Session 6 | Hail studies

Session 6

Hail studies
Orals WE1
| Wed, 19 Nov, 09:00–10:45 (CET)|Room Hertz Zaal
Posters TH4
| Attendance Thu, 20 Nov, 14:30–16:00 (CET) | Display Wed, 19 Nov, 09:00–Thu, 20 Nov, 18:30|Poster area, P4–28
Wed, 09:00
Thu, 14:30

Orals: Wed, 19 Nov, 09:00–10:45 | Room Hertz Zaal

09:00–09:30
|
ECSS2025-52
|
keynote presentation
|
Valentin Gebhart, Ellina Agayar, Martin Aregger, Killian Brennan, Pierluigi Calanca, Ruoyi Cui, Olivia Martius, Christoph Schär, Timo Schmid, Iris Thurnherr, Heini Wernli, Lena Wilhelm, and David N. Bresch

Hail represents the costliest atmospheric peril in Switzerland and many other European countries, highlighting the demand for a good understanding and actionable information about hail risk in current and future climate conditions. For this purpose, the four-year research project scClim, now in its closing stage, was initiated to bring together complementary expertise of several Swiss universities and institutions. The project’s goal is to study hail and hail impacts in a unifying framework, including (a) the improvement of radar-based hail observations, (b) the investigation of hail variability and its link to large-scale weather patterns, (c) the implementation and evaluation of high-resolution weather and climate simulations with a hail growth model, and (d) the modeling of hail impacts on different asset types such as buildings or agriculture. In the first part of this talk, we will give an overview of the project, presenting several results of the different subprojects and their connections.

In the second part, we focus on different types of impact-based hail forecasts for Switzerland. The unique data availability for Switzerland, including detailed exposure and impact data from cantonal building insurances, enabled us to implement and evaluate several impact-based hail forecasts based operational weather forecasts from MeteoSwiss with the hail growth module HAILCAST. We analyze two impact-based forecast products that have been tailored to two different user groups, private citizens who receive weather warnings, and larger institutions like federal or cantonal entities.

How to cite: Gebhart, V., Agayar, E., Aregger, M., Brennan, K., Calanca, P., Cui, R., Martius, O., Schär, C., Schmid, T., Thurnherr, I., Wernli, H., Wilhelm, L., and Bresch, D. N.: Hail and its impacts: An interdisciplinary research project in Switzerland, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-52, https://doi.org/10.5194/ecss2025-52, 2025.

09:30–09:45
|
ECSS2025-228
|
Tobias Scharbach, Silke Trömel, Elias Hühn, Michael Kunz, Jannik Fischer, Susanna Mohr, Joshua Soderholm, Dean Sgarbossa, Jordan Brook, Jana Mendrok, and Ulrich Blahak

Understanding the life cycle of hailstorms is crucial for improving numerical weather prediction (NWP) models to accurately forecast severe weather. As part of the project Understanding Large Hail Formation and Trajectories (LIFT), the primary goal of this study is to improve our understanding of large hail formation and hail trajectory models (e.g. HailTrack; Brooks et al., 2021), towards a more accurate prediction of severe hail events. The study employs both the operational C-band radar network of the German Weather Service (DWD) and data collected during the In-situ Collaborative Experiment for Collection of Hail In the Plains (ICECHIP; Adams-Selin et al., 2024) field campaign. The open-source algorithm Pythonic Direct Data Assimilation (PyDDA) is employed for the wind retrievals. PyDDA uses the 3D variational method (3DVAR), minimising the sum of various cost functions depending on radar-measured Doppler winds and atmospheric dynamic conditions (e.g. the continuity equation) and optional other parameters like e.g. radiosoundings. However, minimising the total cost function presents various challenges, e.g. the final wind retrieval depends on adaptable weights of cost function components . Thus, a sensitivity analysis utilising regional convective-allowing simulations of storms in southern Germany obtained from the ICON Rapid Update Cycle (ICON-RUC, hourly updates), part of the DWD's new Seamless INtegrated FOrecastiNg sYstem (SINFONY), is presented. Consistent simulated 3D wind fields are confronted with retrievals obtained from the corresponding forward-simulated (synthetic) observations to optimize the weighting factors. In the final step, the resulting PyDDA-derived 3D wind fields are comparatively analysed with typical radar process signatures of thunderstorms (e.g. columns with enhanced differential reflectivity ZDR), as well as with trajectories from hailsondes. These miniaturised radiosondes are designed to mimic the trajectories of hailstones providing useful insights into a thunderstorms updraft characteristics (e.g. updraft velocities and region) and their further development.

How to cite: Scharbach, T., Trömel, S., Hühn, E., Kunz, M., Fischer, J., Mohr, S., Soderholm, J., Sgarbossa, D., Brook, J., Mendrok, J., and Blahak, U.: 3D wind retrievals for the analysis of hailstorm dynamics in Germany and the USA, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-228, https://doi.org/10.5194/ecss2025-228, 2025.

09:45–10:00
|
ECSS2025-187
|
Kelly Lombardo and Matthew Kumjian

There is an emerging consensus that strong deep-layer shear, particularly in the 1-6 km altitude layer, favors hail production in supercells, whereas strong low-level (i.e., 0-1- km) shear does not. However, the importance of the distribution of shear within the 1-6 km layer is unknown, yet that distribution of shear will affect the storm-relative wind magnitude and direction in the lowest few kilometers of the troposphere. The lower-tropospheric storm-relative winds play an important role in creating optimal hail growth pathways via the mesocyclone.

 To understand how the distribution of shear in the 1-6-km layer affects hail production in supercell storms, we perform two sets of idealized simulations using CM1 and our hail growth trajectory model. The first quantifies the impact of the storm-relative wind magnitude on the midlevel mesocyclone and hail production. We do this by modifying the hodograph shape to increase the storm-relative wind in the 1-3.5 km layer and decrease the storm-relative wind in the 3.5 – 6 km layer (and vice versa), while generally maintaining the overall storm-relative wind direction, 0-1-km SRH, 0-6-km and 1-6-km shear vectors, and Bunkers storm motion vector.  The second set of experiments quantifies the impact of the vertical distribution of shear within the 1-6 km layer on the mesocyclone and hail production. We do this by adjusting the hodograph such that, while the total 1-6 km shear remains fixed, shear in the 1-3.5 km layer is increased and 3.5 km-6 km layer is decreased (and vice versa). This results in changes to the storm-relative wind direction while generally maintaining the storm-relative wind magnitude, 0-1-km SRH, 0-6-km and 1-6-km shear vectors, and Bunkers storm motion vector.

We will discuss how these hodograph modifications affect mesocyclone properties, storm behavior (cycling, splitting), updraft width and intensity, and how all these storm structural changes affect hail production.

How to cite: Lombardo, K. and Kumjian, M.: The Sensitivity of Hail Production in Supercell Storms to the Distribution of Vertical Wind Shear, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-187, https://doi.org/10.5194/ecss2025-187, 2025.

10:00–10:15
|
ECSS2025-185
|
Lydia Spychalla, Matthew Kumjian, Kelly Lombardo, Joshua Soderholm, and Jannick Fischer

Recent hail trajectory modeling studies have identified pathways for large hail growth that are complex and strongly impacted by sub-updraft scale dynamics in the supercooled layer of a storm. In the hail growth region of a supercell, thermal-like behavior, vortex shedding, and dynamical rotors, among other phenomena, cause an updraft to evolve dynamically on short timescales that may not be clearly resolved by operational radars, which perform volume scans on timescales of 5 min or greater.  

Here, we examine the evolution of the mixed phase region of a supercell storm’s updraft modeled in CM1 with 5-second temporal output. This dataset provides a sandbox in which to explore the timescales of evolution for a variety of updraft quantities and can shed light on the temporal resolution necessary to resolve properties of a storm’s updraft important for hail trajectories. Techniques including Fourier analysis, wavelet analysis, and variability indices are presented as tools for identifying and isolating updraft variability on a variety of timescales associated with physical and dynamical processes in the modeled supercell. 

