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21 November 2017 Raman technology for future planetary missions
Hans Thiele, Stefan Hofer, Timo Stuffler, Markus Glier, Jürgen Popp, Omar Sqalli, Andreas Wuttig, Rainer Riesenberg
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Proceedings Volume 10567, International Conference on Space Optics — ICSO 2006; 105671T (2017) https://doi.org/10.1117/12.2308055
Event: International Conference on Space Optics 2006, 2006, Noordwijk, Netherlands
Abstract
Scientific experiments on mineral and biological samples with Raman excitation below 300nm show a wealth of scientific information. The fluorescence, which typically decreases signal quality in the visual or near infrared wavelength regime can be avoided with deep ultraviolet excitation. This wavelength regime is therefore regarded as highly attractive for a compact high performance Raman spectrometer for in-situ planetary research. Main objective of the MIRAS II breadboard activity presented here (MIRAS: Mineral Investigation with Raman Spectroscopy) is to evaluate, design and build a compact fiber coupled deep-UV Raman system breadboard. Additionally, the Raman system is combined with an innovative scanning microscope system to allow effective auto-focusing and autonomous orientation on the sample surface for high precise positioning or high resolution Raman mapping.
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Hans Thiele, Stefan Hofer, Timo Stuffler, Markus Glier, Jürgen Popp, Omar Sqalli, Andreas Wuttig, and Rainer Riesenberg "Raman technology for future planetary missions", Proc. SPIE 10567, International Conference on Space Optics — ICSO 2006, 105671T (21 November 2017); https://doi.org/10.1117/12.2308055
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KEYWORDS
Raman spectroscopy
Head
Deep ultraviolet
Microscopes
Fiber couplers
Fiber lasers
Spectroscopy
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