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1.INTRODUCTIONChemCam is in operation on Mars onboard the Curiosity rover since 2012, with 855,000 shots performed for LIBS analysis [1]. While ChemCam operated only in LIBS mode at its fundamental wavelength (1067 nm for Nd:KGW), SuperCam can either emit at 1064 nm for LIBS or 532 nm for Raman analysis. SuperCam flight model was delivered to CNES in January 2019 and was successfully integrated to Perseverance Rover at NASA JPL. Landing on Mars is scheduled for 18th of February 2021. Some potential analysis method for planetology would require even shorter wavelength than the second harmonic of Nd:YAG. Ar/K dating would benefit from the cleaner laser ablation possible with a UV laser. For Raman analysis, it could improve the signal to noise ratio. Laser Induced Fluorescence (LIF) spectroscopy potential has not been proved yet for planetology but would also require a UV laser. For lunar exploration with a rover smaller than Curiosity class, a laser with a reduced footprint would be interesting. This communication describes the harmonic conversion of laser based on the ChemCam and SuperCam heritage as well as the downsizing of SuperCam laser for lunar exploration. 2.SUPERCAM LASERNew mission requirements drove the evolution from ChemCam to SuperCam laser. The number of shots in burst mode (from 100 shots to 1000 shots) and the repetition rate (from 3 Hz to 10 Hz) were both increased. A new Raman capability in addition to the LIBS mode required a new shorter wavelength produced using a switchable Second Harmonic Generation (SHG) module. Volume and mass were kept identical to ChemCam. The flight model was delivered to CNES/IRAP in January 2019. It was successfully integrated to NASA rover Perseverance summer 2019. It will land on Mars on 18 February 2021. 2.1OscillatorThe oscillator provides the high beam quality and short pulse length needed for LIBS analysis. It is based on a Nd:YAG rod longitudinally pumped by a multicolor diodes stack. The broad emission spectrum of the diodes shift with temperature but always match some absorption peak of the lasing material. This insures pump absorption over large temperature range without the need of any temperature stabilization system for the pumping diodes. Both the diode and the rod are conductively cooled and can operate on a large temperature range (-40 °C to 40 °C for qualification). The oscillator is actively Q-Switched with a RTP Pockels cell to produce nanosecond pulses. Oscillator resonator is linear, closed on one side by the HR coated rod side and by the output coupler on the other side. Reflectivity of the output coupler is 40 %. A polarizer, wave-plate and Pockels cell are associated to Q-switch the cavity. The oscillator provides output energy of about 30 mJ at 1064 nm with a pulse duration < 5 ns and a M2 < 2. 2.2Second harmonic generatorThe Second Harmonic Generator (SHG) is a KTP (type II) crystal, placed at the output of the oscillator. It generates the 532 nm beam used in Raman mode. A RTP electro-optical switch (same Pockels cell as for the oscillator), between the oscillator and SHG, allows the operation mode selection (LIBS or Raman) by switching between linear and circular polarization. In the absence of a high voltage, an infrared beam at 1064 nm is emitted. When the high voltage is applied to the RTP switch, beam is converted to 532 nm for Raman analysis. An SHG conversion efficiency of about 50% is obtained corresponding to about 15 mJ available for Raman spectroscopy. 2.3SuperCam evolutions: Slab amplifiersFollowing the development and manufacturing of the SuperCam model, we studied the possibility to increase further the energy of the laser for both LIBS and Raman applications [2].We added one or two identical slab amplifiers (dimensions 6 x 6 x 22 mm) to increase the energy at the oscillator output. Each amplifier is transversally pumped by one 1800 W diode stack identical to the one used for the oscillator. These slab amplifier geometry is similar to the one from ChemCam amplifier with the following modifications:
