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Particle Scattering in Magnetized Plasmas and Diffusive Shock Acceleration at Perpendicular Interplanetary Shock Waves

机译:磁化等离子体中的颗粒散射,在垂直行星冲击波处散差震动加速度

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Particle scattering in pure magnetic turbulence is investigated by combining the Newton‐Lorentz equation with the well‐established nonlinear guiding center theory. Cross field diffusion coefficients are calculated as well as certain limits in particle energy and turbulence strength. In addition to the well‐known nonlinear results we find a new contribution which describes particle scattering away from a single field line. In particular, perpendicular diffusion can be described as a superposition of scattering due to wandering magnetic field lines and scattering away from a single field line. As an example, the new results are used to calculate the maximum energy of protons accelerated at perpendicular interplanetary shock waves driven by a coronal mass ejection.
机译:通过将Newton-Lorentz方程与建立良好的非线性引导中心理论相结合来研究纯磁湍流中的颗粒散射。计算横场扩散系数以及颗粒能量和湍流强度的某些限制。除了众所周知的非线性结果之外,我们还发现了一种新的贡献,该贡献描述了远离单个场线的粒子散射。特别地,由于漫长的磁场线和远离单场线散射,垂直扩散可以被描述为散射引起的散射。作为示例,新结果用于计算在由冠状大量喷射驱动的垂直行星际冲击波处加速的质子的最大能量。

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