  Gamma-ray bursts, if they are generated in the process of interaction between
relativistic strongly magnetized winds and an ambient medium, may be
accompanied by very short pulses of low-frequency radio emission. The bulk of
this emission is expected to be at the frequencies of $\sim 0.1-1$ MHz and
cannot be observed. However, the high-frequency tail of the low-frequency radio
emission may reach a few ten MHz and be detected, especially if the strength of
the magnetic field of the wind is extremely high.
