Abstract. The processes that contribute to the flat sea surface height (SSH) wavenumber
spectral slopes observed in the tropics by satellite altimetry are examined
in the tropical Pacific. The tropical dynamics are first investigated with a
1â12â global model. The equatorial region from
10ââN to 10ââS is dominated by tropical instability waves
with a peak of energy at 1000âkm wavelength, strong anisotropy, and a
cascade of energy from 600âkm down to smaller scales. The off-equatorial
regions from 10 to 20â latitude are characterized by a narrower
mesoscale range, typical of midlatitudes. In the tropics, the spectral taper
window and segment lengths need to be adjusted to include these larger
energetic scales. The equatorial and off-equatorial regions of the
1â12â model have surface kinetic energy spectra consistent with
quasi-geostrophic turbulence. The balanced component of the dynamics slightly
flattens the EKE spectra, but modeled SSH wavenumber spectra maintain a steep
slope that does not match the observed altimetric spectra. A second analysis
is based on 1â36â high-frequency regional simulations in the
western tropical Pacific, with and without explicit tides, where we find a
strong signature of internal waves and internal tides that act to increase
the smaller-scale SSH spectral energy power and flatten the SSH wavenumber
spectra, in agreement with the altimetric spectra. The coherent M2Â baroclinic
tide is the dominant signal at âŒ140âkm wavelength. At short scales,
wavenumber SSH spectra are dominated by incoherent internal tides and
internal waves which extend up to 200âkm in wavelength. These incoherent
internal waves impact space scales observed by today's along-track
altimetric SSH, and also on the future Surface Water Ocean Topography (SWOT) mission 2-D swath observations, raising
the question of altimetric observability of the shorter mesoscale structures
in the tropics.