Multi-shell models of celestial bodies with an intermediate layer of fluid: dynamics in the case of the large values of the ekman number

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SUMMARY

    In the theory of the rotating mass of liquid, the key role plays Ekman number, which reads µ E=. ωrot ρ f R2c Here, ωrot is the characteristic angular velocity of system`s components, Rc is the characteristic size (e_g, the radius of the outer boundary of the liquid layer), ρ f is the density of the liquid, and µ is the liquid`s viscosity. In the best part of the studies the motion of the bounding surfaces was assumed to be known, and the effect the liquid invokes on their dynamics was not studied (e_g,). In, F . . .

     

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