1992
DOI: 10.1017/s0022112092002180
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The energy decay in self-preserving isotropic turbulence revisited

Abstract: The assumption of self-preservation permits an analytical determination of the energy decay in isotropic turbulence. Batchelor (1948), who was the first to carry out a detailed study of this problem, based his analysis on the assumption that the Loitsianskii integral is a dynamic invariant – a widely accepted hypothesis that was later discovered to be invalid. Nonetheless, it appears that the self-preserving isotropic decay problem has never been reinvestigated in depth subsequent to this earlier work. In the … Show more

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Cited by 113 publications
(93 citation statements)
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“…This is a more robust type of similarity von Kármán self-preservation for magnetohydrodynamic turbulence 301 decay, originally suggested by von Kármán & Lin (1949). Also, see Speziale & Bernard (1992) for a discussion of the so-called 'partial' similarity solutions versus the 'complete' similarity solutions in which the viscous term is retained.…”
mentioning
confidence: 85%
“…This is a more robust type of similarity von Kármán self-preservation for magnetohydrodynamic turbulence 301 decay, originally suggested by von Kármán & Lin (1949). Also, see Speziale & Bernard (1992) for a discussion of the so-called 'partial' similarity solutions versus the 'complete' similarity solutions in which the viscous term is retained.…”
mentioning
confidence: 85%
“…Most of these investigations have focused on decaying isotropic turbulence (e.g. von Kármán & Howarth 1938;Batchelor 1948;George 1992;Speziale & Bernard 1992) or homogeneous shear Two-point similarity in the round jet 311 turbulence (e.g. George & Gibson 1992).…”
Section: Introductionmentioning
confidence: 99%
“…Estimates on the energy decay law for the 3D Euler equations are rare (see ref. 25 and references therein). Moreover, all the estimates concern the infinite space case while we use periodic boundary conditions.…”
Section: Numerical Resultsmentioning
confidence: 99%
“…Moreover, all the estimates concern the infinite space case while we use periodic boundary conditions. For the infinite space case, under the assumption of complete self-preservation, i.e., selfsimilarity for all scales from 0 to ϱ, one finds that the energy should decay as t Ϫ1 (25). If the assumption of complete selfpreservation is not satisfied, the energy is expected to decay as t Ϫ␣ , where ␣ Ͼ 1.…”
Section: Numerical Resultsmentioning
confidence: 99%