AS1.13 | Advancing understanding of the circulation-coupling and Lagrangian evolution of clouds
Orals |
Tue, 16:15
Wed, 14:00
EDI
Advancing understanding of the circulation-coupling and Lagrangian evolution of clouds
Convener: Raphaela Vogel | Co-conveners: Matthias Tesche, Geet GeorgeECSECS, Julia KukuliesECSECS, Leif Denby
Orals
| Tue, 29 Apr, 16:15–18:00 (CEST)
 
Room 1.85/86
Posters on site
| Attendance Wed, 30 Apr, 14:00–15:45 (CEST) | Display Wed, 30 Apr, 14:00–18:00
 
Hall X5
Orals |
Tue, 16:15
Wed, 14:00

Orals: Tue, 29 Apr | Room 1.85/86

Chairpersons: Matthias Tesche, Geet George, Raphaela Vogel
16:15–16:20
16:20–16:30
|
EGU25-18395
|
solicited
|
Highlight
|
On-site presentation
Julia Windmiller, Romain Fiévet, Helene Glöckner, and Bjorn Stevens

The Intertropical Convergence Zone (ITCZ) is a central component of the atmospheric general circulation and is traditionally described as a region of mean surface convergence and high precipitation rates. The ITCZ is also associated with the doldrums, regions of low wind speeds and variable wind directions, although the exact relationship between the two remains unclear. Reexamining this relationship, we show that the doldrums are largely confined to the area between the edges of the ITCZ, which are characterised by enhanced surface convergence. Although this is a region of high time-averaged precipitation, low wind speed events only occur in the absence of precipitation. This suggests that the traditional explanation of the doldrums being the result of ascending air motion is incorrect. We therefore investigate the vertical structure of the doldrums using data collected during the ORCESTRA (Organized Convection and EarthCARE Studies over the Tropical Atlantic) field campaign. ORCESTRA took place in the tropical Atlantic in August and September 2024 and consisted of eight sub-campaigns. Here, we focus on the sampling of vertical air motion that we measured with dropsondes in the deep tropics in general and in the doldrums in particular. In combination with limited-area simulations that provide daily hindcasts of atmospheric conditions in the campaign region, we use these data to characterise for the first time the vertical structure of vertical air motion within regions of low wind speeds. This study can also be seen as an example of a more fundamental goal of the ORCESTRA campaign, which is to gain a better understanding of the mesoscale structure of the ITCZ and the importance of its significant day-to-day variability.

How to cite: Windmiller, J., Fiévet, R., Glöckner, H., and Stevens, B.: Revisiting the Doldrums: New Insights from the ORCESTRA Campaign, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18395, https://doi.org/10.5194/egusphere-egu25-18395, 2025.

Organized convection and rain
16:30–16:40
|
EGU25-5370
|
On-site presentation
Allison Wing, Michael Bell, James Ruppert, Sarah Kennison, Wei-Ting Hsiao, Delián Colón-Burgos, Daniel Klocke, Chaehyeon Chelsea Nam, and Morgan O'Neill

The ORganized Convection and Earthcare Studies over the TRopical Atlantic (ORCESTRA) field campaign occurred in the tropical Atlantic in August and September 2024. ORCESTRA is an international initiative that combined eight different sub-campaigns utilizing seven different ship, aircraft, ground-based, and satellite platforms. Here we focus on preliminary results from PICCOLO (Process Investigation of Clouds and Convective Organization over the atLantic Ocean), the NSF-funded sub-campaign that deployed the CSU SEA-POL radar on the RV Meteor in coordination with the BOWTIE ship campaign to study the nature, governing mechanisms, and impact of mesoscale convective organization within the Atlantic ITCZ. SEA-POL is a ship-stabilized scanning C-band radar that measures dual-polarization and provides advanced retrievals of precipitation and its spatial pattern. PICCOLO has four objectives: (1) evaluate process relationships between precipitation, humidity, and organization; (2) use advanced polarimetric radar retrievals to investigate microphysical, dynamical, and radiative characteristics of convection; (3) investigate the importance of radiative processes in driving mesoscale organization; and (4) use novel observational approaches to compute the entropy budget to advance understanding of the impacts of convection on climate. 

The 40-day cruise primarily sampled within the moist tropics and observed a wide variety of convective states. There was a significant longitudinal contrast, in which conditions east of 40W were rainier and moister with cooler sea surface temperatures, stronger surface winds, and stronger vertical wind shear than areas west of 40W. We use the SEA-POL retrievals to examine the variability of convective structures within the ITCZ including variability in the prevalence of congestus versus deep convection. We also present initial classifications of the spatial organization of convection, its variability, and its influence on precipitation amount and intensity.

How to cite: Wing, A., Bell, M., Ruppert, J., Kennison, S., Hsiao, W.-T., Colón-Burgos, D., Klocke, D., Nam, C. C., and O'Neill, M.: Ship-borne radar observations of organized convection during the ORCESTRA/PICCOLO field campaign, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-5370, https://doi.org/10.5194/egusphere-egu25-5370, 2025.

