AS1.11 | Mesoscale and severe convection over land: processes, modelling advances, predictability, and impacts
Orals |
Wed, 16:15
Thu, 16:15
EDI
Mesoscale and severe convection over land: processes, modelling advances, predictability, and impacts
Convener: Julia CurioECSECS | Co-conveners: Cornelia KleinECSECS, Irene Livia KruseECSECS, Yanyan Cheng, Kalli Furtado, Jian Li
Orals
| Wed, 30 Apr, 16:15–18:00 (CEST)
 
Room 0.11/12
Posters on site
| Attendance Thu, 01 May, 16:15–18:00 (CEST) | Display Thu, 01 May, 14:00–18:00
 
Hall X5
Orals |
Wed, 16:15
Thu, 16:15

Orals: Wed, 30 Apr | Room 0.11/12

Chairpersons: Julia Curio, Cornelia Klein, Irene Livia Kruse
16:15–16:20
Impacts of severe weather
16:20–16:30
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EGU25-6673
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Highlight
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On-site presentation
Recent developments in tornado theory and observations
(withdrawn)
Richard Rotunno and Howard Bluestein
16:30–16:40
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EGU25-11230
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On-site presentation
Artur Surowiecki, Natalia Pilguj, Mateusz Taszarek, Krzysztof Piasecki, Tomáš Púčik, and Harold Brooks

In this work, we use 8 years (2014–2021) of Operational Programme for the Exchange of Weather Radar Information (OPERA) radar data, lightning detection network (ATDnet) data, and severe weather reports to create a climatology of quasi-linear convective systems (QLCSs) in Europe. In the first step, 15-min OPERA radar scans were used to identify 1475 QLCS cases. The manual investigation of each individual led to the recognition of QLCS morphological and precipitation archetypes, areal extent, width, length, duration, speed, forward motion, accompanying hazards, injuries, and fatalities. Severe weather reports, lightning data, and morphological properties were used to classify QLCSs according to their intensity into 1151 marginal (78.0%), 272 moderate (18.5%), and 52 derecho (3.5%) events. Spatio-temporal analysis indicate that QLCSs are the most frequent during summer in Central Europe, while in southern part of Europe their occurrence is extended to late autumn. A bow echo morphological archetype occurred in around 29% of QLCS cases, while a mesoscale convective vortex occurred in almost 9%. Among precipitation modes, trailing and embedded stratiform types accounted for around 50% of QLCSs. Based on ESWD Database we found that the most frequent QLCS-related hazard was lightning (taking up on average 94.4% of the area impacted by QLCS), followed by severe wind gusts (7.9%), excessive precipitation (6.1%), large hail (2.9%), and tornadoes (0.5%). Derechos had the largest coverage of severe wind reports (49.8%), while back-building QLCSs were mostly associated with excessive precipitation events (13.5%). QLCSs caused 104 fatalities and 886 injuries. Nearly half of all fatalities and injuries were associated with only the 10 most impactful QLCS events, mostly warm-season derechos producing severe to extreme widespread wind gusts.

How to cite: Surowiecki, A., Pilguj, N., Taszarek, M., Piasecki, K., Púčik, T., and Brooks, H.: Quasi-Linear Convective Systems and Derechos across Europe: Climatology, Accompanying Hazards, and Societal Impacts, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-11230, https://doi.org/10.5194/egusphere-egu25-11230, 2025.

16:40–16:50
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EGU25-13858
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On-site presentation
Timothy Raupach, Raphael Portmann, Christian Siderius, and Steven Sherwood

Hail can injure people and damage infrastructure, with hailstorms a driving cause of insured losses. Hailstorms are expected to be affected by global warming, primarily via changes to atmospheric instability, wind shear, and the height of the melting level. However, the nuances of expected changes remain uncertain and are generally only studied regionally, partly because global climate models typically lack the fine grid spacing required to explicitly resolve hailstorms. Here, we show global projections using an ensemble of four hail proxies to estimate hail-prone conditions occurrence frequency in eight global climate models. We use a temperature-based framework and show projected changes in global hail hazard frequency in scenarios with two and three degrees of warming over a recent historical period. By analysing changes in the "ingredients" for the proxies we can determine which factors are most pertinent to the changes in hail-prone conditions. Under global warming, the multi-model multi-proxy results show general poleward shifts in hail-prone condition frequency, and shifts from the warm season to the cool season in many regions. The results reinforce the benefit of using proxies designed specifically for hail for such studies, since some more general thunderstorm proxies neglect the effects of temperature and can show significantly different results. Finally, we use our results to analyse changes in hail exposure to various crops worldwide. This work encompasses the first global projections for severe storms using proxies specifically designed for hailstorms.

How to cite: Raupach, T., Portmann, R., Siderius, C., and Sherwood, S.: Global projections of hail hazard frequency under climate change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13858, https://doi.org/10.5194/egusphere-egu25-13858, 2025.

Storm dynamics and land-atmosphere interactions
16:50–17:00
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EGU25-5461
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ECS
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On-site presentation
Hongpei Yang and Yu Du

Secondary convective initiation (SCI) ahead of mesoscale convective systems, such as squall lines, is a globally observed phenomenon. This study employs idealized numerical simulations to investigate the spatiotemporal characteristics of SCI and its connection to squall line evolution. In a typical mid-latitude environment, SCI frequently develops ahead of the squall line, subsequently modifying squall line’s morphology and intensity through processes like merging or shifting the leading edge, depending on their relative distance.

