NUMERICAL TEST OF DIFFERENT APPROXIMATIONS USED IN THE TRANSPORT THEORY OF ENERGETIC PARTICLES

被引:10
作者
Qin, G. [1 ]
Shalchi, A. [2 ]
机构
[1] Harbin Inst Technol, Shenzhen 518055, Peoples R China
[2] Univ Manitoba, Dept Phys & Astron, Winnipeg, MB R3T 2N2, Canada
基金
加拿大自然科学与工程研究理事会;
关键词
cosmic rays; diffusion; turbulence; PERPENDICULAR DIFFUSION; CHARGED-PARTICLES; MAGNETIC-FIELD; TURBULENCE; MODULATION; ACCELERATION; COEFFICIENTS; RECOVERY;
D O I
10.3847/0004-637X/823/1/23
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Recently developed theories for perpendicular diffusion work remarkably well. The diffusion coefficients they provide agree with test-particle simulations performed for different turbulence setups ranging from slab and slab-like models to two-dimensional and noisy reduced MHD turbulence. However, such theories are still based on different analytical approximations. In the current paper we use a test-particle code to explore the different approximations used in diffusion theory. We benchmark different guiding center approximations, simplifications of higher-order correlations, and the Taylor-Green-Kubo formula. We demonstrate that guiding center approximations work very well as long as the particle's unperturbed Larmor radius is smaller than the perpendicular correlation length of the turbulence. Furthermore, the Taylor-Green-Kubo formula and the definition of perpendicular diffusion coefficients via mean square displacements provide the same results. The only approximation that was used in the past in nonlinear diffusion theory that fails is to replace fourth-order correlations by a product of two second-order correlation functions. In more advanced nonlinear theories, however, this type of approximation is no longer used. Therefore, we confirm the validity of modern diffusion theories as a result of the work presented in the current paper.
引用
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页数:7
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共 36 条
[1]   Cosmic Ray 11-Year Modulation for Sunspot Cycle 24 [J].
Ahluwalia, H. S. ;
Ygbuhay, R. C. .
SOLAR PHYSICS, 2015, 290 (02) :635-643
[2]   NUMERICAL ANALYSIS OF THE FOKKER-PLANCK EQUATION WITH ADIABATIC FOCUSING: ISOTROPIC PITCH-ANGLE SCATTERING [J].
Danos, Rebecca J. ;
Fiege, Jason D. ;
Shalchi, Andreas .
ASTROPHYSICAL JOURNAL, 2013, 772 (01)
[3]   Diffusive shock acceleration at interplanetary perpendicular shock waves: Influence of the large scale structure of turbulence on the maximum particle energy [J].
Dosch, A. ;
Shalchi, A. .
ADVANCES IN SPACE RESEARCH, 2010, 46 (09) :1208-1217
[4]   Cosmic-Ray Modulation: an Ab Initio Approach [J].
Engelbrecht, N. E. ;
Burger, R. A. .
BRAZILIAN JOURNAL OF PHYSICS, 2014, 44 (05) :512-519
[5]   COSMIC RAY ACCELERATION AT PERPENDICULAR SHOCKS IN SUPERNOVA REMNANTS [J].
Ferrand, Gilles ;
Danos, Rebecca J. ;
Shalchi, Andreas ;
Safi-Harb, Samar ;
Edmon, Paul ;
Mendygral, Peter .
ASTROPHYSICAL JOURNAL, 2014, 792 (02)
[6]   TOWARD A THEORY OF INTERSTELLAR TURBULENCE .2. STRONG ALFVENIC TURBULENCE [J].
GOLDREICH, P ;
SRIDHAR, S .
ASTROPHYSICAL JOURNAL, 1995, 438 (02) :763-775
[7]   BROWNIAN MOTION IN A GAS OF NONINTERACTING MOLECULES [J].
GREEN, MS .
JOURNAL OF CHEMICAL PHYSICS, 1951, 19 (08) :1036-1046
[8]   The influence of different turbulence models on the diffusion coefficients of energetic particles [J].
Hussein, M. ;
Tautz, R. C. ;
Shalchi, A. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2015, 120 (06) :4095-4111
[9]   COSMIC-RAY PROPAGATION .1. CHARGED PARTICLES IN A RANDOM MAGNETIC FIELD [J].
JOKIPII, JR .
ASTROPHYSICAL JOURNAL, 1966, 146 (02) :480-&