EGU26-3115, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-3115
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 07 May, 09:25–09:35 (CEST)
 
Room M2
Effects of Saharan air layers on clouds over the tropical Atlantic during BOWTIE
Anna Trosits1,2, Andreas Foth2, Moritz Haarig3, Jonas Witthuhn2, Anton Kötsche2, Johanna Roschke2, and Heike Kalesse-Los2
Anna Trosits et al.
  • 1Institute for Atmospheric and Climate Science, ETH Zürich, Zürich, Switzerland (anna.trosits@env.ethz.ch)
  • 2Leipzig Institute for Meteorology, Leipzig University, Leipzig, Germany
  • 3Leibniz Institute for Tropospheric Research (TROPOS), Leipzig, Germany

The radiative effect of clouds is determined by their development, lifetime and microphysical characteristics. The processes influencing cloud properties are diverse and require further investigation to gain a more profound understanding. However, process studies cannot be conducted by modelling alone, as observations are rarely available, particularly over the oceans. This leads to uncertainties in global weather modelling and climate forecasts. In order to disentangle the effects of various influencing factors on clouds in the intertropical convergence zone (ITCZ), recent observations from the BOWTIE campaign are being analysed with regard to the effects of Saharan dust. During the BOWTIE (Beobachtung von Ozean und Wolken – das Trans-ITCZ Experiment) campaign, which was part of the ORCESTRA (Organized Convection and EarthCARE Studies over the Tropical Atlantic) campaign, the research vessel (RV) Meteor crossed the tropical Atlantic from Cape Verde to Barbados in August and September 2024. The proximity to the African continent and the Sahara led to some trajectories of the Saharan air layers (SAL) traversing the atmosphere above the RV Meteor. Three episodes of SAL lasting between two and three days were observed at altitudes spanning from one to five km. The dry and dust-loaden character of the SAL is determined by their origin in the Saharan desert. Analysis of the Raman lidar observations provides information about the time and altitude of the SAL. In synergy with other instruments, such as radiosondes and a motion-stabilised 94GHz cloud radar, the effect on clouds can be investigated. The stabilisation of the cloud radar, which was monitored by STARPAS (STAbilized Radar Platform Alignment Sensor), ensures reliable vertically pointing cloud observations. The findings indicate that SAL reduces cloud vertical development and suppresses weak convection. This behaviour is due to the thermodynamic structure of the SAL with low relative humidity, nearly dry adiabatic temperature gradients and inversions at the top and bottom. Particle-specific properties of acting as cloud condensation nuclei or ice nucleating particles are of secondary order.

How to cite: Trosits, A., Foth, A., Haarig, M., Witthuhn, J., Kötsche, A., Roschke, J., and Kalesse-Los, H.: Effects of Saharan air layers on clouds over the tropical Atlantic during BOWTIE, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-3115, https://doi.org/10.5194/egusphere-egu26-3115, 2026.