Over an 8-hour simulation, SCI becomes increasingly frequent and exhibits periodic explosive growth (outbreaks), primarily driven by distant SCI events (≥ 5 km from the leading edge), while the number of close SCI events (< 5 km) remains stable. Distant SCIs also extend progressively farther over time, with some forming over 100 km ahead. These SCIs are more likely to occur ahead of regions with locally stronger cold pools and higher radar reflectivity within the squall line. In contrast to close SCI events governed by spatial cold pool variability, SCI outbreaks consistently lag behind recurrent surges in cold pool intensity and are closely linked to the passage of n=2 gravity waves. These waves are characterized by upward motion in the lower troposphere and downward motion aloft. Their formation is primarily driven by strong evaporative cooling and the melting of hydrometeors within the squall line, which concurrently enhances the cold pool. As each n=2 wave propagates forward, its ascent induces adiabatic cooling and enhances low-level moisture, significantly humidifying and destabilizing the lower troposphere, thereby promoting each SCI outbreak. Moreover, the repeated wave generation and long-distance wave propagation (>300 km) amplify these effects, increasing SCI frequency and expanding its reach.

How to cite: Yang, H. and Du, Y.: Cold pool and Gravity Waves Drive Secondary Convective Initiation Ahead of Squall Lines, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5461, https://doi.org/10.5194/egusphere-egu25-5461, 2025.

17:00–17:10
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EGU25-7928
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ECS
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On-site presentation
Qian Wei, Jianhua Sun, Yuanchun Zhang, and Linlin Zheng

Using a convection initiation (CI) identification method designed for isolated convection, 11,646 CI events (CIEs) were identified based on composite reflectivity (CR) in the middle reaches of the Yangtze River Basin from May to September of 2016–2020. CIEs occur more frequently in July and August (62.7%) and from 11 BJT to 16 BJT (62.2%) with a diurnal peak at 12 BJT. CI area (area of the connected region with CR  40 dBZ at CI time) has a diurnal peak at 16 BJT, which is related to the frequent occurrence of large-area CIEs (LACIEs, 1%) with a CI area larger than 62 km². Most LACIEs occur under stronger atmospheric instability and higher vertical wind shear with the rapid intensification and expansion of convective regions after CI. Regions with high-frequency CIEs correspond well with mountain terrains. Mountain CIEs, which are under the weak unstable stratification and low vertical wind shear, occur about twice (5,831) as frequently as foothill or plain CIEs. Compared to other terrains, the local heterogeneity of soil moisture (SM) near CI locations is the strongest over the mountains. Mountain CIEs occur at the center of a high SM region located in the transition zone between the positive and negative SM gradients, with the highest SM gradient magnitude located to the north side of CI locations.

How to cite: Wei, Q., Sun, J., Zhang, Y., and Zheng, L.: Statistical Characteristics of Convection Initiation over Different Terrains in the Middle Reaches of the Yangtze River Basin Based on the Doppler Weather Radar Observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7928, https://doi.org/10.5194/egusphere-egu25-7928, 2025.

17:10–17:20
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EGU25-1567
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ECS
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On-site presentation
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Ben Maybee, Cornelia Klein, Christopher Taylor, Helen Burns, John Marsham, Douglas Parker, and Emma Barton

Understanding drivers and controls on Mesoscale Convective Systems (MCSs) is critical for predicting rainfall extremes and its impacts across time scales, from nowcasting to climate change. For MCSs over land, heterogeneity in surface fluxes across length scales presents a primary influence on storms. In West Africa, for example, MCS initiation is enhanced by ~20km scale gradients in soil moisture [1]; mature MCS cores are favoured over ~200km scale dry soil anomalies [2]; and the regional circulation responds to ~2000km scale soil moisture gradients [3], with this response explaining an observed intensification in MCSs over the last 30 years [4].

To better understand how MCSs respond to this spectrum of surface flux gradients, here we present a novel sensitivity experiment framework in which a convection-permitting Control simulation is reinitialised daily from a soil moisture field where we have modified the spectrum of surface variability using wavelet filtering. We conduct two scale experiments: one in which all sub-1000km scale soil moisture variability is suppressed; and one in which we return sub-mesoscale variability. The Control simulation is run at 1.5km over West Africa for 40 days using the Met Office Unified Model and features realistic land-surface and radiation schemes and a full suite of moisture tracers. Combining results from this simulation and outputs from 2-day long sensitivity experiments gives 200 days of CP data, enabling investigation of the impact of land-surface heterogeneity on MCSs in unprecedented detail.

We hereby elucidate the chain of mechanisms through which variability in mesoscale soil moisture anomalies propagates through surface fluxes to planetary boundary layer (PBL) fields and the regional circulation, and crucially, the effect on MCS lifecycles and intensities. We find a substantial reduction in MCSs when all sub-1000km soil moisture variability is suppressed, with numbers recovering when <100km scale variability is reintroduced. Precursor PBL fields found at MCS core locations in all experiments are consistent with those about relatively dry mesoscale soil moisture anomalies. However, the relative control of soil moisture and insolation on heat fluxes is modified in the sensitivity experiments, indicating that PBL conditions preferential for mature MCS cores are achieved via different controls and at different frequencies, affecting storm populations.

References

  • Taylor et al, Frequency of Sahelian storm initiation enhanced over mesoscale soil-moisture patterns. Nature Geoscience 4, 430-433 (2011)
  • Klein and Taylor, Dry soils can intensify mesoscale convective systems. Proceedings of the National Academy of Sciences, 202007998, (2020)
  • Cook, Generation of the African Easterly Jet and Its Role in Determining West African Precipitation, Journal of Climate 12(5), 1165–1184 (1999)
  • Taylor et al, Frequency of extreme Sahelian storms tripled since 1982 in satellite observations. Nature 544, 475-478, (2017).

How to cite: Maybee, B., Klein, C., Taylor, C., Burns, H., Marsham, J., Parker, D., and Barton, E.: How does the spatial scale of surface flux variability affect MCS properties?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1567, https://doi.org/10.5194/egusphere-egu25-1567, 2025.

