Energy Dissipation in Magnetohydrodynamic Turbulence: Coherent Structures or "Nanoflares"?

Abstract

We investigate the intermittency of energy dissipation in magnetohydrodynamic (MHD) turbulence by identifying dissipative structures and measuring their characteristic scales. We find that the probability distribution of energy dissipation rates exhibits a power law tail with index very close to the critical value of -2.0, which indicates that structures of all intensities contribute equally to energy dissipation. We find that energy dissipation is uniformly spread among coherent structures with lengths and widths in the inertial range. At the same time, these structures have thicknesses deep within the dissipative regime. As the Reynolds number is increased, structures become thinner and more numerous, while the energy dissipation continues to occur mainly in large-scale coherent structures. This implies that in the limit of high Reynolds number, energy dissipation occurs in thin, tightly packed current sheets which nevertheless span a continuum of scales up to the system size, exhibiting features of both coherent structures and nanoflares previously conjectured as a coronal heating mechanism.

To appear in The Astrophysical Journal. 12 pages, 10 figures

References in corpus (2)

• Reconnection in Marginally Collisionless Accretion Disk Coronae
• Turbulent Coronal Heating Mechanisms: Coupling of Dynamics and Thermodynamics

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