The scaling properties of dissipation in incompressible isotropic three-dimensional magnetohydrodynamic turbulence -: art. no. 022301

被引:20
|
作者
Merrifield, JA [1 ]
Müller, WC
Chapman, SC
Dendy, RO
机构
[1] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
[2] Max Planck Inst Plasma Phys, D-85748 Garching, Germany
[3] UKAEA, Culham Div, Culham Sci Ctr, Abingdon OX14 3DB, Oxon, England
[4] Harvard Univ, Radcliffe Inst, Cambridge, MA 02138 USA
关键词
D O I
10.1063/1.1842133
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The statistical properties of the dissipation process constrain the analysis of large scale numerical simulations of three-dimensional incompressible magnetohydrodynamic (MHD) turbulence, such as those of Biskamp and Muller [Phys. Plasmas 7, 4889 (2000)]. The structure functions of the turbulent flow are expected to display statistical self-similarity, but the relatively low Reynolds numbers attainable by direct numerical simulation, combined with the finite size of the system, make this difficult to measure directly. However, it is known that extended self-similarity, which constrains the ratio of scaling exponents of structure functions of different orders, is well satisfied. This implies the extension of physical scaling arguments beyond the inertial range into the dissipation range. The present work focuses on the scaling properties of the dissipation process itself. This provides an important consistency check in that we find that the ratio of dissipation structure function exponents is that predicted by the She and Leveque [Phys. Rev. Lett 72, 336 (1994)] theory proposed by Biskamp and Muller. This supplies further evidence that the cascade mechanism in three-dimensional MHD turbulence is nonlinear random eddy scrambling, with the level of intermittency determined by dissipation through the formation of current sheets. (C) 2005 American Institute of Physics.
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页数:6
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