17:20–17:30
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EGU25-5857
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ECS
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On-site presentation
Eliza Karlowska, Andrew G. Turner, and Steven Woolnough

The Lake Victoria region is inhabited by over 40 million people and is a major source of food, water and economic activity in East Africa. As the intertropical convergence zone passes by, this region experiences two rainy seasons that result in extreme precipitation events and flash flooding. Over 80% of extreme rainfall around Lake Victoria is produced by mesoscale convective systems (MCSs), which are characterised by organised convection spanning a few hundred kilometres, and often lasting several hours. Here, we tracked 4,811 MCSs between 2014 and 2019 that moved over Lake Victoria and lasted longer than 3 hours. A clustering algorithm was applied to identify different types of MCSs crossing this region: cross-lake storms that initiate overnight East Africa time, lake-to-land storms that initiate in the morning, and land-to-lake storms that initiate in the afternoon. We examined conditions of the local environment leading to the development of these storms to link them to larger scale climate variability, such as the Madden-Julian Oscillation (MJO). The MJO is an eastward-propagating envelope of suppressed and enhanced convection that originates over the western Indian Ocean. Active MJO convection over the western Indian Ocean (MJO phase 2) creates favourable zonal wind anomalies for the formation of lake-to-land and land-to-lake storms. In addition, MJO phase 2 is also likely to influence specific humidity and temperature anomalies prior to and during the formation of land-to-lake storms. Conditions over the Lake Victoria region during days when no storms occur are similar to the conditions created during active MJO phase 6, i.e., when active MJO convection is over the Maritime Continent. Our analysis is used to inform a machine learning model that will predict the probability of a given storm type occurring over this region in order to improve predictions of high-impact weather over the lake.

How to cite: Karlowska, E., Turner, A. G., and Woolnough, S.: Controls on the convective environment in the Lake Victoria region and their interactions with large-scale climate variability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5857, https://doi.org/10.5194/egusphere-egu25-5857, 2025.

Km-scale modelling
17:30–17:40
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EGU25-9414
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On-site presentation
Andreas F. Prein, Die Wang, Ming Ge, Alexandra Ramos Valle, and Manda Chasteen

Organized deep convection plays a critical role in the global water cycle and drives extreme precipitation events in tropical and mid-latitude regions. However, simulating deep convection remains challenging for modern weather forecasts and climate models due to the complex interactions of processes from microscales to mesoscales. Recent models with kilometer-scale (km-scale) horizontal grid spacings (∆x) offer notable improvements in simulating deep convection compared to coarser-resolution models. Still, deficiencies in representing key physical processes, such as entrainment, lead to systematic biases. Additionally, evaluating model outputs using process-oriented observational data remains difficult. In this study, we present an ensemble of MCS simulations with ∆x spanning the deep convective grey zone (∆x from 12 km to 125 m) in the Southern Great Plains of the U.S. and the Amazon Basin. Comparing these simulations with Atmospheric Radiation Measurement (ARM) wind profiler observations, we find greater ∆x sensitivity in the Amazon Basin compared to the Great Plains. Convective drafts converge structurally at sub-kilometer scales, but some discrepancies, such as too-deep up- and down-drafts and too-weak peak downdrafts in both regions or too-strong updrafts in Amazo- nian storms remain. Overall, we observe higher ∆x sensitivity in the tropics, including an artificial buildup in vertical velocities at five times the ∆x, suggesting a need for ∆x≤250 m. Nevertheless, bulk convergence – agreement of storm average statistics – is achievable with km-scale simulations within a ±10 % error margin, with ∆x=1 km providing a good balance between accuracy and computational cost.

How to cite: Prein, A. F., Wang, D., Ge, M., Ramos Valle, A., and Chasteen, M.: Grid Spacing Sensitivity of Simulated Convective Drafts in Tropical and Mid-Latitude Mesoscale Convective Systems, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9414, https://doi.org/10.5194/egusphere-egu25-9414, 2025.

17:40–17:50
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EGU25-9830
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ECS
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On-site presentation
Puxi Li

Mesoscale convective systems (MCSs), as major contributors to extreme precipitation events, have garnered significant attention in the context of global warming. In 2020, vast areas of East Asia—downstream of the Tibetan Plateau (TP) and home to over 30% of the global population—experienced an anomalously wet rainy season, marked by intense MCS-induced precipitation that resulted in severe socio-economic impacts and extensive losses.

This study leverages the first ensemble run of kilometer-scale (~4 km) WRF simulations for the Water Year 2020 (WY2020) under the CORDEX-FPS-CPTP framework. The performance of these simulations in representing MCS precipitation characteristics has been assessed using the GPM-IMERG precipitation product and the CMA Multi-Source Merged Precipitation Analysis (CMPA).

The results demonstrate that while all ensemble members can generally capture the spatial distribution of MCS precipitation downstream of the TP, notable differences arise among the simulations with single-physics perturbations. Specifically, simulations using the Morrison and WSM5 microphysics schemes exhibit strong agreement with observations. In contrast, simulations employing the SBU_YLin or WDM6 microphysics schemes significantly underestimate MCS precipitation in the region. Regarding planetary boundary layer (PBL) scheme sensitivity, simulations utilizing the YSU and Shin-Hong schemes outperform those employing the MYNN3 scheme.

Despite these variations, a common bias emerges across all seven kilometer-scale WRF simulations: they collectively underestimate the rainfall area of MCSs by 30.9% to 43.0%, while simultaneously overestimating precipitation intensity of MCSs by 59.4% to 64.1%. These results suggest a consistent tendency for K-scale WRF simulated MCS precipitation to exhibit smaller spatial extents yet greater magnitudes compared to observations.