We hypothesize that the treatment of updraft variability in numerical hail trajectory modeling is impactful on the nature of hail trajectories produced (i.e., do hail trajectories have differing complexity if computed in composited storm fields, in frozen snapshots of a storm, or in fully time-varying fields?). To understand the role of temporal variability in hail growth, we run hail trajectories to compare the impact of these different ways of representing storm fields. We examine how allowing or restricting the evolution of a storm impacts the behavior and complexity of numerically modeled hail trajectories.  

On the recent ICECHIP field campaign, Hailsondes (small probes that are released into a storm, accrete mass, and fall out as pseudo-hailstones) were released to measure hail-like trajectories in real storms. We compare our modeled trajectories to Hailsonde trajectories to analyze the realism of modeled hail trajectories in an evolving storm. 

How to cite: Spychalla, L., Kumjian, M., Lombardo, K., Soderholm, J., and Fischer, J.: Timescales of Evolution for Supercell Updrafts and their Impact on Hail Trajectories, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-185, https://doi.org/10.5194/ecss2025-185, 2025.

10:15–10:30
|
ECSS2025-27
|
Killian P. Brennan and Lena Wilhelm

The impact of atmospheric dust on hail formation remains poorly under-
stood, with competing effects suggesting both convective enhancement through
increased cloud condensation particles and suppression of hail activity through
enhanced ice nucleation. While high concentrations of ice nucleating particles,
such as Saharan dust, are often associated with reduced hail size — motivat-
ing cloud seeding efforts — empirical evidence on the influence of dust on hail
frequency is limited and regionally inconsistent.
In this study, we combine a range of observational and reanalysis datasets
— including CAMS reanalyses, crowd-sourced hail reports, lightning and radar
observations, and synoptic and environmental variables from ERA5, to sys-
tematically investigate the relationship between Saharan dust loading and hail
occurrence across Europe. We find a strong and spatially consistent association:
hail days exhibit significantly (7σ) higher dust concentrations than convective
non-hail days, with the median dust load up to 1.8 times greater.
Importantly, this dust-hail link persists across different synoptic weather
regimes, underscoring its robustness. Hail occurrence peaks at moderate dust
concentrations (38 mg m−2 or a dust optical depth of 0.033), consistent with
convective enhancement, before declining at higher values, suggesting possible
microphysical or radiative limitations. Crowd-sourced hail report data reveals
a substantial increase in hail events on high-dust days vs. low dust days. An
influence of the dust concentration on the reported hail diameters was not found.
When included as a predictor in statistical hail models (logistic regression
and generalized additive models), dust consistently ranks as one of the top three
predictors, with model skills improving notably.
Together, our findings highlight Saharan dust as a key, yet underrecognized,
factor modulating hail activity in Europe and demonstrate the need for further
studies on aerosoll — hail interactions.

How to cite: Brennan, K. P. and Wilhelm, L.: Saharan dust linked to European hail events, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-27, https://doi.org/10.5194/ecss2025-27, 2025.

10:30–10:45
|
ECSS2025-309
John Allen, Rebecca Adams-Selin, Victor Gensini, and Andrew Heymsfield and the ICECHIP Science PIs

 

Hail is the leading driver of severe convective storm losses in the United States and globally, with early estimates though June in 2025 approaching 20 billion dollars insured loss in the U.S. alone. Despite this impact, many questions remain unanswered within hail science, ranging from hailstone properties to swath properties, to environmental drivers and storm kinematic and microphysical structures and how these can be remotely sensed. To address this gap the In Situ Collaborative Experiment for the Collection of Hail in the Plains (ICECHIP) campaign was conducted between May 15 and June 28th of 2025. Active periods of convection persisted throughout the campaign yielding over 20 intensive observation periods.

ICECHIP field assets included over 100 ground deployable instruments, multiple atmospheric profiling systems, mobile doppler radars with a team of 15 institutions and 6 countries. Numerous cases ranging from accumulating small to storms with hail in excess of 75mm were sampled, with the largest hailstone observed >140mm and weighing 462 grams. ICECHIP addressed observations necessary for 5 major research themes: 1) embryo development and hailstone growth and fall behavior; 2) in-storm hail trajectory and convective updraft relationships; 3) environmental impacts on hail processes and predictability; 4) surface properties of hailstones and associated impacts; and 5) relationship of hailstone physical properties and growth processes to radar observations.

This presentation will focus on an overview of major project cases and preliminary significant findings. Examples of the data collected include ground observed arrays at horizontal resolutions of a few hundred meters across hailswaths, updraft measurements of both supercell and non-supercellular hail producing storms, dual-doppler and high-resolution radar coverage overlapping detailed ground mapping, and numerous examples of near storm environmental profiles.

How to cite: Allen, J., Adams-Selin, R., Gensini, V., and Heymsfield, A. and the ICECHIP Science PIs: Overview of the In Situ Collaborative Experiment for the Collection of Hail in the Plains (ICECHIP), 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-309, https://doi.org/10.5194/ecss2025-309, 2025.

Posters: Thu, 20 Nov, 14:30–16:00 | Poster area

Display time: Wed, 19 Nov, 09:00–Thu, 20 Nov, 18:30
P4
|
ECSS2025-30
|
Iris Thurnherr, Lena Wilhelm, Tim Raupach, Francesco Battaglioli, Monika Feldmann, Killian Brennan, Ruoyi Cui, Heini Wernli, and Olivia Romppainen-Martius

Historical and future hail trends over Europe generally point to an increased hail threat. However, these trends often diverge at the regional scale. In particular, Western and Southern Europe show conflicting signals with some models and observations indicating more frequent hail events, while others suggest a decline in a warmer climate. Most existing future projections of hail occurrence rely on hail proxies, estimates based on environmental conditions indicative of hail formation, derived from global and regional climate models that use parameterized convection schemes. Recent developments have introduced more advanced statistical hail models and refined proxies. Despite these advancements, systematic comparisons of different hail proxies - especially when derived from a common dataset - remain limited. In this study, we utilize high-resolution (2 km), convection-permitting regional COSMO climate simulations with the embedded online hail diagnostic HAILCAST to assess the present day and future hail occurrence in a 3°C pseudo global warming scenario. We compare hail frequencies and hail frequency changes derived from (i) established hail proxies based on environmental thresholds and statistical models and (ii) the HAILCAST online diagnostic. Our goal is to evaluate how spatial and temporal patterns of hail occurrence differ between methods and to assess the associated uncertainties in hail trend projections across Europe.

How to cite: Thurnherr, I., Wilhelm, L., Raupach, T., Battaglioli, F., Feldmann, M., Brennan, K., Cui, R., Wernli, H., and Romppainen-Martius, O.: Exploring uncertainty in future hail trends: A comparison of proxy-based and diagnostic approaches using convection-permitting climate simulations over Europe, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-30, https://doi.org/10.5194/ecss2025-30, 2025.

P5
|
ECSS2025-43
|
Iris Thurnherr, Monika Feldmann, Killian Brennan, Sandro Beer, Lena Wilhelm, Ruoyi Cui, Michael Sprenger, Heini Wernli, and Olivia Romppainen-Martius

Environmental proxies are widely used to estimate the occurrence of severe convective storms - such as hailstorms and supercells - in both present and future climates, as these storms are typically not resolved in climate models. These environmental proxies rely on atmospheric parameters, including convective available potential energy (CAPE), convective inhibition (CIN), low-level humidity, and vertical wind shear. A core assumption behind their application is climate stationarity: that similar thresholds of environmental conditions will continue to produce similar storm initiation and behavior. However, this assumption remains largely untested. In this study, we explicitly assess the stationarity of convective proxies under climate change using convection-permitting, high-resolution climate simulations over Europe for the present-day and a +3°C pseudo global warming scenario. A storm-tracking algorithm is applied to track supercells and hail storms and their (pre-storm) environments. This approach enables a detailed comparison of the convective environments, their lower bounds, and their projected future changes. Our results show marked changes in both storm characteristics and their environments, such as increases in mean precipitation, hail diameter associated with hailstorms and supercells, and CAPE, CIN and vertical wind shear in the storm inflow regions. Nonetheless, lower bounds on the distributions do not show marked changes. We further examine how shifts in the distribution of convective environments influence simple threshold-based proxies for hail and supercell occurrence, highlighting the implications of environmental changes on convection proxies.

