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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…
Spectral scaling laws in MHD turbulence simulations and in the solar wind
Stanislav Boldyrev, Jean Carlos Perez, Joseph E. Borovsky +1
The question is addressed to what extent incompressible magnetohydrodynamics (MHD) can describe random magnetic and velocity fluctuations measured in the solar wind. It is demonstr…
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…
Extended Scaling Laws in Numerical Simulations of MHD Turbulence
Joanne Mason, Jean Carlos Perez, Fausto Cattaneo +1
Magnetised turbulence is ubiquitous in astrophysical systems, where it notoriously spans a broad range of spatial scales. Phenomenological theories of MHD turbulence describe the s…
MHD Dynamos and Turbulence
Steven M. Tobias, Fausto Cattaneo, Stanislav Boldyrev
A review of MHD dynamos and turbulence.
Magnetic dynamo action in random flows with zero and finite correlation times
Joanne Mason, Leonid Malyshkin, Stanislav Boldyrev +1
Hydromagnetic dynamo theory provides the prevailing theoretical description for the origin of magnetic fields in the universe. Here we consider the problem of kinematic, small-scal…