Fast transients in the form of spiky radio bursts have been observed in
solar flares events, emitting at different ranges in frequency. These
dynamical phenomena show up as high brightness temperature increments
with short durations of the order of milliseconds. In this work, we
present results of the analysis of some properties of radio spike events
observed at frequencies between 0.01 and 8.4 GHz, as reported in
different studies. We analyze the relation of the duration, bandwidth,
emitted flux, polarization and drift rate of the radio spikes with its
observational frequency. Also, we analyze its correlation with other
energetic solar events.