How to cite: Thurnherr, I., Feldmann, M., Brennan, K., Beer, S., Wilhelm, L., Cui, R., Sprenger, M., Wernli, H., and Romppainen-Martius, O.: Will today’s proxies work tomorrow? Revisiting the stationarity assumption for severe convective environments, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-43, https://doi.org/10.5194/ecss2025-43, 2025.

P6
|
ECSS2025-47
Stavroula Stolaki

One of the main objectives of this study is to document and compare the atmospheric environments associated with hailstorms and non hail thunderstorms during the Greek National Hail Suppression Program (GNHSP) that protects an intensively cultivated area of Central Macedonia, Greece. The analysis focuses on identifying thresholds in various thermodynamic and kinematic parameters that might provide a good discrimination between these two environments based on radiosonde measurements. Convective Available Potential Energy (CAPE), lifted condensation level (LCL), wet bulb zero height, lapse rates, relative humidity, as well as vertical wind profile parameters (such as 0-6 km bulk shear) were derived from 06 UTC radiosondes that were held at Thessaloniki’s Airport Makedonia for the operational period between March and September of 2020-2024. Thermodynamic parameters on hailstorm days have higher median values than on non hail storm days, but there is considerable overlap between the distributions. The intramonthly variation of the thermodynamic parameters in the hailstorm environment shows that their values increase from spring to summer, while this does not apply for the kinematic parameters. Discriminating between hailstorm intensity categories, it is found that values of instability and moisture parameters, with some exceptions, are higher for the severe than for the non severe category, however there is again overlap between the distributions. Hail is most likely for high CAPE and this probability increases when bulk shear increases.

How to cite: Stolaki, S.: Radiosonde observations of storm environments in Northern Greece, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-47, https://doi.org/10.5194/ecss2025-47, 2025.

P7
|
ECSS2025-53
Carlos Calvo-Sancho, Yago Martín, Juan Jesús González-Alemán, Cesar Azorin-Molina, and María Luisa Martín

Supercell storms are often associated with severe-weather phenomena such as heavy rainfall, hail, tornados or straight-line winds (downbursts or derechos), all of which can have impactful socio-economic and environmental consequences. Despite these impacts, the lack of data of supercell storms has limited their analysis and characterization of the climatology across Spain. This constraint has been addressed through a voluntary, collaborative effort to create a database of supercell events from January 2011 to December 2021. During the 11-year study period, 2,087 storms with supercell characteristics were identified. Citizen collaboration confirmed 13.7 % of the supercells detected in PPI radar images. The database also includes hail size and/or tornadoes associated with each supercell whenever such information was reported. The results reveal a spatial distribution with high supercell activity in eastern Spain, mainly in Mediterranean areas and the north-eastern part of the Iberian Peninsula.

From 2022 onward, only supercells with high socio-economic impact - specifically, those accompanied by large hail (≥ 5 cm) - have been compiled. In addition, a thorough review of the national newspaper archive is under way to identify and catalogue large-hail events from 2000 to the present. Because photographs to determine hail size are often unavailable, a proxy based on the damage reported in the press has been developed to identify these events. Currently, more than 240 large-hail events have been catalogued in Spain (Peninsula and Balearic Islands) for 2000-2024. Among them, 44 events reported very large hail (≥ 7 cm) and 7 involved giant hail (≥ 10 cm), three of which occurred in the last three years. The convective environments show substantial differences in the different large-hail categories. The trend shows a significant increase in both the number of days with hail and the number of hail events in Spain.    

How to cite: Calvo-Sancho, C., Martín, Y., González-Alemán, J. J., Azorin-Molina, C., and Martín, M. L.: Supercells and large hail in Spain, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-53, https://doi.org/10.5194/ecss2025-53, 2025.

P8
|
ECSS2025-62
|
Kateřina Skripniková and Petr Zacharov

The severe hail observation in Czechia is limited to observations from weather stations and reports from the public. More comprehensive information can be obtained from weather radar measurements. A method based on single-polarisation techniques has been developed to detect severe hail causing significant damage on the Czech territory. However, this is limited by the period of radar measurements. Insight into the climatology of severe hail is gained by studying the environmental conditions suitable for large hail development.

The ALADIN/PERUN reanalysis includes outputs describing the convective environment. The reanalysis has high horizontal (2.3 km) and temporal (1h) resolution in the 1991-2020 time span. The environmental parameters CAPE, CIN and wind shear are tested in this work as precursors of severe hailstorms. Precursor values that can be used to develop a climatology of hail hazard in Czechia are obtained by comparison with radar-based hail detections from the warm parts of the 14 years from 2007 to 2020. The presence of precipitation ice in convective precipitation as identified by the ALADIN/PERUN reanalysis will also be examined.

In addition, case studies of hailstorms in the vicinity of the mountain meteorological observatory at Milesovka, where more focused radar data are available, are prepared and the precursor values are discussed.

How to cite: Skripniková, K. and Zacharov, P.: Climatology of severe hail precursors in Czechia, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-62, https://doi.org/10.5194/ecss2025-62, 2025.

P9
|
ECSS2025-69
Jin-woo Park, Bo-Young Ye, and Mi-Kyung Suk

  Hail, which causes severe property damage, is a highly localized phenomenon that is difficult to observe and predict. The Korea Meteorological Administration's Weather Radar Center has developed radar-based hail products (Potential Hail Area and Hail Risk Altitude) to support forecasters in responding to hail events. The collection of the ground-based hail observations is challenging task, and systematic management is difficult due to the two different data types: the structure data (official meteorological observations data) and unstructured data (various forms of reported data). Therefore, we developed an integrated data management system that combines both data types.

  In this study, the Hail Observation Data Collection System is a web platform developed using Python “Streamlit”. This system consists of three main components: First, the structured and the unstructured hail data is collected, separately. The structured data are automatically processed through APIs and the unstructured data are processed through the manual input of essential fields (date, time, location, reliability, source) and additional fields (detailed address, hail size, etc.). And the dataset forms of each observed hail are normalized and standardized the time of observation, location, and reliability of information, and recorded it in JSON file format. Second, this system integrates and displays to facilitate convenient analysis through the sorting of the date, time, size, and other criteria about hail cases. Third, the comprehensive analysis about spatial-temporal distribution can provide from these hail records for the long-term in Korea.

  Through the establishment of this integrated hail observation data system, the hail observation cases are systematically managed, and these data are being used to perform systematic validation and parameter improvement of radar-based hail detection technique. And the integrated spatial-temporal distribution and statistical analysis of hail data is available to support effective communication between researchers and forecasters. 

 

ACKNOWLEDGEMENTS
This research was supported by “Development of integrated radar analysis and customized radar technology (KMA2021-03021)” of “Development of integrated application technology for Korea weather radar” project funded by the Weather Radar Center, Korea Meteorological Administration.

 

How to cite: Park, J., Ye, B.-Y., and Suk, M.-K.: Establishment and Analysis of the Collection System of the Ground Hail Observation data for the verification of the Hail Detection Tech. using the High-resolution Weather Radar, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-69, https://doi.org/10.5194/ecss2025-69, 2025.

