The Wind perigee passes covered tail distances from 6-24 R-E. By use o
f bulk quantities and the parent distributions, we have found new feat
ures in the PSBL that had been missed previously. The PSBL consists of
a unidirectional earthward streaming ion beam at the edge and another
unidirectional beam inside this edge streaming in the tailward direct
ion. Bidirectional beams are observed with higher densities, further i
nside the PSBL. The plasma in the region supporting the tailward strea
ming beams consists of the beam distribution plus an isotropic compone
nt, whereas the earthward streaming beams consists mainly of the beam
distribution. These distributions yield fast flows (> 400 km/s) in the
earthward direction and slower flows (approximate to 150 km/s) in the
tailward direction. Both regions support counter streaming electron b
eams superposed on an isotropic component. These new findings are subs
tantially different from previous observations and the interpretation
of fast flows and ion beams in terms of a neutral line model needs to
be reexamined.