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首页> 外文期刊>The Astrophysical journal >Particle Acceleration In A Model Of A Turbulent Reconnecting Plasma:a Fractional Diffusion Approach
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Particle Acceleration In A Model Of A Turbulent Reconnecting Plasma:a Fractional Diffusion Approach

机译:湍流重连接等离子体模型中的粒子加速:分数扩散方法

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摘要

High-energy charged particles are produced during solar flares. These may be accelerated by the strong electric fields associated with the magnetic reconnection process which is the source of energy release in flares. A simple model of random acceleration of charged particles due to fragmented electric fields is considered for the case of a turbulent reconnecting plasma in which the fluctuating electric field is highly localized and its magnitude distributed according to power laws. The statistical properties of the acceleration process are expressed in terms of a fractional diffusion equation in velocity space, whose solution displays a power-law tail related only to the statistics of the electric field.
机译:太阳耀斑期间会产生高能带电粒子。这些可能被与磁重连过程相关的强电场所加速,而磁重连过程是火炬中能量释放的来源。对于湍流重新连接等离子体的情况,考虑了一个由碎裂电场引起的带电粒子随机加速的简单模型,在该等离子体中,波动电场高度局部化,其大小根据功率定律分布。加速过程的统计特性用速度空间中的分数扩散方程表示,该方程的解显示仅与电场统计有关的幂律尾部。

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  • 来源
    《The Astrophysical journal》 |2008年第2期|p.111-114|共4页
  • 作者

    N. H. Bian; P. K. Browning;

  • 作者单位

    Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester M13 9PL, UK;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;
  • 关键词

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