Effects of Forcing Mechanisms on the Multiscale Properties of Magnetohydrodynamics

被引:3
|
作者
Yang, Yan [1 ]
Linkmann, Moritz [2 ,3 ]
Biferale, Luca [4 ,5 ]
Wan, Minping [1 ,6 ]
机构
[1] Southern Univ Sci & Technol, Dept Mech & Aerosp Engn, Shenzhen 518055, Peoples R China
[2] Univ Edinburgh, Sch Math, Edinburgh EH9 3FD, Midlothian, Scotland
[3] Univ Edinburgh, Maxwell Inst Math Sci, Edinburgh EH9 3FD, Midlothian, Scotland
[4] Univ Roma Tor Vergata, Dept Phys, Via Ric Sci 1, I-00133 Rome, Italy
[5] Univ Roma Tor Vergata, INFN, Via Ric Sci 1, I-00133 Rome, Italy
[6] Southern Univ Sci & Technol, Guangdong Prov Key Lab Turbulence Res & Applicat, Shenzhen 518055, Guangdong, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2021年 / 909卷 / 02期
关键词
Magnetohydrodynamics; Magnetohydrodynamical simulations; Interplanetary turbulence; SOLAR-WIND; TURBULENCE; SIMULATIONS; ALIGNMENT; SPECTRUM; FIELDS; SCALES;
D O I
10.3847/1538-4357/abdf58
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We performed numerical simulations to study the response of magnetohydrodynamics (MHD) to large-scale stochastic forcing mechanisms parameterized by one parameter, 0 <= a <= 1, going from direct injection on the velocity field (a = 1) to stirring acts on the magnetic field only (a = 0). We study the multiscale properties of the energy transfer by splitting the total flux in channels mediated by (i) the kinetic nonlinear advection, (ii) the Lorentz force, (iii) the magnetic advection, and (iv) the magnetic stretching term. We further decompose the fluxes into two subchannels given by heterochiral and homochiral components in order to distinguish forward, inverse, and flux-loop cascades. We show that there exists a quasi-singular role of the magnetic forcing mechanism for a similar to 1: a small injection on the magnetic field a < 1 can strongly deplete the mean flux of kinetic energy transfer throughout the kinetic nonlinear advection channel. We also show that this negligible mean flux is the result of a flux-loop balance between heterochiral (direct) and homochiral (inverse) transfers. Conversely, both homochiral and heterochiral channels transfer energy forward for the other three channels. Cross-exchange between velocity and the magnetic field is reversed around a = 0.4, and except when a similar to 1, we always observe that heterochiral mixed velocity-magnetic energy triads tend to move energy from magnetic to velocity fields. Our study is an attempt to further characterize the multiscale nature of MHD dynamics by disentangling different properties of the total energy transfer mechanisms, which can be useful for improving subgrid modeling.
引用
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页数:13
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