We have carried out a survey for "giant pulses" in five millisecond pulsars
. We detect individual pulses from the high-E pulsar B1821-24 with energies
exceeding 50 times the mean pulse energy. These giant pulses are concentra
ted in a narrow phase window coincident with the power-law nonthermal pulse
seen in hard X-rays. This is the third example of the giant-pulse phenomen
on. It supports the idea that large B-fields in the outer magnetosphere are
critical to the formation of such pulses and further suggests a direct con
nection between giant pulses and high-energy emission.