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磁场重联中的电子加速机制的数值模拟研究 被引量:1

A NUMERICAL SIMULATION STUDY ON THE MECHANISM OF ELECTRON ACCELERATION IN MAGNETIC RECONNECTION
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摘要 在应用 2 .5维混合模拟方法研究Petschek模型磁场重联的基础上 ,考察了试验电子被加速的特征 .模拟结果表明 ,稳态的低频重联场能将少量试验电子加速到高能 ,电子的能谱为幂律谱 ,但总体分布函数未发生显著变化 .电子在整个加速过程中被束缚在低磁场的加速区内 ,由重联产生的感应电场Ey 分量对其直接加速 ,根据加速时间和加速区域可以将这些电子分为两种情况 :初始位于加速区和漂移到加速区被加速 . Based on the study of Petschek magnetic reconnection by using 2.5D hybrid simulation, the acceleration characteristics of the test electrons are inspected. The results show that a few test electrons, accelerated by the low frequency steady reconnection field, can obtain extraordinarily high energy. The energy spectrum of energetic electrons abides the power law, though no remarkable difference can be found in the velocity distribution function of electrons as a whole. The electrons are confined into an area with weak magnetic field where they are accelerated. They are accelerated directly by the E y component of electric field induced by the magnetic reconnection. Two situations of electron accelerations can be classified by the period and location. In one situation the electrons is located initially in the acceleration area, in the other elections drift into the area from somewhere else. They are both speeded up in the acceleration region.
出处 《地球物理学报》 SCIE EI CAS CSCD 北大核心 2004年第5期747-755,共9页 Chinese Journal of Geophysics
基金 国家自然科学基金 ( 4 0 1740 41 40 2 44 0 0 6) 中国科学院知识创新工程项目 (KJCX2 N0 8) 博士点基金项目 ( 2 0 0 2 0 3 5 80 19)
关键词 磁场重联 电子加速 数值模拟 混合模拟 Magnetic reconnection, Hybrid simulation, Electron acceleration.
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参考文献16

  • 1[1]Priest E R. Solar Magnetohydrodynamics. Dordrecht, Holland: D.Reidel Publ. Co., 1982
  • 2[2]Litvinenko Yu E, Somov B V. Relativistic acceleration of protons in reconnecting current sheets of solar flares. Solar Phys., 1995, 158:317
  • 3[3]Aschwanden M J, Benz A O, Dennis B R, et al. Solar electronbeams detected in hard X-rays and radio-waves( Part 1 ). Astrophysical J. , 1995, 455(1): 347 ~ 365
  • 4[4]Smith D M, Lin R P, Turin P, et al. The RHESSI spectrometer. Solar Phys., 2002, 210(1-2): 33 ~ 60
  • 5[5]Benz A O, Lin R P, Sheiner O A, et al. The source regions of impulsive solar electron events. Solar physics, 2001, 203( 1 ): 131 ~144
  • 6[6]Paesold G, Benz A O, Klein K L, et al. Spatial analysis of solar type Ⅲ events associated with narrow band spikes at metric wavelengths.Astronomy & Astophysics, 2001, 371(1): 333 ~ 342
  • 7[7]Krucker S, Larson D E, Lin R P, et al. On the origin of impulsive electron events observed at 1 AU. Astrophysical J., 1999, 519(2):864 ~ 875 Part 1
  • 8[8]Holman G D, Sui L H, Schwartz R A, et al. Electron bremsstrahlung hard X-ray spectra, electron distributions, and energetics in the 2002July 23 solar flare. Astrophysical J., 2003, 595(2): L97 ~ L101Part 2
  • 9[9]Litvinenko Yu E, Somov B V. Electron acceleration in current sheets in solar flares. Sov. Astron. Lett., 1991, 17:353
  • 10[10]Wu C S. A fast Fermi process-energetic electrons accelerated by a nearly perpendicular bow shock. J. Geophys. Res., 1984, 89:8857

同被引文献16

  • 1Somov BV,Kosugi T.Collisionless reconnection and high-energy particle acceleration in solar flares.Astrophysical Journal,1997,485(2):859~868,Part 1 AUG 20
  • 2Miller J A,Cargill P J,Emslie A G,et al.Critical issues for understanding particle acceleration in impulsive solar flares.J.Geophys.Res,1997,102A:14631~14659
  • 3Smith D M,Lin R P,Turin P,et al.The RHESSI spectrometer.Solar Phys,2002,210(1 -2):33~60
  • 4Forrest D J,Chupp E L.Simultaneous acceleration of electrons and ions in solar flares.Nature,1983,305:291
  • 5Litvinenko Yu E,Somov B V.Electron acceleration in current sheets in solar flares.Sov.Astron.Lett,1991,17:353
  • 6Parker E N.The solar flare phenomenon and the theory of reconnection and annihilation of magnetic field.Astrophys.J.Suppl.Ser,1963,8:117
  • 7Stem D P.The role of O-type neutral lines in magnetic merging during substorms and solar flares.J.Geophys.Res,1979,84:63
  • 8Wagner J S,Gray P C,Kan J R,et al.Particle dynamics in reconnection field configurations.Planet.Space Sci,1981,29:391
  • 9Litvinenko Yu E,Smov B V.Relativistic acceleration of protons in reconnecting current sheets of solar flares.Solar Phys,1995,158:317
  • 10Drake J F,Shay M A,Thongthai W,et al.Production of energetic electrons during magnetic reconnection.Physical Review Letters,2005,94 (9):Art.No.095001,Mar11

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