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The primitive ocean model is consisted of the Navier Stokes equations for a fluid element on the surface of our rotating planet with hydrostatic balance, incompressible continuity equation, temperature equation, and salinity equation.
In the sedimentation equilibrium equation, temperature is inversely proportional to the slope of the density gradient.
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By substituting the temperature profile of the atrium in the set of temperature equations, temperature of each element has been acquired.
Using regression equations, temperature at every 10 m of depth to 50 m is estimated for seven gauged well locations as shown in Table 2.
In this paper, we consider the Navier-Stokes equations and temperature equation arising from the evolution process of the atmosphere.
In Section 2, the main results about the L 1 -stability of weak solutions to the Navier-Stokes equations and temperature equation are stated.
The scalar convection diffusion equation for temperature field is resolved by thermal LBE.
For the heat equation with temperature dependent parameters, simulation results illustrate the convergence behavior.
The adsorption energy of propene was determined by the Langmuir isotherm equation considering temperature dependency.
By substituting the phase distribution into the relevant equation, the temperature distribution can then be determined.
Findley's power law was used to model the experimental results, and extended to include an Arrhenius equation for temperature dependence of the creep response.
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