LIBS

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Portable X-ray fluorescence (XRF) analyzers for analyzing elemental composition of artifacts. Generated by AI. | Image Credit: © Textures & Patterns - stock.adobe.com
New Research Sheds Light on How Ambient Gases Affect LIBS Signal Quality

April 25th 2025

Researchers from Tsinghua University and Qinghai University have uncovered how specific ambient gas properties affect the stability and accuracy of laser-induced breakdown spectroscopy (LIBS) signals.

A welder in protective gear fuses aluminum pieces with precision, © 69-chronicles-stock.adobe.com
LIBS Illuminates the Hidden Health Risks of Indoor Welding and Soldering

April 23rd 2025

A digitally created image showcasing a modern oil rig alongside wind turbines and solar panels, highlighting a fusion of traditional and renewable energy sources. Generated by AI. | Image Credit: © val - stock.adobe.com
New Laser Spectroscopy Technique Promises Breakthrough in Fusion Fuel Monitoring

April 21st 2025

Mars rover exploring rocky Martian landscape under starry night © SerPak-chronicles-stock.adobe.com
New Spectroscopic Evidence of Hydrothermal Activity on Mars Revealed by Perseverance Rover

April 2nd 2025

Ancient cultural site with religious statues and traditional rituals, emphasizing historical and spiritual heritage. Generated by AI. | Image Credit: © tonpreecha - stock.adobe.com
New Multi-Spectroscopic System Enhances Cultural Heritage Analysis

April 2nd 2025

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The SuperCam Remote Sensing Instrument Suite for the Mars 2020 Rover: A Preview

May 1st 2017

The SuperCam remote sensing instrument suite under development for NASA’s Mars 2020 rover performs laser-induced breakdown spectroscopy (LIBS), remote Raman spectroscopy, visible and infrared (VISIR) reflectance spectroscopy, acoustic sensing, and high resolution color imaging. The instrument builds on the successful architecture of the ChemCam instrument which provides LIBS and panchromatic images on the Curiosity rover, adding the remote Raman spectroscopy by frequency doubling the laser and using a gated intensified detector to obtain Raman signals at distances to 12 m. To the visible reflectance spectroscopy used by ChemCam, an AOTF-based infrared spectrometer is added to cover the 1.3-2.6 µm range that contains important mineral signatures. A CMOS detector provides color (Bayer filter) images at a pixel resolution of 19 µrad and an optical resolution of 30 µrad. Sounds are recorded via a Knowles Electret microphone, which is the same one that was unsuccessfully attempted on two earlier missions. The acoustic signals of the LIBS plasmas will provide information on the hardness of the targets, while other sounds (wind, rover sounds) will also be recorded. The laser, telescope, IR spectrometer, and camera reside on the rover’s mast and are provided by CNES, while the LIBS, Raman, and VIS spectrometers and data processing unit are built by LANL and reside in the rover body. A calibration target assembly provided by U. Valladolid, Spain, resides on the back of the rover. The overall mass of the instrument suite is 10.7 kg.