16:40–16:50
|
EGU25-9024
|
ECS
|
On-site presentation
|
Nils Niebaum, Clara Bayley, Mampi Sarkar, Ann Kristin Naumann, and Raphaela Vogel

How much rain evaporation occurs below shallow cumuli is a crucial determinant of the organisation of such clouds, yet both modelling studies and observations which can robustly quantify the amount of evaporation are in short supply. In this study we combine observations of a diverse population of precipitating cumuli from the EUREC4A field campaign with a simple 1-D rain-shaft model, in order to predict the amount of rain evaporation in the sub-cloud layer and the relative influence on it of microphysical vs environmental controls. The rain-shaft uses superdroplet model microphysics so that our analysis benefits from its detailed and yet comprehensible depiction of the droplet size distribution and microphysical processes involved. Surprisingly, we find that evaporated fractions are usually low, below 20%, and that collisional processes between droplets have a very minor influence on rain evaporation, meanwhile dominant roles are played by the droplet size distribution at cloud base and the sub-cloud layer relative humidity profile. The evaporated mass fraction can vary substantially between clouds and even when clouds’ liquid water contents are comparable, evaporated fraction can be upto 50% larger because of small differences to mean cloud droplet radius. These results stress the importance or accurately measuring/modelling droplet size distributions rather than microphysical processes in order to study rain evaporation. We find too that the vertical profile of evaporation rate is above all controlled by the vertical relative humidity profile, which suggests the sub-cloud layer could be highly sensitive to the feedback between evaporation and relative humidity.

How to cite: Niebaum, N., Bayley, C., Sarkar, M., Naumann, A. K., and Vogel, R.: Rain Evaporation Below Shallow Tropical Trade-Wind Cumuli as Predicted by a New Super-Droplet Model, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-9024, https://doi.org/10.5194/egusphere-egu25-9024, 2025.

16:50–17:00
|
EGU25-4547
|
On-site presentation
Ryan Eastman, Justin Stopa, Ralph Foster, Doug Vandemark, and Hauke Schulz

Synthetic Aperture Radar (SAR) is capable of detecting wind and rain signatures at a 5-meter resolution on the ocean surface without interference from overlying cloud cover. Here, wind signatures represent the spatial distributions of capillary waves produced by gusts and lulls in the surface winds. These distinct wind signatures vary based on the 3-dimensional structure of the lower boundary layer and fall into two dominant categories: mesoscale convective (MC), and wind streaks (WS). MC boundary layers tend to be associated with gentler motions and lighter winds while WS are associated with stronger overturning “rolls” and heavier winds. SAR can detect rain columns as drops disturb the ocean surface and can also discern cold pools and atmospheric boundaries associated with precipitation. A machine learning routine has been developed to classify SAR images based on these signatures.

 

SAR images classified as MC, WS, or containing boundaries or rain columns are compared to a variety of satellite cloud data in order to independently verify the classification system, and to gain insight into whether these classified PBL states have an effect on cloud and precipitation processes. Randomly spaced and located SAR images taken only at sunrise and sunset during the year 2018 are linked to polar orbiting A-Train satellite observations. Observations are linked by using Lagrangian PBL trajectories, following the cloud-level winds forward and backward from the SAR image to the 1:30 and 13:30 A-Train observation times. This “brackets” the SAR image with satellite data observed 12-hours apart, or in the case of daytime-only data, 24-hours apart. Comparisons are made in four marine subtropical stratocumulus regions.

 

Results show that SAR-observed rain columns and cold pools are associated with higher rain rates as seen by AMSR/2 89 GHz rain rate estimates tuned by CloudSat. PBLs with wind streaks are associated with stronger rain rates and greater cloud liquid water path compared with mesoscale convective PBLs, even after controlling for wind speed. Further analysis shows that WS PBLs tend to be cloudier, shallower, and contain fewer cloud drops. This work highlights the importance of small-scale turbulent boundary layer processes in controlling cloud processes on sub-daily timescales, and motivates investment in future SAR observations over the ocean.

How to cite: Eastman, R., Stopa, J., Foster, R., Vandemark, D., and Schulz, H.: Sensitivity of Warm Rain Rates to Lower PBL Structure as Observed by Synthetic Aperture Radar over the Subtropical Ocean, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4547, https://doi.org/10.5194/egusphere-egu25-4547, 2025.

