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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physics.plasm-ph 2years
2026 2verdicts
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New ergodicity-based ACF estimator and integral timescale methodology for solar wind turbulence claimed to eliminate artificial interval-length dependence.
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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.
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The integral and correlation scales of solar wind turbulence
New ergodicity-based ACF estimator and integral timescale methodology for solar wind turbulence claimed to eliminate artificial interval-length dependence.