To explore potential improvements, we expanded the model domain from [15.0°N–50.0°N; 65.0°E–125.0°E] to [5.0°N–55.0°N; 45.0°E–160.0°E; almost doubled] and conducted additional WY2020 simulations. Preliminary results indicate that the expanded domain not only enhances the model’s ability to capture heavy MCS rainfall centers during Mei-yu season, particularly over the Western North Pacific Ocean (south to Japan), but also better reproduces MCS precipitation features than other K-scale WRF runs. Remarkably, the expanded domain simulation even outperforms the GPM data in representing MCS precipitation over the middle and lower reaches of the Yangtze River basin in eastern China, compared to CMPA.

The K-scale WY2020 ensemble run represents a valuable resource for advancing our understanding of the K-scale model uncertainties on MCS and the hydrological cycle over the TP and its downstream regions.

How to cite: Li, P.: Simulating Mesoscale Convective Systems Downstream of the Tibetan Plateau at Kilometer-Scale: Insights from the First Ensemble Run of ‘WY2020’ in CORDEX-FPS-CPTP, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9830, https://doi.org/10.5194/egusphere-egu25-9830, 2025.

17:50–18:00
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EGU25-10450
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ECS
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On-site presentation
Harriet Gilmour, Robin Chadwick, Jennifer Catto, Kate Halladay, and Neil Hart

South America is highly vulnerable to storms and extreme precipitation. Mesoscale Convective Systems (MCSs), a prevalent storm type in tropical and subtropical South America, can be particularly damaging due to the organised, deep convection that fuels heavy precipitation over wide areas. Future warming will likely bring changes to MCS characteristics and precipitation extremes across the region. However, the relatively coarse spatial resolution of current regional climate models fails to explicitly resolve convective processes, making future changes to MCSs uncertain. Here, the representation of modelled MCSs is investigated in decade-long convection-permitting climate simulations over South America run by the UK Met Office. Changes to MCSs under global warming are then assessed using a future climate simulation. Simulated MCSs are tracked using a cloud tracking algorithm (tobac) and compared with those in satellite observations for seasonality, storm characteristics and regional differences. The simulations perform well at capturing the observed MCS climatology, including spatial frequency and seasonal cycle. However, the simulations overestimate MCS frequency over the Amazon Basin by a factor of 2 and underestimate MCS frequency over the La Plata Basin, likely due to a weak bias in the simulated South American Low-Level Jet.  In general, regional variations in MCS characteristics are also well simulated, but precipitation-related characteristics show larger model-observed differences. Simulated MCSs overestimate precipitation intensity and underestimate precipitation area. This results in an underestimation of the MCS contribution to total rainfall of 20-30% in the model, particularly in subtropical South America. The results from this work suggest that MCSs are generally well-captured by the CPM and have been used to inform results for future changes to MCSs over South America under climate change.

How to cite: Gilmour, H., Chadwick, R., Catto, J., Halladay, K., and Hart, N.: Mesoscale convective systems over South America: Representation in km-scale climate simulations and future change, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-10450, https://doi.org/10.5194/egusphere-egu25-10450, 2025.

Posters on site: Thu, 1 May, 16:15–18:00 | Hall X5

Display time: Thu, 1 May, 14:00–18:00
Chairpersons: Julia Curio, Cornelia Klein
Impacts of severe weather
X5.35
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EGU25-15921
Kateřina Skripniková and Zbyněk Sokol

Data from lightning detection sensors and dual-polarized weather radars are used for high-resolution analysis of hailstorms developing around the Ore Mountains ridge. Measured radar and lightning parameters provide information on storm dynamics and are indicative of severe hailfall occurrence. Our case study deals with a multicellular hailstorm that developed during a summer afternoon near the ridge of the Ore Mountains from Germany to Czechia.

On 27 June 2022, hailstorms formed on both the windward and leeward sides of the Ore Mountains ridge. The multicellular storm evolved in warm air ahead a warm front advancing to the east. Severe hail was reported in many places, with hailstones up to 5 cm in diameter. And high lightning activity was detected.

Both radar and lightning detection data were used to study the hailstorm evolution thoroughly. Lightning data from the ENTLN network provide lightning activity parameters from the entire area of interest. Radar data from the Czech weather service C-band radar network are covering the area of interest as well. Data from the X-band radar situated on the Milesovka hill are used in the radar range, which is 30 km from the Milesovka observatory. This measurement does not cover the entire study area of the storms, but provides more detailed information, also due to the frequent RHI scanning in the scanning strategy.

How to cite: Skripniková, K. and Sokol, Z.: A case study of hailstorm dynamics during mountain ridge crossing, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-15921, https://doi.org/10.5194/egusphere-egu25-15921, 2025.

X5.36
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EGU25-16917
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ECS
Iris Thurnherr, Lena Wilhelm, Ruoyi Cui, Monika Feldmann, Sandro Beer, Christoph Schär, and Heini Wernli

Thunderstorm-related severe weather, particularly hail, causes extensive damage to life and infrastructure across Europe. However, the effect of a warmer climate on the occurrence of hail is still not fully understood. To date, most projections of hail occurrence under future climate scenarios have relied on hail proxies derived from global and regional climate models that use parameterized representations of convection. Recently, convection-permitting regional climate simulations with a high computational resolution of 2 km, using the COSMO model with the online hail diagnostic HAILCAST, have provided new insights. The simulations revealed spatially contrasting changes in hail frequency under a 3°C global warming scenario, showing a substantial decrease in summer hail frequency in southwestern Europe and an even larger increase in central and eastern Europe. In this study, we leverage these high-resolution model outputs to assess future projections of hail occurrence. Specifically, we compare differences in hail day frequencies between a warmer future climate and the present day climate as derived from (i) traditional hail proxies using environmental variables (e.g. CAPE and wind shear) and (ii) the HAILCAST online diagnostic. Through this comparison, we aim to better understand two key questions: (1) how accurately hail proxies capture the spatial and temporal patterns of hail occurrence in comparison to HAILCAST, and (2) whether the relationship between environmental variables and hail occurrence remains stationary under changing climatic conditions.

