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Thus, for a complete understanding of the turbulence effect of the incident wind on the fluctuations of the roof-corner surface pressures, the incident wind needs to be considered as a three-dimensional velocity vector, as it is in reality.
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As concrete examples, we consider the stochastic equations for the Maxwell and Oldroyd fluids that are of great importance in the investigation towards the understanding of the elastic turbulence.
Such approach in the mathematical investigation for the understanding of the Newtonian turbulence phenomenon was pioneered by Bensoussan and Temam in [5] where they studied the Stochastic Navier-Stokes Equation (SNSE).
Large Volume Plasma Device (LVPD) has been successfully contributing towards understanding of the plasma turbulence driven by Electron Temperature Gradient (ETG), considered as a major contributor for the plasma loss in the fusion devices.
The major problem that remains to be resolved involves the understanding of the effect of turbulence on the cellular detonation structure, the propagation of high-speed deflagrations and the transition from deflagration to detonations.
Direct numerical simulations play an important role in both the understanding of compressible turbulence dynamics and the calibration of turbulence closure models.
This paper, dedicated to Norbert Peters, follows his lead in developing theoretical understanding of the complex flow-turbulence interactions occurring in the propagation of premixed flames.
The understanding of the wave activities and turbulence processes in the Venus magnetosheath will also enable us to predict the possible conditions in the terrestrial magnetosphere when the magnetic field is weak.
The knowledge of the kinetic of reactions, the understanding of the synergistic interaction between turbulence and combustion, and the likelihood of transition to extreme events such as detonation, are the necessary steps for engineering purposes, and in particular for the sound design of prevention and protective measures.
These results contribute to the understanding of the limiting factor effects of flow turbulence on algal production that can inform the optimization of the benthic algal cultivation.
The present work aims to develop a better understanding of wave and turbulence processes in the planetary magnetosheath region.
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