We highlight one result of a time-dependent analysis of reconnection a
t the terrestrial magnetopause, namely, that the Petschek-type reconne
ction process is inevitably accompanied by the generation of surface w
aves. These waves propagate along the magnetopause at a speed which is
generally different from that of the shocks and discontinuities bound
ing the region of heated and accelerated plasma, the so-called outflow
region of reconnected plasma. The surface waves play a central role i
n the reconnection process because it is through them that the perturb
ations of the magnetic field and velocity normal to the magnetopause a
re transmitted along the current sheet from the source region to the s
ystem at large. Since reconnection acts as a source of surface waves,
the present general view that transient phenomena at the magnetopause
are due either to surface waves (generated by, for example, variations
in the solar wind) or to transient reconnection should be revised in
the interests of a more unified treatment.