  We present the results of our intensive radio observing campaign of the dwarf
nova SS Cyg during its 2010 April outburst. We argue that the observed radio
emission was produced by synchrotron emission from a transient radio jet.
Comparing the radio light curves from previous and subsequent outbursts of this
system (including high-resolution observations from outbursts in 2011 and 2012)
shows that the typical long and short outbursts of this system exhibit
reproducible radio outbursts that do not vary significantly between outbursts,
which is consistent with the similarity of the observed optical, ultraviolet
and X-ray light curves. Contemporaneous optical and X-ray observations show
that the radio emission appears to have been triggered at the same time as the
initial X-ray flare, which occurs as disk material first reaches the boundary
layer. This raises the possibility that the boundary region may be involved in
jet production in accreting white dwarf systems. Our high spatial resolution
monitoring shows that the compact jet remained active throughout the outburst
with no radio quenching.
