Small scale structures in three-dimensional magnetohydrodynamic turbulence

dc.creatorMininni, P. D.
dc.creatorPouquet, A.
dc.creatorMontgomery, D. C.
dc.date2006-07-28
dc.date.accessioned2026-07-07T07:55:10Z
dc.date.available2026-07-07T07:55:10Z
dc.descriptionWe 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 Reynolds number.
dc.description4 pages, 3 figures
dc.identifierhttps://arxiv.org/abs/physics/0607269
dc.identifierhttp://arxiv.org/abs/physics/0607269
dc.identifierPhys. Rev. Lett. 97, 244503 (2006)
dc.identifierdoi:10.1103/PhysRevLett.97.244503
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/126877
dc.subjectFluid Dynamics
dc.subjectPlasma Physics
dc.titleSmall scale structures in three-dimensional magnetohydrodynamic turbulence
dc.typetext

Files

Collections