EGU23-16379, updated on 07 Jul 2023
https://doi.org/10.5194/egusphere-egu23-16379
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

The diurnal warm layer and its consequences for the upper ocean: from EUREC4A-OA observations and the global coupled ICON-ESM

Florian Schuette1,3, Diego Lange2, Dian Putrasahan3, Ruben Carrasco4, Pierre L'Herguet5, Dongxiao Zhang6, Sabrina Speich7, Jin-Song von Storch3, and Johannes Karstensen1
Florian Schuette et al.
  • 1GEOMAR Helmholtz-Centre for Ocean Research Kiel, PO, Kiel, Germany (fschuette@geomar.de)
  • 2Universität Hohenheim, Stuttgart, Germany
  • 3Max-Planck-Institut für Meteorologie, Hamburg, Germany
  • 4Helmholtz-Zentrum Hereon, Geestacht, Germany
  • 5Université de Bretagne Occidentale, Brest, France
  • 6National Oceanic and Atmospheric Administration Pacific Marine Environmental Laboratory, Seattle, USA
  • 7Ecole Normale Supérieure Department of Geosciences Laboratoire de Météorologie Dynamique, Paris, France

The uppermost 0-20m depth of the ocean within the mixed layer (ML) were investigated on diurnal scales using data collected during the EUREC4A campaign in the western tropical Atlantic. The results are compared against data from the global coupled Earth System model ICON. In both datasets is the diurnal impulse generator the penetrating shortwave solar radiation, heating the first meters of the ocean. During day on top of the ML a stably stratified near-surface layer, called the diurnal warm layer (DWL), can be formed. Depending on the wind conditions or the amount of incoming solar radiation the depth of such a DWL can reach from several centimeters to tens of meters. Associated to the stable stratification (and the wind) shear is produced which propagates down with time. At that point, the model and the observations start to differ. Using high-resolution current measurements of ADCP’s mounted on saildrones the detailed structure of the descending shear layer is observed. The cycle of shear instability leads the diurnal mixing cycle, typically by 2–3 h, consistent with the time needed for instabilities to grow and break (observed by microstructure measurements). In the morning, the turbulence decays and the upper ocean restratifies. At this point, wind accelerates the near-surface flow to form a new unstable shear layer, and the cycle begins again. Since the study area is located around 15°N, the excited layers are affected by the Coriolis force, which causes the descending shear layer to rotate around the inertial frequency of 1.8 days. Compared to the global coupled earth system model, these processes cannot be represented in such detail here. This leads to lower shear (and also mixing) at the different time and depth. Different model configurations show that even small differences in the upper 20m of the ocean, such as those observed, can lead to quite large changes in the model, e.g., a different strength of the ocean current system down to 1000m depth.

How to cite: Schuette, F., Lange, D., Putrasahan, D., Carrasco, R., L'Herguet, P., Zhang, D., Speich, S., von Storch, J.-S., and Karstensen, J.: The diurnal warm layer and its consequences for the upper ocean: from EUREC4A-OA observations and the global coupled ICON-ESM, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-16379, https://doi.org/10.5194/egusphere-egu23-16379, 2023.