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- W3098556150 abstract "Abstract Randomly distributed convective storms can self-aggregate in the absence of large-scale forcings. Here we present a 1D shallow-water model to study the convective self-aggregation. This model simulates the dynamics of the planetary boundary layer and represents convection as a triggered process. Once triggered, convection lasts for finite time and occupies finite length. We show that the model can successfully simulate self-aggregation, and that the results are robust to a wide range of parameter values. In the simulations, convection excites gravity waves. The gravity waves then form a standing wave pattern, separating the domain into convectively active and inactive regions. We analyze the available potential energy (APE) budget and show that convection generates APE, providing energy for self-aggregation. By performing dimensional analysis, we develop a scaling theory for the size of convective aggregation, which is set by the gravity wave speed, damping time scale, and number density of convective storms. This paper provides a simple modeling framework to further study convective self-aggregation." @default.
- W3098556150 created "2020-11-23" @default.
- W3098556150 creator A5028212408 @default.
- W3098556150 date "2021-02-01" @default.
- W3098556150 modified "2023-09-23" @default.
- W3098556150 title "A Shallow-Water Model for Convective Self-Aggregation" @default.
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- W3098556150 doi "https://doi.org/10.1175/jas-d-20-0031.1" @default.
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