Adiabatic invariants for the dynamics of rotating 3-dimensional fluid
Alexander M. Balk
TL;DR
This paper identifies three adiabatic invariants in rapidly rotating 3D fluid dynamics with beta effect, explaining energy buildup in zonal jets, which enhances understanding of planetary atmosphere behaviors.
Contribution
It introduces the concept of three adiabatic invariants in 3D rotating fluid dynamics, linking them to zonal jet formation and energy distribution.
Findings
Identification of three adiabatic invariants in the system
Explanation of energy accumulation in zonal jets
Insight into planetary atmosphere dynamics
Abstract
The 3-dimensional fluid dynamics under rapid rotation with beta effect is shown to possess three adiabatic-type invariants; their presence leading to the energy accumulation in zonal jets.
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Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Astro and Planetary Science · Fluid Dynamics and Turbulent Flows