An Orchestra Without a Conductor: Slow Rossby Waves Set the Climate's Rhythm ✎

Original: "Three-dimensional slow Rossby waves in rotating spherical density stratified convection"
arXiv:1705.06207 · 2017-05-17 · arXiv non-exclusive · independent analysis · 3 min
Three-dimensional Rossby waves with periods of several years explain the observed oscillations of the Southern Oscillation.

Over the tropical Pacific, air pressure breathes with periods from two to fourteen years. The barometer on Tahiti rises while it falls in Darwin, Australia, and the entire planet's climate shudders: El Niño arrives. Meteorologists call this the Southern Oscillation and have tracked it for 138 years, but until now they couldn't answer a simple question: where do such periods come from? The classic Rossby waves usually cited as examples live no longer than a hundred days, but here we're talking years. So a different mechanism is needed.

Rossby waves are giant meanders in air currents that arise from Earth's rotation. They resemble the slow oscillations of a giant rope that some invisible hand tugs from the side. In standard theory, these waves are two-dimensional: they live only in the horizontal plane, like ripples on a pond. But the atmosphere isn't flat; it's layered: near the ground the air is dense, while at an altitude of ten kilometers it's thin, like a soufflé. This layering, or stratification, gives rise to a third type of wave: three-dimensional slow Rossby waves that move not only sideways but also upward.

Imagine an orchestra without a conductor, where each musician plays at their own tempo. Convection is the bustling violins, quickly running through their strings. And slow Rossby waves are the double basses, setting the overall rhythm several bars ahead. Without them, the orchestra would dissolve into noise, but with them, music emerges: that very multi-year climate variability.

The authors built a mathematical model of a rotating spherical atmosphere with layers of different densities. They found that three-dimensional Rossby waves can have periods from 2.5 to 14 years, exactly those observed in the Southern Oscillation index. For instance, a wave with azimuthal number m=1 and vertical scale 7.3 km yields a period of 13.88 years, while a wave with scale 16.3 km gives 3.96 years. These vertical scales are comparable to the height of the tropopause, the boundary between the lower and upper atmospheric layers, where regime changes occur.

The key point: the waves don't just exist on their own; they are excited by an instability that feeds on the thermal energy of convective motions. This is like a boiling pot of soup producing slow, large bubbles that rise to the surface amid rapid churning. Before this work, it was unclear why the Southern Oscillation spectrum shows such periods rather than chaos. Now it's clear: slow Rossby waves act like a metronome that synchronizes climate oscillations.

The Southern Oscillation index is measured by the pressure difference between Tahiti and Darwin. When pressure is high in Tahiti and low in Darwin, the ocean off Peru cools: that's La Niña. When the opposite occurs, El Niño arrives, and warm water floods the eastern Pacific. The periods of these switches range from 2 to 7 years, but longer cycles up to 14 years are also visible in the data.

Today, this theory could improve forecasting of El Niño and associated droughts, floods, and crop failures. If we understand which orchestra is playing in the atmosphere, we can predict when it will change tempo. And in the future, the same equations could help describe atmospheres of other planets, where rotation and layers of gas of varying density also exist. The orchestra without a conductor keeps playing, but now we know its score.

The periods of slow Rossby waves are comparable to the time spent in school: from 2.5 to 14 years. The Southern Oscillation Index is measured by the pressure difference between Tahiti and Darwin, and its fluctuations are visible even after smoothing over 5 months.

\omega_R^{(3D)} = \frac{8m\Omega H_\rho}{R(1+\sigma^2)}
The frequency depends on the azimuthal number m, the angular rotation rate Ω, the scale height Hρ, and the parameter σ=2kHρ
\omega_R^{(2D)} = \frac{2\Omega m}{\ell(\ell+1)}
The frequency is determined by rotation and the spherical harmonic degree ℓ
Concepts
rossby wave Southern Oscillation index El Niño-Southern Oscillation ENSO relative ONI Oceanic Niño index La Niña Kelvin wave natural variability ERSST recharge oscillator model solar wind waves Westerly wind burst decadal variability density waves spring predictability barrier Warm water volume zebiak cane model Teleconnection seasonal forcing