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Fig. 1 Snapshot from dynamo model 4: a radial magnetic field (B_r) (in colors) and the tangential flow (vec {u}_h) (black arrows).
Fig. 6 Intense high-latitude normal polarity magnetic flux patch (HN) in dynamo model 1 (Fig. 5): radial magnetic field B r (colors) and the tangential flow (vec {u}_{h}) (arrows) at a mid-depth and at b the top of the free stream just below the Ekman boundary layer.
Fig. 5 A snapshot from dynamo model 1: radial magnetic field B r (colors) and the tangential flow (vec {u}_{h}) (arrows) at a mid-depth and at b the top of the free stream just below the Ekman boundary layer.
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We decomposed the tangential flow into toroidal and poloidal parts using ({vec u_{text {tor}}}= nabla times mathcal {T} hat {r}) and ({vec u_{text {pol}}}= nabla _{h} mathcal {P}), where (mathcal {T}) and (mathcal {P}) are the respective flow potentials.
Under such conditions, the tangential flow is purely toroidal.
The tangential flow was turbulent.
The tangential flow is dominantly toroidal, and the radial component of the flow is only 0.62 of the tangential component.
The toroidal flow dominates over the poloidal, and the tangential flow dominates over the radial.
The fluid flow in hydraulic fractures can be divided into two major types: tangential flow and normal flow, Fig. 3.
The tangential flow has a large field-aligned component which produces a weak Ad h (Fig. 8e).
The following are the conditions for solving the temperature: cylindrical, implicit method, convection, and conduction while ignoring tangential flow.
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