Towards a theoretical understanding of Arctic amplification dynamics

This paper develops a theoretical framework for understanding Arctic amplification through the lens of nonlinear potential vorticity (PV) dynamics, static stability feedbacks, and stratosphere-troposphere coupling. Using scaling arguments, Green’s function solutions, and a modified Eady model, we show how surface-warming-induced static stability perturbations modulate PV inversion efficiency and extend remote influences. We identify a critical threshold in the diabatic number D D that marks the transition from a dry-nonlinear to a moist-nonlinear regime where diabatic PV generation outweighs baroclinic advection. A regime diagram constructed from the nonlinearity ratio R=| σ ^ /σ ̄| R = ∣ σ ′ / σ ¯ ∣ (where σ is static stability) and D D reveals four quadrants; the Arctic already resides in a nonlinear background ( R > 0.3 R > 0 . 3 for most CMIP6 models) and under continued warming, it migrates vertically into the moist-nonlinear state via increasing D D . Under SSP2-4.5, the ensemble-mean D D crosses the 0.03 threshold by mid-century ( D=0.031 D = 0 . 031 ); under SSP5-8.5, D D reaches 0.039 by end-century, with 88% of models exceeding the threshold. Reduced stability amplifies baroclinic growth rates and shifts most unstable modes toward high-latitude blocking wavelengths. Extending the framework to the stratosphere, we show that the refractive index for vertically propagating Rossby waves decreases with weakened zonal winds, a robust signal across models, enabling deeper wave penetration. Observational support from ERA5 reanalysis reveals a vertical contrast in PV anomalies - strong positive anomalies in the lower troposphere and a wave-like pattern aloft, consistent with the transition to diabatically driven dynamics. A positive feedback loop linking surface warming, reduced stability, enhanced inversion efficiency, amplified streamfunction anomalies, increased poleward heat transport, and strengthened vertical wave coupling suggests a loop gain that would be arrested by nonlinear saturation. These results establish polar amplification as arising from coupled interactions of static stability, PV dynamics, diabatic heating, and stratosphere-troposphere coupling, with direct implications for predicting midlatitude extreme weather events.