Idler beam quality at 6.3 µm from HgGa 2 S 4 OPO is compared for linear, planar ring and RISTRA cavities. The last one produces smooth, circular profile and much higher focal fluence. OCIS codes: (190.4970) Parametric oscillators and amplifiers; (160.4330) Nonlinear optical materials.Recently, the concept of Rotated Image Singly-Resonant Twisted RectAngle (RISTRA) cavity for optical parametric oscillators (OPOs) was shown to be a very successful tool for achieving high output beam quality (low M 2 values) also in the mid-IR spectral range, using ZnGeP 2 nonlinear crystals pumped near 2 µm [1,2]. However, our first attempt to employ such cavity design with CdSiP 2 (CSP), which can be pumped at 1064 nm with negligible two-photon absorption (TPA), failed and basically only smoothing of the idler spatial distribution was observed [3]. Obviously some of the prerequisites, on the first place the absent spatial walk-off in the 90°-phase-matchable CSP, were not satisfied in this experiment. Therefore, we decided to examine the RISTRA concept with the most promising non-oxide mid-IR crystal for 1-µm pumped OPOs, HgGa 2 S 4 (HGS), with which we obtained idler energy of 3 mJ at ~6.3 µm with a linear cavity [4]. Here we compare RISTRA cavity with linear and ring cavities whose parameters are as close as possible and investigate the effect of the spatial walk-off by changing the pump beam diameter.The most important advantage of the defect chalcopyrite type HGS (point group 4 ) over the commercially available chalcopyrite AgGaS 2 (AGS) is the ~1.8 times higher nonlinear coefficient d 36 at slightly increased band-gap value (2.79 eV for HGS vs. 2.7 eV for AGS), i.e. at somewhat improved damage resistivity. Due to its wide band-gap, HGS, similar to AGS, can be pumped near 1 µm by short or ultrashort pulse laser sources (e.g. Nd:YAG at 1064 nm) without any TPA.The pump source was a diode-pumped Q-switched Nd:YAG laser / amplifier emitting ~8-ns pulses with maximum energy of 250 mJ at 1064 nm at a nominal repetition rate of 100 Hz. To improve the spatial beam profile (eliminate diffraction rings producing hot spots) a vacuum diamond pinhole was installed in the focus of a telescope. The M 2 parameter measured behind the telescope amounted to ~2. After an attenuator the polarization state of the pump beam was horizontal which defines the critical plane or the walk-off plane in the optically negative HGS, while vertical will be the non-critical plane. The beam size (at e -2 level intensity) was reduced by a second telescope to D=2.25 mm (small diameter) for the first series of measurements while it was D=5.35 mm (large diameter, comparable to the crystal aperture) without this telescope for the second series of measurements. The repetition rate was reduced to 10 Hz in both cases, either by a mechanical shutter synchronized to the internal Pockels cell driver of the laser or by driving the Pockels cell at 10 instead of 100 Hz although the pump diodes were operated at 100 Hz. Table 1. Mid-IR OPOs based on RISTRA cavities pumped by mu...