Observations of Turbulence Generated by Magnetic Reconnection

被引:147
作者
Eastwood, J. P. [1 ]
Phan, T. D. [1 ]
Bale, S. D. [1 ,3 ]
Tjulin, A. [2 ]
机构
[1] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[2] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BW, England
[3] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
关键词
LOWER-HYBRID WAVES; FIELD; DISSIPATION; BETA;
D O I
10.1103/PhysRevLett.102.035001
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Spacecraft observations of turbulence within a magnetic reconnection (guide field similar to 0) ion diffusion region are presented. In the inertial subrange, electric and magnetic fluctuations both followed a -5/3 power law; at higher frequencies, the spectral indices were -1 and -8/3, respectively. The dispersion relation was found to be consistent with fast-mode-whistler waves rather than kinetic Alfven-ion cyclotron waves. Lower hybrid waves, which could be enhanced by whistler mode conversion, were observed, but the associated anomalous resistivity was not found to significantly modify the reconnection rate.
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页数:4
相关论文
共 25 条
[21]   The onset of turbulence in collisionless magnetic reconnection [J].
Rogers, BN ;
Drake, JF ;
Shay, MA .
GEOPHYSICAL RESEARCH LETTERS, 2000, 27 (19) :3157-3160
[22]   Stochastic Fermi acceleration of subrelativistic electrons and its role in impulsive solar flares [J].
Selkowitz, R ;
Blackman, EG .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2004, 354 (03) :870-882
[23]  
Sonnerup B. U. O., 1979, MAGNETIC FIELD RECON, P47
[24]   Solar wind magnetic fluctuation spectra: Dispersion versus damping [J].
Stawicki, O ;
Gary, SP ;
Li, H .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2001, 106 (A5) :8273-8281
[25]   THEORETICAL MODELS OF MAGNETIC-FIELD LINE MERGING .1. [J].
VASYLIUNAS, VM .
REVIEWS OF GEOPHYSICS, 1975, 13 (01) :303-336