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How do tidal waves interact with convective vortices in rapidly-rotating planets and stars? (2022)

First Author: Dandoy V

Attributed to: Modelling turbulence induced by hydrodynamic instability in differentially-rotating flow funded by EPSRC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2211.05900

Publication URI: https://arxiv.org/abs/2211.05900

Type: Other