We describe a deep narrowband [S II] imaging survey of similar to 0.7
deg(2) covering the rho Ophiuchi cloud core (L1688). We detect seven n
ew jet/Herbig-Haro (HH) objects in our survey, of which three are new
detections and four confirm candidates from a recent survey by Wilking
et al. Together with the five previously known objects, this brings t
he total to 12 known jet/HH objects in the cloud. In addition to this,
we propose six new candidate HH objects. The most likely sources to p
ower the new jet/HH objects appear to be optically visible stars; howe
ver, a conclusive association between the HH objects and pre-main-sequ
ence stars is difficult, as several candidate driving sources lie in c
lose vicinity of the new knots. Practically all of the HH objects are
located on the perimeter of the cloud. The lack of optical emission to
ward the center of the cloud and the high spatial concentration of the
youngest protostars toward the densest regions strongly suggest that
jets inside the cloud are obscured from our view at optical wavelength
s. A near-infrared H-2 survey is required to penetrate into the cloud
and to study the outflow activity in this extremely active star-formin
g region.