with the duration of the amplified pulses. At the same time the use of backward SRS removes this limitation. In the present work results of theoretical as well as experimental study of amplification of picosecond Stokes pulses with backward SRS in methane in the field of counterpropagating nano- and subnanosecond pumping pulses arc given. A modified installation from 131 was used in the experiments, in which the SRS-mirror in pulse laser pumping unit II was also used for compressing the pump pulses when necessary, and in amplification unit III instead of Ti:S-amplifiers SRS-cuvettes of length LI = 120 and L2 = 25 cm were placed. We present here only the main parameters of this laser installation. At the output of the second cascade of the SS-compressor (unit I) the Stokes pulses (,t S = 0.63 F4m) had an energy of Ws < 8 mJ with a pulse length of T S < 20 ps. The pulse laser pumping unit (2 L = 0.532/~m) made it possible to obtain energies W1 <_ 300 mJ in the nanosecond (rl < 4 nsc) pulse mode and W2 < 110 mJ in the subnanosecond (r2 < 0.65 ns) pulse mode. A delay line additionally inserted between units I and III made it possible to change the moment of arrival of the pump pulses by Ato = +--1.3 ns relative to the arrival time of the signal pulse. Furthermore, the meeting point of the pulses in the SRS-cuvette was adjusted by moving it longitudinally. Thus, by changing the focusing, the meeting point of the pulses, and the methane pressure in the cuvette, the conditions of interaction were optimized to achieve the maximum output energy of the first Stokes pulse for specified input energies of the pump signal pulses. To transform the energy of the pump pulses efficiently with backward SRS, as in the case of laser amplifiers 13 I, it is necessary that the energy density of the Stokes pulses be close to the saturation energy density. In the quasistationary case, where the duration of timewise smooth laser and Stokes pulses TL, S is much more than the time of transverse relaxation T2 of the excited molecules, the saturation energy flux density is found by Fsa t = ;tL(nL+ns)/gc S = 2/gc [61, where nL, S are the refractive indices of the SRS-medium at the laser and Stokes frequencies, g is the specific gain (in intensity) of the Stokes component [7 l, which depends on the pressure; c is the velocity of light. At a methane pressure of p -- 30 aim the time of dephasing of the oscillations is T2 = 16 ps, the gain g = 0.86 cm/GW [71, and the saturation energy density is Fsa t = 78 mJ/cm 2. Thus, assuming by analogy with laser amplifiers [3 ] that in the nonstationary mode of amplification of short Stokes pulses the saturation energy Fsa t has the same (relatively low) order of magnitude, one can hope to achieve rather high efficiencies of
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