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Create a fast and robust radial profile of the tropical cyclone rotating wind from inputs Vmax, R34kt, Rmax, and latitude
A package that creates fast, robust, physics-based radial profiles of the tropical cyclone rotating wind and pressure from inputs Vmax, R34kt, and latitude. Based on the latest observationally-validated science on the structure of the wind field and pressure.
Cite this package: . Also a paper is in prep with co-authors Dandan Tao and Robert Nystrom
Objective: To provide a faster and easier-to-use approximation to the physics-based wind model code of Chavas+ (2015 JAS). That model is state-of-the-art, but slow. We want something faster/simpler that also better fits observations while staying true to the physics.
The Chavas+ (2015) model has been extensively validated for real-world TCs, in terms of both physics and hazards/impacts:
Physics:
Hazards/impacts: 4. When used as forcing for a surge model, it reproduces the historical record of U.S. peak storm surge remarkably well (Gori+ 2023 JGR-A). It performs better than prevailing empirical wind field model Wang+ 2022 JGR-A). 5. When used as forcing for a physics-based rainfall model, it reproduces the climatology of U.S. tropical cyclone inland rainfall remarkably well -- and dramatically better than existing empirical wind field models (Xi+ 2020 J. Hydromet.). 6. When used to model all hazards (wind, coastal surge, inland flooding), predicts the county-level distribution of economic damage quite well (Gori+ 2025 ERL, accepted).
Full modeling pipeline:
Currently, this code uses a quadratic profile inside the eye (r$<$Rmax), a modified‐Rankine vortex between Rmax and R34kt (inner model), and the E04 model beyond R34kt. It is very similar to the full physics-based wind profile model of Chavas et al. (2015) (code here), but is simpler and much faster, and also includes a more reasonable eye model.
The model starts from the radius of 34kt, which is the most robust measure of size we have: it has long been routinely-estimated operationally; it is at a low enough wind speed to be accurately estimated by satellites over the ocean (higher confidence in data); and it is less noisy because it is typically outside the convective inner-core of the storm. The model then encodes the latest science to estimate 1) Rmax from R34kt (+ Vmax, latitude), 2) the radius of vanishing wind R0 from R34kt (+ latitude, an environmental constant), and 3) the minimum pressure Pmin from Vmax, R34kt, latitude, translation speed, and environmental pressure. Hence, it is very firmly grounded in the known physics of the tropical cyclone wind field while also matching the input data. It is also guaranteed to be very well‐behaved for basically any input parameter combination.
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Create a fast and robust radial profile of the tropical cyclone rotating wind from inputs Vmax, R34kt, Rmax, and latitude
We found that tcwindprofile demonstrated a healthy version release cadence and project activity because the last version was released less than a year ago. It has 1 open source maintainer collaborating on the project.
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