Thanks to improved thermal properties of Nd:YAG compared to Nd:KGW, a thousand shot sequence at 10 Hz can be performed compared to the 100 shots/3 Hz shooting sequence of ChemCam. 3.EXPERIMENTAL SET-UP3.1SuperCam test platformWe assembled a tabletop version of SuperCam as a flexible platform for low TRL studies (TRL 3-4). We can flexibly add various modules as depicted in figure (1). The oscillator described in paragraph 2.1 is built using optical components from the SuperCam program. As the mechanical mount are off the shelf components, and the system is opened without any covers, it is not representative in term of thermal behavior of the SuperCam Flight model. For convenience, the diode stack is cooled and temperature stabilized at 20°C by a Peltier module. For the purpose of this study, we kept a constant output energy of 20 mJ at 1064 nm for the oscillator. We choose to have this constant energy level to preserve a low M2 parameters for the oscillator (M2<1.2). Subsequent amplification in slabs allows us to recover higher energy at the fundamental wavelength before frequency conversion. The repetition rate can be set at 3 Hz or 10 Hz. Following the oscillator, we choose the laser configuration by adding the following modules:
We used dichroic mirrors to separate third or fourth harmonic, 1064 nm and 532 nm beams are transmitted while harmonic beam is reflected. 3.2Third harmonic generation module We selected the following non-linear crystal:
Both crystals are mounted on mechanical stages allowing phase matching by rotation of the crystals. 3.3Fourth harmonic generation moduleWe selected the following non-linear crystal: BBO crystal for FHG was used in program like the MOMA instruments for ExoMars mission. 3.4Measurement set-upThe measurement set-up includes:
We took special care to remove fundamental wavelength and second harmonic generated signals using additional two additional dichroic mirrors and a Pelin Broca prism for spatial and temporal measurements. 4.EXPERIMENTAL RESULTS4.1SuperCam test platform at 1064 nmThe SuperCam laser assembled on a breadboard allows us to test different configurations to increase the energy of the oscillator. We measured energy, pulse duration and beam profile (near field, far field and M2 factor) for each configurations at the fundamental wavelength of the emission of the laser. We summarized results in table 1. All measurements were performed at 3 Hz except for the 2 slabs and beam expander configuration (3 Hz and 10 Hz). Table 1.SuperCam performance at 1064 in four optical configurations.
The spatial profile in the near field and far field is preserved when the beam is amplified in the different configurations. The platform can deliver energy from 20 mJ (oscillator only) to 115 mJ (two amplifiers including beam expander). Pulse width (FWHM) is 6 ns for all configurations. 4.2Third Harmonic GenerationThird harmonic generation for each set-up is optimized by angle tuning of SHG and THG crystals. The highest level in energy of the third harmonic is not obtained for the highest level of second harmonic. Usually, a conversion efficiency of 40 % for the second harmonic is optimal to maximize THG energy output. We have summarized in table the maximum energy achievable for each configuration. Table 2.SuperCam performance at 355 nm for 4 different optical configurations.
We can deliver with the various platform tested from 5.8 mJ at 355 nm (oscillator only) to 37.4 mJ at a repetition rate of 3 Hz. Energy stability is better than 2.5% RMS except for the most energetic configuration (3.8% RMS for 2 slabs and beam expander). M2 parameter is lower than 2 on both axis for all configurations. FWHM pulse duration is reduced to 5 ns due to temporal filtering in the harmonic generation process. For the configuration using two slab amplifiers and a beam expander (maximum energy in the fundamental), there is a decrease of converted energy by 10% when running the laser at 10 Hz rather than 3 Hz. We attribute this decrease in harmonic conversion efficiency to increased thermal lensing and aberration within the slab amplifiers. 4.3Fourth Harmonic GenerationFourth harmonic generation for each set-up is optimized by angle tuning of SHG and FHG crystals. The highest level in energy of the fourth harmonic is obtained for the highest level of second harmonic. We have summarized in table the maximum energy achievable for each configuration. Table 3.SuperCam performance at 355 nm for 4 different optical configurations.
