Observational results with Chandra [J].
Bamba, A ;
Yamazaki, R ;
Yoshida, T ;
Terasawa, T ;
Koyama, K .
ASTROPHYSICAL JOURNAL, 2005, 621 (02) :793-802
[4]   Small-scale structure of the SN 1006 shock with Chandra observations [J].
Bamba, A ;
Yamazaki, R ;
Ueno, M ;
Koyama, K .
ASTROPHYSICAL JOURNAL, 2003, 589 (02) :827-837
[5]   PARTICLE-ACCELERATION AT ASTROPHYSICAL SHOCKS - A THEORY OF COSMIC-RAY ORIGIN [J].
BLANDFORD, R ;
EICHLER, D .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1987, 154 (01) :1-75
[6]   Discovery of 35 new supernova remnants in the inner galaxy [J].
Brogan, CL ;
Gelfand, JD ;
Gaensler, BM ;
Kassim, NE ;
Lazio, TJW .
ASTROPHYSICAL JOURNAL, 2006, 639 (01) :L25-L29
[7]   Interpreting multipoint observations of substructure at the quasi-perpendicular bow shock: Simulations [J].
Burgess, D. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2006, 111 (A10)
[8]   Simulations of electron acceleration at collisionless shocks: The effects of surface fluctuations [J].
Burgess, D. .
ASTROPHYSICAL JOURNAL, 2006, 653 (01) :316-324
[9]   Nonthermal emission from a supernova remnant in a molecular cloud [J].
Bykov, AM ;
Chevalier, RA ;
Ellison, DC ;
Uvarov, YA .
ASTROPHYSICAL JOURNAL, 2000, 538 (01) :203-216
[10]   Supernova remnants in molecular clouds [J].
Chevalier, RA .
ASTROPHYSICAL JOURNAL, 1999, 511 (02) :798-811