When Hurricane Milton made landfall on Florida's Gulf Coast in October 2024, it offered the catastrophe modeling community something genuinely instructive: a major hurricane whose wind field defied the assumptions baked into many conventional models. As Milton crossed the peninsula, strong vertical wind shear — driven by interaction with the jet stream — modified the storm's wind field asymmetry from the typical right side of the track. As a result, the strongest winds were not located where a simpler asymmetric model based only on storm motion would have placed them. For insurers and reinsurers trying to understand localized loss potential in near-real time, that mismatch matters.
Milton is one reason my colleagues and I spent several years systematically rebuilding the wind hazard component of Verisk's U.S. tropical cyclone model from the ground up. The result is a fundamentally different approach to representing how hurricane winds behave — one grounded in direct surface observations, responsive to the actual environment a storm moves through, and capable of capturing the structural variability that drives the difference between a loss event and a catastrophe.

The problem with the previous generation
Most parametric wind field models in operational use today share a common lineage. They describe wind speed as a function of radial distance from the storm center in terms of a fairly small number of structural parameters, commonly the maximum wind speed, radius of maximum winds, and profile shape factors. Parameters in these models have often been calibrated on wind observations taken well above the ground level, requiring additional assumptions in order to compute winds at the surface (10 meter). The asymmetry imposed on these profiles has typically been tied to storm motion: the right quadrant is assumed to be stronger simply because the storm's translation speed adds to the rotational winds on that side.
This is physically reasonable, but only on average; it leaves out a great deal of what actually shapes a storm's wind field. Vertical wind shear, baroclinic interactions as storms move poleward, sea surface temperature gradients, the storm's own life cycle stage — all of these influence where peak winds occur and how quickly they decay outward. A model that can only express asymmetry through motion is, by design, blind to these effects.
There is a second, less-discussed, but just as important, limitation: most of these models were calibrated on winds measured at flight level — typically around one to three kilometers altitude — and then translated to the surface through conversion schemes that carry their own substantial uncertainties. The surface is where exposure sits. It is not where most historical calibration data came from.
A new parametric foundation
The updated wind field model, documented in peer-reviewed work published in the Journal of Applied Meteorology and Climatology in late 2024, begins with a reworking of the parametric wind profile itself. Building on the dual-exponential radial profile framework developed by Prof. Hugh Willoughby and colleagues (Willoughby et al., 2006), we expanded the model's structural degrees of freedom significantly. Where the previous formulation constrained the profile shape to a limited set of parameters, the updated model unlocks each component of the profile — the inner core shape, the dual outer decay scales, the transition width — and allows them to vary in a logical yet stochastic way.
The practical result is a model that can accurately represent the full range of observed tropical cyclone structures. Compact, intense storms like Hurricane Charley (2004), with its narrow eye and sharply peaked wind maximum, can be fit precisely. So can broad, asymmetric systems like Hurricane Sandy (2012), whose outer wind field extended hundreds of kilometers from a weakening center. These are not edge cases — they represent the genuine structural diversity that the historical record contains, and that loss estimates need to reflect.
Asymmetry tied to the environment, not just motion
The more consequential innovation may be how asymmetry is handled. In the updated framework, each structural parameter carries its own wavenumber-1 expansion (Fourier series) — meaning each element of the wind profile can independently vary around the storm in response to environmental conditions. The direction and magnitude of that variation is not assumed; it is learned from data and connected to the physical environment.
Vertical wind shear, which is a result of several dynamic atmospheric processes, is the primary driver. In weakly sheared environments, the wind maximum tends to sit in the right-forward quadrant relative to storm motion, as conventional models assume. But as shear magnitude increases, that maximum wind tends to rotate — counterclockwise from the conventional location — and can shift to the forward or even left side of the storm. This is not a modeling artifact. It is a well-documented physical relationship confirmed by aircraft reconnaissance observations, and ignoring it means systematically misplacing peak winds in storms. In particular, such events are more likely to be found at the tails of the season and in higher-latitude environments where shear is most pronounced.
By coupling the statistical description of wind field structure directly to the environmental state — including shear, sea surface temperature, relative humidity, and storm life cycle stage — the model produces wind fields that evolve realistically as conditions change. A storm moving into a high-shear environment does not just weaken in intensity; it reorganizes structurally in ways the model now captures.
