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Rotating Fluids

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Fluid Dynamics

Part of the book series: Graduate Texts in Physics ((GTP))

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Abstract

The most spectacular effect of rotation on a fluid flow is certainly the huge hurricanes surging up in the Earth’s atmosphere when the waters of the ocean are warm enough. These huge flows, so typical in pictures of the Earth, would not exist if the Earth were not rotating. They owe their existence to the Coriolis acceleration.

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Notes

  1. 1.

    See Longuet-Higgins (1964).

  2. 2.

    A detailed discussion of this question may be found in Greenspan (1969).

  3. 3.

    We recall that we set χ proportional to \(e^{i(\omega t+m\varphi )}\).

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Rieutord, M. (2015). Rotating Fluids. In: Fluid Dynamics. Graduate Texts in Physics. Springer, Cham. https://doi.org/10.1007/978-3-319-09351-2_8

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