Dissipation and particle energization in moderate to low beta turbulent plasma via PIC simulations

[1]  J. Birn,et al.  General magnetic reconnection, parallel electric fields, and helicity , 1988 .

[2]  V. Petrosian Stochastic Acceleration by Turbulence , 2012, 1205.2136.

[3]  K. D. Makwana,et al.  Energy dynamics and current sheet structure in fluid and kinetic simulations of decaying magnetohydrodynamic turbulence , 2014, 1412.4723.

[4]  Gang Li Identifying Current-Sheet-like Structures in the Solar Wind , 2007 .

[5]  K. Bowers,et al.  Ultrahigh performance three-dimensional electromagnetic relativistic kinetic plasma simulationa) , 2008 .

[6]  L. Davis,et al.  Large-Amplitude Alfvn Waves in the Interplanetary Medium' , 1971 .

[7]  S. Sridhar,et al.  Toward a theory of interstellar turbulence. 2. Strong Alfvenic turbulence , 1994 .

[8]  M. Hoshino,et al.  Relativistic Reconnection and Particle Acceleration , 2012 .

[9]  W. Matthaeus,et al.  MHD-driven Kinetic Dissipation in the Solar Wind and Corona , 2000 .

[10]  S. Schwartz,et al.  Universality of solar-wind turbulent spectrum from MHD to electron scales. , 2009, Physical review letters.

[11]  A. C. Fabian,et al.  Turbulent heating in galaxy clusters brightest in X-rays , 2014, Nature.

[12]  Martin J. Rees,et al.  Theory of extragalactic radio sources , 1984 .

[13]  H. Karimabadi,et al.  Coherent structures, intermittent turbulence, and dissipation in high-temperature plasmas , 2013 .

[14]  Xiaocan Li,et al.  NONTHERMALLY DOMINATED ELECTRON ACCELERATION DURING MAGNETIC RECONNECTION IN A LOW-β PLASMA , 2015, 1505.02166.