Parallel and Perpendicular Diffusion Coefficients of Energetic Charged Particles with Adiabatic Focusing

被引:9
作者
Wang, J. F. [1 ]
Qin, G. [1 ]
机构
[1] Harbin Inst Technol, Sch Sci, Shenzhen 518055, Peoples R China
关键词
diffusion; magnetic fields; scattering; turbulence; COSMIC-RAY TRANSPORT; NONLINEAR PARALLEL; FLUCTUATIONS; PROPAGATION; TURBULENCE; RECOVERY;
D O I
10.3847/1538-4357/aae927
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is very important to understand stochastic diffusion of energetic charged particles in the nonuniform background magnetic field in plasmas of astrophysics and fusion devices. Using different methods considering an along-field adiabatic focusing effect, various authors derived a parallel diffusion coefficient kappa(parallel to) and its correction T to kappa(parallel to 0), where kappa(parallel to 0) is the parallel diffusion coefficient without an adiabatic focusing effect. In this paper, using the improved perturbation method developed by He & Schlickeiser and iteration process, we obtain a new correction T' to kappa(parallel to 0). Furthermore, by employing the isotropic pitch-angle scattering model D-mu mu( =) D(1-mu(2)), we find that T' has a different sign from that of T. In this paper, the spatial perpendicular diffusion coefficient kappa(perpendicular to) with the adiabatic focusing effect is also obtained.
引用
收藏
页数:10
相关论文
共 42 条
  • [21] Qin G., 2014, ApPhR, V6, P1
  • [22] Roelof E. C., 1969, LECT HIGH EN ASTR, V111
  • [23] Cosmic-ray diffusion approximation with weak adiabatic focusing
    Schlickeiser, R.
    Shalchi, A.
    [J]. ASTROPHYSICAL JOURNAL, 2008, 686 (01) : 292 - 302
  • [24] A new type of cosmic-ray anisotropy from perpendicular diffusion. I. Modification of the spatial diffusion tensor and the diffusion-convection cosmic-ray transport equation
    Schlickeiser, R.
    Dohle, U.
    Tautz, R. C.
    Shalchi, A.
    [J]. ASTROPHYSICAL JOURNAL, 2007, 661 (01) : 185 - 189
  • [25] Cosmic ray transport in non-uniform magnetic fields: consequences of gradient and curvature drifts
    Schlickeiser, R.
    Jenko, F.
    [J]. JOURNAL OF PLASMA PHYSICS, 2010, 76 : 317 - 327
  • [26] Schlickeiser R, 2002, ASTR AST LI
  • [27] Parallel and perpendicular transport of heliospheric cosmic rays in an improved dynamical turbulence model
    Shalchi, A
    Bieber, JW
    Matthaeus, WH
    Schlickeiser, R
    [J]. ASTROPHYSICAL JOURNAL, 2006, 642 (01) : 230 - 243
  • [28] Analytical investigation of the two-dimensional cosmic ray Fokker-Planck equation
    Shalchi, A
    [J]. ASTRONOMY & ASTROPHYSICS, 2006, 448 (03) : 809 - 816
  • [29] Evidence for the nonlinear transport of galactic cosmic rays
    Shalchi, A
    Schlickeiser, R
    [J]. ASTROPHYSICAL JOURNAL, 2005, 626 (02) : L97 - L99
  • [30] Nonlinear parallel and perpendicular diffusion of charged cosmic rays in weak turbulence
    Shalchi, A
    Bieber, JW
    Matthaeus, WH
    Qin, G
    [J]. ASTROPHYSICAL JOURNAL, 2004, 616 (01) : 617 - 629