How to cite: Thurnherr, I., Wilhelm, L., Cui, R., Feldmann, M., Beer, S., Schär, C., and Wernli, H.: Comparison of future hail trends across Europe based on the HAILCAST diagnostic and hail proxies, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16917, https://doi.org/10.5194/egusphere-egu25-16917, 2025.

X5.37
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EGU25-5635
Ulrike Lohmann, Nikolaos Papaevangelou, and Manuel Brülisauer

Hailstorms can cause a lot of damage for agriculture and property. Therefore, efforts exist to mitigate hail damage by means of seeding a developing hailstorm with ice nucleating particles. Motivated by the Swiss hail mitigation campaign, we examined the impact of silver iodide (AgI) perturbations on a convective storm observed over northern Switzerland on July 6, 2019. We evaluated the effectiveness of an early seeding strategy and investigated the concept of beneficial competition, where increased number of INPs lead to the formation of smaller, less damaging hailstones. We used the Consortium for Small-Scale Modeling Regional Weather and Climate Model (COSMO) to simulate this case. AgI particles were added as a prognostic variable to the hailstorm during its cumulus stage and were released in the updraft region near the cloud base with concentrations ranging from 0.2/cm3 to 2000/cm3 in ensemble simulations. While seeding delayed the onset of precipitation, increased the graupel concentration and reduced supercooled liquid water, especially in the upper part of the convective cloud, no systematic change in the overall hail size has been found.

The lightning potential index (LPI) depends both on simultaneous occurrence of liquid water and ice species, as well as on the updraft strength. LPI increased in all seeding simulations in terms of intensity and spatial extent, because seeding increased the updraft strength and the graupel weighted ice mixing ratio.

How to cite: Lohmann, U., Papaevangelou, N., and Brülisauer, M.: Simulations of selective seeding of hailstorms over Switzerland: impacts for precipitation and lightning, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5635, https://doi.org/10.5194/egusphere-egu25-5635, 2025.

Storm dynamics and land-atmosphere interactions
X5.38
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EGU25-18567
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ECS
Nicolas Da Silva, Diana Monroy, Ashly Wilson, and Jan Haerter

Mesoscale Convective Systems (MCSs) are organized collections of thunderstorms that typically consist of narrow, intense regions of convective precipitation alongside broader, lighter areas of stratiform precipitation. These systems are the primary contributors to extreme precipitation events across Europe (Da Silva & Haerter, 2023). While both convective and stratiform precipitation rates are expected to increase with temperature according to thermodynamic expectations (the Clausius-Clapeyron relationship), their statistical superposition may intensify at an even faster rate due to increased proportion of convective-type precipitation within MCSs under warmer conditions (Da Silva & Haerter, 2025, accepted).

Both the intensity and proportion of convective-type precipitation in MCSs play a critical role in determining flood risks, but the spatial and temporal organization of convection is equally significant for shaping the characteristics and severity of flooding. Larger, long-lived clusters of convection within MCSs are indeed more likely to trigger severe flooding compared to smaller, isolated clusters.

In this study, we analyze the spatio-temporal characteristics of convective clusters within MCSs. MCSs are identified and tracked using both radar precipitation data (RADOLAN radar; Bartels et al., 2004) and lightning records from the EUropean Cooperation for LIghtning Detection (EUCLID; Schulz et al., 2016) network over Germany. Convective-type precipitation is classified based on its proximity to lightning strikes. To explore links between these clusters and local environmental conditions, we incorporate data from German Weather Service (Deutscher Wetterdienst, DWD) weather stations and the ERA5 reanalysis dataset (Hersbach et al., 2020).

We measure the spatial clustering of convection within MCSs using two novel spatial organization indices that quantify deviations from random distributions. Our preliminary findings suggest that convective clusters within MCSs become wider at higher temperatures, consistent with observations of larger CAPE (Convective Available Potential Energy) environments. Additionally, we observe a geographic trend in the location of convective clusters: they are more frequently concentrated in the southern portions of MCSs. However, under warmer conditions, a larger fraction of MCSs exhibit convective clusters on their northern edges. We hypothesize that this shift is driven by stronger convective instability ahead of the northern flanks of MCSs at higher temperatures. This effect may be linked to increased near-surface baroclinicity and horizontal temperature gradients at warmer temperatures.

The temporal evolution of these convective clusters is further analyzed through the framework of directed percolation, a statistical physics approach that allows us to investigate the growth and connectivity of convective cells over time. Through this lens, we aim to better understand the lifecycle of convective clusters within MCSs, including their formation, propagation, and eventual dissipation. By combining spatial and temporal analyses, this study provides critical insights into how environmental conditions influence the organization of convection within MCSs, thereby advancing our ability to predict and mitigate flood risks in a warming climate.

How to cite: Da Silva, N., Monroy, D., Wilson, A., and Haerter, J.: Spatio-temporal aggregation of convective cell clusters in European MCSs, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18567, https://doi.org/10.5194/egusphere-egu25-18567, 2025.

