How Well Do Simplified Models Capture Complex Ocean Dynamics? A Numerical-Analytical Comparison on the Theory of a Stratified Rotating Fluid
Summary
Understanding how ocean circulation transitions between stable and oscillatory states under ther-
mal, rotational, and wind forcing remains fundamental to climate modelling. This study integrates
analytical modelling with numerical simulations to identify stability thresholds where steady cir-
culation gives way to self-sustained oscillations. We extend Maas’ low-order moment framework
to derive explicit stability criteria in non-dimensional parameter space: buoyancy forcing strength
(Ra′), rotation rate (f ′), and diffusion (μ). These predictions are tested in the Miami Isopycnic
Coordinate Ocean Model (MICOM) through systematic parameter sweeps. The numerical exper-
iments confirm the analytical predictions: increases in Ra′ or f ′ trigger limit cycle oscillations;
μ modulates stability; wind torque lowers oscillation thresholds and induces coexistence of steady
and oscillatory attractors; and bathymetry shifts but does not eliminate the propensity for oscil-
lations. Spectral analysis reveals integer harmonics generated through bilinear coupling between
fundamental modes and their higher harmonics. Our results demonstrate that low-order moment
models successfully capture the essential stability behaviour of a comprehensive ocean model across
different forcings and parameter regimes, including vertical structure response, Hopf bifurcation
thresholds, and wind-driven multi-stability.