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UV Raman spectroscopy - A technique for biological and mineralogical in situ planetary studies

机译:紫外拉曼光谱-一种用于生物和矿物原位行星研究的技术

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We report on the great advantages of using deep UV Raman system for in situ planetary applications. Among them are to be mentioned: (1) higher scattering efficiency compared to VIS-IR Raman excitation wavelengths, (11) electronic resonance effects which increase the intrinsically weak Raman signal thus improving the S/N ratio of the detected Raman signals and (111) spectral separation of Raman and fluorescence signals. All these advantages are making UV Raman a valuable technique for in situ planetary applications. Mineral as well as biological samples were analyzed using Raman deep UV excitation and the results are presented. For the mineral samples a comparison with excitation in the NIR-VIS spectral regions is made. The impact of fluorescence on Raman data acquisition at different laser excitation wavelengths is assessed. Making use of the resonance effects, spectra of microorganisms were recorded with a high S/N ratio, allowing afterwards a very precise identification and classification (to the strain level) of the measured samples. (c) 2007 Elsevier B.V. All rights reserved.
机译:我们报告了在原位行星应用中使用深紫外线拉曼系统的巨大优势。其中要提到的是:(1)与VIS-IR拉曼激发波长相比更高的散射效率;(11)电子共振效应会增加本征弱的拉曼信号,从而提高检测到的拉曼信号的信噪比;(111) )拉曼光谱和荧光信号的光谱分离。所有这些优点使UV拉曼光谱成为用于原位行星应用的有价值的技术。使用拉曼深紫外激发分析矿物质和生物样品,并给出结果。对于矿物样品,将其与NIR-VIS光谱区域中的激发进行了比较。评估了荧光对不同激光激发波长下拉曼数据采集的影响。利用共振效应,以高信噪比记录了微生物的光谱,之后可以对被测样品进行非常精确的识别和分类(以应变水平分类)。 (c)2007 Elsevier B.V.保留所有权利。

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