Magnetospheric Multiscale Observations of Markov Turbulence on Kinetic Scales
Wieslaw M. Macek, Dariusz Wojcik, and James L. Burch

TL;DR
This study analyzes magnetic field fluctuations in Earth's magnetosheath at kinetic scales, demonstrating that turbulence can be modeled by Markov processes, with results aligning with theoretical Fokker-Planck solutions and revealing universal scale invariance.
Contribution
It applies Markov process analysis to kinetic-scale turbulence in Earth's magnetosheath, extending previous large-scale studies and confirming the universality of turbulence characteristics across scales.
Findings
Markov processes describe turbulence at kinetic scales.
Fokker-Planck solutions match observed probability densities.
Turbulence exhibits universal scale invariance across kinetic regimes.
Abstract
In our previous studies we have examined solar wind and magnetospheric plasmas turbulence, including Markovian character on large inertial magneto-hydrodynamic scales. Here we present the results of statistical analysis of magnetic field fluctuations in the Earth's magnetosheath based on Magnetospheric Multiscale mission at much smaller kinetic scales. Following our results on spectral analysis with very large slopes of about -16/3, we apply Markov processes approach to turbulence in this kinetic regime. It is shown that the Chapman-Kolmogorov equation is satisfied and the lowest-order Kramers-Moyal coefficients describing drift and diffusion with a power-law dependence are consistent with a generalized Ornstein-Uhlenbeck process. The solutions of the Fokker-Planck equation agree with experimental probability density functions, which exhibit a universal global scale invariance through…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies · Complex Systems and Time Series Analysis
