From the geometry of Foucault pendulum to the topology of planetary waves

Pierre Delplace; Antoine Venaille

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arXiv · 2006.08488

From the geometry of Foucault pendulum to the topology of planetary waves

Pierre Delplace·Antoine Venaille

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Abstract

The physics of topological insulators makes it possible to understand and predict the existence of unidirectional waves trapped along an edge or an interface. In this review, we describe how these ideas can be adapted to geophysical and astrophysical waves. We deal in particular with the case of planetary equatorial waves, which highlights the key interplay between rotation and sphericity of the planet, to explain the emergence of waves which propagate their energy only towards the East. These minimal ingredients are precisely those put forward in the geometric interpretation of the Foucault pendulum. We discuss this classic example of mechanics to introduce the concepts of holonomy and vector bundle which we then use to calculate the topological properties of equatorial shallow water waves.

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Pierre Delplace, Antoine Venaille. 2020-06-08. From the geometry of Foucault pendulum to the topology of planetary waves. https://arxiv.org/abs/2006.08488

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