  A small number of pulsars are known to emit giant pulses, single pulses much
brighter than average. Among these is PSR J0534+2200, also known as the Crab
pulsar, a young pulsar with high giant pulse rates. Long-term monitoring of the
Crab pulsar presents an excellent opportunity to perform statistical studies of
its giant pulses and the processes affecting them, potentially providing
insight into the behavior of other neutron stars that emit bright single
pulses. Here, we present an analysis of a set of 24,985 Crab giant pulses
obtained from 88 hours of daily observations at a center frequency of 1.55 GHz
by the 20-meter telescope at the Green Bank Observatory, spread over 461 days.
We study the effects of refractive scintillation at higher frequencies than
previous studies and compare methods of correcting for this effect. We also
search for deterministic patterns seen in other single-pulse sources, possible
periodicities seen in several rotating radio transients and fast radio bursts,
and clustering of giant pulses like that seen in the repeating fast radio burst
FRB121102.
