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- W2070249242 abstract "Strong incompressible three-dimensional magnetohydrodynamic turbulence is investigated by means of high-resolution direct numerical simulations. The simulations show that the configuration space is characterized by regions of positive and negative cross-helicity, corresponding to highly aligned or antialigned velocity and magnetic field fluctuations, even when the average cross-helicity is zero. To elucidate the role of cross-helicity, the spectra and structure of turbulence are obtained in imbalanced regions where cross-helicity is nonzero. When averaged over regions of positive and negative cross-helicity, the result is consistent with the simulations of balanced turbulence. An analytical explanation for the obtained results is proposed." @default.
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- W2070249242 date "2009-01-14" @default.
- W2070249242 modified "2023-09-30" @default.
- W2070249242 title "Role of Cross-Helicity in Magnetohydrodynamic Turbulence" @default.
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- W2070249242 doi "https://doi.org/10.1103/physrevlett.102.025003" @default.
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