Particle transport through localized interactions with sharp magnetic field bends in MHD turbulence

被引:25
作者
Lemoine, Martin [1 ]
机构
[1] Sorbonne Univ, CNRS, Inst Astrophys Paris, F-75014 Paris, France
关键词
astrophysical plasmas; PITCH-ANGLE DIFFUSION; SOLAR-WIND TURBULENCE; COSMIC-RAY TRANSPORT; MAGNETOHYDRODYNAMIC TURBULENCE; CHARGED-PARTICLES; PHASE COHERENCE; ENERGETIC PARTICLES; ACCELERATION; SCATTERING; WAVES;
D O I
10.1017/S0022377823000946
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
When a particle crosses a region of space where the curvature radius of the magnetic field line shrinks below its gyroradius r(g), it experiences a non-adiabatic (magnetic moment violating) change in pitch angle. The present paper carries that observation into magnetohydrodynamic (MHD) turbulence to examine the influence of intermittent, sharp bends of the magnetic field lines on particle transport. On the basis of dedicated measurements in a simulation of incompressible turbulence, it is argued that regions of sufficiently large curvature exist in sufficient numbers on all scales to promote scattering. The parallel mean free path predicted by the power-law statistics of the curvature strength scales in proportion to r(g)(0.3) l(c)(0.7) (l(c) is the coherence scale of the turbulence), which is of direct interest for cosmic-ray phenomenology. Particle tracking in that numerical simulation confirms that the magnetic moment diffuses through localized, violent interactions, in agreement with the above picture. Correspondingly, the overall transport process is non-Brownian up to length scales greater than or similar to l(c).
引用
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页数:17
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