  A search for pulse signals in a area with declinations of $+52\degr <\delta
<+55\degr$ was carried out on the LPA LPI radio telescope. When processing ten
months of observations recorded in six frequency channels with a channel width
of 415 kHz and a total bandwidth of 2.5 MHz, 22 thousand events were found with
a pronounced dispersion delay of signals over frequency channels, i.e. having
signs of pulsar pulses. It turned out that the found pulses belong to four
known pulsars and two new rotating radio transients (RRATs). An additional
pulse search conducted in 32-channel data with a channel width of 78 kHz
revealed 8 pulses for the transient J0249+52 and 7 pulses for the transient
J0744+55. Periodic radiation of transients was not detected. The analysis of
observations shows that the found RRATs are most likely pulsars with nullings,
where the proportion of nulling is greater than 99.9\%.
