Spherical model for turbulence

We have studied the inhomogeneous rate of the transfer of the energy flux indicating multifractal and intermittent be- haviour of solar wind turbulence in the inner heliosphere..

A chaotic cascade model for 3-D homogeneous isotropic Navier-Stokes turbulence was then proposed by Yamada and Ohkitani (1987), who modified the Gledzer model by com- plexifying

In such a set- ting, it can be computationally infeasible to perform a full similarity evaluation between the query and every database model just to identify the few most

good results, accurately predicting the transition onset, laminar seperation bubble formation and the turbulent reattachment Fig 8(b).. These flow features were not noticed in any

We present a detailed study of the collapse of a spherical perturbation in Dvali-Gabadadze-Porrati (DGP) braneworld gravity for the purpose of modeling simulation results for the

If both ends of the type II orbit are below ( above ) the thermodynamic line then the we get a warm direct ( inverse ) cascade spectrum with a point sink and the right ( left ) end

This asymptotical model for large activation energies gives the radius of the ame as the solution of a nonlinear Abel integral equation of the second type.. The analysis

While the European unemployment rate in their model increases significantly with an increase in turbulence, the unemployment rate in my model declines slightly. While in Ljungqvist