Noble gas tracers of ventilation during deep-water formation in the Weddell Sea

7th International Symposium on Gas Transfer at Water Surfaces

Nicholson, D.P.^1 ; Khatiwala, S.^2 ; Heimbach, P.^3,4

Marine Chemistry and Geochemistry Department, Woods Hole Oceanographic Institution, 266 Woods Hole Road, Woods Hole

MA

02543, United States^1

Department of Earth Sciences, University of Oxford, South Parks Road, Oxford

OX1 3AN, United Kingdom^2

Institute for Computational Engineering and Sciences, Jackson School of Geosciences, University of Texas at Austin, 201 East 24th Street, Austin

TX

78712, United States^3

Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge

MA

02139, United States^4

关键词: Deep-water formation;    Dynamic adjustment;    High Latitudes;    Model simulation;    Oceanic uptake;    Saturation anomalies;    Seasonal cycle;    Stationary solutions;   

Others  :  https://iopscience.iop.org/article/10.1088/1755-1315/35/1/012019/pdf
DOI  :  10.1088/1755-1315/35/1/012019

来源: IOP

【 摘 要 】

To explore the dynamics and implications of incomplete air-sea equilibration during the formation of abyssal water masses, we simulated noble gases in the Estimating the Circulation & Climate of the Ocean (ECCO) global ocean state estimate. A novel computation approach utilizing a matrix-free Newton-Krylov (MFNK) scheme was applied to quickly compute the periodic seasonal solutions for noble gas tracers. MFNK allows for quick computation of a cyclo-stationary solution for tracers (i.e., a spun-up, repeating seasonal cycle), which would otherwise be computationally infeasible due to the long time scale of dynamic adjustment of the abyssal ocean (1000's of years). A suite of experiments isolates individual processes, including atmospheric pressure effects, the solubility pump and air-sea bubble fluxes. In addition to these modeled processes, a volumetric contribution of 0.28 ± 0.07% of glacial melt water is required to reconcile deep-water observations in the Weddell Sea. Another primary finding of our work is that the saturation anomaly of heavy noble gases in model simulations is in excess of two-fold more negative than is suggested from Weddell Sea observations. This result suggests that model water masses are insufficiently ventilated prior to subduction and thus there is insufficient communication between atmosphere and ocean at high latitudes. The discrepancy between noble gas observations and ECCO simulations highlights that important inadequacies remain in how we model high-latitude ventilation with large implications for the oceanic uptake and storage of carbon.