P10
|
ECSS2025-79
Stavros Kolios

One major weather hazard is the hail produced by cloud convective systems. Hail detection from satellites plays a critical role in reducing property damage, improving severe weather forecasting and disaster preparedness, supporting agricultural resilience, and advancing climate science. Nevertheless, even nowadays, hail is difficult to timely and accurately detected, remaining a challenging topic for the scientific community to develop even more accurate methods and algorithms for hail detection. The study is an effort to examine the role of a newly established remote sensing index, namely “Hail Potential Index” (HPI) to detect cloud areas with high possibility of hail production using the Meteosat Third Generation (MTG-1) multispectral imagery. The positive impact of this index evaluated both as an independent index and as input parameter in an Artificial Neural Network (ANN) model to detect hail produced by Mesoscale Convective Systems (MCS). Using a set of hail reports on the ground as reference datasets, a set of evaluation statistics were calculated to examine its efficiency in satellite-based hail detection. Metrics such as Probability of Detection (85%), the False Alarm Ratio (11%), the Critical Success Index (81%) and correlation coefficient reaching (0.87), highlight the satisfactory results of using the HPI index to detect hail produced by organized cloud convection using exclusively the latest Meteosat imagery.

How to cite: Kolios, S.: The efficiency of a new remotely sensed index for hail detection using Meteosat Third Generation multispectral imagery, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-79, https://doi.org/10.5194/ecss2025-79, 2025.

P11
|
ECSS2025-86
Kevin Manka, Daniel Butt, Connell Miller, and Julian Brimelow

Hailpads are a widely used method for recording hailstone impact data by capturing indentations made by hailstones during hailstorms. As a simple and low-cost approach, hailpads are often deployed in vast networks to collect spatially-distributed data. However, the subsequent process of analyzing these indentations is often long and intensive (taking up to several hours for a single hailpad), and subjective. This research presents a novel, automated approach to identify the major/minor axes and depth distributions of hailpad dents via an image processing and machine learning pipeline, aimed at reducing the time and effort required to analyze the constituent dents of a hailpad. Using high-precision 3D scans, hailpads are depth mapped and then binarized based on user-prescribed adaptive thresholding, contrast equalization, and area filtering parameters. Next, the resulting binary masks are used as input to a convolutional neural network (CNN), which separates dents in clustered and non-clustered regions via instance segmentation. Built on a training dataset of simulated hailpad binary masks, the model was evaluated with a 93.0% Intersection over Union (IoU) score on predicted dent masks. In further comparisons against manual analyses and third-party commercial 3D scan assessments, the model excels in identifying individual impacts from within densely grouped regions. However, the overall prediction distributions are hindered to varying degrees by the influence of false positives in dent detection from non-hail artifacts in the input binary masks. Overall, this automated approach demonstrates the potential to considerably expedite hailstone dent identification and lays the groundwork for extracting more physical properties in the future, such as approximations for volume, impact velocity, and accumulated impact energy.

How to cite: Manka, K., Butt, D., Miller, C., and Brimelow, J.: Automated Hailpad Dent Detection and Segmentation Using Machine Learning, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-86, https://doi.org/10.5194/ecss2025-86, 2025.

P12
|
ECSS2025-87
|
Jack Hamilton, Julian Brimelow, and Simon Eng

A destructive hailstorm hit Calgary, Alberta, Canada on August 5th, 2024, resulting in $3.25 billion CAD of insured losses – this made it the second costliest natural hazard event in Canadian history, in terms of insured losses. The storm caused widespread damage to the northern areas of the city. We will present results on the storm’s evolution, meteorological environment, and behaviour, to better understand the mechanisms behind its intensity and to inform the forecasting and mitigation of future hailstorms. On this day, the Northern Hail Project (NHP) field teams also collected in-situ data along the storm’s track; the largest hailstone that was found measured 52 mm in diameter. Hail was recorded at four NHP hail-monitoring stations located in the affected areas of the city. Colleagues from the Insurance Institute for Business & Home Safety (IBHS) also captured high-resolution data from an array of hail disdrometers deployed ahead of the storm. 

Synoptic conditions on the day were broadly supportive for the development of severe thunderstorms, although the environment did not suggest conditions were in place to support an exceptionally damaging hailstorm. Examination of ERA5 reanalysis data revealed a favourable kinematic profile, characterized by 20 m/s of 0-6 km bulk wind shear, as well as surface-based CAPE near 1,200 J/kg and 19 mm of precipitable water. The storm initiated over a zone of enhanced surface convergence and upslope flow along the front range of the Rocky Mountains northwest of Calgary. Once away from the terrain, the storm rapidly intensified and began producing large quantities of damaging hail. Just prior to entering the city limits, the storm became outflow dominant, producing measured wind gusts up to 65 km/h. These winds significantly increased the level of hail damage. The storm continued to produce severe hail after leaving the city.  

Ultimately, it was the combination of an outflow-driven storm, over an urban area, which produced such extensive damage. Therefore, insights gained from this investigation, particularly the detailed in-situ observations and environmental analysis by the NHP, underscore the importance of high-resolution monitoring to advance hailstorm forecasting and impact mitigation. 

How to cite: Hamilton, J., Brimelow, J., and Eng, S.:  The $3.25 billion Calgary, Alberta Hailstorm: a Meteorological Case Study and In-Situ Observations from the Northern Hail Project, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-87, https://doi.org/10.5194/ecss2025-87, 2025.

P13
|
ECSS2025-120
Iciar Guerrero-Calzas, Foteini Baladima, Alberto Sanchez-Marroquin, Ana Cortés, Mauricio Hanzich, and Josep Ramón Miró

Hailstorms are among the most destructive convective weather phenomena, causing extensive damage to agriculture, infrastructure, and property. Improving hail prediction and hindcasting requires a deep understanding of the atmospheric conditions under which hail forms. This study analyzes hail occurrence across Europe using ERA5 reanalysis data and ground-based hail observations to characterize the meteorological environments conducive to hail events.

Hail-prone conditions are identified based on a dataset of key atmospheric variables - including convective parameters, moisture and temperature profiles, and dynamic indices - at 0.25° spatial resolution on a daily timescale. Feature selection is performed using statistical relevance, variance, and correlation criteria to select variables that best capture the thermodynamic and dynamic processes involved in hail formation while minimizing redundancy.

To explore patterns linking atmospheric conditions to hail events, this study applies dimensionality reduction and clustering techniques. The resulting classification reveals distinct synoptic and mesoscale regimes associated with hailstorms, highlighting spatial and seasonal variability across Europe. These clusters expose region-specific hail environments and highlight the atmospheric states most likely to generate hail.

These regime-based classifications offer direct insights for improving convective-scale numerical weather prediction. By associating each cluster with specific model physics, this framework provides guidance for optimizing convection-permitting simulations - such as those using the Weather Research and Forecasting (WRF) model - to more accurately hail events/processes. Ultimately, this work contributes to improve hail prediction capability and robust climate-scale risk assessment of hailstorms across a range of European weather regimes.

How to cite: Guerrero-Calzas, I., Baladima, F., Sanchez-Marroquin, A., Cortés, A., Hanzich, M., and Miró, J. R.: Clustering Large-Scale Atmospheric Patterns Associated with Hailstorms, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-120, https://doi.org/10.5194/ecss2025-120, 2025.

P14
|
ECSS2025-141
Francesco De Martin, Agostino Manzato, Nicola Carlon, Martin Setvák, and Mario Marcello Miglietta

On July 24, 2023, the new European record for hail size was set in northeast (NE) Italy with a 19-cm wide hailstone, recorded during a supercell outbreak. During this event, severe storms were triggered in the Alps, moved eastward, intensified rapidly in the foothills, and generated damaging hailstorms in the plains. A detailed analysis of the available observations highlights that the second supercell developed in an atmospheric environment with an unusually weak-to-moderate potential instability. However, numerical simulations revealed a high-Θe tongue over the Adriatic Sea, which was lifted by a southerly flow above the cold pool generated by the thunderstorm outflow, associated with an initial supercell. This raised the moist layer to 1–2km above mean sea level in the area affected by the record-breaking hailstorm. The vertical profile was characterized by an intense south-westerly flow in the mid-troposphere. Additionally, there was anomalously high water-vapor transport in the layer 2–5 km above mean sea level. Consequently, high CAPE seems unnecessary for the occurrence of giant hailstorms in the region.

