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Disturbance of the Front Region of Magnetic Reconnection Outflow Jets due to the Lower-Hybrid Drift Instability

机译:由于较低的混合漂移不稳定,磁力重新连接流出喷射的前部区域的干扰

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摘要

A 3D fully kinetic simulation shows that the lower-hybrid drift instability disturbs the front of magnetic reconnection outflow jets and additionally causes energy dissipation. The result is very consistent with a disturbance observed at the dipolarization front (DF) in Earth's magnetotail by the Magnetospheric Multiscale (MMS) mission. A fully kinetic dispersion relation solver, validated by the MMS observations, further predicts that the disturbance of the reconnection jet front could occur over different parameter regimes in space plasmas including Earth's DF and solar flares.
机译:3D完全动力学模拟表明,较低混合漂移不稳定性扰动磁力重新连接流出喷射器的前部,并且另外导致能量耗散。结果非常一致地通过磁磁性多尺度(MMS)使命在地球磁磁铁中的双极化前部(DF)观察到的干扰。由MMS观察验证的完全动力学色散关系求解器进一步预测,在包括地球的DF和太阳耀斑的时空等离子体中,可以在不同的参数制度上发生重新连接前沿的扰动。

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  • 来源
    《Physical review letters》 |2019年第23期|235101.1-235101.6|共6页
  • 作者单位

    Austrian Acad Sci Space Res Inst A-8042 Graz Austria;

    Nagoya Univ Inst Space Earth Environm Res Nagoya Aichi 4648601 Japan;

    Austrian Acad Sci Space Res Inst A-8042 Graz Austria;

    Beihang Univ Sch Space & Environm Beijing 100083 Peoples R China;

    Univ Calif Berkeley Space Sci Lab Berkeley CA 94720 USA;

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  • 正文语种 eng
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