Local Anisotropy, Higher Order Statistics, and Turbulence Spectra
W. H. Matthaeus, S. Servidio, P. Dmitruk, V. Carbone, S. Oughton, M., Wan, and K. T. Osman

TL;DR
This paper investigates the emergence of local correlation anisotropy in magnetohydrodynamics, revealing its connection to higher order statistics and its implications for turbulence spectra in space and astrophysical plasmas.
Contribution
It demonstrates that local anisotropy is intensified with localized mean fields and links this phenomenon to higher order correlations, challenging traditional interpretations of turbulence spectra.
Findings
Local anisotropy is stronger in localized mean field estimates.
Sensitivity of local anisotropy to phase randomization links it to higher order correlations.
Local structure functions do not directly measure the energy spectrum.
Abstract
Correlation anisotropy emerges dynamically in magnetohydrodynamics (MHD), producing stronger gradients across the large-scale mean magnetic field than along it. This occurs both globally and locally, and has significant implications in space and astrophysical plasmas, including particle scattering and transport, and theories of turbulence. Properties of local correlation anisotropy are further documented here by showing through numerical experiments that the effect is intensified in more localized estimates of the mean field. The mathematical formulation of this property shows that local anisotropy mixes second-order with higher order correlations. Sensitivity of local statistical estimates to higher order correlations can be understood in connection with the stochastic coordinate system inherent in such formulations. We demonstrate this in specific cases, illustrate the connection to…
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