  We report the discovery of coherent radio emission from the young,
rapidly-rotating magnetic Bp star HD 133880 at a frequency of 610 MHz with the
Giant Metrewave Radio Telescope (GMRT). This is only the second magnetic star
in which coherent radio emission has been detected. In our observations of HD
133880 covering the full rotational cycle of the star (except for a phase
window 0.17-0.24), we witness an abrupt order-of-magnitude flux enhancement
along with $\approx100$ percent right circular polarization. We attribute this
phenomenon to coherent Electron Cyclotron MASER Emission. We attribute the lack
of left circularly polarised emission to the asymmetric topology of the star's
magnetic field. The phase of enhancement, $0.73$, differs from the previously
reported phase of enhancement, $0.16$, (at 610 MHz Chandra et al. 2015) by
one-half cycle. However, no flux enhancement is found at phase $0.16$ in our
data, which could be due to an unstable or drifting emission region, or a
consequence of the reported changes of the star's rotational period. Either of
these factors could have shifted the enhancement to the above-mentioned phase
window not sampled by our observations.
