The repeated samplings of the Jovian magnetosheath during the Ulysses
encounter with Jupiter provided an opportunity to probe the planetary
depletion layer. Of the 10 complete crossings of the Jovian magnetopau
se, only three contained clear signatures of an overlying depletion la
yer. All of these occurred on the flanks of the magnetosphere near the
dusk terminator; crossings on the dayside were ambiguous or clearly l
acked a depletion layer signature. In this paper we present a detailed
analysis of the observations by the Ulysses solar wind plasma and mag
netometer experiments and discuss conditions favorable and unfavorable
for depletion layer observation.