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Table S2 from Characterization of columnar inertial modes in rapidly rotating spheres and spheroids.

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Version 2 2020-10-15, 10:20
Version 1 2017-07-21, 11:08
journal contribution
posted on 2017-08-07, 08:13 authored by Stefano Maffei, Andrew Jackson, Philip W. Livermore
Some values of G in the no-slip case calculated for di↵erent values of N and m for the 3-D inertial modes with the lowest vertical complexity and with the smallest (in absolute value) eigenfrequency.

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    Proceedings of the Royal Society A: Mathematical, Physical & Engineering Sciences

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    Keywords

    inertial modesquasi-geostrophyEarth's outer core

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