17:00–17:10
|
EGU25-20029
|
ECS
|
On-site presentation
Edoardo Foschi, Louise Nuijens, Paco Lopez-Dekker, and Owen O'Driscoll

Shallow convection and precipitation in the marine atmospheric boundary layer can modulate near-surface winds on scales from 100 m - 100 km. This may substantially influence the exchange of heat and momentum across the air-sea interface and turbulent mixing on either side of the interface. Here we analyze spatial patterns of near-surface wind and momentum flux down to a 100 m scale as a function of Richardson number and as a function of the development in moist precipitating convection in many large-domain large eddy simulations (DALES) as part of the BOTANY ensemble. To assess the modulation effect that convection has on surface momentum fluxes, we decompose the LES wind stress across the simulations into contributions from different scales and processes, and answer how these dependencies change as simulations develop deeper moist convection and consequently precipitation. At the ocean surface, DALES currently uses a rough-wall boundary condition with a bulk flux formulation that relates surface fluxes to resolved-scale variables at the first grid level, consistent with Monin-Obukhov similarity theory. Knowing that the representation of wind stress in LES is likely flawed, we reflect on the largest uncertainties given the model assumptions and how observations from space and from the recent ORCESTRA/BOWTIE campaigns can help validate and improve the formulation of wind stress. 

How to cite: Foschi, E., Nuijens, L., Lopez-Dekker, P., and O'Driscoll, O.: Shallow convection modulation of wind stress patterns in marine atmospheric boundary layer, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20029, https://doi.org/10.5194/egusphere-egu25-20029, 2025.

Circulation and cloud feedbacks
17:10–17:20
|
EGU25-3571
|
ECS
|
On-site presentation
Anna Mackie, Michael P. Byrne, and Chris J. Short

Understanding of cloud-circulation coupling in a warming world is underpinned by global climate models (GCMs) with coarse horizontal resolutions necessitating the use of convective parameterizations. Global convection-permitting models are now emerging, but their high computational cost is a barrier to their use for studies of climate change. 

Here, we present results from 2-year atmosphere-only, limited domain simulations at a horizontal resolution of ~4.5km over a region of the west Pacific using the Met Office Unified Model. The limited-area model is driven at the lateral boundaries by an existing ~25km global model. Two simulations are analysed: a control run with present-day SSTs and a perturbed run with a prescribed SST warming of approximately 4K. 

There are substantial differences in cloud-circulation coupling between the high-resolution simulations and the global driving model. In particular, we find – on average – large cloud radiative effects (CREs) associated with strongly subsiding gridpoints, in comparison to the relatively small CREs for this circulation regime as expected from previous GCM studies and indeed in the global driving model. We demonstrate that this systematic difference in subsiding CRE between models arises from the existence of complex circulation structures in the high-resolution simulations, which are absent in the global simulations. For the highest (>80%) percentiles of column relative humidity, subsiding gridpoints have O(5 Wm-2) weaker cooling compared to ascending gridpoints with similar column relative humidity. We discuss how this strong subsidence regime responds to warming, and potential implications for cloud feedbacks.

How to cite: Mackie, A., Byrne, M. P., and Short, C. J.: Cloud-circulation coupling in convection-permitting simulations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-3571, https://doi.org/10.5194/egusphere-egu25-3571, 2025.

17:20–17:30
|
EGU25-13780
|
On-site presentation
George Tselioudis and Joe Kelly

We analyze the CERES solar radiative balance trends of the past 23 years, with the objective to separate the contribution to the solar absorption trends of shifts in the atmospheric general circulation and changes in cloud controlling processes. Regimes of large cloud cover and strong cloud radiative cooling are defined in the low latitude and the high latitude zones, representing the tropical rainy zone and the midlatitude storm zones respectively, and the trends in the areal coverage of those regimes over the past 23 years are examined along with the trends in the cloud solar radiative effect within each regime. This allows the decomposition of the global solar cloud radiative trends into circulation induced changes and those induced by cloud controlling processes. The results show that the general circulation component of the cloud solar radiative changes, which manifests itself as a contraction of the midlatitude storm zones and the tropical rainy zone, is the largest term in the solar absorption trend, causing decreased sunlight reflection of 0.37 W/m2 per decade. We explore the relationship between the cloud regime contraction and the main atmospheric circulation indices, including the width of the Hadley circulation and the location of the midlatitude jet, in order to understand the processes responsible for the cloud regime changes.

How to cite: Tselioudis, G. and Kelly, J.:  Contraction of the world’s storm-cloud zones and the relationship to atmospheric circulation changes, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13780, https://doi.org/10.5194/egusphere-egu25-13780, 2025.

17:30–17:40
|
EGU25-14463
|
On-site presentation
Maria Rugenstein and Senne Van Loon

The radiative effect of shallow clouds, especially in the subtropical ocean upwelling regions, is very efficient and mostly controlled by local sea surface temperatures and the lower tropospheric inversion strength. The latter caused the radiative feedback of shallow clouds to switch from positive to negative over the last couple of decades and likely controls cloud feedbacks in the future. Drivers of lower tropospheric inversion strength are not well understood theoretically and vary strongly between reanalyses. We employ convolutional neural networks and explainable artificial intelligence to create maps of drivers of lower tropospheric inversion strength in the subtropical ocean upwelling regions. We quantify the relative relevance of local and remote surface temperatures and find that the edges of regions of deep convection matter much more than their center. The West Pacific Warm Pool is much less and the subtropical Atlantic more relevant than expected. Our results quantify how the theories of tropospheric weak temperature gradient and the convection circus tent play out for setting local free tropospheric temperatures and the local tropospheric inversion stength. Currently, our method is based on large ensemble climate model simulations and the results are robust across models. Applying this framework to observations, it might be possible to constrain the spread of this cloud controlling factor across reanalyses and constrain its future evolution, hence improving projections of the radiative effect of shallow clouds.

