Thermal conduction in magnetized turbulent gas

被引:80
作者
Cho, J
Lazarian, A
Honein, A
Knaepen, B
Kassinos, S
Moin, P
机构
[1] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA
[2] Stanford Univ, Ctr Turbulence Res, Stanford, CA 94305 USA
关键词
galaxies : clusters : general; ISM : general; MHD; turbulence;
D O I
10.1086/376492
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using numerical methods, we systematically study in the framework of ideal MHD the effect of magnetic fields on heat transfer within a turbulent gas. We measure the rates of passive scalar diffusion within magnetized fluids and make the comparisons (1) between MHD and hydrodynamic simulations, (2) between different MHD runs with different values of the external magnetic field (up to the energy equipartition value), and (3) between thermal conductivities parallel and perpendicular to the magnetic field. We do not find apparent suppression of diffusion rates by the presence of magnetic fields, which implies that magnetic fields do not suppress heat diffusion by turbulent motions.
引用
收藏
页码:L77 / L80
页数:4
相关论文
共 18 条
[1]  
BEGELMAN MC, 1990, MNRAS, V244, P26
[2]   The thermal pressure of the hot interstellar medium derived from cloud shadows in the extreme ultraviolet [J].
Berghofer, TW ;
Bowyer, S ;
Lieu, R ;
Knude, J .
ASTROPHYSICAL JOURNAL, 1998, 500 (02) :838-846
[3]   Relative dispersion in fully developed turbulence: The Richardson's law and intermittency corrections [J].
Boffetta, G ;
Sokolov, IM .
PHYSICAL REVIEW LETTERS, 2002, 88 (09) :4
[4]   Simulations of magnetohydrodynamic turbulence in a strongly magnetized medium [J].
Cho, J ;
Lazarian, A ;
Vishniac, ET .
ASTROPHYSICAL JOURNAL, 2002, 564 (01) :291-301
[5]   On the soft X-ray spectrum of cooling flows [J].
Fabian, AC ;
Mushotzky, RF ;
Nulsen, PEJ ;
Peterson, JR .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 321 (01) :L20-L24
[6]   COOLING FLOWS IN CLUSTERS OF GALAXIES [J].
FABIAN, AC .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1994, 32 :277-318
[7]   TOWARD A THEORY OF INTERSTELLAR TURBULENCE .2. STRONG ALFVENIC TURBULENCE [J].
GOLDREICH, P ;
SRIDHAR, S .
ASTROPHYSICAL JOURNAL, 1995, 438 (02) :763-775
[8]  
ISHIHARA T, 2001, APS M DFD01
[9]   A high-order WENO finite difference scheme for the equations of ideal magnetohydrodynamics [J].
Jiang, GS ;
Wu, CC .
JOURNAL OF COMPUTATIONAL PHYSICS, 1999, 150 (02) :561-594
[10]   Reconnection in a weakly stochastic field [J].
Lazarian, A ;
Vishniac, ET .
ASTROPHYSICAL JOURNAL, 1999, 517 (02) :700-718