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The case of a rough inner sphere results in a reduction of the critical inner rotation rate for dynamo action by a factor of 10.
The theory predicts a complicated behavior of the maximal current as a function of the diffusion layer thickness (or of the disk rotation rate for the RDE technique), with a maximum and a minimum separated by the range with an anomalous variation: increase of the maximal current with increase of the diffusion layer thickness ("autocatalytic interval").
The theory predicts a complicated behavior of the maximal current as a function of the diffusion layer thickness (or the disk rotation rate for the RDE technique), with a maximum and a minimum separated by the range with an anomalous variation: increase of the maximal current with increase of the diffusion layer thickness ("autocatalytic interval").
The latest estimate of Saturn's rotation (as an indicated rotation rate for Saturn as a whole) based on a compilation of various measurements from the Cassini, Voyager and Pioneer probes was reported in September 2007 is 10 hours, 32 minutes, 35 seconds.
A weighted linear fit to the centers of the robust Gaussian fits indicates a rotation rate for the auroral feature of ∼45±3%3% rigid corotation, as mentioned above.
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Favourable mixing was obtained at smaller impeller rotation rates for larger fills, but at larger impeller rotation rates for smaller fills.
An exact analytic expression for the rotation rate of an anisotropic triangular particle is obtained.
The average maximum increase is some 1.5-fold which corresponds to an effective rotation rate of 100 000 rpm (1667Hz) for a silent solution in order to achieve the same transport rates.
We present a convenient software tool for quickly and accurately calculating Roche lobe properties for mass ratio in the range 0.01 to 100, for Roche lobe fill-out factor in the range 0.1 to 1.0, and for dimensionless rotation rate of the star in the range 0.1 to 2.0.
A model for calculating the rotation rate of the underwater vehicle is also proposed and verified.
We perform two simulations, one for the PDE with a rotation rate of (Omega _{rm{PDE}}= 1) (left( dfrac{hbox {rotation}}{hbox {days}}right)) and a second one for the TLE with a rotation rate of (Omega_{mathrm{TLE}}= dfrac{1}{365}) (left( dfrac{hbox {rotation}}{hbox {days}}right)).
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Justyna Jupowicz-Kozak
CEO of Professional Science Editing for Scientists @ prosciediting.com