The relevance of surface quasi-geostrophic dynamics (SQG) to the upper ocean and the atmospheric tropopause has been recently demonstrated in a wide range of conditions. Within this context, the properties of SQG in terms of kinetic energy (KE) transfers at the surface are revisited and further explored. Two well-known and important properties of SQG characterize the surface dynamics: (i) the identity between surface velocity and density spectra (when appropriately scaled) and (ii) the existence of a forward cascade for surface density variance. Here we show numerically and analytically that (i) and (ii) do not imply a forward cascade of surface KE (through the advection term in the KE budget). On the contrary, advection by the geostrophic flow primarily induces an inverse cascade of surface KE on a large range of scales. This spectral flux is locally compensated by a KE source that is related to surface frontogenesis. The subsequent spectral budget resembles those exhibited by more complex systems (primitive equations or Boussinesq models) and observations, which strengthens the relevance of SQG for the description of ocean/atmosphere dynamics near vertical boundaries. The main weakness of SQG however is in the small-scale range (scales smaller than 20-30 km in the ocean) where it poorly represents the forward KE cascade observed in non-QG numerical simulations.
IntroductionFundamental questions of ocean and atmosphere dynamics are how their equilibrium energy spectrum is established and what are the underlying spectral energy transfers. One difficulty is that there is a variety of contributing processes, and different fluid regions and dynamical regimes must be distinguished. In particular, regions close to boundaries, such as the ocean surface or the atmospheric tropopause, behave differently than does the interior. For boundaries Blumen (1978) developed a surface quasi-geostrophic (SQG) theory that serves as a counterpart to a model of three-dimensional geostrophic turbulence (Charney 1971). While the latter is driven by large-scale interior potential vorticity (PV) contrasts and is not influenced by boundary anomalies, SQG dynamics is entirely driven by the density (or potential temperature in the atmosphere) anomaly evolution at the boundary. As such, frontogenesis (in 166 X. Capet, P. Klein, B. L. Hua, G. Lapeyre and J. C. McWilliams its QG limit) is the key process in SQG systems. SQG theory has been recently used to describe the three-dimensional dynamics of the upper troposphere (Juckes 1994;Hakim, Snyder & Muraki 2002;Tulloch & Smith 2006) and the upper oceanic layers LaCasce & Mahadevan 2006;Isern-Fontanet et al. 2006). To better understand the range of applicability of the SQG theory, have further revisited theoretically and numerically the question of the coupling of the boundary dynamics (driven by the surface density) with the interior dynamics (driven by the interior PV gradients). Using the dynamical analogy (suggested by Bretherton 1966) of the surface density as a boundary PV delta-function...