Idealized Cumulus Cloud-Scale Motions and the Dynamics of Isolated and Coupled Flows
Dario P. Falcone, Matthew R. Igel, Joseph A. Biello

TL;DR
This paper introduces the KRoNUT and DoNUT models to analyze cloud-scale motions, revealing how different forcings influence cloud morphology and interactions, providing new insights into cloud dynamics and stability.
Contribution
The paper develops a novel conceptual and differential equation-based model for cloud-scale motions, enabling analysis of cloud morphology evolution and interactions.
Findings
Cloud motions tend to evolve toward a steady state.
Vertical growth is influenced by advection and diffusion.
Interactions depend on specific height ratios and circulation parameters.
Abstract
Developing an understandable theory for the dynamic evolution of the morphology of clouds remains intractable. To break this deadlock, we introduce a new conceptual model for cloud-scale motions named the Kinematics Representation of Non-rotating Updraft Tori (KRoNUT) model, where non-rotating reflects the absence of motion in the azimuthal direction. Using this model, we conduct a series of relaxation experiments whereby we ``turn off'' the baroclinic term associated with a pre-existing cloud-scale circulation. We then implement a moment reduction technique to generate a system of differential equations named the Dynamics of Non-rotating Updraft Tori (DoNUT) equations, which describe the temporal evolution of a cloudy circulation under various combinations of forcings, namely turbulent diffusion, self-advection, and cross-advection from a neighboring cloud-scale flow. The solutions of…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsMeteorological Phenomena and Simulations · Plant Water Relations and Carbon Dynamics · Solar and Space Plasma Dynamics
