Coherent structures and the saturation of a nonlinear dynamo

被引:28
作者
Rempel, Erico L. [1 ]
Chian, Abraham C. -L. [1 ,2 ,3 ]
Brandenburg, Axel [4 ,5 ,6 ]
Munoz, Pablo R. [1 ]
Shadden, Shawn C. [7 ]
机构
[1] WISER, Inst Aeronaut Technol ITA, BR-12228900 Sao Jose Dos Campos, SP, Brazil
[2] CNRS, LESIA, Observ Paris, F-92190 Meudon, France
[3] WISER, Natl Inst Space Res INPE, BR-12227010 Sao Jose Dos Campos, SP, Brazil
[4] KTH Royal Inst Technol, NORDITA, SE-10691 Stockholm, Sweden
[5] Stockholm Univ, SE-10691 Stockholm, Sweden
[6] Stockholm Univ, Dept Astron, SE-10691 Stockholm, Sweden
[7] Univ Calif Berkeley, Dept Mech Engn, Berkeley, CA 94720 USA
基金
欧洲研究理事会; 美国国家科学基金会; 瑞典研究理事会; 巴西圣保罗研究基金会;
关键词
chaotic advection; dynamo theory; MHD turbulence; SOLAR ENERGETIC PARTICLES; TURBULENT DYNAMO; MAGNETIC-FIELDS; VORTEX; FLOWS; CHAOS; IDENTIFICATION; SIMULATIONS; DEFINITION; TRANSPORT;
D O I
10.1017/jfm.2013.290
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Eulerian and Lagrangian tools are used to detect coherent structures in the velocity and magnetic fields of a mean-field dynamo, produced by direct numerical simulations of the three-dimensional compressible magnetohydrodynamic equations with an isotropic helical forcing and moderate Reynolds number. Two distinct stages of the dynamo are studied: the kinematic stage, where a seed magnetic field undergoes exponential growth; and the saturated regime. It is shown that the Lagrangian analysis detects structures with greater detail, in addition to providing information on the chaotic mixing properties of the flow and the magnetic fields. The traditional way of detecting Lagrangian coherent structures using finite-time Lyapunov exponents is compared with a recently developed method called function M. The latter is shown to produce clearer pictures which readily permit the identification of hyperbolic regions in the magnetic field, where chaotic transport/dispersion of magnetic field lines is highly enhanced.
引用
收藏
页码:309 / 329
页数:21
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