Spatial structures in ionospheric electron density revealed in a tomographi
c image have been identified with auroral forms and related to their source
s in precipitating particles observed by DMSP satellites. The observations
of plasma enhancements relate to discrete auroral arcs seen in the post-noo
n sector, identified by both red- and green-line emissions measured by a me
ridional scanning photometer. The features lie within a very narrow latitud
inal band on L-shells where the satellite detectors observed electron preci
pitation classified as from the boundary plasma sheet (BPS). The harder par
ticles are identified with an E-region structure, while further north the p
recipitation is softer, resulting in a localised F-layer blob and 630.0 nm
emissions. A steep gradient in plasma density represent a signature in the
ionosphere of the central plasma sheet (CPS)/BPS boundary. A transition to
a less-structured F-layer is found on crossing the convection reversal boun
dary.