Since the launch of ERS-1 in 1991, a sequence of satellites equipped with altimeters have continuously observed sea surface height (SSH) at global scales. Although satellite altimetry has changed our understanding of many oceanographic phenomena at large and mesoscales (e.g., El Niño, Rossby waves, mesoscale eddies), the temporal and spatial resolution of the present constellation is insufficient to observe the two-dimensional structure of SSH variability at scales shorter than 150 km (Morrow et al., 2019). The upcoming Surface Water and Ocean Topography (SWOT) mission will change this paradigm by mapping the sea surface via two parallel 50-km-wide swaths, capable of resolving processes with wavelengths as small as ∼15 km.Recent work motivated by SWOT has explored the different dynamical processes that contribute to the sea surface height variability at meso (100-300 km) and large submesoscales (15−100 km). Observational and numerical studies focusing both on regions of strong baroclinic jets (e.g., Callies et al., 2015;Qiu et al., 2018; and less energetic currents (e.g., Chereskin et al., 2019), have found SSH spectra consistent with quasi-geostrophic (QG) turbulence theory, which predicts a wavenumber (k) spectrum that decays with a spectral slope ranging from k −5 to k −11/3 for wavenumbers in the mesoscale-to-submesoscale range. However, for spatial scales shorter than the so-called "transition scale" (Qiu et al., 2018), inertia-gravity waves (IGWs) play an important role in SSH variability, and the spectral slope of the SSH spectrum is typically shallower than the QG turbulence prediction of k −11/3 (Rocha, Qiu et al., 2017). Here, we refer to the low-wavenumber region of the SSH spectrum, that has a clear negative spectral slope, as the red zone (Figure 1, left).Beyond this transition scale, at wavelengths ranging from tens of kilometers to a few kilometers, multiple dynamical processes such as internal waves, submesocale fronts, infra-gravity waves, and surface wave groups are expected to contribute to the SSH wavenumber spectrum; however, the lack of observations in this range of wavenumbers makes it difficult to understand the role of each process, and results from numerical ocean models