This hypothesis is then assessed performing a statistical analysis p for the 2018–2023 period in NE Italy, using hail reports from the Pretemp database and observed high-rez Udine soundings. The results show that hail size has a much lower correlation with potential instability compared to kinematic parameters of the mid-troposphere and water-vapor transport. While thermodynamic parameters have better skill in predicting the occurrence of hail (or hail > 2 cm), the kinematic parameters (like water-vapor transport at 600 hPa, VT600= Wind x q at 600 hPa) of the mid-troposphere are better predictors for very large (> 5 cm) and giant (> 8 cm) hail events.

How to cite: De Martin, F., Manzato, A., Carlon, N., Setvák, M., and Miglietta, M. M.: Dynamic and statistical analysis of giant hail environments in northeast Italy, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-141, https://doi.org/10.5194/ecss2025-141, 2025.

P15
|
ECSS2025-168
Johanna Philipps, Hans Feyen, and Katharina Schröer

Hailstorms frequently cause severe damage to agriculture in Switzerland highlighting the need to better understand the characteristics of damaging hail events and their spatial and temporal patterns. Such knowledge is essential for improving the assessment and modeling of current and future hail risk to crops.

So far, approaches to assess crop hail damage have included radar, hail pad, and satellite-based methods, however they are often restricted to specific crops or hampered by the limited availability of exposure data and damage reports. Current challenges further include the uncertainty of radar-derived hail size estimates, which are often used as a proxy for hail intensity, as well as the uncertain relationship between hail size and actual crop damage.

To address these challenges and improve the link between observed hail characteristics and agricultural damage, this study combines various radar-based hailstorm indicators, such as the probability of hail (POH), maximum expected severe hail size (MESHS) and thunderstorm radar tracking data, with extensive and high-resolution exposure and damage data provided by the crop insurer Swiss Hail. This includes the policies insured at municipality level as well as damage reports for various crop types from 2014 to 2024. To evaluate which hazard indicators are most relevant for crop damage prediction, a random forest regression approach with feature selection techniques is applied.

First results indicate that combining multiple indicators can achieve robust model performance, particularly when including both municipality-scale hail characteristics (i.e. hail area and duration indicators, MESHS, velocity and mean reflectivity) as well as larger-scale information about the probability of hail and number of storms over a day. The most informative indicator is a proxy integrating the spatial extent and duration of hail occurrence within a municipality.

Based on these findings we perform a risk assessment of potential damage development under prospective future climatological conditions. To do so, we consider recent scientific findings on expected changes in hailstorm frequency and severity through a storyline-scenario approach. The scenarios are built through sampling characteristic hail days from the storm-object-based stochastic hail event set HailStoRe developed for the Swiss Hail Climatology.

How to cite: Philipps, J., Feyen, H., and Schröer, K.: Risk assessment for crop hail damage in Switzerland under current and potential future scenarios, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-168, https://doi.org/10.5194/ecss2025-168, 2025.

P16
|
ECSS2025-180
|
Francesco Sioni, Andrea Perbellini, Antonio Palmeri, Agostino Manzato, and Lorenzo Giovannini

The northeastern Italian plains are particularly prone to severe weather, due to the combined influence of moisture from the nearby Adriatic Sea and the orographic features of this region. These factors contribute to significant hailstorms with large to giant hailstones. This study investigates two of such events that occurred in this region.

In the early morning of 1 August 2021 a supercell developed, locally producing hailstones with diameters up to 9 cm. The second event, on 24 July 2023, involved two supercells, one of which produced a hailstone with the European record-breaking diameter of 19 cm. Notably, both events resulted in the largest hailstones being observed in the same location—the village of Azzano Decimo.

The main focus of this work is the best-possible simulation of these two events by means of the Weather Research and Forecasting (WRF) model at 1 km resolution, coupled with the HAILCAST hail growth parameterization, which provides estimates of the maximum hail size at the ground. The 1 August 2021 event is first examined through several simulations performed using different setups. The results highlight a significant sensitivity to the forcing meteorological model and the initialization time. In particular, WRF gives better results with ECMWF-IFS initial and boundary conditions with respect to GFS, especially when simulations are initialized more than 24 hours before the event. Moreover, results are significantly affected by the microphysical scheme and the land surface model, whereas the planetary boundary layer parameterization seems to have a minor influence. However, the development of the supercell is properly simulated, with hailstone diameters comparable to observations, only when data from radiosoundings of Udine Rivolto are nudged into the model.

To validate the model setup, the 24 July 2023 event was also simulated, incorporating all available radiosonde data. The model was able to reasonably simulate two supercells with hailstone diameters up to 10 cm. This study shows the significant impact that radiosonde data nudging can have on convective simulations, recommends a WRF setup that produces reliable numerical predictions, and demonstrates the effectiveness of HAILCAST in accurately simulating giant hail events.

The upcoming physical analysis, taking advantage of the best simulations and of the observations available for the two events (including polarimetric radar variables and ground-based weather stations), will investigate common patterns to identify the dynamic and thermodynamic conditions that contribute to large hail production in this peculiar region of the northeastern Italian plains.

How to cite: Sioni, F., Perbellini, A., Palmeri, A., Manzato, A., and Giovannini, L.: Numerical simulations of two giant hail events in northeastern Italy with WRF-HAILCAST, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-180, https://doi.org/10.5194/ecss2025-180, 2025.

P17
|
ECSS2025-189
Sophie Löbel, Ulrich Blahak, Markus Schultze, and Alberto de Lozar

Large hail can cause considerable damage (e.g. crop losses in agriculture or damage to house roofs) and so the predictioon of its maximum size is of particluar interest to the population. Our aim is to provide an estimation of the size of large hailstones at the surface from the forecasts of the Rapid Update Cycle ICON-RUC. The ICON-RUC produces hourly updated forecasts for Germany with a two-moment microphysics scheme, which particularly improves the prediction of severe convective storms. The prognostic variables of the two-moment scheme are the mass and the number concentrations of each hydrometeor, including hail. This allows a direct calculation of the mass-weighted mean diameter for hail, which can serve as an indication of the larger particles in the distribution.

Unfortunately, there are no area-wide hail observations over Germany that could be taken as the real truth.  However, the DWD's weather warning app (WarnWetter) offers the option of submitting reports on the current weather situation. This also includes hail. Although the accuracy of the individual reports cannot be determined, the data as a whole can still be a good help to evaluate the predicted hail size in the model. In addition, there are estimates of hail size from radar reflectivities, which can also be used to determine the adjustment for estimating the maximum hailstone size on the surface.

Days from the 2024 convective season are evaluated. These are matched with the hailsizes from the radar database for quality control and then compared to  model forecasts from the ICON-RUC. This provides information on how accurate the hail forecast is (location and time errors) and whether the estimate of the (average) hail size is realistic. In addition, we investigate how to correct the mean averaged hail size in order to obtain a realistic maximum possible diameter on the ground. In the end, this should help to improve the overall hazard assessment of a thunderstorm and thus minimize the hazard risk.

How to cite: Löbel, S., Blahak, U., Schultze, M., and de Lozar, A.: Evaluation of the hailstone size of certain hail events over Germany in 2024, comparison with ICON-RUC forecasts and estimation of the maximum hail size., 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-189, https://doi.org/10.5194/ecss2025-189, 2025.

