New, deep, wide-field [SII] images of the HL Tauri region show the ext
ended spatial structure of the HH 30 jet and counter-jet. At an angula
r distance of similar to 300 arcsec toward the NE, the HH 30 jet ends
in a group of scattered condensations. This previously undetected stru
cture might correspond to a broken-up working surface. Our images also
include HH 262, which is shown to have a previously undetected extend
ed emission region.