Phase Conjugate Laser Optics

Chapter 5.4.4.3 - Long-pulse second harmonic conversion

5.4.4.3   Long-pulse second harmonic conversion   We adopted a design
for the frequency doubler that is very similar to that used for the 15-ns system. It
consists of a type II KD*P doubler using two crystals in an alternating-Z geometry


Figure 5.20. (a) A measured near field beam profile for the 30-J, 500-ns laser system showing both (b) horizontal and (c) vertical irradiance line-outs.

[41]. In the case of the 500-ns, 30-J output, however, it was necessary to add a set of
beam-shaping optics between the output of the laser and the doubler in order to
increase the irradiance incident on the crystals. Since the frequency converter is
outside the SBS wavefront-corrected path, it is desirable to reshape the beam
without concern for introducing wavefront error due to the imperfect alignment of a
telescope. For this reason, a set of two 45o prisms are used to reduce the 25-mm
output beam in one dimension by a factor of 2.5, resulting in a beam size of
10 × 25 mm2 in the KD*P crystals. A second set of prisms restores the 527-nm
beam to a 25-mm square after the crystals. A dichroic mirror outside of the laser
enclosure is used to separate the unconverted 1053-nm light from the 527-nm
output. A typical external conversion efficiency of 60% is obtained at up to 30 J /
pulse corresponding to a peak input irradiance of 24 MW/cm2. Under these
conditions, routine operation of >45 W in 500-ns pulses at 3 Hz is achieved. Figure
5.22 shows a 10-minute portion of a run with an average input energy of 27 J and
average output energy of 16 J / pulse at 527 nm.

Due to the increased length of the doubler crystals required for the long-pulse,
low-irradiance laser output (60 mm total), the second harmonic converter introduces
greater wavefront distortion than that used for the 15-ns laser system. Figure 5.23
shows the measured far-field profile at 16 J / pulse and 3 Hz. Because of weak
absorption (~ 0.15%/cm) at 1053 nm, the converted green beam exhibits ~ 0.2λ
spherical wavefront error at full average power which can be compensated by a
small adjustment of the far-field diagnostic system. As can be seen from the line-

Figure 5.21. Far-field beam profile for the near field shown in Fig 5.20. The distribution represents a divergence of 1.1_ the diffraction limit. The dashed vertical lines show the theoretically expected first minima in the line-outs for both a round and a square near-field distribution.

outs in Figs. 5.23b and 5.23c, higher-order distortions are also observed which lower
the measured Strehl by 2× from the single shot value. In the final user application of
the system, an external telescope was used to further expand the laser output before
entering the beam director. The very small thermal focus introduced by the doubler
was easily corrected in the focusing adjustment of this telescope.

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