Preprints
https://doi.org/10.5194/egusphere-2026-5329
https://doi.org/10.5194/egusphere-2026-5329
23 Sep 2026
 | 23 Sep 2026
Status: this preprint is open for discussion and under review for Hydrology and Earth System Sciences (HESS).

A temperature-conditioned spatial-temporal storm generator with evolving convective cell life cycles

Chien-Yu Tseng, Li-Pen Wang, and Christian Onof

Abstract. Convective rainfall varies at multiple scales: individual cells evolve within storms, while the population of cell intensities can differ substantially between storms. Existing object-based stochastic storm generators commonly represent cell occurrence and movement but provide limited representation of these two sources of variability. This study develops a spatial-temporal convective storm generator that explicitly represents both. At the cell scale, radar-derived tracks are represented using three lifespan-based classes, ranging from complete growth-peak-decay lifecycles to short-lived and transient cells, with dependence among evolving intensity and geometric properties preserved using copulas. At the storm scale, each event is assigned a storm-specific distribution of cell intensities. Its location and spread are modelled using Generalised Additive Models for Location, Scale and Shape (GAMLSS), with near-surface air temperature representing systematic environmental dependence and event-level random effects representing residual storm-to-storm variability. The framework was calibrated using 169 warm-season convective storms observed over Birmingham, UK, between 2005 and 2017. The resulting generator reproduces the observed cell-property distributions, dependence structures, storm-scale organisation and temporal clustering. Importantly, using a single pooled cell-intensity distribution largely removes the observed between-storm intensity variability, whereas the storm-specific formulation recovers the observed variance partition while retaining within-storm dispersion. This improves the distributions of event-maximum cell intensity and substantially improves their extreme-value behaviour, with observed return levels remaining within the 5-95% simulation intervals across return periods of 2-100 years. The resulting framework links storm-scale environmental variability to populations of dynamically evolving convective cells, providing a computationally efficient basis for large-ensemble spatial-temporal rainfall generation and future climate-conditioned applications.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
Share
Chien-Yu Tseng, Li-Pen Wang, and Christian Onof

Status: open (until 04 Nov 2026)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
Chien-Yu Tseng, Li-Pen Wang, and Christian Onof
Chien-Yu Tseng, Li-Pen Wang, and Christian Onof
Metrics will be available soon.
Latest update: 23 Sep 2026
Download
Short summary
Short, intense storms can cause severe urban flooding, but producing enough realistic storms to assess future risk is difficult. We developed a fast computer model that simulates how individual storm cells grow, move and decay, while allowing their intensity to vary with temperature and between storms. This better reproduced observed differences between storms and rare extremes, providing a practical way to generate large sets of storms for flood-risk and climate-change studies.
Share