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