EGU26-14270, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-14270
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Tuesday, 05 May, 16:50–17:00 (CEST)
 
Room L2
Cold Pools Drive Short-Term Thermohaline Variability in the Ocean Skin Layer
Riaz Bibi1, Leonie Jaeger1, Carsten Rauch1, Samuel Mintah Ayim1, Lisa Gassen1, Mariana Ribas-Ribas1, Sean W. Freeman2,3, Kyra Britton2, Leah D. Grant4, Nicholas M. Falk4, Christine A. Neumaier4, Susan van den Heever4, Diana L. Monroy5, Jan Härter5, and Oliver Wurl1
Riaz Bibi et al.
  • 1Institute for Chemistry and Biology of the Marine Environment (ICBM), School of Mathematics and Science, Carl von Ossietzky University of Oldenburg, Oldenburg, Germany
  • 2Department of Atmospheric and Earth Science, The University of Alabama in Huntsville, Huntsville, AL
  • 3Earth System Science Center, The University of Alabama in Huntsville
  • 4Department of Atmospheric Science, Colorado State University, Fort Collins, Colorado
  • 5Department of Physics and Astronomy, University of Potsdam, Potsdam, Germany

Atmospheric cold pools are transient sub-mesoscale to mesoscale weather phenomena generated by convective precipitation. They are characterized by cool, dense air spreading laterally, which strongly alters near-surface atmospheric conditions and the thermohaline properties of the ocean skin layer (< 1 mm) and near-surface layer (NSL: < 1 m). The spatial extent and thermodynamic intensity of atmospheric cold pools are moderated by mixing within the moist marine boundary layer (MBL), the lowest ~0.5–1 km of air above the ocean. Despite this moderation, accompanying wind surges and intense precipitation drive short-lived intensifications of atmosphere–ocean fluxes that can abruptly restructure upper-ocean thermohaline structure, an aspect that remains poorly constrained by in situ measurements and is underrepresented in coupled atmosphere–ocean models.

Here we present observations of atmospheric cold pool passages over the tropical Atlantic Ocean, combining ship-based meteorological measurements, aerial drones, weather balloon profiles, and high-resolution observations from the autonomous surface vehicle HALOBATES. Equipped with meteorological and oceanographic sensors sampling at high-resolution (1 Hz), HALOBATES resolves the ocean skin layer and the NSL dynamics, allowing us to identify and characterize cold pools as they passed over the study area during the R/V METEOR M211 field campaign (14 June–27 July 2025).

Between 13 and 18 July 2025, cold pool passages were identified by rapid air-temperature drops of 0.6–1.8 °C and, during rainy events, rainfall rates of up to 37 mm h⁻¹. All cold pools induced transient ocean surface cooling, leading to sea surface temperature anomalies (Tskin-TNSL) of 0.02 – 0.35 °C, and amplified cooling in the skin layer relative to the NSL. To quantify the cooling and recovery of the ocean skin layer following the cold pool passage, we consider two different skin-layer depths: the infrared (IR) skin layer observed by thermal cameras and the skin layer measured in situ by HALOBATES. This comparison shows that skin-temperature responses evolve on timescales of only a few minutes and therefore require high temporal resolution in situ measurements to be adequately resolved.

Salinity responses depended critically on precipitation: cold pools that passed the study area without measurable rainfall produced negligible changes, whereas intense-rain events freshened the skin by up to 1.3 g kg-1 and the NSL by 0.4 g kg-1, forming shallow freshwater lenses that re-stratified the upper meter within approximately 15 minutes. Pronounced cold pool passages were accompanied by enhanced latent and sensible heat fluxes, with maximum increases of −140 W m⁻² and −30 W m⁻², respectively, driven primarily by increased wind speeds and indicating intensified ocean-to-atmosphere heat exchange. These observations demonstrate that cold pools strongly affect short-term variability in upper-ocean thermohaline structure through short-lived intense peaks in atmosphere–ocean fluxes, emphasizing the need to include these transient events in future coupled atmosphere–ocean models.

How to cite: Bibi, R., Jaeger, L., Rauch, C., Mintah Ayim, S., Gassen, L., Ribas-Ribas, M., W. Freeman, S., Britton, K., D. Grant, L., M. Falk, N., A. Neumaier, C., van den Heever, S., L. Monroy, D., Härter, J., and Wurl, O.: Cold Pools Drive Short-Term Thermohaline Variability in the Ocean Skin Layer, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14270, https://doi.org/10.5194/egusphere-egu26-14270, 2026.