NONTHERMAL ACCELERATION FROM RECONNECTION SHOCKS

被引:15
作者
BLACKMAN, EG
FIELD, GB
机构
[1] Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138
关键词
D O I
10.1103/PhysRevLett.73.3097
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Reconnection shocks in a magnetically dominated plasma must be compressive. Nonthermal on acceleration can occur across built-in slow shocks and across outflow fast shocks when the outflow is supermagnetic and the field is line yield. Electron acceleration may be initiated by injection from the dissipation region. Reconnection and shock acceleration thus cooperate and nonthermal acceleration should be a characteristic feature. © 1994 The American Physical Society.
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页码:3097 / 3100
页数:4
相关论文
共 17 条
[1]  
[Anonymous], 1958, S INT ASTRONOMICAL U, DOI [DOI 10.1017/S0074180900237704, 10.1017/S0074180900237704]
[2]   MAGNETIC RECONNECTION [J].
BISKAMP, D .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1994, 237 (04) :179-247
[3]   MAGNETIC AND ELECTRIC-FIELD WAVES IN SLOW SHOCKS OF THE DISTANT GEOMAGNETIC TAIL - ISEE-3 OBSERVATIONS [J].
CORONITI, FV ;
MOSES, SL ;
GREENSTADT, EW ;
TSURUTANI, BT ;
SMITH, EJ .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1994, 99 (A6) :11251-11263
[4]  
EILEK JA, 1991, BEAMS JETS ASTROPHYS
[5]  
ELLISON DC, 1992, PARTICLE ACCELERATIO
[6]   SLOW-MODE SHOCKS - A SEMIPERMANENT FEATURE OF THE DISTANT GEOMAGNETIC TAIL [J].
FELDMAN, WC ;
BAKER, DN ;
BAME, SJ ;
BIRN, J ;
GOSLING, JT ;
HONES, EW ;
SCHWARTZ, SJ .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1985, 90 (NA1) :233-240
[7]   FAST-SHOCK FORMATION IN LINE-TIED MAGNETIC RECONNECTION MODELS OF SOLAR-FLARES [J].
FORBES, TG .
ASTROPHYSICAL JOURNAL, 1986, 305 (01) :553-563
[8]  
JARDINE M, 1989, ESA SP285 ESCTEC
[9]   THE PLASMA PHYSICS OF SHOCK ACCELERATION [J].
JONES, FC ;
ELLISON, DC .
SPACE SCIENCE REVIEWS, 1991, 58 (3-4) :259-346
[10]   THE GENERALIZED DIFFUSION-CONVECTION EQUATION [J].
JONES, FC .
ASTROPHYSICAL JOURNAL, 1990, 361 (01) :162-172