EGU24-18021, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-18021
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Cross-front wind forcing of a dense submesoscale filament

Lars Umlauf1, Mira Schmitt1, and Jen-Ping Peng2
Lars Umlauf et al.
  • 1Leibniz-Institute for Baltic Sea Research, Rostock, Germany (lars.umlauf@io-warnemuende.de)
  • 2University of Western Australia, Perth, Australia (jen-ping.peng@uwa.edu.au)

In this study, the effects of cross-front winds on a submesoscale dense filament are investigated using high-resolution turbulence and velocity observations, and idealized numerical simulations. Our study area is the Baltic Sea, which is characterized by strong frontal gradients and pronounced submesoscale dynamics. Embedded in a large-scale frontal region, our observations reveal the existence of a 3-4 km wide, dense filament with an asymmetric structure resulting from the interactions between cross-front winds and the two submesoscale fronts laterally bounding the filament. These two fronts are driven by either downgradient winds, directed from the lighter surrounding waters toward the dense center of the filament, or upgradient winds, directed in the opposite direction. While the effect of a wind stress that is aligned with the frontal jet has been investigated in numerous previous studies, especially field data focusing on the role of cross-front winds are largely lacking at the moment. We find that for downgradient winds, when the surface Ekman transport and the frontal jet are aligned, both the frontal jet and the cross-front secondary circulation are enhanced. The latter supports a tendency for frontal re-stratification, suppression of turbulence, and mixed-layer shoaling. For the front with upgradient wind forcing, the Ekman transport and the frontal jet nearly cancel, and also the cross-front secondary circulation is strongly suppressed. Restratification by the secondary circulation is weak in this case, and the well-mixed turbulent surface layer is approximately twice as deep compared to the other side of the filament with downgradient forcing. We show that these mechanisms are consistent with results from idealized numerical simulations of frontal regions with downgradient and upgradient wind forcing.

How to cite: Umlauf, L., Schmitt, M., and Peng, J.-P.: Cross-front wind forcing of a dense submesoscale filament, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-18021, https://doi.org/10.5194/egusphere-egu24-18021, 2024.