Link Between the Time‐Space Behavior of Rainfall and 3D Dynamical Structures of Equatorial Waves in Global Convection‐Permitting Simulations

Abstract

Abstract Equatorial waves (EWs) control a considerable portion of tropical rainfall variability but numerical models often struggle to capture them. Increased computing power now enables global simulations with resolved deep convection, which is believed to produce more realistic EWs. Here we identify EWs in global ICON simulations with varying horizontal resolution by (a) filtering rainfall based on space‐time spectral analysis and (b) projecting wind and geopotential onto theoretical wave patterns. The simulations demonstrate that Kelvin, mixed‐Rossby gravity and equatorial Rossby waves are consistently represented, regardless of model resolution and convective treatment. For smaller‐scale inertio‐gravity waves, however, explicit convection appears to be a prerequisite. Surprisingly, the associated rainfall signals are not accompanied by corresponding wind patterns but appear to be connected to mesoscale convective systems. This demonstrates the importance of analyzing rainfall and dynamical aspects of EWs jointly for a robust assessment.

Keywords

• equatorial waves
• wave identification
• DYAMOND
• representation of convection
• space‐time filtering
• spatial projection