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Cited article:

Evolution of Magnetohydrodynamic Turbulence in the Expanding Solar Wind: Residual Energy and Intermittency

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Residual Energy and Broken Symmetry in Reduced Magnetohydrodynamics

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A Three-dimensional Model for the Evolution of Magnetohydrodynamic Turbulence in the Outer Heliosphere

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Quantification of the Cross-helicity Turbulent Cascade in Compressible MHD Simulations

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Scaling of Turbulent Viscosity and Resistivity: Extracting a Scale-dependent Turbulent Magnetic Prandtl Number

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Three-dimensional local anisotropy of velocity fluctuations in the solar wind

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Can Hall Magnetohydrodynamics Explain Plasma Turbulence at Sub-ion Scales?

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Kinetic Range Spectral Features of Cross Helicity Using the Magnetospheric Multiscale Spacecraft

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Solar Wind Turbulent Cascade from MHD to Sub-ion Scales: Large-size 3D Hybrid Particle-in-cell Simulations

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Impact of Residual Energy on Solar Wind Turbulent Spectra

Trevor A. Bowen, Alfred Mallet, John W. Bonnell and Stuart D. Bale
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Influence of Intermittency on the Quasi-perpendicular Scaling in Three-dimensional Magnetohydrodynamic Turbulence

Liping Yang, Jiansen He, Chuanyi Tu, Shengtai Li, Lei Zhang, Xin Wang, Eckart Marsch and Linghua Wang
The Astrophysical Journal 846 (1) 49 (2017)
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Variance anisotropy in compressible 3‐D MHD

S. Oughton, W. H. Matthaeus, Minping Wan and Tulasi Parashar
Journal of Geophysical Research: Space Physics 121 (6) 5041 (2016)
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