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Large-scale flows are dominated by vortical motions1 and appear to be weaker than expected in the solar interior2.
Convection and large-scale flows couple to build wreath-like global-scale magnetic structures in the stellar convection zones.
There are sometimes large-scale flows, such as when a hot star forms on the outer edge of a cold, quiescent dark molecular cloud and ionizes an H II region in its vicinity.
Nonlinear model reduction for large-scale flows is an essential component in many fluid applications such as flow control, optimization, parameter space exploration and statistical analysis.
Given the importance of turbulence in this type of large-scale flows we have used Large Eddy Simulation (LES) to incorporate it in the calculation, using a Detached Eddy Simulation (DES) approach to solve the flow near walls.
These findings may prove useful for design of lab experiments, computational studied of flows through real rock fractures, or inclusions in simulators for large-scale flows in highly fractured rocks.
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Davies, G. F. Ocean bathymetry and mantle convection 1. Large-scale flow and hotspots.
And snowy weather patterns depend on the large-scale flow of the atmosphere, which is changing, too.
Information about the large-scale flow in large columns cannot be readily obtained by direct measurements.
"Global climate models," he says, echoing Dixon, "are designed to deal with large-scale flow of the atmosphere, and they do very well with that".
Analysis of an ice rise in that ice shelf suggests an even longer period of stability of the large-scale flow regime spanning several thousands of years7.
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