首页> 外文会议>Proceedings of the 32nd International Cosmic Ray Conference >Charged particles time-dependent transverse transport
【24h】

Charged particles time-dependent transverse transport

机译:带电粒子的时间依赖性横向传输

获取原文
获取原文并翻译 | 示例

摘要

The temporal dependence of the perpendicular transport coefficient of charged particles in magnetostatic turbulence is studied for times smaller than the time needed to charged particles to travel the turbulence correlation length. This time window is left unexplored in most transport models. In our analysis all magnetic scales are taken to be much larger than the particle gyroradius, so that perpendicular transport is assumed to be dominated by the guiding center motion. Particle drift from the local magnetic field lines and magnetic field lines random walk are evaluated separately for slab and 3D isotropic turbulence. Contributions of wavelength scales shorter and longer than the turbulence coherence length are compared. In contrast to slab case, particles in 3D isotropic turbulence unexpectedly diffuse from local magnetic field lines; this result questions the common assumption that particle magnetization is independent on turbulence geometry. These results may have significant impact on turbulence in supernova remnant blast waves and interplanetary shocks.
机译:研究静磁湍流中带电粒子垂直传输系数的时间依赖性,其时间小于带电粒子经过湍流相关长度所需的时间。在大多数运输模型中,此时间窗口尚未开发。在我们的分析中,所有磁性尺度都被认为比粒子陀螺半径大得多,因此垂直传输被假定为由引导中心运动主导。针对平板和3D各向同性湍流,分别评估了来自局部磁场线和随机游走磁场线的粒子漂移。比较了短于和长于湍流相干长度的波长尺度的贡献。与平板情况相反,3D各向同性湍流中的粒子意外地从局部磁场线中扩散出来。这个结果质疑了粒子磁化强度与湍流几何形状无关的普遍假设。这些结果可能会对超新星残余爆炸波和行星际冲击中的湍流产生重大影响。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号