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1.
A planetary environment and analysis chamber (PEACh) has been developed at Washington University in St. Louis, in order to perform in situ multiple spectroscopic measurements on geological samples under relevant planetary environmental conditions and to support future planetary missions, with particular interest on Mars. The pressure in the chamber can range from ambient to 3 × 10−2 mbar. The simulated atmospheric composition and pressure are regulated via a combination of needle and ball valves connecting the chamber with containers filled with premixed gas. The temperature of the samples can be controlled in a range from ambient to − 100 °C. The in situ analytical techniques implemented (and to be implemented) are laser Raman spectroscopy, laser‐induced breakdown spectroscopy (LIBS), near‐IR reflectance spectroscopy, mid‐IR attenuated total reflectance spectroscopy, and microscopic imaging. The coordinated spectroscopic sensing on the same geological sample under well‐controlled atmospheric conditions in the PEACh establishes a way to link the results from the laboratory experiments to the spectral data obtained by landed and orbital planetary exploration missions, which will facilitate understanding the surface processes by which mineral phases occur and their association with atmospheric changes. Copyright © 2011 John Wiley & Sons, Ltd.  相似文献   

2.
Well‐resolved Raman spectra of samples of nitrogen‐containing compounds were detected using a portable Raman instrument (Ahura First Defender XL) outdoors at a low ambient temperature of −15 °C and at an altitude of 2860 m (Pitztall, Austria). The portable Raman spectrometer tested here is equipped with a 785‐nm diode laser and a fixed frontal probe. Solid form of formamide, urea, 3‐methylpyridine, aniline, indene, 1‐(2‐aminoethyl)piperazine, indoline and benzofuran were detected unambiguously under high‐mountain field conditions. The main Raman features (strong, medium and partially weak bands) were observed at the correct wavenumber positions (with a spectral resolution 7–10 cm−1) in the wavenumber range 200–1600 cm−1. The results obtained demonstrate the possibility of employing a miniaturised Raman spectrometer as a key instrument for investigating the presence of nitrogen‐containing organic compounds and biomolecules outdoors under low temperature conditions. Within the payload designed by European Space Agency (ESA) and National Aeronautics and Space Administration (NASA) for future missions, focussing not only on Mars, Raman spectroscopy represents an important instrumentation for the detection of organic nitrogen‐containing compounds relevant to life detection on planetary surfaces or near sub‐surfaces. Copyright © 2009 John Wiley & Sons, Ltd.  相似文献   

3.
We demonstrate the use of a light‐emitting diode (LED) based experimental setup for collecting polarization‐resolved Raman spectra with good spectral resolution. The combination of a commercial red LED (630 nm), a 1‐nm bandwidth laser‐line filter, and a polarizing prism is used as a light source. Polarization‐resolved spectra in dimethyl sulfoxide are recorded and compared with the corresponding laser‐Raman spectra. The LED‐excited spectra exhibit a resolution slightly lower than those in the laser case but still close to the resolution of the spectrometer. All relevant spectral features of dimethyl sulfoxide including the symmetric and antisymmetric stretching modes of the CSC moiety are resolved with the experimental setup providing a spectral resolution of approximately 20 cm−1. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

4.
Raman spectroscopy can be used for analysing both mineral and organic phases, thus allowing characterisation of the microbial‐scale geological context as well as the search for possible traces of life. This method is therefore very useful for in situ planetary exploration missions. Compared with the myriad of sample preparation techniques available in terrestrial laboratories, the possibilities for sample preparation during in situ missions on other planetary bodies are extremely limited and are generally restricted to abrasion of rock surfaces or crushing of the target samples. Whereas certain techniques need samples to be prepared in powder form, such as X‐ray diffraction, this kind of preparation is not particularly suitable for optical microscopy and/or Raman spectroscopy. In this contribution, we examine the effects of powdering rock and mineral samples on optical observations and Raman analyses. We used a commercial Raman spectrometer, as well as a Raman laser spectrometer that simulates the instrument being developed for the future ExoMars 2018 mission. The commercial Raman spectrometer documents significant modifications to the spectra of the powdered samples, including broadening of the peaks and shifts in their position, as well as the appearance of new peaks. These effects are caused by localised heating of the sample under the laser beam and amplification of nominal surface effects due to the increase in surface area in finer grain sizes. However, most changes observed in the Raman spectra using the Raman laser spectrometer system are negligible because the relatively large (50 µm diameter) laser spot size produces lower irradiance. Furthermore, minor phases were more easily detectable in the powdered samples. Most importantly, however, this sample preparation method results in the loss of the textural features and context, making identification of potential fossilized microbial remains more problematic. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