How to cite: Rugenstein, M. and Van Loon, S.: Understanding drivers of local lower tropospheric stability, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-14463, https://doi.org/10.5194/egusphere-egu25-14463, 2025.

17:40–17:50
|
EGU25-18477
|
ECS
|
On-site presentation
Geoffrey Pugsley, Edward Gryspeerdt, and Vishnu Nair

Stratocumulus clouds play an important role in the Earth’s energy balance due to their widespread spatial coverage and radiative properties. However, the impact of aerosol on stratocumulus cloud fraction (CF) remains poorly constrained resulting in large uncertainties for the effective radiative forcing due to aerosol cloud interactions (ERFaci). Stratocumuli undergo a strong diurnal cycle driven by variations in cloud top radiative cooling, which alters the processes sustaining the cloud. Despite this, many previous observational studies have only considered the state of the cloud field during the daytime due to the availability of satellite data.

In this work we use a Lagrangian tracking method, combined with geostationary satellite data, to investigate the CF response to aerosol over the entire
diurnal cycle. Strong variations in the cloud response to aerosol are found with the diurnal cycle. This brings satellite-based studies into closer alignment with ground- and insitu-based measurement campaigns, emphasising the importance of nighttime cloud processes for understanding aerosol cloud interactions and constraining the ERFaci.

How to cite: Pugsley, G., Gryspeerdt, E., and Nair, V.: How does the cloud fraction response to aerosol change over the diurnal cycle?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18477, https://doi.org/10.5194/egusphere-egu25-18477, 2025.

17:50–18:00
|
EGU25-13654
|
On-site presentation
James Ruppert, Emily Luschen, Rosimar Rios-Berrios, Shun-Nan Wu, and Yunji Zhang

Our emphasis on distinct tropical convective cloud modes has evolved over the decades in step with advancements in our understanding of tropical convection, its governing dynamics, and its role in large-scale weather and climate. While an early undilute plume view of tropical convection emphasized the role of latent heating from deep cumulonimbi in tropical ascending motion, a later emphasis on shallow to congestus clouds came with our improved grasp of water vapor’s essential role as governor to convective cloud development and organization. Here I discuss the unique role of stratiform and anvil clouds in this context, which play a surprisingly active role in the mesoscale organization of deep convection. While stratiform and anvil clouds are the biproducts of deep convection, consuming remnant buoyancy from their parent cumulonimbi, their much larger spatial and temporal footprints cause radiative forcing that fosters the upscale growth of moist convection and its coupling with the larger-scale environment. These clouds are therefore uniquely capable of coupling convection with the larger scale owing to their very long inherent lifecycles, compared to the fundamental scales of deep convection. In this presentation, I first motivate these arguments through consideration of scales. I next present the results from numerical model experiments and observations of tropical convection supporting the argument that longwave forcing by stratiform and anvil clouds actively promote convective upscale development and intensification. This forcing acts by reducing downdraft mass flux in stratiform regions, which in turn yields more upward motion per unit precipitation in the overall convective system. This constitutes a destabilization of the moist convective system, fostering its intensification, compared to if cloud–radiative forcing was absent. The results of this study imply that stratiform and anvil clouds and their radiative forcing are essential elements to any realistic conceptual model of tropical moist convection, and hence, to the tropical hydrologic cycle.

How to cite: Ruppert, J., Luschen, E., Rios-Berrios, R., Wu, S.-N., and Zhang, Y.: The active role of stratiform and anvil clouds through longwave radiative feedback, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13654, https://doi.org/10.5194/egusphere-egu25-13654, 2025.

Closing remarks

Posters on site: Wed, 30 Apr, 14:00–15:45 | Hall X5

Display time: Wed, 30 Apr, 14:00–18:00
Chairpersons: Geet George, Matthias Tesche, Raphaela Vogel
ORCESTRA and its sub-campaigns
X5.1
|
EGU25-16165
Daniel Klocke, Allison Wing, Marcus Dengler, Hans Segura, Geet Georges, Louise Nuijens, Micheal Bell, Heike Kalesse-Los, James Ruppert, and Hauke Schmidt

