Analysis of the scale dependence of the atmosphere-ocean thermal coupling using cross-spectral methods.
Abstract:
The obtained analytical solutions are found to be linearly dependent on the power spectral density of the model’s forcing terms associated with ocean and atmosphere dynamics, and help to distinguish between the atmosphere- and ocean-driven coupling regimes in the cross-spectra computed from satellite-based estimates of SST/SST-tendency and THF. Similar to recent conclusions drawn for SST and 10-m wind speed, our new results show that the transition between regimes occurs at wavelengths near the atmospheric first baroclinic Rossby radius of deformation, and that the dispersion of correlated signals indicative of the ocean-driven regime resembles that of oceanic planetary waves. We further demonstrate that the use of realistic spectral variance distributions for the theoretical model’s oceanic and atmospheric forcing signals enables the model to reproduce the observed cross-scale transition reasonably well. This correspondence suggests that the transition is linked to the distinct spectral power distribution of intrinsic variability in each medium, occurring because (a) the atmospheric SST modulation is significant at large scales but weaker over the ocean mesoscales, mainly because the mesoscale wind variance is itself weaker; concurrent with (b) the strong ocean-driven SST modulation over mesoscale ranges.