Output energy at 266 nm is 3.1 mJ for the oscillator and up to 23.4 mJ for two slabs with the beam expander set-up. Energy stability (12 % RMS) and conversion efficiency are low in the oscillator configuration because of insufficient peak power incident on the BBO crystal. Adding one or two slabs drastically improves energy stability (better than 2.5 % RMS) and conversion efficiency (up to 19 %) thanks to higher peak power. M2 is lower than 3.4 on both axis in all configurations. Temporal width (FWHM) is measured to be 6ns. We expected shorter duration due to the nonlinear process but are limited by the detector spectral response in the UV. As for THG, the conversion efficiency drops by 10% when running at a higher repetition rate. We noticed for all configuration the high sensitivity of angular phase matching of the fourth harmonic generator. In the case of the highest energy version including the beam expander, it is also critical to adjust its divergence precisely to be within the narrow acceptance of the BBO crystal. These constraints could be relaxed by using a shorter BBO crystal (larger acceptance angle) at the cost of a lower harmonic conversion efficiency. 4.4Discussion and model designFrom our measurements, we wrote preliminary specifications for a UV laser operating at 355 nm or 266 nm. The designed lasers would be single wavelength, without the capacity to switch between fundamental and UV. Repetition rate is chosen to be 10 Hz to have a fixed thermal load and hence constant beam divergence during the burst sequence. Mechanical design is herited from SuperCam. Thermal dissipation is purely conductive in the laser (no active cooling using Peltier module). Non-linear crystal oven are temperature controlled using heaters as for SuperCam KTP crystal. Additional driving electronics for Q-switch and diodes adds 600 g to the laser mass. In table 4, we have summarized performances of both laser versions. Thermal effects experienced during burst shooting were taken into account (thermal dissipation, interplay between diode spectrum and Nd:YAG absorption spectrum) to estimate preliminary performances of the lasers. Different configurations with lower repetition rate and/or lower energy are possible, leading to smaller footprint for the laser. Table 4.Preliminary specifications for SuperCam type UV model at 355 nm and 266 nm operating at 10 Hz.
5.MINICAM LASERIn parallel to a UV version of SuperCam, we investigated through CAD simulation a simplified version (MiniCam) for LIBS only application. The idea was to have a smaller/lighter version of SuperCam that can be integrated on a lander or rover smaller than Curiosity/Perseverance class for a potential lunar mission. The performance of the laser in LIBS mode are identical to SuperCam (30 mJ at 1064 nm) performance, so the cavity design is kept (see section 2). To minimize risk and keep qualification to a minimum, we decided to use titanium as for ChemCam and SuperCam, and keep laser welding technology to seal the laser. By removing the Raman functionality (Polarization switch and SHG crystal), the laser is shortened and mass is reduced. We also optimized the oscillator structure by adapting geometry and mass repartition. Consequently, we moved the laser collar along the laser axis. The mass for MiniCam is 333 g (193 g reduction). For the electronics of the laser, delivering pulse current to the diode and high voltage to the Q-switch unit, modification were driven by the return of experience on SuperCam. A large margin was kept on SuperCam diode current (230 A for 220 μs pulse at 10 Hz) in the design phase to ensure energy target (30 mJ for LIBS) could be met over a large temperature range. As the current applied to SuperCam diode stack is never higher than 160 A over the whole qualification temperature range (-40 °C to 40 °C), we choose this value as the new maximum to be delivered by the electronics. Mass for electronic was reduced from 468 g to 308 g. Reducing current allowed us to reduce the number of capacitors and surface of the PCB board. 6.SUMMARY AND OUTLOOKWe have investigated the performances of UV models emitting at 355 nm or 266 nm on SuperCam test platform and estimated potential performances for flight models at the highest energy and repetition rate achievable. We also designed a new version of SuperCam focusing on size reduction for LIBS application. 7.ACKNOWLEDGEMENTThe work is funded by the Centre National d’Etudes Spatiales (CNES) under the R&T grant “Conversion dans l’UV du laser Supercam (R-S18/SU-0003-070)”. REFERENCESForni, O.,
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