Servidio S, Haynes C T, Matthaeus W H, Burgess D, Carbone V, Veltri P
Dipartimento di Fisica, Università della Calabria, I-87036 Cosenza, Italy.
School of Physics and Astronomy, Queen Mary University of London, Mile End Road, London E1 4NS, United Kingdom.
Phys Rev Lett. 2016 Aug 26;117(9):095101. doi: 10.1103/PhysRevLett.117.095101. Epub 2016 Aug 24.
Particle dynamics are investigated in plasma turbulence, using self-consistent kinetic simulations, in two dimensions. In the steady state, the trajectories of single protons and proton pairs are studied, at different values of plasma β (ratio between kinetic and magnetic pressure). For single-particle displacements, results are consistent with fluids and magnetic field line dynamics, where particles undergo normal diffusion for very long times, with higher β's being more diffusive. In an intermediate time range, with separations lying in the inertial range, particles experience an explosive dispersion in time, consistent with the Richardson prediction. These results, obtained for the first time with a self-consistent kinetic model, are relevant for astrophysical and laboratory plasmas, where turbulence is crucial for heating, mixing, and acceleration processes.
利用二维自洽动力学模拟研究了等离子体湍流中的粒子动力学。在稳态下,研究了单个质子和质子对在不同等离子体β值(动压与磁压之比)下的轨迹。对于单粒子位移,结果与流体和磁力线动力学一致,其中粒子在很长时间内经历正常扩散,β值越高扩散性越强。在中间时间范围内,当间距处于惯性范围时,粒子在时间上经历爆炸性扩散,这与理查森预测一致。这些首次通过自洽动力学模型获得的结果与天体物理和实验室等离子体相关,在这些等离子体中,湍流对于加热、混合和加速过程至关重要。