On April 6, 1993 an SEB disturbance commenced with a bright white spot
at 15.5 degrees S latitude, The spot was followed by a dark column ly
ing only 24 degrees from the eastern edge of the Great Red Spot. A con
tinuous CCD and photographic survey at visual wavelengths of the el ml
during the four months following the eruption has allowed us to obtai
n the best imaging records of the evolution of an SEB disturbance, wit
h a spatial resolution and temporal coverage of unprecedent quality, A
high resolution zonal wind velocity profile in the 8 degrees S to 25
degrees S latitude range has been obtained tracking the cloud elements
pertaining to the SEBD and nearby features, The SEBD central and nort
hern 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 th
e GRS and by the interaction of the SEBD spots with preexisting featur
es in the STrZ, The new phenomena observed included: (i) A temporal de
lay in the development of the SEBD southern branch spots, that moved w
ith lower velocities (at about 30 m sec(-1)) than those observed on th
e 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-live
d anticyclonic vortex in the STrZ, The revival of the SEB was complete
in November 1993, entering the belt during 1993 in an SEBD1 phase (as
described in paper I) which was characterized at continuum wavelength
s by the formation of a STrZ belt at similar to 23.5 degrees S and by
the presence of synoptic and rapidly changing white spots at 11.5 degr
ees S, This activity formed tilted cloud patterns of turbulence in the
northern half of the belt in a region that corresponds to the cycloni
c southern half of the strong eastward jetstream at similar to 7 degre
es S. (C) 1996 Academic Press, Inc.