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Residual Energy in Weak and Strong MHD Turbulence
Stanislav Boldyrev, Jean Carlos Perez, Yuxuan Wang
Recent numerical and observational studies revealed that spectra of magnetic and velocity fluctuations in MHD turbulence have different scaling indexes. This intriguing feature has…
Residual energy in magnetohydrodynamic turbulence and in the solar wind
Stanislav Boldyrev, Jean Carlos Perez, Vladimir Zhdankin
Recent observations indicate that kinetic and magnetic energies are not in equipartition in the solar wind turbulence. Rather, magnetic fluctuations are more energetic and have som…
Residual Energy in Magnetohydrodynamic Turbulence
Yuxuan Wang, Stanislav Boldyrev, Jean Carlos Perez
There is mounting evidence in solar wind observations and in numerical simulations that kinetic and magnetic energies are not in equipartition in magnetohydrodynamic turbulence. Th…
Strong magnetohydrodynamic turbulence with cross helicity
Jean Carlos Perez, Stanislav Boldyrev
Magnetohydrodynamics (MHD) provides the simplest description of magnetic plasma turbulence in a variety of astrophysical and laboratory systems. MHD turbulence with nonzero cross h…
Numerical simulations of imbalanced strong magnetohydrodynamic turbulence
Jean C Perez, Stanislav Boldyrev
Magnetohydrodynamics (MHD) is invoked to address turbulent fluctuations in a variety of astrophysical systems. MHD turbulence in nature is often anisotropic and imbalanced, in that…
Spectrum of weak magnetohydrodynamic turbulence
Stanislav Boldyrev, Jean Carlos Perez
Turbulence of magnetohydrodynamic waves in nature and in the laboratory is generally cross-helical or non-balanced, in that the energies of Afvén waves moving in opposite direction…