“…In its climatological mean, late-winter cooling of the upper Labrador Sea induces strong vertical mixing down to a depth of several hundred meters (Fig. 2c, contours) that forms a core of very dense waters within the SPG's center, which in turn strengthens the zonal gradient of upper-ocean densities and, thereby, the gyre's circulation (Born and Stocker 2014). After the SPG shift, however, ocean deep mixing is locally hampered as fresher, hence lighter, surface conditions develop in the Labrador Sea (Figs.…”