We are conducting an unbiased search at lambda 2.12 mu m for embedded
molecular hydrogen jets thought to be associated with very young stell
ar objects, deeply embedded in dense cores in the Orion A molecular cl
oud. As a first result, we show a 0.4 x 0.5 degree mosaic centred on t
he L 1641-N complex, revealing a number of previously unknown knots an
d chains of H-2 emission. A 5 x 5 arcmin close-up of L 1641-N shows it
to be a very active region, with at least one parsec-scale jet origin
ating in the small embedded cluster: we also show 10 mu m imaging to h
elp identify the outflow source. Elsewhere in the mosaic, several knot
s in the HH 34 jet are detected for the first time in H-2 and a new, d
eeply embedded jet is discovered next to it. These preliminary results
demonstrate the power of H-2 imaging surveys in studying the large-sc
ale role of jets and outflows in star formation.