The 1991-1992 Acoustic Mid-Ocean Dynamics Experiment (AMODE) in the Sargasso Sea included an acoustic tomography array (Figure 1) deployed for about a year. The tomography data were used to show that the mode-1, diurnal (O1, K1) internal tides of the region were resonantly trapped between Puerto Rico and their turning latitudes at about 30°N (Dushaw, 2006;Dushaw & Worcester, 1998). The observed waves were a different manifestation of the trapped, Equatorial Pacific internal waves described by Wunsch and Gill (1976), different in that they were tidally-forced and observed deterministically, rather than wind-forced and observed statistically. By their amplitude and phase structures across the tomography array and other properties, the Sargasso Sea diurnal internal tides were shown to be large standing waves with inordinately large energy density.The observations by tomography are a natural filter selecting mode-1 internal tides (Dushaw, 2003;Dushaw et al., 1995Dushaw et al., , 2011Munk et al., 1995). References to the "internal tide" in this paper are restricted to the first internal-wave mode. As observed during AMODE, the temperature variations of the internal tides were temporally coherent (Dushaw, 2006) (see also Hendry, 1977). The waves are also observed by satellite altimetry (Carrere et al., 2021;Dushaw, 2015;Dushaw et al., 2011;Ray & Mitchum, 1996), although the diurnal waves have almost no signal in sea-surface height near their turning latitude, being nearly inertial. With excellent temporal resolution, measurements by tomography naturally complement those of altimetry. Indeed, tomography was used to show that these semidiurnal or diurnal internal waves, with O (150 or 500) km wavelengths and O (3 or 6) m/s phase speeds, are predictable in many regions of the world's ocean, much as the ordinary tides are predictable