  We use dual-site radio observations of interplanetary scintillation (IPS)
with extremely long baselines (ELB) to examine meridional flow characteristics
of the ambient fast solar wind at plane-of-sky heliocentric distances of 24-85
solar radii (R\odot). Our results demonstrate an equatorwards deviation of
3-4{\deg} in the bulk fast solar wind flow direction over both northern and
southern solar hemispheres during different times in the declining phase of
Solar Cycle 23.
