EGU26-21637, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-21637
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 05 May, 15:35–15:45 (CEST)
 
Room M2
Convective Organization through Gravity Waves from a Conceptual Model
Ashly Wilson and Jan Haerter
Ashly Wilson and Jan Haerter
  • University of Potsdam, Physics and Astronomy, Computational Physics, Potsdam Eiche, Germany (wilsonashly8@gmail.com)

Convective Organization through Gravity Waves from a Conceptual Model

Ashly Wilson and Jan O. Haerter

Department of Physics and Astronomy, University of Potsdam, Karl-Liebknecht Str. 24/25,

14476 Potsdam, Germany

Correspondence: Ashly Wilson (ashly.wilson@uni-potsdam.de)

Organized convection plays a crucial role in driving extreme weather events, such as

Thunderstorm clusters and tropical cyclones have far-reaching implications for human lives and

infrastructure. It is known that the global tropical circulation is mainly thermally driven (Lau

& Lim, 1982) and that diabatic heating over Earth’s continents plays a key role in

causing Walker and Hadley type circulations. It has long been postulated that tropical deep convection

might couple to different geophysical flows. In a 2D conceptual model, we here propose a two-way interaction where gravity waves can trigger new convection, whereas convection also releases gravity waves.

In our model, a convective ”kick” (in the form of momentum ) (Bretherton and Piotr Smolarkiewicz

1988) initiates gravity waves, which subsequently interact with one another by linear superposition. When a critical amplitude is exceeded, a new convective “kick” results. The physical motivation of the aforementioned convective “kick” is localized heating from convergence in the planetary boundary layer resulting from the interaction between gravity waves, which can act as a source of convection. This enhanced convection, in turn, generates new oscillations within the otherwise stratified troposphere, perpetuating the feedback cycle. The interplay of these processes is proposed as a mechanism of self-organization of convection. Boussinesq equations in the absence of the Earth’s rotation are used. Convection is modeled as a triggered function (Dirac Delta) (Da Yang, 2021).

By extending these concepts, our model provides a simplified yet insightful framework

to explore the dynamics of convective aggregation. Preliminary results suggest that the nonlinear feedback proposed can give rise to a fully-clustered convective system, similar to that seen in convective self-aggregation. Our approach opens avenues for future investigations into the role of gravity waves in

modulating large-scale atmospheric patterns and extreme weather phenomena.

​Keywords: Convective Organization, Convectively Coupled Gravity Waves, Triggered

Convection

​Abstract for oral session

How to cite: Wilson, A. and Haerter, J.: Convective Organization through Gravity Waves from a Conceptual Model, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21637, https://doi.org/10.5194/egusphere-egu26-21637, 2026.