  The long-term observations of the Galactic Centre as well as the Galactic
anti-Centre regions in hard X-rays (10-300 keV) were made in experiments on
board Prognoz-9 satellite and "Mir" orbital station (GRIF experiment). Some
transient pulsars including A0535+262, GS1722-36, 4U1145-619, A1118-615,
EXO2030+37, Sct X-1, SAX J2103.5+4545, IGR 16320-4751, IGR 16465-4507 were
observed. The pulsation flux components of A0535+26 and GS1722-36 X-ray
emission were revealed at significant level. For other observed pulsars the
upper limits of pulsation intensity were obtained. The mean pulsation profiles
of A0535+26 in different energy ranges as well as the energy spectra were
obtained at different stages of outburst decreasing. The pulsation
intensity-period behavior does not contradict the well-known correlation
between spin-up rate and X-ray flux, while the stable character of the energy
spectrum power index indicates on the absence of thermal component. The energy
spectrum and mean pulsation profiles were also obtained for one time interval
of GS1722-36 observations. The upper limits of pulsation fluxes obtained for
other observed transient pulsars at the orbital phases more than 0.14
correspond the quiescent state or final stage of the first type outburst.
