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First, the upstream and downstream parts of the system are shown to exhibit the ISS property with respect to certain boundary input terms governed by the core flow in the vicinity of the bluff body.
Fig. 11 Quasi-geostrophic core flow in 2015 to degree 16, derived from the CHAOS-6 magnetic field to degree 13, and secular variation to degree 16, following the method of Gillet et al.
Kinetic energy is derived from thermo-compositional convection of an electrically conducting fluid although mechanical mechanisms, such as libration and precession, may also drive core flow in smaller bodies (e.g., Le Bars et al. 2015).
The experiment procedures consist of first establishing a stable oil water core flow in the horizontal test section of the facility by introducing into the pipe, through a 'T-Junction' inlet, oil and water with superficial oil and water velocities of 0.4 0.5 m/s and 0.2 m/s, respectively.
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When decane saturation in the core was above residual saturation, decane volatilization occurred near the inlet, the relative decane saturation throughout the core dropped uniformly, and decane in the core flowed in the liquid phase to the shell to replenish volatilized decane.
We note the detailed implementation of the technique and evidence for the usefulness of core flows in secular variation forecasting is given in Whaler and Beggan (2015).
In this paper, the results of core flow experiments in limestone formations are presented.
These responses can be used to better understand the core flow and, in particular, to improve accuracies of predicting geomagnetic variability in the future.
Enameled steel, stainless steel with 2.5 μm roughness, oxidized polymers or oxidized commercial steel can all be used to better the effectiveness of core-flow in the transportation of heavy oils.
The operation of oil production or transportation line in the core flow mode consists in injecting small amounts of water to create a lubrication layer around the viscous oil and avoid oil wall contact.
As the core flow is plausibly in the TG balance over a large area of the core surface, a majority of the non-geostrophic SV should not originate from the advection of radial MF by the ageostrophic flow.
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