No abstract

І н ф о р м а ц і й н і с и с т е м и , м е х а н і к а т а к е р у в а н н я UDC 629.7.058

No abstract

No abstract

It is shown that the errors of calibration coefficients of the multichannel imaging eat" may be a reason for the spurious source if the selection crikria for gamma-ray flashes are used. Besides that, the influence of bright stars and discriminator's threshold on the calculated g a m -r a y flux was also estimated. It is shown that the requiremenls for the equipment are rather high for accurate registration of Faint (IO-" quanta cm-' s-I) gamma-ray flux of very high energy (10" eV). The calculations were made using a method of Bash simulation.