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 BPI Seminar Series series.

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• Cambridge Energy Seminars
• NanoDTC Energy Materials Talks
• Open Plan Area, BP Institute, Madingley Rise CB3 0EZ
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