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a,b to the shape of the tetrad given by (3c) is presented here as a model assumption. Alternatively, one could start with the pressure anisotropy tensor (defined over spherical volume of size R) and study its Lagrangian dynamics which, if the present assumption is correct, should be consistent with (3b) and (3c).
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i,jδ(t) term in (5b). It, however, plays no role as long as one works with pure inertial range, coarse-grained quantities.
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43
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These sorts of singular solutions have been earlier noted by others (e.g., Childress and Siggia - private communications).
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50
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85034536925
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note
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2 which underlies the singularity (Ref. 33).
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51
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85034532680
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note
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By ribbon, we mean configuration with two unequal stretching directions.
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2>=0. It can be easily added.
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55
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85034551531
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note
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This is not an essential approximation, and proper integration may be performed numerically.
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85034529339
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note
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3> + (3/4)<ω·S·ω>=0, which allows us to relate average energy flux to the average enstrophy production.
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61
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85034544587
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note
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The degree of alignment, of course, would vary if conditioned on σ or e as an independent variable.
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62
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85034548263
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note
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As the trajectory enters the σ<0 upper right quadrangle, matrix presented for isotropic tetrad.
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63
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85034537450
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note
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While the question of existence of finite times' singularities is still being debated, it is clear that it has to be generated by some nonlocal effect, rather than by local stretching effect (Refs. 62-66).
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64
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note
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An earlier effort to construct a stochastic generalization of RE dealt with only local gradients and resulted in a very different type of model (Ref. 68).
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85034548393
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2v(r)> "anomaly" contribution.
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72
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85034554585
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note
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Note that the "tails" here refer to the intermediate asymptotics where λ is much larger than its root-mean-square (r.m.s.) value but smaller than the characteristic large scale velocity over r. The latter condition is imposed by the bound on velocity difference PDF imposed by the single point PDF (Ref. 71).
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73
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