PARTICLE-ACCELERATION IN AN EVOLVING ACTIVE-REGION BY AN ENSEMBLE OF SHOCK-WAVES

被引:24
作者
ANASTASIADIS, A
VLAHOS, L
机构
[1] Department of Physics, University of Thessaloniki
关键词
ACCELERATION OF PARTICLES; SHOCK WAVES; SUN; CORONA; FLARES; MAGNETIC FIELDS;
D O I
10.1086/174290
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a model for the acceleration and transport of energetic particles (electrons and ions) inside an active region. We propose that the agent for the acceleration is an ensemble of oblique shock waves, generated inside an evolving and constantly changing active region. The acceleration is based on the ''shock drift'' mechanism, using the adiabatic treatment. The high-energy particles are losing energy via Coulomb collisions and radiation. We calculate the energy distribution of the particles, their acceleration time, and their maximum energy as a function of the number of shock waves present. The high-energy particles are transported inside a chaotic magnetic field and are reflected randomly when they meet a magnetic mirror point. Finally we compare our numerical results with the observations.
引用
收藏
页码:819 / 826
页数:8
相关论文
共 66 条
[1]  
ACHTERBERG A, 1990, ASTRON ASTROPHYS, V231, P251
[2]  
ANASTASIADIS A, 1993, ASTRON ASTROPHYS, V275, P427
[3]  
ANASTASIADIS A, 1991, ASTRON ASTROPHYS, V245, P271
[4]  
Armstrong T.P., 1985, GMS, V35, P271, DOI [10.1029/GM035p0271, DOI 10.1029/GM035P0271]
[5]   HARD X-RAY TIME PROFILES AND ACCELERATION PROCESSES IN LARGE SOLAR-FLARES [J].
BAI, T ;
RAMATY, R .
ASTROPHYSICAL JOURNAL, 1979, 227 (03) :1072-1081
[6]  
BENZ AO, 1992, LECT NOTE PHYS, V399, P106
[7]   MAGNETIC-FIELD AMPLIFICATION AND SATURATION IN 2-DIMENSIONAL MAGNETOHYDRODYNAMIC TURBULENCE [J].
BISKAMP, D ;
WELTER, H .
PHYSICS OF FLUIDS B-PLASMA PHYSICS, 1990, 2 (08) :1787-1793
[8]  
BLANDFORD RD, 1980, APJ, V237, P7931
[9]  
BLANDFORD RD, 1991, PHYS REP, V154, P1
[10]  
CARGILL PJ, 1988, ASTRON ASTROPHYS, V189, P254