The BOWTIE ship-based field experiment explored the influence of convective storm processes and their oceanic interactions on the Atlantic Inter-Tropical Convergence Zone (ITCZ) in August and September 2024. This research is driven by evidence suggesting that storm-scale dynamics is pivotal for shaping the broader structure of the ITCZ and its connection to global circulation patterns and energy transport. Utilizing the German research vessel METEOR, the expedition involved extensive sampling within the ITCZ from its Northern to Southern edge - while transiting the tropical Atlantic from East to West - with detailed atmospheric and oceanic vertical profiling. The research focuses on obtaining vertically resolved cross-sections of the ITCZ and its surrounding conditions, with an emphasis on the atmosphere-ocean boundary layers. Key measurements include precipitation, cloud and humidity profiles, wind, sea-surface temperature, as well as physical and biogeochemical upper ocean characteristics with state-of-the-art instrumentation. BOWTIE is embedded within the international initiative ORCESTRA that combines eight different sub-campaigns. During BOWTIE the research vessel METEOR also served as a platform for two additional subcampaigns of ORCESTRA, which contributed UAVs (STRINQS) and a dual-polarization C-band radar (CSU’s SEA-POL, through PICCOLO) to the ship’s instrumentation. We will present an overview of BOWTIE and first results from the comprehensive measurments.

How to cite: Klocke, D., Wing, A., Dengler, M., Segura, H., Georges, G., Nuijens, L., Bell, M., Kalesse-Los, H., Ruppert, J., and Schmidt, H.: BOWTIE: A ship-based field campaign to explore the inner life of the Atlantic ITCZ, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16165, https://doi.org/10.5194/egusphere-egu25-16165, 2025.

X5.2
|
EGU25-20399
|
ECS
|
Anja Stallmach, Anna Weber, and Bernhard Mayer

Near-surface winds are a key component for the coupling of the atmosphere- ocean system. Convergence and divergence patterns can be inferred from measurements of the surface wind vector, enabling the characterization of meso- and synoptic-scale atmospheric dynamics. Observations over remote areas, such as the Atlantic ocean, are mostly limited to satellites and buoys. Geostationary satellites derive wind data primarily from cloud tracking and thus do not measure surface winds. In contrast, polar-orbiting satellites can provide surface wind data predominantly using active remote sensing instruments, such as scatterometers, wind-lidars or synthetic aperture radars, providing better spatial but certainly lower temporal resolution. Finally, buoy measurements are point-observations and cannot be employed for large-scale wind field analyses. This work aims to explore an alternative approach for quantifying surface wind fields over the ocean by analysing high-spatial resolution imagery from airborne observations.


Measurements of specularly reflected solar radiation (sunglint) by the hyperspectral and polarized imager specMACS aboard the German research aircraft HALO are employed for the development of a surface wind retrieval. Size and shape of the sunglint are predetermined by wind speed and direction: With ocean surface roughness directly corresponding to near-surface wind speed, the specMACS retrieval makes use of the relationship between ocean wave slope distribution and angular variation of sunglint radiance. SpecMACS measurements of spectral radiances are evaluated against simulated spectral radiances for different solar zenith and azimuth angles, as well as surface wind speeds and directions. The radiative transfer simulations are done with the Monte Carlo (MYSTIC) solver of the libRadtran radiative transfer package.


The overarching goal of this work is the development of an operational surface wind retrieval after analysing selected cases as an initial step. The retrieval requires a view of the ocean surface from the aircraft. We aim to explore to what extent the wind retrieval can be employed for (a) partially cloud-covered scenes or (b) scenes with an optically thin cirrus layer above or below the aircraft. A first application will be the analysis of data acquired during the recent ’Persistent EarthCare underflight studies of the ITCZ and organized convection’ (PERCUSION) sub-campaign in the tropical Atlantic. Research concerned with the horizontal wind field structure of atmospheric phenomena, e.g. the doldrums in the deep tropics, will benefit from along flight-track surface wind observations. Continuous surface wind data also further supplement dropsonde point-measurements.

How to cite: Stallmach, A., Weber, A., and Mayer, B.: Development of a surface wind retrieval by analysing sunglint geometry from specMACS radiance measurements, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-20399, https://doi.org/10.5194/egusphere-egu25-20399, 2025.

