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We present liquid sodium convection experiments in a spherical vessel, designed to model the convective state of planetary cores such as the Earth's.
It can be said that the REA can model the convective drying of sewage sludge well.
In this model, the convective parameterizations are replaced by the cloud microphysics, which is expressed in terms of GCM state variables.
In addition, to model the convective effect of flow in the duct, a uniform, unidirectional flow field is treated.
Especially, in this model, the convective heat transfer process caused by pressure difference and gravity is studied.
In this study, the REA (reaction engineering approach) is implemented for the first time to model the convective drying of sewage sludge, a highly shrinkable material.
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Numerous theoretical and experimental expressions aiming at modelling the convective heat exchange of buoyancy-driven flows along vertical surfaces have been proposed.
The system of nonlinear hyperbolic equations that models the convective transport of the fluid phases is approximated by a modified central scheme to take into account the explicit spatially discontinuous flux functions and the effects of spatially variable porosity.
In the research for this paper, a GA PNN hybrid system was used for modelling the convective heat transfer characteristics and pressure drop of TiO2 water a nanofluid in a fully developed turbulent flow based on an experimentally obtained train and test data set.
The Swift-Hohenberg (SH) equation describes the pattern formation in fluid layers confined between horizontal well-conducting boundaries, which was proposed by Swift and Hohenberg [1] as a model for the convective instability in the Rayleigh-Bénard convection.
We know that a localized one-dimensional version of the model is the local one-dimensional Swift-Hohenberg equation u_{t}=-(1+partial_{xx})^{2} u+mu u-u^{3}, (1.1) which was originally derived by Swift and Hohenberg [1] as a model for the convective instability in the Rayleigh-Bénard convection.
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