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• W2089914592 abstract "We investigate using direct numerical simulations with grids up to 1536(3) points, the rate at which small scales develop in a decaying three-dimensional MHD flow both for deterministic and random initial conditions. Parallel current and vorticity sheets form at the same spatial locations, and further destabilize and fold or roll up after an initial exponential phase. At high Reynolds numbers, a self-similar evolution of the current and vorticity maxima is found, in which they grow as a cubic power of time; the flow then reaches a finite dissipation rate independent of the Reynolds number." @default.
• W2089914592 created "2016-06-24" @default.
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• W2089914592 date "2006-12-14" @default.
• W2089914592 modified "2023-09-23" @default.
• W2089914592 title "Small-Scale Structures in Three-Dimensional Magnetohydrodynamic Turbulence" @default.
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• W2089914592 doi "https://doi.org/10.1103/physrevlett.97.244503" @default.
• W2089914592 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/17280293" @default.
• W2089914592 hasPublicationYear "2006" @default.
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