P18
|
ECSS2025-207
|
Matthew Kumjian, Lydia Spychalla, and Kelly Lombardo

Hailstone growth trajectory models are increasingly being used to understand complex processes in hailstorms and to elucidate environmental controls on hail production. These trajectory models often are microphysically detailed, explicitly representing all relevant hail growth processes. Less attention has been paid to hailstone aerodynamic behaviors. Typically, hailstone motion throughout the storm is modeled by a combination of hailstone fall speed and advection: A hailstone’s vertical motion is the difference between the storm’s vertical velocity and the hailstone’s terminal velocity, and its horizontal motion is given by the storm’s horizontal winds. The hailstone is assumed to instantaneously adjust to the storm’s wind fields at each time step.

However, relative to other hydrometeors, hailstones have substantial mass, and thus inertia, which prevents an instantaneous adjustment to the storm’s wind fields. Especially for larger (more massive) hailstones, the adjustment timescale can be several seconds. This means the hailstone can move through the storm with a horizontal velocity vector that is different than the storm’s horizontal wind vector. This has implications for the vector at which hailstones impact surfaces (and thus damage potential), as well as for hailstone growth. Typically, hailstone growth by collection is assumed to occur only in the vertical; hailstone inertia can lead to collection in three dimensions, which can increase growth rates.

In this study, we examine the impact of including hailstone momentum/inertia on their trajectories and growth. The theory is developed, and implemented in a series of simple, idealized flows. Then, hailstone inertia is implemented in a full-physics trajectory model. The impact of explicitly considering hailstone inertia is quantified and compared to other sources of uncertainty in trajectory models (including uncertainty in fall speeds).

How to cite: Kumjian, M., Spychalla, L., and Lombardo, K.: Hailstone Inertial Adjustment to Storm Wind Fields and Implications for Growth, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-207, https://doi.org/10.5194/ecss2025-207, 2025.

P19
|
ECSS2025-210
|
Lena Wilhelm, Valentin Gebhart, Olivia Martius, and Aessia Boukhatmi

 The rapid expansion of photovoltaic (PV) systems is transforming the renewable energy landscape, but extreme weather events, particularly hailstorms, pose an increasing threat to energy production and infrastructure longevity. Recent studies show that both hail frequency and intensity in Switzerland have risen over the past six decades (Wilhelm et al., 2024) and are projected to continue increasing in a warming climate (Thurnherr et al., 2025), leading to growing damage costs for PV installations in Switzerland. We present a newly launched interdisciplinary research project — a collaboration between scientific institutions, (re-)insurance companies, and industry partners, aimed at improving hail risk assessment and resilience strategies for PV systems in Switzerland. Using an open-source inventory of installed PV systems and high-resolution radar-based hail data, we identified hail damage hotspots in regions including Ticino, Thun, Basel, and Lucerne. By linking energy production data with damage claims, we find that hail can reduce the median operational lifetime of PV systems by up to two years. Preliminary analyses further suggest that tilt
 angle, orientation, and module type significantly influence vulnerability to hail. Building on these insights, we will conduct a comprehensive analysis of multiple aspects of PV hail damage. This includes:
1. Identifying the hailstorm and PV system characteristics, such as hail size, storm orientation, tilt angle, and module type, that influence real-world damages;
2. Producing high-resolution risk maps that distinguish current and future ”high-risk” from ”low-risk, high-capacity” areas using convection-permitting simulations under a 3°C warming scenario;
3. Quantifying the short-, medium-, and long-term economic impacts of hail damage on PV systems;
4. Evaluating technical and strategic adaptation options to enhance system resilience.
Our approach combines meteorological, energy production, and damage data to quantify evolving hail risks and guide actionable solutions. This work will support more resilient PV planning and help energy providers, insurers, and policymakers adapt to an era of intensifying extreme weather.

How to cite: Wilhelm, L., Gebhart, V., Martius, O., and Boukhatmi, A.: Hail risk to photovoltaic systems in Switzerland, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-210, https://doi.org/10.5194/ecss2025-210, 2025.

P20
|
ECSS2025-223
|
Mathis Tonn, Susanna Mohr, Jannik Wilhelm, Christian Sperka, Markus Augenstein, and Michael Kunz

Severe hail events are comparatively rare, yet they contribute a significant portion of the total insured losses each year in Germany and worldwide. Single events with large hailstones in the past have caused major damage, such as the severe Reutlingen hailstorm on July 28, 2013, with hail diameters up to 10 cm, causing costs of more than EUR 1 billion. Additionally, hailstorms with smaller hailstones often cause substantial damage to building facades and roofs, photovoltaic systems, vehicles, and agricultural areas. Given the considerable potential for damage, it is crucial to gain a better understanding of the behavior of hailstorms in the context of a changing climate.

As a data basis for hail, twenty summer half-years (2005 – 2024) of potential hail tracks in different intensity classes over Germany are used. These tracks were derived using a modified version of the TRACE3D tracking algorithm based on 3D radar data from the C-Band radar network of the German Weather Service (DWD). From these hail events, the ambient thermodynamic and dynamic conditions are extracted and compared with ambient conditions of non-events, taken from a similar environment on days without cell activity. This establishes that the most suitable proxy variables for the hail events of different intensity classes can be determined.

Preliminary findings suggest that the use of a combination of a lifted index for atmospheric stability, the moisture content of the layer above the lifted condensation level, and the layer thickness between the equilibrium level and the -10°C isotherm are especially promising. Besides others, these parameters serve as the basis for a logistic regression used for estimating hail occurrence from ERA5 data. We combine the parameters with information about the triggering, such as fronts and anomalies in potential vorticity.

Longer periods than only twenty years are required to determine the extent to which climate change influences hail frequency and intensity. For this purpose, the hail model can also be applied to climate simulations to estimate future changes in hail frequency under various warming scenarios. 

How to cite: Tonn, M., Mohr, S., Wilhelm, J., Sperka, C., Augenstein, M., and Kunz, M.: Estimation of hail frequency in Germany and its trends under climate change , 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-223, https://doi.org/10.5194/ecss2025-223, 2025.

P21
|
ECSS2025-229
Amruta Vurakaranam, Christian Berndt, Katharina Lengfeld, Lukas Josipovic, Markus Schultze, and Katharina Schröer

Hail remains one of the most challenging and least understood severe weather hazards in Germany, posing significant challenges for forecasting and contributing to substantial economic losses, particularly in agriculture, infrastructure, and related insurance sectors. While the occurrence and probability of hail have been studied, estimating hail size remains a key open research question from both a forecasting and a climatological perspective.

This study is part of the HAIPI project (Hailstorm Analysis, Impact, and Prediction Initiative) funded by the German weather service DWD, which aims to improve hail size estimation by leveraging various newly developed datasets. These include advanced polarimetric radar products, numerical weather prediction (NWP) outputs, lightning data, and crowd-sourced observations from platforms such as the European Severe Weather Database (ESWD) and the DWD WarnWetter app.

We present first results from a set of tree-based machine learning approaches, including Random Forests and Gradient Boosting methods. These models incorporate atmospheric variables such as convective available potential energy (CAPE), wind shear, and radar products from the DWD’s KONRAD3D forecast system. A comparative analysis of model performance is conducted for both binary classification—distinguishing between severe and non-severe hail using various threshold definitions—and multiclass classification, categorizing hail sizes into three groups: Category 1 (<2 cm), Category 2 (2–5 cm), and Category 3 (≥5 cm).

A preliminary model achieves around 70% accuracy with balanced performance across hail size classes, demonstrating strong potential for operational forecasting. Feature importance analysis identifies radar-derived vertical extent features (e.g., vertical_extent, echo_top_threshold_55dBZ) and model-based reflectivity metrics (e.g., cell_based_VIL) as key predictors. These initial findings highlight the value of integrating radar, model-based, and crowd-sourced data to improve hail size prediction.

