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一种用于行星物质研究的远程拉曼系统及其应用。

A Remote Raman System and Its Applications for Planetary Material Studies.

作者信息

Qu Hongkun, Ling Zongcheng, Qi Xiaobin, Xin Yanqing, Liu Changqing, Cao Haijun

机构信息

Shandong Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, School of Space Science and Physics, Institute of Space Sciences, Shandong University, Weihai 264209, China.

Key Laboratory of Space Active Opto-Electronics Technology, Chinese Academy of Sciences, Shanghai 200083, China.

出版信息

Sensors (Basel). 2021 Oct 21;21(21):6973. doi: 10.3390/s21216973.

Abstract

A remote Raman prototype with a function of excitation energy adjusting for the purpose of obtaining a Raman signal with good signal-to-noise ratio (SNR), saving power consumption, and possibly avoiding destroying a target by high energy pulses, which may have applications for Chinese planetary explorations, has been setup and demonstrated for detecting different minerals. The system consists of a spectrograph equipped with a thermoelectrically cooled charge-coupled device (CCD) detector, a telescope with 150 mm diameter and 1500 mm focus length, and a compact 1064 nm Nd:YAG Q-switched laser with an electrical adjusted pulse energy from 0 to 200 mJ/pulse. A KTP crystal was used for second harmonic generation in a 1064 nm laser to generate a 532 nm laser, which is the source of Raman scatting. Different laser pulse energies and integration time were used to obtain distinguishable remote Raman spectra of various samples. Results show that observed remote Raman spectra at a distance of 4 m enable us to identify silicates, carbonates, sulfates, perchlorates, water/water ice, and organics that have been found or may exist on extraterrestrial planets. Detailed Raman spectral assignments of the measured planetary materials and the feasible applications of remote Raman system for planetary explorations are discussed.

摘要

为了获得具有良好信噪比(SNR)的拉曼信号、节省功耗并可能避免高能脉冲对目标的破坏,已搭建并演示了一种具有激发能量调节功能的远程拉曼原型,该原型可用于中国的行星探测,以检测不同的矿物质。该系统由一台配备热电冷却电荷耦合器件(CCD)探测器的光谱仪、一台直径150毫米、焦距1500毫米的望远镜以及一台紧凑的1064纳米调Q Nd:YAG激光器组成,该激光器的电调脉冲能量为0至200毫焦/脉冲。使用KTP晶体在1064纳米激光中进行二次谐波产生,以产生532纳米激光,这是拉曼散射的光源。使用不同的激光脉冲能量和积分时间来获得各种样品的可区分远程拉曼光谱。结果表明,在4米距离处观测到的远程拉曼光谱使我们能够识别在外星行星上已发现或可能存在的硅酸盐、碳酸盐、硫酸盐、高氯酸盐、水/水冰和有机物。讨论了所测行星物质的详细拉曼光谱归属以及远程拉曼系统在行星探测中的可行应用。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/39f1/8587591/c11ac6867962/sensors-21-06973-g001.jpg

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