One of the most interesting and unexplained spatial structures in the
Io plasma torus located near Io's orbit about Jupiter is the east-west
(or alternatively dawn-dusk) asymmetry in the planetocentric distance
of the so called plasma ''ribbon,'' the brightest and most prominentl
y observed radial feature of the torus. The average radial position of
the ribbon on the sky plane in both its ground-based measured S+ opti
cal emission (6716 Angstrom, 6731 Angstrom) and its Voyager measured S
++ ultraviolet emission (685 Angstrom) is observed to be located close
r to the planet and well within Io's orbit when it is west of Jupiter
at the dusk (or receding) ansa and farther from the planet and very ne
ar Io's orbit when it is east of Jupiter at the dawn (or approaching)
ansa. In addition, the ribbon is also observed to move about this aver
age position as a function of its ansa System III longitude. It is sho
wn that the location of this asymmetrical radial structure for the Sribbon arises naturally in the presence of an east-west electric field
from a space and time dependent plasma source that is highly concentr
ated at Io's instantaneous orbital location (and hence initially locat
ed at a constant distance from the planet) and a plasma transport rate
that increases radially outward. Model calculations reproduce both th
e observed average east-west asymmetry and the System III longitude de
pendence of the S+ ribbon location in the plasma torus. In the absence
of an east-west electric field, however, the model-calculated density
peak for the S+ ribbon is located essentially symmetrically about Jup
iter just inside Io's orbit and does not exhibit the observed east-wes
t asymmetry. Since the S+ ribbon during its slow outward transport wil
l undergo electron impact ionization, the radial location of the S++ r
ibbon can be expected to be created naturally with the same System III
longitude dependence as for the S+ ribbon and at a position radially
just beyond that of the S+ ribbon, as has been observed.