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The first station of the Long Wavelength Array (LWA1) was used to studyPSR~B0031-07 with simultaneous observations at 38 and 74~MHz. We found that 158(0.35\%) of the observed pulses at 38~MHz and 221 (0.49\%) of the observedpulses at 74~MHz qualified as giant pulses in a total of 12 hours ofobservations. Giant pulses are defined as having flux densities of a factor of$\geq$ 90 times that of an average pulse at 38~MHz and $\geq$ 80 times that ofan average pulse at 74~MHz. The cumulative distribution of pulse strengthfollows a power law, with an index of $-$4.2 at 38~MHz and $-$4.9 at 74~MHz.This distribution has a much more gradual slope than would be expected ifobserving the tail of a Gaussian distribution of normal pulses. The dispersionmeasure value which resulted in the largest signal-to-noise for dedispersedpulses was DM $=10.9$~pc~cm$^{-3}$. No other transient pulses were detected inthe data in the wide dispersion measure range from 1 to 5000~pc~cm$^{-3}$.There were 12 giant pulses detected within the same period from both 38 and74~MHz, meaning that the majority of them are not generated in a wide band.

Simultaneous Observations of Giant Pulses from Pulsar PSR B0031-07 at 38 MHz and 74 MHz