We propose to image with CAM-CVF some well known bipolar outflows
 in the two pure rotational lines of molecular hydrogen at 9.665um
 (0-0 S(3)) and 12.279um (0-0 S(2)), and to obtain SWS01 full scans
 in selected bright outflow positions.
 The two H2 lines selected are among the brightest H2 pure-rotational
 lines, which are foreseen to be excited in warm (T>~200 K)
 molecular gas both in regions shocked at moderate velocities and in
 photodissociation regions, probing therefore physical conditions
 complementary to that of the roto-vibrational near-IR H2 lines
 observed from the ground. The outflows selected in this proposal will
 also be mapped spectroscopically with the LWS as part of the LWS PMS
 GT program: all the obtained ISO spectroscopic observations, together
 with ground based broad band and spectroscopic NIR imaging, will
 be used to: 1) understand the connection between the outflow
 morphological and physical structure and the evolutionary status of
 the driving source; 2) study in details the physics of the shocked
 regions in the outflow in order to discriminate between different
 excitation models.