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shows a simple model of geodynamo used for benchmark codes. The view is from center towards one of the poles, and the cones show convective flow towards higher temperature (light green to dark green with increasing velocity) in a spiraling form caused by rotation.
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Amit Chourasia1, Ashley Willis2, Maggie Avery1, Chris Davies1,3, Catherine Constable1, David Gubbins3.
1UC San Diego, 2University of Sheffield, 3University of Leeds
NSF Grants: ACI-1053575, TG-EAR130004
CC BY 3.0