Observations of Turbulence Generated by Magnetic Reconnection
被引:147
作者:
Eastwood, J. P.
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Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Eastwood, J. P.
[1
]
Phan, T. D.
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Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Phan, T. D.
[1
]
Bale, S. D.
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Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USAUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
Bale, S. D.
[1
,3
]
Tjulin, A.
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Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London SW7 2BW, EnglandUniv Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
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
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.