X5.3
|
EGU25-6335
|
ECS
Anna Trosits, Andreas Foth, and Heike Kalesse-Los

Convection, which influences cloud and precipitation properties as well as, the radiative effects of clouds, needs to be better understood for a comprehensive picture of interconnected climate processes all over the globe and requires a better representation for accurate climate projections. Meanwhile, the modelling of these phenomena is already a challenge itself, the quality and quantity of high-resolution observational data of convective clouds are limited, especially over the (tropical) oceans. The recent measurement campaign BOW-TIE (“Beobachtung von Ozean und Wolken – das Trans ITCZ Experiment”) on board the research vessel Meteor in August and September 2024 focussed on atmospheric and oceanic measurements inside the Atlantic ITCZ (intertropical convergence zone), between Mindelo (Cabo Verde) and Bridgetown (Barbados). Our working group from the Leipzig Institute for Meteorology concentrated on the investigation of the microphysical properties of clouds and precipitation by deploying a continuously measuring remote sensing suite mainly consisting of a motion-stabilized, vertically-pointing 94 GHz cloud radar and a microwave radiometer (MWR; to derive liquid water path (LWP) and integrated water vapor (IWV)) on the research vessel. In combination with data obtained with the ceilometer deployed by the MPI for Meteorology Hamburg, the synergetic Cloudnet processing chain can be employed. Cloudnet products include a hydrometeor target classification as well as cloud microphysical properties like the effective radius of cloud droplets and ice crystals, the hydrometeors phase, ice water content (IWC), and liquid water content (LWC). All observed and derived cloud and precipitation characteristics are contrasted between the Eastern and Western Atlantic. A first insight reveals the dominance of shallow convective clouds in the Eastern Atlantic, while the Western Atlantic also evinces convective clouds with a height up to six kilometers and cirrus clouds more frequently. Related to the frequency of occurrence of the different cumulus cloud types, the distribution of the microphysical properties like the effective radius of hydrometeors, IWC, and LWC allows for a more detailed glimpse into differences of the processes in the Eastern and Western ITCZ. With that, the convective processes above the tropical Atlantic Ocean are studied concerning microphysics and their distribution and contribute to an improved understanding of cloud-affecting processes.

How to cite: Trosits, A., Foth, A., and Kalesse-Los, H.: First insights into the diverse remote sensing observations of convection during BOW-TIE, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6335, https://doi.org/10.5194/egusphere-egu25-6335, 2025.

X5.4
|
EGU25-7132
|
ECS
Wei-Ting Hsiao, Allison Wing, Sarah Kennison, Michael Bell, and James Ruppert

As convective aggregation has been found to be supported by radiative heating in idealized simulations, this study seeks to answer whether such a property of convection exists in the observed convective organization. Data was collected during the ORCESTRA field campaign over the tropical Atlantic in August and September 2024. Cloud properties, precipitation, atmospheric radiative fluxes, and the derived degree of convective organization are measured by the Sea-Pol radar and other instruments on a shipborne platform (RV Meteor) supported by sub-campaigns including PICCOLO and BOW-TIE. We analyze how atmospheric radiative effects support the spatial organization of tropical deep convection, and also inversely, how the convective organization affects the strength of convective-radiative feedback. In particular, the strength of convective-radiative feedback is assessed by the temporal covariance between atmospheric radiative heatings and either moist static energy tendency or precipitation rate. We will show the observed dependency of convective-radiative feedback on the occurrence of various convective organization phenomena, including mesoscale convective organization and the passage of tropical waves. The effect of radiative heating and its induced circulation on the state of convective organization during the field campaign will also be derived from mechanism-denial numerical simulations.

How to cite: Hsiao, W.-T., Wing, A., Kennison, S., Bell, M., and Ruppert, J.: Interaction between cloud-radiative effects and convective systems measured during the ORCESTRA field campaign in Aug-Sep 2024, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7132, https://doi.org/10.5194/egusphere-egu25-7132, 2025.

X5.5
|
EGU25-17730
|
ECS
Geet George, Robert Mackenzie, Owen O'Driscoll, Daniel Klocke, Louise Nuijens, Pier Siebesma, and Team Menapia

STRINQS stands for Soundings and TuRbulent eddy measurements in the ITCZ with a Network of QuadcopterS and is one of the sub-campaigns under the umbrella of ORCESTRA, an international collaboration of measurement campaigns with the larger goal of understanding mesoscale organization of convection in the tropical Atlantic. STRINQS made measurements of the ITCZ boundary layer by employing four meteorological quadcopters, designed and developed by Menapia. Co-ordinated flights were conducted with the German research vessel Meteor as base, a part of the BOWTIE subcampaign in ORCESTRA. The quadcopters, designed to sustain performance in heavy rain and strong wind, provide high-resolution atmospheric soundings of temperature, humidity, pressure, and winds while allowing for high flight ceilings. There are two sets of meteorological sensors in each quadcopter, with a sampling frequency of 10 Hz. Additionally, a sonic anemometer configured on a 1 m arm above the quadcopter body helps provide wind measurements without disturbances due to the wake of the propellers during non-descending trajectories. The team had to initially overcome multiple logistical and technical challenges, unfortunately including mishaps. However eventually, between the period of 30th August and 9th September, the team successfully conducted around 45 vertical profiles reaching altitudes of up to 1500 m (the permitted flight ceiling for STRINQS) in addition to flying horizontal hexagonal patterns that traversed distances between 2 and 4 km horizontally. Some flights recorded intriguing case-studies such as profiling the boundary-layer thrice in a span of 40 minutes as an organized squall-line rain event passed over the ship, thus providing contrasting conditions before, during and after the storm. The meteorological sensors' data show promising results in the drone's capability to sample the boundary layer, but some corrections still need to be made to the retrieval of wind measurements, particularly vertical wind, which is known to be a challenging measurement from UAV (uncrewed aerial vehicle) platforms. Post data-processing and preliminary analyses, the data will be made publicly available in state of the art data formats. Although STRINQS only partially achieved its scientific goal of statistical sampling, the learnings on the measurement capabilities of such methods have been significant. With this demonstration of using a ship as a launchpad for coordinated flights of heavyduty quadcopters even in heavy rain events, STRINQS signals the possibilities of such strategies in future campaigns to provide a rich spatial characterization of the boundary layer.