X5.39
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EGU25-1319
Liangliang Li, Wenshou Tian, Jian Li, Jinlong Huang, Rui Wang, and Jiali Luo

From 19 to 21 July 2021, Henan province of China experienced an extreme precipitation event that caused massive flooding and great loss of lives. This event is thus far the second heaviest precipitation event observed by rain gauges in this region. Based on the ERA5 reanalysis data, the ECMWF operational global ensemble forecasts and numerical simulations using the ARW-WRF model, impacts of an upper tropospheric cold low (UTCL) on the extreme precipitation are examined. It is found that due to the influence of the persistent intrusion of stratospheric high potential vorticity (PV) air, a long-lived UTCL was detached from the upper level flow a week prior to the extreme precipitation event. The UTCL then moved westward, reaching the Yellow Sea and the East China Sea and maintaining there until the precipitation event ended. During this event, a broad northeast-southwest oriented area of ascending motion associated with the UTCL could be observed in front of the UTCL and strong ascending motions developed in the upper troposphere above Henan province. Analysis of the ECMWF operational global ensemble forecasts reveals that the amount of precipitation over Henan is positively correlated with the UTCL intensity. The UTCL impact on the extreme precipitation and the underlying mechanisms are further investigated based on results of numerical experiments. The control experiment reasonably reproduces the UTCL location as well as the distribution and evolution of the extreme precipitation. When the UTCL intensity is reduced in the initial condition using the piecewise PV inversion for sensitivity experiment, the upper tropospheric divergence reduces correspondingly and the dynamical ascending motion weakens in the second precipitation stage. As a result, the amount and intensity of precipitation both decrease. When the UTCL is completely removed from the initial condition, the sensitivity experiment indicates that the upper tropospheric divergence and dynamical ascending motion further weaken, resulting in a large decrease in precipitation intensity during the whole precipitation period. These findings highlight that the occurrence of the long-lived UTCL is a crucial factor that affects the intensity of the extreme precipitation event.

How to cite: Li, L., Tian, W., Li, J., Huang, J., Wang, R., and Luo, J.: Impacts of an upper tropospheric cold low on the extreme precipitation in Henan Province, China in July 2021, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-1319, https://doi.org/10.5194/egusphere-egu25-1319, 2025.

X5.40
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EGU25-2623
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ECS
Christian Dominguez

The North American Monsoon (NAM) contributes the most significant amount of annual precipitation from July to September over northwestern Mexico. The increase in deep convection during the NAM is due to the emergence of extensive cumulonimbus cloud agglomerations, known as Mesoscale Convective Systems (MCSs). Previous studies suggest that upper tropospheric inverted troughs (IVs) (200 hPa), which occur over the NAM region, induce favorable environmental conditions for the development and intensification of MCSs. This talk shows the relationship of VIs with the organization of MCSs that occur over the NAM region. GOES-13 infrared satellite images (2010-2013) and the CLAUS database (1984-2008) are used to identify the trajectory of MCSs. ERA5 reanalysis data (1984–2008) characterize the atmospheric and thermodynamic conditions induced by VIs and upwellings. The results show that MCSs developed mainly in July and August, beginning to decline during September. A similar behavior is observed in the VIs, as most  of them originate from tropical upper tropospheric trough (TUTT) detachments. It is concluded that 22.8% of all MCSs formed during the study period interacted with VIs and produced more intense precipitation, unlike MCSs that did not interact. Although this percentage is small, MCSs that interacted with VIs induced more moisture to be transported to mid-atmospheric levels (500 hPa), compared to those that did not interact. Therefore, detecting these systems is essential to determine the existence of intense precipitation events over the NAM region.

How to cite: Dominguez, C.: The influence of inverted troughs on the formation of mesoscale convective systems during the North American Monsoon, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2623, https://doi.org/10.5194/egusphere-egu25-2623, 2025.

X5.41
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EGU25-20189
Maria Cristina Lemos da Silva, Helber Gomes, Matheus José Arruda Lyra, Dirceu Herdies, Fabricio Daniel dos Santos Silva, Heliofábio Barros Gomes, and Hakki Baltaci

Land use in the city of Maceió is rapidly changing from its natural state to accommodate a growing population and tourism. These changes include increased urbanization. There has been a significant increase in the frequency and intensity of extreme events occurring in recent years in the Northeast region of Brazil (NEB), especially in its metropolitan areas. It is believed that this may be associated with the exacerbated land use (LU) in these areas. Therefore, the objective of this work is to evaluate how an intense simulation event using the WRF model would be affected if the size of the Maceió metropolitan region were increased. Furthermore, the study will investigate the effects that the LU has on the intensity of this extreme event and its structure. To achieve this, the land use around the metropolitan region of Maceió was changed to a slightly larger urban area in the input files and then re-executed under the same parameters. Control and experimental simulation were compared using vertical profiles, flow fields and instability indices. The heavy rains that occurred on March 17, 2020 over Maceió were caused by an intense confluence of air at low levels (1000 hPa) observed on the state's coast in the early hours of the day. This conference occurred due to a small low pressure center that was present near the coast of Bahia, which could also be observed in the Sea Level Pressure field. The Convective Available Potential Energy (CAPE) field also indicated intense instability over the region, with values above 1000 J/Kg after 16 UTC over a large part of the north/east sector of Alagoas. Skew T Log-P thermodynamic profiles demonstrated high levels of instability throughout the 17th, gaining more strength between 16-21 UTC, with a maximum CAPE of 1864 J/Kg at 18 UTC. Throughboth simulations, it was reported that in the LU experiment there was an increase in the intensity and spatial distribution of the occurrence over the city of Maceió, as well as being associated with an increase in instability. Impacts were also identified on sensible and latent heat fluxes, and vertical shear. These results, despite being initial, show that there is a sensitivity in the use of land in convection and, consequently, in the intensity of learning.

How to cite: Silva, M. C. L. D., Gomes, H., Lyra, M. J. A., Herdies, D., Silva, F. D. D. S., Gomes, H. B., and Baltaci, H.: Effects on urbanization on a WRF-simulated heavy precipitation over the Maceió city, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20189, https://doi.org/10.5194/egusphere-egu25-20189, 2025.

