FRACTALS AND MULTIFRACTALS IN FLUID TURBULENCE

By Katepalli R. Sreenivasan. 1991

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Citations in the corpus

Interstellar Turbulence I: Observations and Processes (2004, result): “If the perimeter-area dimension of a projected 3D structure is the same as the perimeter-area dimension of a slice, then the ISM value of ∼ 1.4 for projected contours is consistent with analogous measures in laboratory turbulence (Sreenivasan 1991).”
Permeability‐porosity relationship: A reexamination of the Kozeny‐Carman equation based on a fractal pore‐space geometry assumption (2006, methodology): “This implies q = (2 DS)/(3 DV) ffi 1 and means that we consider random fractals with no axes of symmetry [Mandelbrot, 1983; Sreenivasan, 1991].”
Multifractality in combustion noise: predicting an impending combustion instability (2014, background): “…turbulent velocity measures are multifractal (Sreenivasan & Meneveau 1986; Meneveau & Sreenivasan 1987; Prasad, Meneveau & Sreenivasan 1988; Sreenivasan & Meneveau 1988; Meneveau & Sreenivasan 1989, 1991 to name a few pioneering studies; see Sreenivasan 1991 for an excellent review on the subject).”
PHYSICAL PROPERTIES AND GALACTIC DISTRIBUTION OF MOLECULAR CLOUDS IDENTIFIED IN THE GALACTIC RING SURVEY (2010, background): “This seemingly universal value of D, also observed in atmospheric clouds, could result from the intrinsic structure of supersonic, intermittent turbulent flows (Sreenivasan & Meneveau 1986; Meneveau & Sreenivasan 1990; Sreenivasan 1991).”
A Fractal Analysis of the H I Emission from the Large Magellanic Cloud (2000, background): “The similarity of these gas structures to the distribution of smoke particles and other passive tracers in incompressible laboratory turbulence (Sreenivasan 1991) and to the distribution of density in simulations of compressible turbulence (Elmegreen 1999 ; Rosolowsky et al. 1999 ; MacLow &…”
Coherent structures in wall-bounded turbulence (2017, methodology): “There is a well-developed theory of the intermittency associated with a singular behaviour in the limit of very high Reynolds numbers (Sreenivasan 1991), but we will use a less rigorous definition.”
Three-dimensional delayed-detonation models with nucleosynthesis for Type Ia supernovae (2012, methodology): “Following Kerstein (1988), Sreenivasan (1991) and Woosley (2007) we useD = 2.36.”