How to cite: George, G., Mackenzie, R., O'Driscoll, O., Klocke, D., Nuijens, L., Siebesma, P., and Menapia, T.: Boundary-layer measurements of the ITCZ with meteorological quadcopters off a trans-Atlantic ship expedition, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17730, https://doi.org/10.5194/egusphere-egu25-17730, 2025.

Trade cumulus dynamics
X5.6
|
EGU25-7235
Raphaela Vogel and Martin Janssens

Two thirds of variability in cloud cover in the trade-wind regions is associated with cloudiness near the top of the cloud layer, which mostly occurs in the form of stratiform layers. Stratiform inversion cloud is also the cloud component that changes most across different patterns of cloud organization and potentially also under climate change. Unfortunately, our understanding of the factors controlling the occurrence and lifetime of stratiform layers and how they link to the structure of the trade inversion is limited. Because the trade inversion can be as thin as 10-100m, even high-resolution large-eddy simulations have serious issues in accurately representing the sharpness of the inversion and its associated cloudiness. The EUREC4A field campaign released >850 dropsondes from the HALO aircraft upstream Barbados in January-February 2020 in 200 km diameter circles, constituting a sounding dataset which lends itself particularly well to investigate the structure and variability of the trade inversion. Here we use the dropsonde data in conjunction with lidar-retrieved cloud-top height distributions and high resolution large-eddy simulations (the cloud botany ensemble) to investigate controls on inversion strength and height, document their variability at different scales, and assess their connection with cloudiness.    

How to cite: Vogel, R. and Janssens, M.: Mesoscale controls on trade-wind inversion structure and cloudiness during EUREC4A, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-7235, https://doi.org/10.5194/egusphere-egu25-7235, 2025.

X5.7
|
EGU25-18408
Silke Gross, Manuel Gutleben, Martin Wirth, and Florian Ewald

Clouds and convection play a key role in structuring atmospheric circulation and in determining the climate sensitivity. However, it is still not understood how clouds and convection will respond to warming of the atmosphere. This is due to an insufficient representation of clouds and moist convection in climate models. A better understanding of the coupling between water vapor, convection, cloud formation and circulation is needed. Shallow marine convection shows the largest frequency of occurrence amongst clouds. But besides being uniform clouds of similar structure, they can occur in different larger scale patterns of organization. The trade wind region is characterized by a complex structure of water vapor, aerosols and clouds. Depending on the season and larger scale circulation, it was found, that lofted layers of water vapor and aerosols can have a quite significant impact on the atmospheric stability, and with that on cloud structure and evolution.

Airborne lidar measurements with the combined water vapor differential absorption and high spectral resolution lidar system WALES provide simultaneous measurements of the water vapor mixing ratio and of aerosol properties. The WALES instrument was deployed in a series of airborne experiments aiming to better understand the coupling of clouds and convection over the sub-tropical and tropical Atlantic Ocean. The first campaign of this series, the NARVAL experiment, was conducted in wintertime out of Barbados. It was followed by the NARVAL-II experiment in August 2016, the EUREC4A experiment in January/February 2020 and the PERCUSION campaign in August and September 2024. The latter especially focused on the transition of shallow to deep convection and the ITCZ. Another add on of this campaign was the contrasting measurements over the east and west Atlantic Ocean. We used these measurements to investigate how the complex structure of water vapor and aerosol impact the stability of the atmosphere and with that the evolution and structure of clouds. We found that the impact is different, if the water vapor and aerosol are within distinct layers. During summertime, when they are well separated from the marine boundary layer, the radiative effect of the layers dominates. The evolution of shallow marine clouds below the SAL is suppressed. In wintertime, the e.g. dust is transported at lower altitudes and the dust layer is frequently mixed into the marine boundary layer. During this time of the year the effect of the layer on the evolution and lifetime of marine trade wind convection is much more complex, as the dust particles within the SAL might additionally act as cloud or ice nuclei.

In our presentation we will give an overview of the performed measurements and the radiative transfer calculations that were performed based on our findings. Those calculations together with the observations better help to understand the impact of lofted layers on cloud evolution and structure.

How to cite: Gross, S., Gutleben, M., Wirth, M., and Ewald, F.: Impact of elevated water vapor and aerosol layers on the stability of the sub-tropical atmosphere and the structure and evolution of shallow marine clouds, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18408, https://doi.org/10.5194/egusphere-egu25-18408, 2025.

