Boundary-driven MHD flux-braiding simulations at different Rm reveal Rm-dependent current sheet properties with fragmentation at high Rm consistent with plasmoid instability, supporting braiding for coronal heating.
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An a posteriori framework implemented in PyMHD estimates numerical dissipation in Alfvénic, dynamo, and MRI-driven MHD turbulence, showing it has distinct spectral and anisotropic properties from physical dissipation.
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Distribution of energy release events due to magnetic braiding
Boundary-driven MHD flux-braiding simulations at different Rm reveal Rm-dependent current sheet properties with fragmentation at high Rm consistent with plasmoid instability, supporting braiding for coronal heating.
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Characterization of Numerical Dissipation in Simulations of Magnetohydrodynamic Turbulence
An a posteriori framework implemented in PyMHD estimates numerical dissipation in Alfvénic, dynamo, and MRI-driven MHD turbulence, showing it has distinct spectral and anisotropic properties from physical dissipation.