Weak magnetohydrodynamic turbulence and intermittency

• Published in: Journal of fluid mechanics 2015-05, Vol.770, p.066301; 096601; 225001; 014501; 154501; 015301; 194501; 035106; 066302; 125102; 046312-066301; 096601; 225001; 014501; 154501; 015301; 194501; 035106; 066302; 125102; 046312, Article R1
• Main Authors: Meyrand, R., Kiyani, K. H., Galtier, S.
• Format: Article
• Language: English
• Subjects: Astrophysics; Fluid flow; Fluid mechanics; Intermittency; Magnetic fields; Magnetohydrodynamic turbulence; Mathematical analysis; Mathematical models; Numerical analysis; Physics; Plasma Physics; Rapids; Turbulence; Turbulent flow; Two dimensional
• ISSN: 0022-1120; 1469-7645
• DOI: 10.1017/jfm.2015.141

Three-dimensional numerical simulation is used to investigate intermittency in incompressible weak magnetohydrodynamic turbulence with a strong uniform magnetic field $\boldsymbol{b}_{\mathbf{0}}$ and zero cross-helicity. At leading order, this asymptotic regime is achieved via three-wave resonant interactions with the scattering of a wave on a 2D mode for which $k_{\Vert }=0$ . When the interactions with the 2D modes are artificially reduced, we show numerically that the system exhibits an energy spectrum with $k_{\bot }^{-3/2}$ , whereas the expected exact solution with $k_{\bot }^{-2}$ is recovered with the full nonlinear system. In the latter case, strong intermittency is found when the vector separation of structure functions is taken transverse to $\boldsymbol{b}_{\mathbf{0}}$ . This result may be explained by the influence of the 2D modes whose regime belongs to strong turbulence. In addition to shedding light on the origin of this intermittency, we derive a log-Poisson law, ${\it\zeta}_{p}=p/8+1-(1/4)^{p/2}$ , which fits the data perfectly and highlights the important role of parallel current sheets.