We present the numerical simulation of a single internal working surfa
ce which farms along the body of a supersonic jet with periodic variat
ions in the magnitude of its velocity. The structure, the evolution an
d the observational properties of this flow are analysed. We make a qu
alitative comparison with previous analytic predictions, simulations o
f the complete jet and observations of Herbig-Haro jets. The apparent
lag of the knots of emission with respect to the jet flow (which has b
een observed in some jets) can be explained by this model.