A method for automated analysis of data from a survey of scintillating
radio sources to be obtained using the Large Phased Array of the Lebe
dev Physical Institute has been developed. Difference and median filte
rs are used to remove effects interfering with the detection of scinti
llating sources. The parameters for these filters are chosen so as to
maximize the signal-to-noise ratio, which is very important when searc
hing for extremely weak scintillating sources. Model calculations are
used to give the probability of missing a signal as a function of sign
al-to-noise ratio for a given acceptable probability of false detectio
n of 0.001. The analysis method presented will make it possible to obt
ain a scintillating source survey complete to radio sources having sci
ntillation dispersions equal to the noise dispersion, with the expecte
d number of false detections being one in 1000. Estimates of the error
s of the measured coordinates of the scintillating radio sources and o
f the scintillation dispersions as functions of the signal-to-noise ra
tio are obtained.