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Structure of Current Sheets with Quasi-Adiabatic Dynamics of Particles in the Solar Wind

机译:太阳风中颗粒的准绝热动力学的现有纸张结构

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摘要

Within the self-consistent hybrid model based on the quasi-adiabatic approximation of the proton dynamics, a fine structure of strong current sheets (SCSs) in the solar wind has been investigated, including the heliospheric current sheet. The motion of electrons is fast and considered in the Boltzmann approximation. The simulation results have been shown that the SCS profiles have a multiscale enclosed structure with a narrow central current sheet that is enclosed in a wider sheet, similar to the heliospheric current sheet surrounded by the plasma sheet. The features of the SCS structure are determined by the relative contributions of the current of demagnetized protons in serpentine orbits and drift currents of electrons. The model predicts and describes the properties of SCSs observed by spacecraft. It has been shown that the multiscale structure of current sheets is an inherent intrinsic property of current sheets in the solar wind.
机译:在基于质子动力学的准绝热近似的自一致的混合模型中,研究了太阳风中的强电流纸张(SCS)的精细结构,包括螺旋镜电流板。电子的运动是快速的,并且在Boltzmann近似中考虑。已经示出了模拟结果,SCS型材具有多尺度封闭结构,其具有窄的中央电流片,其封闭在更宽的薄片中,类似于等离子体片材围绕的螺旋体电流片。 SCS结构的特征由蛇形轨道中的偏磁质子的电流和电子的漂移电流的电流的相对贡献决定。该模型预测并描述了航天器观察到的SCS的特性。已经表明,当前纸张的多尺度结构是太阳风中当前纸张的固有的固有特性。

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  • 来源
    《Cosmic research》 |2018年第6期|462-470|共9页
  • 作者单位

    Moscow MV Lomonosov State Univ Skobeltsyn Inst Nucl Phys Moscow 119992 Russia|Russian Acad Sci Space Res Inst Moscow 117997 Russia;

    Russian Acad Sci Space Res Inst Moscow 117997 Russia|Moscow MV Lomonosov State Univ Fac Phys Moscow 119991 Russia|Natl Res Univ Higher Sch Econ Moscow 101000 Russia;

    Russian Acad Sci Pushkov Inst Terr Magnetism Ionosphere & Radio Wa Troitsk 142092 Moscow Oblast Russia;

    Russian Acad Sci Space Res Inst Moscow 117997 Russia|St Petersburg State Univ St Petersburg 199034 Russia;

    Russian Acad Sci Space Res Inst Moscow 117997 Russia;

    Russian Acad Sci Space Res Inst Moscow 117997 Russia;

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