Vema Channel (nominal location 30S, 40W) is a major passage for the flow of Antarctic Bottom Water on its way northward from the Argentine Basin to the Brazil Basin. New data based on approximately year-long current meter deployments at abyssal depths yield mean or time-averaged kinetic energies as strong as 240 cm2s−2, and eddy kinetic energies from 8 to 40 cm2s−2. We observe a persistent northward flow of AABW with maximum speed near 40 cm s−1, as is found at abyssal depths in the vicinity of the Gulf Stream. The highest value of mean kinetic energy in Vema Channel (240 cm2 s−2) is much larger than that (∼20 cm2 s−2) found in the flow of Antarctic Bottom Water near the Ceara Rise, and comparable to values of 220 cm2 s−2 for the southward flow of North Atlantic Deep Water on the Blake-Bahama Outer Ridge. Existing observations of mean kinetic energy at locations near the Gulf Stream System do not exceed 100 cm2 s−2 in the abyssal depth range.Eddy kinetic energies of 8 cm−2 s−2 are comparable to estimates (at similar depths) from areas at roughly equivalent latitudes, like MODE (Mid-Ocean Dynamics Experiment, nominal location 28N, 70W). However, abyssal kinetic energies as large as 40 cm2 s−2 are normally found only near strong current regimes, in contrast to values of roughly 1 cm2 s−2 in the ocean interior. Values of 18 to 64 cm2 s−2 have been observed near the southward flow of North Atlantic Deep Water on and adjacent to the Blake-Bahama Outer Ridge near 30N, and up to 20 cm2 s−2 in the flow of Antarctic Bottom Water over the Ceara Rise. The strongest abyssal eddy field yet observed, ∼100 to 150 cm2 s−2, occurs near the Gulf Stream.