On April 6, 1993 an SEB disturbance commenced with a bright white spot at 15.5°S latitude. The spot was followed by a dark column lying only 24° from the eastern edge of the Great Red Spot. A continuous CCD and photographic survey at visual wavelengths of the event during the four months following the eruption has allowed us to obtain the best imaging records of the evolution of an SEB disturbance, with a spatial resolution and temporal coverage of unprecedent quality. A high resolution zonal wind velocity profile in the 8°S to 25°S latitude range has been obtained tracking the cloud elements pertaining to the SEBD and nearby features. The SEBD central and northern branches developed according to the classical morphology patterns and values of the zonal winds as described in paper I. However, this SEBD event was marked by the unusual proximity of the onset site to the GRS and by the interaction of the SEBD spots with preexisting features in the STrZ. The new phenomena observed included: (i) A temporal delay in the development of the SEBD southern branch spots, that moved with lower velocities (at about 30 m sec-1) than those observed on the average in other events; (ii) The interaction of a preexisting STrZ disturbance with the GRS and the SEBD southern branch features; (iii) The interaction of the features of the central branch with a long-lived anticyclonic vortex in the STrZ. The revival of the SEB was complete in November 1993, entering the belt during 1994 in an SEBD1 phase (as described in paper I) which was characterized at continuum wavelengths by the formation of a STrZ belt at ∼23.5°S and by the presence of synoptic and rapidly changing white spots at 11.5°S. This activity formed tilted cloud patterns of turbulence in the northern half of the belt in a region that corresponds to the cyclonic southern half of the strong eastward jetstream at ∼7°S. © 1996 Academic Press, Inc.