  We present a large survey of giant pulses from the Crab Pulsar as observed
with the first station of the Long Wavelength Array. Automated methods for
detecting giant pulses at low frequencies where scattering becomes prevalent
are also explored. More than 1400 pulses were detected across four frequency
bands between 20 - 84 MHz over a seven month period beginning in 2013, with
additional followup observations in late 2014 and early 2015. A handful of
these pulses were detected simultaneously across all four frequency bands. We
examine pulse characteristics, including pulse broadening and power law indices
for amplitude distributions. We find that the flux density increases toward
shorter wavelengths, consistent with a spectral turnover at 100 MHz. Our
observations uniquely span multiple scattering epochs, manifesting as a notable
trend in the number of detections per observation. These results are
characteristic of the variable interface between the synchrotron nebula and the
surrounding interstellar medium.

Solar and Stellar Astrophysics;High Energy Astrophysical Phenomena