EGU24-15978, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-15978
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

An attempt to calibrate a density-dependent groundwater flow model for a high energy subterranean estuary using particle swarm optimization and integrating salinity-, temperature- and 3H/He age observations 

Janek Greskowiak1, Rena Meyer1, Jairo Cueto2, Nico Skibbe3, Anja Reckhardt4, Thomas Günther3, Stephan Seibert1, Kai Schwalfenberg4, Dietmar Pommerin4, Mike Müller-Petke3, and Gudrun Massmann1
Janek Greskowiak et al.
  • 1Institute for Biology and Environmental Sciences, Carl von Ossietzky Universität Oldenburg, Oldenburg, Germany
  • 2Institute for Geosciences, Christian-Albrechts-Universität Kiel, Kiel, Germany
  • 3Department for Geoelectrics and Electromagnetics, Leibniz-Institute for Applied Geophysics, Hannover, Germany
  • 4Institute for Chemistry and Biology of the Marine Environment, Carl von Ossietzky Universität Oldenburg, Oldenburg, Germany

Subterranean estuaries below high-energy beaches are understudied, despite being potential powerful biogeochemical reactors at the land/sea transition zone affecting the quality of coastal waters. Highly transient hydro(geo)logical boundary conditions and density-effects lead to dynamic subsurface flow and transport patterns which are difficult to understand and hard to replicate by models. A comprehensive and unique 1-year dataset of hydraulic heads, salinity and temperature data in combination with apparent 3H/He ages was obtained at a beach research site on Spiekeroog Island in North Germany. The site includes 3 multilevel groundwater monitoring wells and a vertical electrode chain with 10 temperature sensors, all positioned on a transect aligned along the principal cross-shore flow direction and all reaching down to 24 m depth below ground surface. The data-set was used to set up and calibrate a site-specific groundwater flow and transport model, aiming to approximate the highly dynamic groundwater flow patterns on that transect. The simulation time needed to be 20 years because of the long model spin-up. Due to the complex and nonlinear nature of the system, model calibration was carried out via particle swarm optimization, which is superior to gradient-based optimization techniques with respect to finding a global minimum of the objective function. The calibration results were reasonable. The dynamics of hydraulic head data were well captured, however, simulated values were constantly higher than those observed. The observed salinities were best captured for the multilevel wells near the mean high water and low water line. At the highest multilevel well located at the upper beach right at the dune base, simulations matched observations less well. Similarly, groundwater temperatures and ages were best replicated at the location in the infiltration zone near the high-water line. Groundwater ages and their temporal dynamics at the dune base and mean low water line could only be replicated down to 12 m depth. Deviations between simulations and observations are likely due to 3D flow effects in longshore direction, which could not be captured with the 2D vertical cross-sectional model approach. However, long model run times hindered calibration of a full-blown 3D density-dependent, 20-year long-term groundwater flow and transport model. The next step is to estimating the importance of longshore hydraulic gradients. Finally, the model will be extended for hydrobiogeochemical reactions to assist in the analysis and understanding of the observed hydrochemical data at this site.                    

How to cite: Greskowiak, J., Meyer, R., Cueto, J., Skibbe, N., Reckhardt, A., Günther, T., Seibert, S., Schwalfenberg, K., Pommerin, D., Müller-Petke, M., and Massmann, G.: An attempt to calibrate a density-dependent groundwater flow model for a high energy subterranean estuary using particle swarm optimization and integrating salinity-, temperature- and 3H/He age observations , EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-15978, https://doi.org/10.5194/egusphere-egu24-15978, 2024.