THE IMPLICIT CONTRIBUTION OF SLAB MODES TO THE PERPENDICULAR DIFFUSION COEFFICIENT OF PARTICLES INTERACTING WITH TWO-COMPONENT TURBULENCE

被引:8
作者
Shalchi, A. [1 ]
机构
[1] 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
diffusion; magnetic fields; turbulence; COSMIC-RAYS; CHARGED-PARTICLES; MAGNETIC-FIELD; ENERGETIC PARTICLES; NUMERICAL TEST; RANDOM-WALK; TRANSPORT; ACCELERATION; MODULATION; LINES;
D O I
10.3847/0004-637X/830/2/130
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We explore the transport of energetic particles in two-component turbulence in which the stochastic magnetic field is assumed to be a superposition of slab and two-dimensional modes. It is known that in magnetostatic slab turbulence, the motion of particles across the mean magnetic field is subdiffusive. If a two-dimensional component is added, diffusion is recovered. It was also shown before that in two-component turbulence, the slab modes do not explicitly contribute to the perpendicular diffusion coefficient. In the current paper, the implicit contribution of slab modes is explored and it is shown that this contribution leads to a reduction of the perpendicular diffusion coefficient. This effect improves the agreement between simulations and analytical theory. Furthermore, the obtained results are relevant for investigations of diffusive shock acceleration.
引用
收藏
页数:8
相关论文
共 47 条
[1]  
Abramowitz M., 1974, HDB MATH FUNCTIONS
[2]   Temporal Changes in the Rigidity Spectrum of Forbush Decreases Based on Neutron Monitor Data [J].
Alania, M. V. ;
Wawrzynczak, A. ;
Sdobnov, V. E. ;
Kravtsova, M. V. .
SOLAR PHYSICS, 2013, 286 (02) :561-576
[3]   How cosmic ray electron propagation affects radio-far-infrared correlations in M 31 and M 33 [J].
Berkhuijsen, E. M. ;
Beck, R. ;
Tabatabaei, F. S. .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 435 (02) :1598-1609
[4]   PROTON AND ELECTRON MEAN FREE PATHS - THE PALMER CONSENSUS REVISITED [J].
BIEBER, JW ;
MATTHAEUS, WH ;
SMITH, CW ;
WANNER, W ;
KALLENRODE, MB ;
WIBBERENZ, G .
ASTROPHYSICAL JOURNAL, 1994, 420 (01) :294-306
[5]   THEORETICAL EXPLANATION OF THE COSMIC-RAY PERPENDICULAR DIFFUSION COEFFICIENT IN THE NEARBY STARBURST GALAXY NGC 253 [J].
Buffie, K. ;
Heesen, V. ;
Shalchi, A. .
ASTROPHYSICAL JOURNAL, 2013, 764 (01)
[6]  
CHUVILGIN LG, 1993, ASTRON ASTROPHYS, V279, P278
[7]  
Corrsin S, 1959, ATMOSPHERIC DIFFUSIO
[8]   AN AB INITIO MODEL FOR THE MODULATION OF GALACTIC COSMIC-RAY ELECTRONS [J].
Engelbrecht, N. E. ;
Burger, R. A. .
ASTROPHYSICAL JOURNAL, 2013, 779 (02)
[9]   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)
[10]  
Fisk L. A., 1973, P 13 INT COSM RAY C, V1, P367