Rotational Dynamics of Planetary Cores: Instabilities Driven By Precession, Libration and Tides
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Publisher
Springer International Publishing
Link
http://link.springer.com/content/pdf/10.1007/978-3-030-22074-7_4
Reference82 articles.
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3. Barker, & Lithwick. (2013). Non-linear evolution of the tidal elliptical instability in gaseous planets and stars. Monthly Notices of the Royal Astronomical Society, 435(4), 3614–3626.
4. Barker, Braviner, & Ogilvie. (2016). Nonlinear tides in a homogeneous rotating planet or star: Global modes and elliptical instability. Monthly Notices of the Royal Astronomical Society, 459(1), 924–938. https://doi.org/10.1093/mnras/stw701 , arXiv:1603.06839 .
5. Bayly. (1986). Three-dimensional instability of elliptical flow. Physical Review Letters, 57(17), 2160–2163. https://doi.org/10.1103/PhysRevLett.57.2160 .
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