  The survey of northern hemisphere were made at a frequency of 111 MHz. The
total accumulation time at each point of the sky was at least one hour. 75
sources of pulse emission were detected. More then 80% of these sources are
known pulsars observed in the side lobes of the antenna. From one to several
hundreds pulses were detected in twelve known pulsars. For four pulsars
(J0157+6212, J1910+5655, J2337+6151, J2354+6155) the narrowness of the
strongest pulses and the ratio of peak flux densities in the strongest pulse
and in the average profile indicate that they can be pulsars with giant pulses.
One new rotating radio transient (RRAT) J0812+8626 with a dispersion measure
DM=40.25 pc/cm3 was detected.
