  We have surveyed 68 deg^2 along the Galactic Plane for single, dispersed
radio pulses. Each of 3027 independent pointings was observed for 68 s using
the Arecibo telescope at 430 MHz. Spectra were collected at intervals of 0.5 ms
and examined for pulses with duration 0.5 to 8 ms. Such single pulse analysis
is the most sensitive method of detecting highly scattered or highly dispersed
signals from pulsars with large pulse-to-pulse intensity variations. A total of
36 individual pulses from five previously known pulsars were detected, along
with a single pulse not associated with a previously known source. Follow-up
observations discovered a pulsar, PSR J1918+08, from which the pulse
originated. This pulsar has period 2.130 s and dispersion measure 30 pc cm^-3,
and has been seen to emit single pulses with strength up to 8 times the
average.
