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The mean-field calculations are done in a quasi-linear approximation for the turbulence, for realistic spherical geometry, with compressibihy included and using a profile of the solar internal rotation rate obtained from helioseismic inversions.
The trends of differential rotation versus stellar rotation rate obtained for simulations including the effect of the magnetic field are weaker compared with hydro simulations 0.44 in the MHD case and ΔΩ∝0.89 in the hydro case), hence showing a better agreement with the observations.
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The rotation rates of these initial models are motivated by realistic rotation rates obtained by stellar evolution calculations.
Thereafter, the equivalent azimuth beam rotation rate in Figure 2 can be obtained as follows ω r = v R c - θ 2 - θ 0 T (5).
From these coordinates, we obtain the solar rotation rate in this period.
In this work, it is shown that by controlling the solid liquid interface shape and provoking changes in the pulling to rotation rate ratio, it is possible to obtain the desired engineered domain structure, overloading problems such as the high electric field necessary for LiNbO3 domain reversal and the domain widening of the electroded area taking place in photolithographic techniques.
An exact analytic expression for the rotation rate of an anisotropic triangular particle is obtained.
Comparison between trends in effects of rotation rate, chamber pressure and reactant flow as obtained from experimental growth results and modeling computations is reported.
This work proposed new design correlations for the model parameters in terms of flow rate, rotation rate, flow properties of materials, number of blades and blade angle, obtained by means of multiple regressions.
We perform an analysis of the kinetics of grain rotation: assuming that its rate is limited by grain boundary diffusion, we obtain very good agreement between the observed and predicted rates and the rotation rate is predicted to be very sensitive to the grain size.
Reasonable fits were obtained for both models at different experimental conditions (e.g. Cu2+ bulk concentration, rotation rate).
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CEO of Professional Science Editing for Scientists @ prosciediting.com