Modeling Planetary-Scale Fluid Flows in the Laboratory
Erwin Schrödinger International Institute for Mathematics and Physics (ESI) via YouTube
Overview
Syllabus
Introduction
Rotational system
Experimental observations
Equations
Polar amplification
Persistence
Ocean circulation
The opening of the Drake Passage
Oversimplified model
Fluid dynamics
Ice Albedo feedback
Tidally logged exoplanets
Experiment modification
Laboratory model
Differentially rotating planets
Future experiments
Summary
Taught by
Erwin Schrödinger International Institute for Mathematics and Physics (ESI)