How to cite: Vurakaranam, A., Berndt, C., Lengfeld, K., Josipovic, L., Schultze, M., and Schröer, K.: Exploring Tree-Based Machine Learning Methods for Estimation of Hail Sizes, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-229, https://doi.org/10.5194/ecss2025-229, 2025.

P22
|
ECSS2025-236
|
Christian Sperka, Markus Augenstein, Mathis Tonn, and Michael Kunz

Hail is among the most destructive hazards associated with severe convective storms. Nevertheless, direct observational records are limited. We therefore based our analysis of changes in hail frequency and intensity in response to climate change on severe convective cell tracks identified over 20 years from 3D radar data of the German Weather Service (DWD). These tracks are supplemented and validated with lightning detections, hail reports from the European Severe Weather Database, and insurance claims.

To establish a link between hail occurrence and its environmental drivers, convolutional neural networks (including U-Net architectures) are trained on convective parameters from ERA5 reanalysis to predict hail events. These models facilitate the simulation of hail climatologies and the estimation of hail occurrence for periods without observational data, thereby extending trend analyses into the more distant past.

Trend analyses of the radar-based tracks show a distinct spatial pattern: while a significant increase in hail activity in southern Germany is observed, no or slightly negative trends in northern Germany have been identified. The ML models demonstrate a high degree of success in replicating this distinct spatial pattern, thus indicating that the observed trends are likely driven by changes in large-scale convective environments rendered by the models. Current efforts are centered on the quantification of the relative importance of individual convective parameters for hail prediction. This will offer further insight into the physical drivers behind these changes.

The insights gained into the physical mechanisms behind hail formation enhance our ability to interpret and constrain hail projections in future climate scenarios. This bridges the gap between past climatologies and future risks.

How to cite: Sperka, C., Augenstein, M., Tonn, M., and Kunz, M.: Hail Trend Estimation in Germany utilizing Radar-based Hail Tracks, Convective Parameters, and Machine Learning Techniques, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-236, https://doi.org/10.5194/ecss2025-236, 2025.

P23
|
ECSS2025-237
Susanna Mohr, Mathis Tonn, Markus Augenstein, and Michael Kunz

A nationwide 3D spatio-temporal homogeneous radar composite for Germany has been created using 16 single-polarization C-band radars, covering now a period of 20 years. This dataset enables a detailed analysis of hail statistics, including regional differences, as well as preliminary estimates of long-term changes and emerging trends.

The TRACE3D tracking algorithm for severe convective cells with potential hail signals (> 55 dBz) was used to identify 13,324 potential hail tracks (PHTs) during the summer half-year (2005 – 2024). The spatial distribution of these PHTs reveals distinct regional patterns, including a north-south gradient influenced by the proximity of northern Germany to the North Atlantic and by orographic features. The highest hail frequency occurs south of Stuttgart, in the Neckar Valley, over the Swabian Jura, and over the foothills of the Alps. Most tracks are shorter than 45 km and last less than 75 minutes (both 75th percentile). Around 50% of the tracks follow a flow direction between south and west, aligning with typical mid-tropospheric conditions that favor convection. Furthermore, half of the days with PHTs are associated with atmospheric blocking regimes, such as Scandinavian, European, and Greenland blocking.

Temporally, hail events in Germany are unevenly distributed, with 63 % of days recording no PHTs and only infrequent periods of intense hail activity with many tracks on a day. Although many hail days usually tend to be isolated (~ 43 %), clustering of hail days can occur under specific synoptic conditions; however, such sequences rarely extend beyond two weeks.

Trend analyses reveal a high annual variability in the number of PHTs, with no clear nationwide trend over the past 20 years. However, significant regional differences emerge: In northern and central Germany, there are generally no statistically significant trends, although a slight downward tendency can be observed. In contrast, southern Germany exhibits a significant increase in the number of days with PHTs.

How to cite: Mohr, S., Tonn, M., Augenstein, M., and Kunz, M.: A 20-year spatio-temporal analysis of 3D radar-based hail tracks in Germany: Trends and regional differences, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-237, https://doi.org/10.5194/ecss2025-237, 2025.

P24
|
ECSS2025-240
Alexey Bugrimov, Alexander Chernokulsky, Sergey Davletshin, Konstantin Pustovalov, Andrey Shikhov, and Alexander Sprygin

Large hail is a hazardous convective phenomenon that causes significant socioeconomic damage. Although climate change has led to an increase in severe convective events in several Russian regions, the statistics of large hail occurrences in Russia remain understudied. For the first time, this work compiles a comprehensive database of hail events in Russia from 1906 to 2024. Sources include ESWD data, routing meteorological observations, news and social network information, and existing scientific literature. The database contains over 12,000 hail reports, including more than 4,000 reports of large hail. 

A comparative analysis of hail events and lightning activity, based on WWLLN data from 2016 to 2024, reveals a statistically significant difference in the characteristics of lightning between hail and non-hail cases. The skill score analysis enables the determination of the optimal frequency of lightning flashes for identifying severe hail occurrences. Lightning data were used to specify the time and place for some hail cases in the presented database.

Analysis of the collected database revealed an exponential distribution of hail sizes, with a median diameter of 2 cm and a 95th percentile of 5 cm. The spatial distribution of hail generally reflects population density, with the highest frequencies (including hail larger than 10 cm in diameter) occurring in southern and central European Russia and southern Western Siberia. The temporal distribution of hail reports revealed a pronounced annual cycle, with a peak in June, as well as a diurnal cycle, with a peak around 16:00 local time.

To evaluate the atmospheric conditions associated with hail formation, thermodynamic and dynamic indices were calculated for hail events during the warm season (May–August) between 2010 and 2020, using ERA5 reanalysis data at an hourly temporal resolution and a 25 km spatial resolution. Statistically significant relationships were found between index values and the occurrence and size of hail. The most informative indices and their threshold values were identified for diagnosing hail of various sizes.

The study was supported by the Russian Science Foundation (grant no 24-17-00357).

How to cite: Bugrimov, A., Chernokulsky, A., Davletshin, S., Pustovalov, K., Shikhov, A., and Sprygin, A.: Climatology and formation environments of large hail in Russia, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-240, https://doi.org/10.5194/ecss2025-240, 2025.

P25
|
ECSS2025-253
|
Clotilde Augros, Vincent Forcadell, Louis Tariot, Pierre Lepetit, Olivier Caumont, Thibaut Montmerle, and Kevin Dedieu

Hail is a significant severe weather hazard in France, capable of causing substantial damage to agriculture, vehicles, infrastructure and solar installations. For example, a severe hailstorm over Paris on 3 May 2025 resulted in insured losses exceeding €300 million. Despite the operational use of weather radar for hail detection and size estimation, current methods (such as fuzzy logic hydrometeor classification algorithms or hail proxies using vertical profiles of reflectivity) remain limited in their ability to estimate the occurrence of severe hail (>2 cm) and discriminate its size on the ground. Notably, they overlook information embedded in storm morphology.

At Météo-France, a new approach using convolutional neural networks (CNNs) has been developed to better exploit storm morphology, initially for severe hail detection. This method uses a single-timestep input comprising 19 radar-derived features, including quality-controlled polarimetric variables and storm severity diagnostics (e.g. ECHOTOP45, VIL, MESH…). These are fed into a CNN trained to predict severe hail occurrence over 30x30 km² areas. Hail cases were selected using the ESWD, while non-hail cases came from storms over densely populated areas without hail reports. Experimental results show that CNNs outperform existing hail proxies, especially when those proxies are used as input features (Forcadell et al., 2024).

This methodology has been adapted for estimating hail size, which is framed as a multi-class classification problem involving three categories: medium (20–35 mm), large (35–50 mm) and giant (≥50 mm) hail. A new radar dataset was created by extracting image sequences centred on convective cell centroids, which were tracked using a dedicated algorithm. Each sample spans six timesteps over 25 minutes, thus incorporating the storm’s temporal evolution. Several CNN architectures were tested; models using multiple prior timesteps proved more robust than those based on a single timestep. Feature importance analysis identified radar echo top as the most predictive input, followed by polarimetric variables below the freezing level.