X5.42
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EGU25-7625
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ECS
Xiao Yiqing, Li Ming, and Ma Yongyong

Doppler radar, FY-4B satellite data, wind profile radar, ERA-5 reanalysis data, automatic weather station and other multi-source observation data are used to analyze the causes and forecast deviation of a rainstorm on the eastern foot of Qinling mountains in Shaanxi province of China on 19th July 2024, and the results indicated that the rainstorm had strong suddenness, locality and convection. The main water vapor and energy for the rainstorm were provided by the southwest low-level jet at 700 hPa, and the strengthening of the jet stream and the decrease in the height of the jet stream core had a good correlation with the occurrence of heavy precipitation. The mesoscale convective system(MCS) causing rainstorm was formed by the the merging and strengthening of locally generated cold clouds in the convergence and upward movement zone of 700 hPa jet stream front and mesoscale convective clouds moving from southwest to east. And the convective system continued to develop along the mountain direction, forming a "train effect" that strengthens local heavy rainfall. Topography played an important role in this rainstorm.  On the one hand, the Qinling Mountains block the low-level jet stream at 700hPa, causing water vapor to strongly accumulate on the windward slope and converge and rise. On the other hand, the Qinling Mountains produced a significant topographic uplift movement on the ground and southerly winds at 850 hPa, thereby strengthening precipitation together. The 24-hour precipitation forecast was significantly missed by several numerical models because of deviation of 700 hPa jet location and intensity, but the CMA-BJ model had good prediction on the falling area and intensity of heavy rainfall for 3 h. Conducting analysis of similar rainstorm events, summarizing the deviation characteristics of the numerical models, considering the triggering and maintenance mechanisms of convection, and the important role of terrain would help improve the forecasting and early warning capabilities of such rainstorm.

 

How to cite: Yiqing, X., Ming, L., and Yongyong, M.: Analysis on the Causes and Forecast Deviation of Rainstorm on the Eastern Foot of Qinling Mountains, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7625, https://doi.org/10.5194/egusphere-egu25-7625, 2025.

X5.43
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EGU25-5421
Yu Du, Dong Fu, and Hongpei Yang

Previous studies have investigated the optimal configuration of squall lines affected by linear vertical wind shear and cold pools, as described by the RKW theory. However, the interaction dynamics between low-level jets (LLJs) with nonlinear vertical wind shear, and cold pools remain insufficiently understood. This study utilizes idealized numerical simulations to examine the impacts of LLJs on cold pools and their subsequent role in initiating convection, focusing on the sensitivity to LLJ height and strength. The simulations reveal that, under the influence of an LLJ, a cold pool typically evolves into a two-step structure with two distinct heads, and its intensity diminishes more rapidly compared to scenarios with quasi-linear shear or no wind. Two prominent regions of vertical velocity are identified near these heads, with oneassociated with the elevated cold pool head and elevated convection initiation. Variations in parcel lifting above and below the jet core arise from differences in horizontal vorticity induced by LLJ shear, resulting in two distinct clusters of parcel trajectories. A lower or weaker LLJ leads to earlier convection initiation due to larger initial vertical velocity driven by LLJ-cold pool interactions. Convection intensity peaks when the LLJ height aligns with levels of high CAPE and when vorticity pairing above the jet core reaches its optimal state, consistent with RKW theory.

How to cite: Du, Y., Fu, D., and Yang, H.: The Interaction Between Low-level Jets and Cold Pools and Their Impacts on Convection Initiation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5421, https://doi.org/10.5194/egusphere-egu25-5421, 2025.

X5.44
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EGU25-5357
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ECS
Wenyi Li, Riyu Lu, and Lin Wang

Mesoscale convective systems (MCSs) frequently occur over southern China during early summer, often leading to significant precipitation and associated socioeconomic impacts. This study investigates the differences in MCS frequency and related precipitation in southern China before and after the onset of the South China Sea summer monsoon (SCSSM) during 2001-2020, using high-resolution satellite data from the Global Precipitation Measurement mission and iterative rain cell tracking (IRT) method that combines cloud and precipitation criteria.

Our analysis indicates that during two pentads after the SCSSM breaks out, the frequency of MCSs significantly decreases in southern China, especially over the middle and lower reaches of Yangtze River basin (MLYRB). Accordingly, the heavy rainfall amounts decrease sharply. For instance, the number of grids with hourly precipitation between 10 and 30 mm drops by over 40% over MLYRB after the monsoon onset. It is found that the remarkable weakening of lower-level vertical wind shear and abnormal descending motion over southern China are unfavorable for the formation of MCSs. Corresponding to the SCSSM onset, on the one hand, atmosphere warms much less over the tropical oceans, including the SCS, than over the extratropical lands, resulting in smaller magnitude of meridional air temperature gradient and a subsequent decrease in vertical wind shear. On the other hand, the lower-level northerly winds induced by the SCSSM onset result in the suppressed ascent flows over southern China.

How to cite: Li, W., Lu, R., and Wang, L.: The Influence of South China Sea Summer Monsoon Onset on Mesoscale Convective Systems in Southern China, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5357, https://doi.org/10.5194/egusphere-egu25-5357, 2025.

