convection model oor Sjinees
convection model
Vertalings in die woordeboek Engels - Sjinees
对流模型
Geskatte vertalings
Vertoon algoritmies gegenereerde vertalings
voorbeelde
Advanced filtering
Voorbeelde moet herlaai word.
The experimental breakthrough curves fit well with the analytical solution of the modified convection–dispersion model.
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In addition, a modified convection–dispersion model for particle transport and deposition was developed, considering dispersive flux on the deposition kinetics.
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A method was developed for estimating the approximate initial sulfate concentration in the source layer and the redistribution time since the oxidizing event, using a semi-generic convection–dispersion model.
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The SSM serves two purposes: it provides estimates for the helium abundance and mixing length parameter by forcing the stellar model to have the correct luminosity and radius at the Sun's age, it provides a way to evaluate more complex models with additional physics, such as rotation, magnetic fields and diffusion or improvements to the treatment of convection, such as modelling turbulence, and convective overshooting.
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In fact, the only way to determine the two free parameters of the stellar evolution model, the helium abundance and the mixing length parameter (used to model convection in the Sun), are to adjust the SSM to "fit" the observed Sun.
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The results of numerical and analytical modeling show that both permeation and convection can introduce oxygen into anoxic wells to near saturation concentrations.
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The second model postulates a massive convective event at the onset of burning of an outer helium shell, causing the little remaining atmospheric Hydrogen to be turned over into the interior of the star.
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Numerical simulations of convection in a simplified model of the Yarragadee Aquifer show that: (1) the spacing of convective upwellings can be predicted from aquifer thickness and permeability anisotropy; (2) convective upwellings may be circular or elongate in plan view; (3) convective upwellings create significant temperature enhancements relative to the conductive profile; (4) convective flow rates are similar to regional groundwater flow rates; and (5) convection homogenises salinity within the aquifer.
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Using sand tank experiments and numerical models, local-scale solute-transport processes associated with free convection in both the region surrounding as well as within discrete low-permeability strata are explored.
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The forced convection ventilation design of this model ensures consistent and stable temperature.
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Projections of precipitation over tropical land regions are more uncertain than those at higher latitudes, but, despite significant inadequacies in modelling tropical convection and atmosphere-ocean interactions, and the added uncertainty associated with tropical cyclones, some robust features emerge in models.
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This illustration is taken from a model of convection in the Earth's mantle . Convective heat transfer , often referred to simply as convection , is the transfer of heat from one place to another by the movement of fluids .
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Forced convection chamber furnace NA 15/65 as table-top model
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All the process takes place by forced convection of undirected hot air.The machines roasters TMR ROASTERS MODELS have modular architecture with an external heat generating unit.
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Computer models predicted steady strengthening as the depression tracked westward before turning to the north. Of the intensity models, the Geophysical Fluid Dynamics Laboratory predicted an intensity of 135 mph (217 km/h) within 36 hours, with other forecasts being more conservative in their predictions.[10] Deep convection continued to develop to the south of the center, and the depression intensified into Tropical Storm Wilma at 0600 UTC on October 17, while located about 200 miles (320 km) southeast of Grand Cayman.
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In 1997, the existence of the core was suggested by gravitational measurements,[27] indicating a mass of from 12 to 45 times the Earth's mass or roughly 3%–15% of the total mass of Jupiter.[26] [29] The presence of a core during at least part of Jupiter's history is suggested by models of planetary formation involving initial formation of a rocky or icy core that is massive enough to collect its bulk of hydrogen and helium from the protosolar nebula . Assuming it did exist, it may have shrunk as convection currents of hot liquid metallic hydrogen mixed with the molten core and carried its contents to higher levels in the planetary interior.
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16 sinne gevind in 7 ms. Hulle kom uit baie bronne en word nie nagegaan nie.