Role of resolved and parameterized eddies in the Labrador Sea balance of heat and buoyancy

• Main Authors: Smith, Gregory C., Yashayaev, Igor, Saenko, Oleg A., Dupont, Frédéric, Myers, Paul G., Yang, Duo
• Format: Other/Unknown Material
• Language: English
• Published: 2014
• Subjects: envir; geo; Greenland; Labrador Sea
• Online Access: https://doi.org/10.7939/R3F47H82P; https://era.library.ualberta.ca/items/a86cb12d-9cef-451a-be34-a19437e814c0

Deep convection in the Labrador Sea is an important component of the global ocean ventilation. The associated loss of heat to the atmosphere from the interior of the sea is thought to be mostly supplied by mesoscale eddies, generated either remotely or as a result of convection itself—processes that are not resolved by low-resolution ocean climate models. The authors first employ a high-resolution (°) ocean model forced with high-resolution (33 km, 3 h) atmospheric fields to further elaborate on the role of mesoscale eddies in maintaining the balance of heat and buoyancy in the Labrador Sea. In general agreement with previous studies, it is found that eddies remove heat along the coast and supply it to the interior. Some of the eddies that are generated because of the barotropic instability off the west coast of Greenland are recaptured by the boundary current. In the region of deep convection, the convergence of heat and buoyancy by eddies significantly increases with the deepening of the winter mixed layer. In addition, the vertical eddy flux plays an important part in the heat budget of the upper Labrador Sea, accounting for up to half of the heat loss to the atmosphere north of 60°N. A low-resolution (1°) model with parameterized eddies is then applied to show that it does capture, qualitatively, the general structure of eddy buoyancy advection along the Labrador Current. However, the 1° model is deficient in this regard in the most eddy active region off the west coast of Greenland, although some improvements can be made by forcing it with the high-resolution atmospheric fields.