X5.45
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EGU25-2340
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ECS
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Debjit Paul and Sarvesh Kumar Dubey

Mesoscale Convective Systems (MCSs) account for over 50% of annual rainfall across the tropics and many regions of the subtropics and midlatitudes. They are often associated with strong lightning and extremely heavy rainfall, which can lead to floods. Consequently, comprehending the spatio-temporal attributes and long-term trends of MCSs is crucial for better preparedness to avoid natural hazards in current and future climatic conditions. In contrast to other MCS hotspots around the globe, investigations on the long-term alterations of MCSs in South Asia are still scarce. Our work employs high-resolution satellite brightness temperature and precipitation data, together with a novel MCS tracking method (PyFLEXTRKR), to generate a database of MCS occurrences in South Asia during the last two decades (2001-2020), and then perform a detailed analysis to understand their climatological characteristics, the environmental conditions favouring them and the long term trend. Bay of Bengal, Western Ghats, and Southern Peninsula of India are the sites where the highest number of MCSs develop. Additionally, there is a distinct seasonality in MCS activity, with the summer monsoon season seeing the highest formation of convective systems. During this season, especially over the Bay of Bengal, we observe the strong characteristics of the MCS, such as its larger area, longer duration, and greater rain rate. To a certain degree, the formation of small (<104 km2) and medium-sized (104 km2–4.4 x 104 km2) MCSs is equally dispersed between the ocean and land, whereas the large (4.4 x 104 km2–1.6 x 105 km2) MCSs form mostly across the oceans. On the other hand, the Super (> 1.6x105 km2) MCSs are exclusively found over the Bay of Bengal, primarily during the monsoon season. The percentage of rainfall contributed by MCSs over South Asia varies with the seasons, and the highest amount is received during the monsoon season. There is also a disparity over land and ocean, with land areas receiving 40%-50% and oceans receiving 55%-65% of their annual mean rainfall. Compared to the other types of convections, the MCSs contribute to the major fraction of total rainfall produced over both land and ocean, especially towards the higher magnitudes of rainfall. The ability to produce strong rainfall by any MCS strongly depends on its spatial extent (rcorr = 0.83 (0.88) over land (ocean)), followed by lifetime (rcorr = 0.48 (0.65) over land (ocean)), whereas the brightness temperature is negatively correlated weakly (rcorr = -0.24 (-0.37) over land (ocean)). The analysis of the large-scale environmental conditions reveals a gradual build-up of favorable conditions six hours before the initiation, with a noticeable increase within a 100-kilometer radius just three hours before the initiation. Our analysis shows that within the last 20 years, MCSs have increased in frequency and spatial extent. Furthermore, the precipitation associated with MCS has shown a notable upward trend. The rising frequency and severity of MCSs are propelled by increasingly conducive water vapor rich environment, which are expected to escalate with global warming. This could significantly impact the hydroclimate of South Asia, particularly the probability of severe events.

How to cite: Paul, D. and Dubey, S. K.: Comprehending the Attributes and Strengthening of Mesoscale Convective Systems over South Asia, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-2340, https://doi.org/10.5194/egusphere-egu25-2340, 2025.

Km-scale modelling
X5.46
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EGU25-17755
Juan Pedro Montávez, Eloisa Raluy-López, Domingo Muñoz-Esparza, and Jeremy Sauer

High-resolution simulations, both at mesoscale and microscale, have become increasingly prevalent, often leveraging high-resolution terrain datasets. However, terrain-following coordinate models can encounter numerical instabilities in regions where terrain slopes exceed critical thresholds, generally around 35º. To address this issue, terrain smoothing is typically required. Current approaches usually involve applying global smoothing methods across the entire domain, which inevitably results in a loss of terrain detail and resolution to prevent numerical instabilities in regions where it is not necessary. Moreover, as the model resolution increases, the number of grid points with steep slopes grows, underscoring the need for alternative terrain smoothing strategies.

This study presents the development and implementation of a local terrain smoothing approach designed to mitigate numerical instabilities in a mesoscale model (the WRF model) and a microscale model (NCAR-RAL’s GPU-accelerated FastEddy® LES model). Various smoothing techniques were evaluated, including both simultaneous and sequential approaches. Following a thorough performance analysis—considering the number of iterations required for convergence, computational cost, and, most importantly, the degree of terrain distortion—the most effective method was selected and implemented. The final approach applies a Gaussian filter (σ = 25) over a 3x3 grid centered on each steep-slope point, with a blending factor of 0.2 at the edges. This ensures that the central point is smoothed while the surrounding points retain 80% of their original terrain characteristics. Each steep slope is addressed individually but processed simultaneously across iterations. A higher blending factor results in greater terrain distortion, while a lower blending factor significantly increases computational time, often preventing convergence within the imposed iteration limit.

This terrain smoothing method has been fully implemented in FastEddy® and is now used operationally and routinely within the model. This implementation will be made publicly available in the next release of FastEddy®, hosted on GitHub (https:// github.com/NCAR/FastEddy-model, starting with version 3.0). For WRF, the method has been integrated as an additional step in the WPS workflow, following the execution of the geogrid program. The proposed local smoothing approach helps preventing the occurrence of CFL errors in high-resolution simulations over complex terrain without relying on excessively high values of the time off-centering parameter (epssm) to dampen vertically propagating sound waves, which can lead to excessive high-frequency damping, negatively impacting the accuracy of the simulations.

In conclusion, this study presents a simple yet effective method for avoiding terrain-driven numerical instabilities in high-resolution simulations, ensuring the maximal preservation of terrain resolution in both microscale and mesoscale models. This approach can be easily applied to other models, offering a straightforward solution to enhance numerical stability while maintaining high-resolution terrain features in diverse simulation environments.

Acknowledgements: The authors acknowledge the ECCE project (PID2020-115693RB-I00) of the Ministerio de Ciencia e Innovación/Agencia Estatal de Investigación (MCIN/AEI/10.13039/501100011033). ERL thanks her predoctoral contract FPU (FPU21/02464) to the Ministerio de Universidades of Spain.

How to cite: Montávez, J. P., Raluy-López, E., Muñoz-Esparza, D., and Sauer, J.: A Local Terrain Smoothing Approach for Stabilizing Microscale and High-Resolution Mesoscale Simulations: Application to FastEddy® and WRF, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17755, https://doi.org/10.5194/egusphere-egu25-17755, 2025.