Magnetic Helicities and Dynamo Action in Magneto-rotational Turbulence

被引:4
|
作者
Bodo, G. [1 ]
Cattaneo, F. [2 ]
Mignone, A. [3 ]
Rossi, P. [1 ]
机构
[1] Osserv Astron Torino, INAF, Str Osserv 20, I-10025 Pino Torinese, Italy
[2] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
[3] Univ Turin, Dipartimento Fis, Via Pietro Giuria 1, I-10125 Turin, Italy
来源
ASTROPHYSICAL JOURNAL | 2017年 / 843卷 / 02期
基金
美国国家科学基金会;
关键词
accretion; accretion disks; dynamo; magnetohydrodynamics (MHD); turbulence; FINITE THERMAL-DIFFUSIVITY; STRATIFIED SHEARING BOXES; MAGNETOROTATIONAL TURBULENCE; DISKS; FIELD; SATURATION; MODELS; ALPHA;
D O I
10.3847/1538-4357/aa7680
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine the relationship between magnetic flux generation, taken as an indicator of large-scale dynamo action, and magnetic helicity, computed as an integral over the dynamo volume, in a simple dynamo. We consider dynamo action driven by magneto-rotational turbulence (MRT) within the shearing-box approximation. We consider magnetically open boundary conditions that allow a flux of helicity in or out of the computational domain. We circumvent the problem of the lack of gauge invariance in open domains by choosing a particular gauge-the winding gauge-that provides a natural interpretation in terms of the average winding number of pairwise field lines. We use this gauge precisely to define and measure the helicity and the helicity flux for several realizations of dynamo action. We find in these cases that the system as a whole does not break reflectional symmetry and that the total helicity remains small even in cases when substantial magnetic flux is generated. We find no particular connection between the generation of magnetic flux and the helicity or the helicity flux through the boundaries. We suggest that this result may be due to the essentially nonlinear nature of the dynamo processes in MRT.
引用
收藏
页数:10
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