Abstract
AbstractThe turbulence of collisionless magnetized plasmas, as observed in space, astrophysical, and magnetically confined fusion plasmas, has attracted considerable interest for a long-time. The entropy cascade in collisionless magnetized plasmas is a theoretically proposed dynamics comparable to the Kolmogorov energy cascade in fluid turbulence. Here, we present evidence of an entropy cascade in laboratory plasmas by direct visualization of the entropy distribution in the phase space of turbulence in laboratory experiments. This measurement confirms the scaling laws predicted by the gyrokinetic theory with the dual self-similarity hypothesis, which reflects the interplay between the position and velocity of ions by perpendicular nonlinear phase mixing. This verification contributes to our understanding of turbulent heating in the solar corona, accretion disks, and magnetically confined fusion plasmas.
Funder
Ministry of Science and Technology, Taiwan
Publisher
Springer Science and Business Media LLC
Subject
General Physics and Astronomy
Reference37 articles.
1. Kolmogorov, A. N. The local structure of turbulence in incompressible viscous fluid for very large Reynolds’ numbers. Dokl. Akad. Nauk SSSR 30, 301–305 (1941).
2. Kraichnan, R. H. Inertial ranges in two-dimensional turbulence. Phys. Fluids 10, 1417 (1967).
3. Champagne, F. H. The fine-scale structure of the turbulent velocity field. J. Fluid Mech. 86, 67–108 (1978).
4. Howes, G. G. et al. Gyrokinetic simulations of solar wind turbulence from ion to electron scales. Phys. Rev. Lett. 107, 035004 (2011).
5. Chen, C. H. K. et al. The evolution and role of solar wind turbulence in the inner heliosphere. ApJS 246, 53 (2020).
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