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• W1996829340 abstract "We consider freely decaying, statistically axisymmetric turbulence evolving in the presence of a background rotation, an imposed stratification or a uniform magnetic field. We focus on the case of Saffman turbulence in which E ( k → 0) ~ k 2 and show that, if the large scales evolve in a self-similar manner, then u ⊥ 2 ℓ ⊥ 2 ℓ ∥ = constant in rotating, stratified and magnetohydrodynamic turbulence. This may be contrasted with E ( k → 0) ~ k 4 turbulence, in which u ⊥ 2 ℓ ⊥ 4 ℓ ∥ ≈ constant. (Here the subscripts ⊥ and ∥ indicate directions perpendicular and parallel to the axis of symmetry, and ℓ ⊥ , ℓ ∥ and u ⊥ are suitably defined integral scales.) This constraint on the integral scales allows us to make simple, testable predictions for the temporal evolution of ℓ ⊥ , ℓ ∥ and u ⊥ in all three systems. There are only limited data sets against which to compare these predictions, but they are consistent with those data which are currently available." @default.
• W1996829340 created "2016-06-24" @default.
• W1996829340 creator A5026897833 @default.
• W1996829340 date "2010-08-23" @default.
• W1996829340 modified "2023-10-16" @default.
• W1996829340 title "On the decay of Saffman turbulence subject to rotation, stratification or an imposed magnetic field" @default.
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• W1996829340 doi "https://doi.org/10.1017/s0022112010003496" @default.
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