Antarctic Bottom Water (AABW), which fills the global ocean abyss, is derived from dense water that forms in several distinct Antarctic shelf regions. Previous modeling studies have reached conflicting conclusions regarding export pathways of AABW across the Southern Ocean and the degree to which AABW originating from distinct source regions are blended during their export. This study addresses these questions using passive tracer deployments in a 61‐year global high‐resolution (0.1°) ocean/sea‐ice simulation. Two distinct export “conduits” are identified: Weddell Sea‐ and Prydz Bay‐sourced AABW are blended together and exported mainly to the Atlantic and Indian Oceans, while Ross Sea‐ and Adelie Land‐sourced AABW are exported mainly to the Pacific Ocean. Northward transport of each tracer occurs almost exclusively (>90%) within a single conduit. These findings imply that regional changes in AABW production may impact the three‐dimensional structure of the global overturning circulation.
Previous studies have concluded that the wind-input vorticity in ocean gyres is balanced by bottom pressure torques (BPT), when integrated over latitude bands. However, the BPT must vanish when integrated over any area enclosed by an isobath. This constraint raises ambiguities regarding the regions over which BPT should close the vorticity budget, and implies that BPT generated to balance a local wind stress curl necessitates the generation of a compensating, non-local BPT and thus non-local circulation. This study aims to clarify the role of BPT in wind-driven gyres using an idealized isopycnal model. Experiments performed with a single-signed wind stress curl in an enclosed, sloped basin reveal that BPT balances the winds only when integrated over latitude bands. Integrating over other, dynamically-motivated definitions of the gyre, such as barotropic streamlines, yields a balance between wind stress curl and bottom frictional torques. This implies that bottom friction plays a non-negligible role in structuring the gyre circulation. Non-local bottom pressure torques manifest in the form of along-slope pressure gradients associated with a weak basin-scale circulation, and are associated with a transition to a balance between wind stress and bottom friction around the coasts. Finally, a suite of perturbation experiments is used to investigate the dynamics of BPT. To predict the BPT, the authors extend previous theory that describes propagation of surface pressure signals from the gyre interior toward the coast along planetary potential vorticity contours. This theory is shown to agree closely with the diagnosed contributions to the vorticity budget across the suite of model experiments.
The formation and northward export of Antarctic Bottom Water (AABW) supplies the deepest branch of the global meridional overturning circulation (MOC;Lumpkin & Speer, 2007;Talley, 2013). This export ventilates the global abyss, with AABW comprising over one-third of the volume of the subsurface ocean (Gebbie & Huybers, 2011). In addition to supplying oxygen (Gordon, 2009;Orsi et al., 2001), AABW serves as a reservoir of carbon dioxide many times larger than the atmosphere's (Russell et al., 2006;Skinner et al., 2010). The spread of AABW is, therefore, arguably the most climatically important branch of the MOC on centennial to millennial time scales (Marshall & Speer, 2012).Despite the global importance of AABW export, there are currently no direct measurements of its total meridional transport in the Southern Ocean. In contrast, deep ocean transports in the Atlantic basin are sampled by the Rapid Climate Change-Meridional Overturning Circulation and Heatflux Array (RAPID;Johns et al., 2011), Overturning in the Subpolar North Atlantic Program array (OSNAP;Schiermeier, 2013) and South Atlantic Meridional Overturning Circulation -Basin-wide Array (SAMBA; Ansorge et al., 2014), with additional arrays in preparation (Frajka-Williams et al., 2019). Estimates of AABW transport have been derived from inverse model calculations, but the available measurements permit only the multi-decadal mean transports to be estimated (Lumpkin & Speer, 2007;Naveira Garabato et al., 2016;Sloyan & Rintoul, 2001). While multi-decadal changes in the properties and transport of AABW have been inferred
A mechanism is presented, based on multiscale interactions via nonlinear wind-induced surface heat exchange (WISHE), that produces eastward-propagating, intraseasonal convective anomalies in the tropical atmosphere. Simulations of convectively coupled disturbances are presented in two intermediate-complexity atmospheric models. One is a shallow water model with a simple WISHE-motivated heating term. The other model is also based on a first baroclinic mode but has an additional prognostic equation for humidity and a simple representation of moist convection based on a quasi-equilibrium approximation. In spite of many differences between the models, they robustly produce a coherent signal in westerly winds and convection that travels eastward at 4–10 m s−1. It is shown here that this slow signal is a forced response to an eastward-propagating Yanai (mixed Rossby–gravity) wave group. The response takes the form of a forced Kelvin wave that is driven nonlinearly, via WISHE, by meridional wind anomalies of the Yanai wave group and that travels considerably more slowly than the free convectively coupled Kelvin waves in these models. The Yanai waves are destabilized in the models used here by WISHE in the presence of mean easterlies, but more generally they could also be excited by stratiform instability in the absence of mean easterlies so that the mechanism described here could also operate without mean easterlies. Similarities to and differences from the Madden–Julian oscillation (MJO) and convectively coupled tropical waves are discussed.
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