These findings, detailed in Forcadell, V. (2024), form the basis for ongoing work. New datasets covering 2024 and 2025 hail events are currently being assembled to improve generalization and further validate the model. The methodology and updated evaluation results of this CNN-based hail size estimation algorithm will be presented.

References
Forcadell, V. (2024). PhD Thesis, Université de Toulouse. https://theses.hal.science/tel-05070872
Forcadell, V., et al. (2024). Atmos. Meas. Tech., 17(22), 6707–6734. https://doi.org/10.5194/amt-17-6707-2024

How to cite: Augros, C., Forcadell, V., Tariot, L., Lepetit, P., Caumont, O., Montmerle, T., and Dedieu, K.: Towards Improved Hail Detection and Size Estimation Using Convolutional Neural Networks, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-253, https://doi.org/10.5194/ecss2025-253, 2025.

P26
|
ECSS2025-255
Gokul Kavil Kambrath and Michael Kunz

Hailstorms are among the most damaging convective weather hazards in Europe, causing significant losses to infrastructure, vehicles, agriculture, and energy systems. However, reliably detecting and characterizing hail in real time remains a major challenge.

This study aims to improve existing hail detection approaches by combining polarimetric radar observations and environmental data using machine learning techniques. We utilize dual-polarization radar data from the C-band radar operated at the Karlsruhe Institute of Technology (KIT), which provides key variables, such as reflectivity, differential reflectivity, specific differential phase, and correlation coefficient. Convective cells are identified and tracked using the storm tracking algorithm TRACE3D, which performs object-based tracking and incorporates morphological analyses and pattern recognition to extract features indicative of severe convection, including size, shape, echotop height, temporal development, and motion characteristics. These cell objects are linked to environmental predictors derived from numerical weather prediction models, including Convective Available Potential Energy (CAPE), Lifted Index (LI), and storm-relative helicity (SRH), which are known to strongly influence hail formation. Ground-truth verification is supported by hail size reports from the European Severe Weather Database (ESWD), crowd-sourced observations via the DWD WarnWetter app, and insurance claim records. For the estimation of hail probability and hailstone size, we apply machine learning models such as logistic regression, random forest, and convolutional neural networks (CNNs), using combined radar and environmental features as input.

At the time of the conference, we anticipate presenting first results on model performance, predictor relevance, and detection accuracy. The object-based approach of our study enables integration into operational radar systems and supports more accurate, timely hail warnings for improved risk mitigation in weather-sensitive sectors.

How to cite: Kavil Kambrath, G. and Kunz, M.: Near-real-time probabilistic Hail Detection based on polarimetric radar quantities and environmental conditions using machine learning methods, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-255, https://doi.org/10.5194/ecss2025-255, 2025.

P27
|
ECSS2025-262
|
Tomas Pucik, Mateusz Taszarek, Pieter Groenemeijer, and Francesco Battaglioli

Recent years have brought devastating hailstorms across Europe with large economic losses and hundreds of injuries. We study 315 European hailstorm cases from 2021 to 2024 that produced at least two reports of hail 5 cm or larger (i.e., very large), using the European Severe Weather Database, their proximity environments using the ERA-5 reanalysis, and storm motion inferred from the composite radar data (such as OPERA). 

Supercells are often considered by the forecasters to be long-lived storms. However, as evidenced in our study, only 77 out of 315 studied hailstorms produced large hail for at least 100 km, and only 86 lasted at least one hour. All 4 supercells of 24 July 2023 that affected Italy, Slovenia, and Croatia had hail swaths longer than 200 km, including the storm that set the European hail record of 19 cm. On 13 July 2023, a single supercell tracked for at least 686 km and lasted more than 9 hours. Here we look at how the pre-convective environment influences the length of the hail swath, a characteristic less explored in the existing literature compared to the observed hail size.

We first considered the individual 1-D vertical profiles of temperature, moisture, and horizontal wind representing the conditions in the area with the largest observed hailstone per hailstorm. We found that the storms with longer hail swaths formed in environments of higher storm-relative helicity, stronger inflow, lower cloud bases, and weaker cold pool potential. Of the kinematic parameters, observed storm motion was best correlated with the hail swath length.

In the second part of the study, we investigate the spatial distribution of pre-convective environments parallel and perpendicular to the hailstorm path, using the radar-derived storm-motion vectors. We hypothesize that longer-lived hailstorms feature larger areas of favourable environments parallel to the path. We also wonder whether the longer-lived hailstorms stay near low-level boundaries or move away from them to prevent the upscale growth. Results of this study advance our understanding of the controls of the supercell and their hail production maintenance.

How to cite: Pucik, T., Taszarek, M., Groenemeijer, P., and Battaglioli, F.: Anything from 10 to 686 km, or what influences the hail swath length in supercells?, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-262, https://doi.org/10.5194/ecss2025-262, 2025.

P28
|
ECSS2025-312
John Allen, Ian Giammanco, Rebecca Adams-Selin, Brenna Meisenzahl, Jake Sorber, Julian Brimelow, Aaron Kennedy, Hannah Vagasky, Daniel Dawson, Sabrina Servey, Kyle Brooks, Kaleb Clover, Madeleine Richer, Mark Gartner, Talia Kurtz, and Teagen Schultz

Detailed ground observations of hailstones are historically rare, particularly as it relates to properties that describe hail beyond its maximum single axis diameter, or in sampling the hail swath in substantive detail. To address this gap the In Situ Collaborative Experiment for the Collection of Hail in the Plains (ICECHIP) campaign was conducted between May 15 and June 28th of 2025. Active periods of convection persisted throughout the campaign yielding over 20 intensive observation periods. These included measurement of hail in numerous storms producing 50 mm or greater hail, with both in situ measurement platforms and post-storm transects of the hailswaths sampled close to time of fall in cooled environments and regularly thereafter  at horizontal resolutions in the hundreds of meters. 

Five types of instruments focused on direct hail capture: impact disdrometers with video cameras and hailpads formed the bulk of the sensing array, deployed ahead of the storm. These were complemented by mesonet pods for near-storm environment and SUMHOs, (Super Mobile Hail Observatory) deployable instrumented supersites that funnel hail into cooled storage with colocated hailpad, and measure hailstone fall speed using vertical pointing radar. High resolution and speed video cameras additionally captured hail fall speed and orientation. These were operated in a range of array configurations to best sample storm evolution or the swath at impressive resolution. Post storm sampling accumulated thousands of hailstones, and performed 2-3 axial dimensional measurements along with mass, and for a subset of stones exceeding 2cm, compressive strength testing via crushing.

This presentation will focus on three exemplary cases, a supercell in northeast Colorado producing a 14 mile-wide swath with hail diameters reaching 90 mm, a merging supercell that produced giant hailstones measuring as large as 150mm, and a non-supercell case producing extremely soft accumulating hail. Hailstone size and sphericity distributions, compressive strength properties and mass will be compared across the respective swaths to provide preliminary insights into the variability of hail and its potential for damage under different classes of storms.

How to cite: Allen, J., Giammanco, I., Adams-Selin, R., Meisenzahl, B., Sorber, J., Brimelow, J., Kennedy, A., Vagasky, H., Dawson, D., Servey, S., Brooks, K., Clover, K., Richer, M., Gartner, M., Kurtz, T., and Schultz, T.: Ground Observations from the In Situ Collaborative Experiment for the Collection of Hail in the Plains, 12th European Conference on Severe Storms, Utrecht, The Netherlands, 17–21 Nov 2025, ECSS2025-312, https://doi.org/10.5194/ecss2025-312, 2025.