Turbulence subject to a strong background rotation

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• Peter Davidson, Engineering, Uni of Cambridge
• Thursday 10 October 2013, 11:30-12:30
• Open Plan Area, BP Institute, Madingley Rise CB3 0EZ.

If you have a question about this talk, please contact Catherine Pearson.

Turbulence subject to a strong background rotation is common in both geophysics and astrophysics, with motion in planetary cores being the most striking example. It is well known that such turbulence is dominated by the formation of long-lived columnar cyclones, and these columnar vortices control most of the large scale processes, such as mixing and magnetic field generation. However, there is still no agreement as to how these cyclones form. In this seminar we provide a partial answer to this question.

This talk is part of the Institute for Energy and Environmental Flows (IEEF) series.

This talk is included in these lists:

• All Talks (aka the CURE list)
• Cambridge Energy Seminars
• Department of Earth Sciences seminars
• Institute for Energy and Environmental Flows (IEEF)
• NanoDTC Energy Materials Talks
• Open Plan Area, BP Institute, Madingley Rise CB3 0EZ
• history
• ps635

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