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首页> 外文期刊>Spectrochimica Acta, Part B. Atomic Spectroscopy >Study of sub-mJ-excited laser-induced plasma combined with Raman spectroscopy under Mars atmosphere-simulated conditions
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Study of sub-mJ-excited laser-induced plasma combined with Raman spectroscopy under Mars atmosphere-simulated conditions

机译:火星大气模拟条件下亚mJ激发激光诱导等离子体与拉曼光谱的结合研究

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摘要

Laser-Induced Breakdown Spectroscopy (LIBS) and Raman spectroscopy are complimentary techniques.LIBS yields elemental information while Raman spectroscopy yields molecular information about a sample,and both share similar instrumentation configurations.The combination of LIBS and Raman spectroscopy in a single instrument for planetary surface exploration has been proposed,however challenges exist for developing a combined instrument.We present LIBS and Raman spectroscopy results obtained using a diode pumped,intracavity doubled,Q-switched,Nd:YLF laser operating at 523 nm,which overcomes some of the difficulties associated with a combined instrument.LIBS spectra were obtained with 170 u J per pulse at 4 Hz repetition rate in a low pressure Mars-simulated atmosphere and Raman spectra produced with 200 mW at 100 kHz.The Nd:YLF laser is switchable between LIBS and Raman spectroscopy modes only by a change in Q-switch repetition rate.Emissions from Ca,Ca II,Fe,Fe II,Mg,Na,and O atom were identified in the mu-LIBS spectrum of oolithic hematite.Evidence was found for a change in plasma dynamics between 7 and 5 Torr that could be explained as a decrease in plasma temperature and electron density below 5 Torr.This is relevant to future Mars exploration using LIBS as the mean surface pressure on Mars varies from 3.75 to 6 Torr.LIBS plasma dynamics should be carefully evaluated at the pressures that will be encountered at the specific Mars landing site.
机译:激光诱导击穿光谱(LIBS)和拉曼光谱是互补技术,LIBS产生元素信息,而Raman光谱产生有关样品的分子信息,并且两者共享相似的仪器配置.LIBS和拉曼光谱的组合在单个仪器上用于行星表面提出了探索性的方法,但是开发组合仪器仍然存在挑战。我们介绍了使用在523 nm下工作的二极管泵浦,倍频倍频,Q开关,Nd:YLF激光器获得的LIBS和拉曼光谱结果,克服了一些相关的难题在低压火星模拟的大气中,以4 Hz的重复频率,每个脉冲以170 u J的脉冲获得LIBS光谱,在100 kHz时以200 mW产生的拉曼光谱获得.Nd:YLF激光可在LIBS和拉曼之间切换光谱模式只能通过改变Q开关重复率来确定。Ca,Ca II,Fe,Fe II,Mg,Na和O原子的发射被识别在卵石赤铁矿的mu-LIBS光谱中被证实。等离子体动力学在7至5 Torr之间变化的证据可以解释为等离子体温度和电子密度在5 Torr以下的降低,这与未来的火星探测有关LIBS在火星上的平均表面压力在3.75到6 Torr之间变化.LIBS等离子体动力学应在特定的火星着陆点遇到的压力下进行仔细评估。

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