Calibration at the surface, at scale
Underpinning all of this is a substantial expansion of the observational dataset used for model calibration. The previous generation relied primarily on model parameters calibrated on wind measurements taken high above the surface by aircraft reconnaissance flights. The updated calibration draws on over 700,000 individual surface wind observations from stepped-frequency microwave radiometer (SFMR) and global positioning system (GPS) data spanning more than two decades from nearly 1200 flights into 169 tropical cyclones, ranging from tropical storms to Category 5 hurricanes.
Critically, these are surface observations — 10-meter wind speeds from SFMR instruments, GPS dropwindsondes, land-based towers, offshore buoys, and satellite-derived datasets including synthetic aperture radar. The model is calibrated and validated directly at the level where damage occurs, eliminating the altitude correction step and the uncertainty it introduces.
The payoff is an unbiased parametric model that fits observed wind fields with random errors across the full intensity range comparable to the measurement uncertainty in the observations taken in extreme environments of tropical cyclones.
Downscaling: Resolution where it matters
Once the initial wind field is established, translating it to a surface hazard footprint requires accounting for land surface friction. This is where models often trade accuracy for computational tractability. Our updated downscaling scheme addresses several specific limitations in the previous approach.
The surface roughness representation has been rebuilt utilizing the latest 30-meter land use and land cover data from the U.S. Geological Survey. While our model computes winds at a coarser resolution than this dataset, sub-grid information is now preserved when upscaling to the final model resolution and adds meaningful detail to resolved terrain features. Meanwhile, friction assignments across land cover classes have been updated to align with current scientific literature — most notably that open water surfaces are treated as smoother than in the current implementation. And simultaneously, the fetch-weighting scheme, which accounts for the upwind terrain a given wind parcel has traversed, has been redefined to emphasize local conditions more strongly. The net effect is that coastal winds are enhanced and more realistically confined to areas directly influenced by the maritime boundary, while inland penetration of strong sustained winds are appropriately attenuated. Notably however, areas where localized terrain features, such as gaps in land cover or inland water bodies, can still create corridors for elevated hazard.
Azimuthal resolution in the friction scheme has also been increased substantially, allowing the model to resolve situations where wind direction aligns with specific terrain features — the kind of localized enhancement that drives disparate loss outcomes across short distances.
A new approach to gusts
The final innovation addresses a persistent gap between modeled outputs and what insurers actually observe and care about. The previous model produced maximum one-minute sustained wind speeds — a standard meteorological convention, and the basis for Saffir-Simpson categorization. But wind damage is better explained by gusts, and the relationship between sustained winds and gusts varies considerably with wind intensity and surface roughness.
Rather than applying a static conversion factor from the literature — where published estimates are loosely defined, span a wide range, and often conflict — we built an empirical gust formulation coached in our new modeling paradigm and derived from our curated observational datasets. High-frequency wind measurements from towers, buoys, and offshore platforms across multiple storms and in various terrain conditions were used to characterize the sustained-to-gust relationship as a function of wind and storm intensity, and surface type. The result is a model-native gust and duration formulation that translates directly to three-second maximum gusts — the quantity most relevant for structural damage assessment and the one most commonly reported by observing networks.
Validation against independent observations across a large number of historical events shows mean biases below 0.5 mph catalog-wide, with error metrics well within observational tolerances even at the coastline, where variability is greatest.
What this means for risk assessment
The implications for catastrophe model users are practical as well as scientific. More accurate representation of wind field asymmetry — tied to the environment rather than motion alone — improves loss estimates most significantly for storms at the shoulders of the season and in the northern tier of the U.S., where shear is highest and where conventional models most frequently misplace peak winds. Events like Milton, where the loss footprint was shaped as much by shear-induced asymmetry as by raw intensity, are now representable in the stochastic catalog.
The improved frictional downscaling produces more defensible localized loss estimates, particularly in coastal zones where the previous model's broad fetch representation smoothed over meaningful differences in terrain. And the gust formulation adds variance to inland wind fields in a physically consistent way, addressing a known source of underestimation in damage to residential and light commercial construction.
Taken together, these advances represent a meaningful shift in what parametric representations of tropical cyclone wind fields in catastrophe risk models can accomplish. The goal was not to build a more complicated model — it was to build one that more completely reflects what the observations tell us about how hurricanes actually work. For a modeling community that is increasingly asked to justify its assumptions against real events, that distinction is worth making.
- The parametric wind field model described in this article is documented in: Uhlhorn, E. W., S. Tolwinski-Ward, and S. Lorsolo, 2024: An asymmetric model of the tropical cyclone surface wind field and probabilistic climatology of structural parameters. J. Appl. Meteor. Climl., 63, 1569–1587.