Scale dependence of energy transfer in turbulent plasma
Yan Yang, Minping Wan, William H. Matthaeus, Luca Sorriso-Valvo,, Tulasi N. Parashar, Quanming Lu, Yipeng Shi, Shiyi Chen

TL;DR
This paper investigates how different measures of energy transfer in turbulent plasma vary with scale, revealing that they are concentrated near each other but dominate at different scales, with implications for understanding plasma heating.
Contribution
It provides a scale-dependent analysis of multiple energy transfer proxies in turbulent plasma, highlighting their spatial correlation and scale-specific dominance.
Findings
Energy dissipation proxies are spatially close but decorrelate over a few ion inertial lengths.
Different proxies dominate at different scales, with large scales for electromagnetic work and small scales for pressure-strain.
The third-order law applies mainly within the inertial range of turbulence.
Abstract
In the context of space and astrophysical plasma turbulence and particle heating, several vocabularies emerge for estimating turbulent energy dissipation rate, including Kolmogorov-Yaglom third-order law and, in its various forms, (work done by the electromagnetic field on particles), and (pressure-strain interaction), to name a couple. It is now understood that these energy transfer channels, to some extent, are correlated with coherent structures. In particular, we find that different energy dissipation proxies, although not point-wise correlated, are concentrated in proximity to each other, for which they decorrelate in a few (s). However, the energy dissipation proxies dominate at different scales. For example, there is an inertial range over which the third-order law is…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Magnetic confinement fusion research