X5.8
|
EGU25-13564
|
ECS
Examining Downstream Impacts of Mesoscale Sea Surface Temperature Anomalies on Trade Cumulus Clouds in Satellite Observations
(withdrawn)
Xuanyu Chen, Isabel McCoy, Ryan Eastman, Martin Janssens, Hauke Schulz, Geet George, and Juliana Dias
Cloud tracking
X5.9
|
EGU25-16875
Matthias Tesche, Felix Müller, and Torsten Seelig

The temporal development of cloud properties along the trajectory of a tracked clouds can show a behavior that is clearly unrealistic. For instance, a low-level cloud that is partly obscured by faint high-level clouds above can show development of cloud-top temperature with jumps of 40 K or more. To assess the general development of clouds tracked over central Europe, we have applied the ISCCP cloud classification to those clouds. It is found that the majority of the tracked clouds shows transitions between time steps that are either between identical cloud types (e.g. cumulus to cumulus) or represent reasonable development (e.g. stratus to stratocumulus or vice versa). The additional consideration of objective weather types enables an assessment of the large-scale conditions under which different cloud types are most abundant.

How to cite: Tesche, M., Müller, F., and Seelig, T.: Track ‘n’ Type: Do tracked clouds show a realistic behavior with respect to cloud type?, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16875, https://doi.org/10.5194/egusphere-egu25-16875, 2025.

X5.10
|
EGU25-17353
|
ECS
Felix Müller, Torsten Seelig, Hauke Schulz, Diego Villanueva, and Matthias Tesche

We compare satellite data from the EUREC4A campaign (observed by the Advanced Baseline Image onboard the GOES-16 satellite) and model output from ICON-LEM tailored for the EUREC4A campaign [1]. All datasets are located east of Barbados in the Caribbean Sea. We build on previous cloud tracking analyses for the GOES satellite dataset [2].

We use a cloud tracking algorithm [2] to find lifetime and cloud size distributions. The trajectories can be classified into the four mesoscale cloud patterns “sugar” to “fish” based on C3ONTEXT data which makes it possible to investigate how well these patterns are represented in the model data. We compare the distributions of cloud sizes, lifetimes and the average development of cloud size over the cloud’s lifetimes.

Cloud modelling is a very important tool for climate research. However, it is not an easy task to validate model data and assess a model’s performance. The cloud tracking enables us to provide a unique quality assessment of the model data. Lifetime information is interesting because it encompasses multiple dynamic scales from micro to planetary regimes, while cloud size and cloud cover are important factors for the radiative properties of the clouds in a region and characterise the clouds’ general behavior.

 

[1] Schulz, Hauke & Stevens, Bjorn (2023) “Evaluating Large-Domain, Hecto-Meter, Large-Eddy Simulations of Trade-Wind Clouds Using EUREC4A Data” in Journal of Advances in Modeling Earth Systems, doi: 10.1029/2023MS003648

[2] Seelig et al. (2023) “Do optically denser trade-wind cumuli live longer?”, in Geophysical Research Letters, doi: 10.1029/2023GL103339

How to cite: Müller, F., Seelig, T., Schulz, H., Villanueva, D., and Tesche, M.: Tracking Clouds: Assessing the representation of mesoscale cloud patterns in the EUREC4A model data, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-17353, https://doi.org/10.5194/egusphere-egu25-17353, 2025.

X5.11
|
EGU25-19918
William Jones and Philip Stier

Tropical anvil clouds have significant impacts on the atmosphere due to their cloud radiative effect (CRE), and their response to warming remains one of the largest uncertainties in future climate projections. Recent research has highlighted both the importance of changes in anvil cloud structure and changes in convective mass flux in a warmer climate to CRE feedbacks. However, understanding of these processes is limited due to a lack of observations linking convective processes to anvil cloud properties across their entire lifetimes. We apply the tobac-flow algorithm to a year of Meteosat SEVIRI observations over Africa and the tropical Atlantic to detect and track convective cores and their subsequent anvil clouds to investigate the impact of convective dynamics on anvil clouds. By combining this cloud tracking dataset with retrieved cloud properties and broadband fluxes, changes in the intensity and organisation of convection can be linked to changes in anvil CRE. Overall, both more intense and more organised convection tends to result in anvils with positive CRE, as these storms produce higher, colder anvil clouds and, over land, anvils that exist for longer at night. However, when controlling for the anvil temperature and time of day, more intense convection tends to result in positive CRE, while more organised convection results in a negative CRE. We attribute these differences to changes in anvil structure, as we observe that more organised convection tends to produce thicker anvils, while more intense convection results in thinner anvils. The contrasting effects of different convective processes on anvil CRE highlight the importance of understanding the mechanisms through which convective dynamics affect anvil structure, and indicate that different changes in convective processes may lead to regional differences in anvil cloud feedbacks.

How to cite: Jones, W. and Stier, P.: Contrasting effects of convective intensity and organisation on anvil cloud radiative effect observed using cloud tracking, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-19918, https://doi.org/10.5194/egusphere-egu25-19918, 2025.