Turbulence in Magnetic Reconnection Jets from Injection to Sub-Ion Scales

被引:1
|
作者
Richard, Louis [1 ,2 ]
Sorriso-Valvo, Luca [1 ,3 ,4 ]
Yordanova, Emiliya [1 ]
Graham, Daniel B. [1 ]
Khotyaintsev, Yuri, V [1 ]
机构
[1] Swedish Inst Space Phys, S-75121 Uppsala, Sweden
[2] Uppsala Univ, Dept Phys & Astron, Space & Plasma Phys, S-75120 Uppsala, Sweden
[3] CNR ISTP Ist Sci & Tecnol Plasmi, I-70126 Bari, Italy
[4] KTH Royal Inst Technol, Sch Elect Engn & Comp Sci, Space & Plasma Phys, S-11428 Stockholm, Sweden
基金
瑞典研究理事会;
关键词
SOLAR-WIND TURBULENCE; ASTROPHYSICAL GYROKINETICS; PLASMA TURBULENCE; FLUX ROPES; CASCADE; WAVES; ACCELERATION; CONSEQUENCES; DISSIPATION; HYPOTHESIS;
D O I
10.1103/PhysRevLett.132.105201
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We investigate turbulence in magnetic reconnection jets in the Earth's magnetotail using data from the Magnetospheric Multiscale spacecraft. We show that signatures of a limited inertial range are observed in many reconnection jets. The observed turbulence develops on the timescale of a few ion gyroperiods, resulting in intermittent multifractal energy cascade from the characteristic scale of the jet down to the ion scales. We show that at sub-ion scales, the fluctuations are close to monofractal and predominantly kinetic Alfve ' n waves. The observed energy transfer rate across the inertial range is similar to 108 J kg-1 s-1, which is the largest reported for space plasmas so far.
引用
收藏
页数:7
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