  We discuss properties of the expected radio emission from Soft Gamma-ray
Repeaters (SGRs) during their bursting activity in the framework of the model
of Thompson, Lyutikov and Kulkarni (2002), in which the high energy emission is
powered by the dissipation of super-strong magnetic fields in the
magnetospheres through reconnection-type events. Drawing on analogies with
Solar flares we predict that coherent radio emission resembling solar type-III
radio bursts may be emitted in SGRs during X-ray bursts. The radio emission
should have correlated pulse profiles with X-rays, narrow-band-type radio
spectrum with $\Delta \nu \leq \nu$ with the typical frequency $ \nu \geq 1 $
GHz, and, possibly, a drifting central frequency. We encourage sensitive radio
observations of SGRs during the bursting activity.