5.
Well‐resolved Raman spectra of organic acids were obtained with 785 nm excitation using a portable Raman instrument (Ahura First Defender XL) under low temperature −5 °C atmospheric conditions at an altitude of 2000 m (Axamer Lizum, Innental, Austria). The portable Raman spectrometer tested in this setting permits fast and unambiguous detection of solid forms of these organic acids (formic, acetic, valeric, hexanoic, heptanoic, isophthalic, ascorbic and mellitic) under field conditions. This demonstrates the possibility to use a miniaturized Raman spectrometer as a key instrument for investigating the presence of organic compounds and biomolecules under low temperature conditions. These results are important for future missions focusing not only on Mars, where Raman spectroscopy will be a key non‐destructive analytical tool for the in situ identification of organic compounds relevant to life detection on planetary surfaces or near sub‐surfaces. Copyright © 2009 John Wiley & Sons, Ltd.  相似文献   

6.
Raman spectral signatures have been obtained for a series of organic minerals using a compact portable Raman instrument equipped with 785‐nm laser excitation. Well‐resolved Raman spectra of crystalline salts of carboxylic acids, whewellite and mellite, as well as of the aromatic mineral idrialite were recorded. For comparative purposes, an amorphous fossil resin, baltic amber, was also investigated. The results obtained confirm that portable Raman instruments can be considered as excellent tools for field geological applications, including the detection of organic minerals in the frame of outcrops of sedimentary rocks or coal beds. Organic minerals can be added to the list of established biomarkers, including porphyrins, hydrocarbons and organic acids, which are important for the study with regard to future exobiological missions such as the ESA ExoMars mission to detect the presence of extinct or extant life on Mars. Copyright © 2009 John Wiley & Sons, Ltd.  相似文献   

7.
The identification of iron sulfates on Mars by the Mars Exploration Rovers (MERs) and the Mars Reconnaissance Orbiter emphasized the importance of studying iron sulfates in laboratory simulation experiments. The copiapite group of minerals was suggested as one of the potential iron sulfates occurring on the surface and subsurface on Mars, so it is meaningful to study their spectroscopic features, especially the spectral changes caused by cation substitutions. Four copiapite samples with cation substitutions (Fe3+, Al3+, Fe2+, Mg2+) were synthesized in our laboratory. Their identities were confirmed by powder X‐ray diffraction (XRD). Spectroscopic characterizations by Raman, mid‐IR, vis‐NIR and laser‐induced‐breakdown spectroscopy (LIBS) were conducted on those synthetic copiapite samples, as these technologies are being (and will be) used in current (and future) missions to Mars. We have found a systematic ν1peak shift in the Raman spectra of the copiapite samples with cation substitutions, a consistent atomic ratio detection by LIBS, a set of systematic XRD line shifts representing structural change caused by the cation substitutions and a weakening of selection rules in mid‐IR spectra caused by the low site symmetry of (SO4)2− in the copiapite structures. The near‐infrared (NIR) spectra of the trivalent copiapite species show two strong diagnostic water features near 1.4 and 1.9 µm, with two additional bands near 2.0 µm. In the vis‐NIR spectra, the position of an electronic band shifts from 0.85 µm for ferricopiapite to 0.866 µm for copiapite, and this shift suggests the appearance of a Fe2+ electronic transition band near 0.9 µm. Copyright © 2010 John Wiley & Sons, Ltd.  相似文献   

8.
Well‐resolved Raman spectra of gypsum, anglesite and baryte were detected using a portable Raman instrument (Ahura First Defender XL) in the laboratory and outdoor under atmospheric conditions. Spectra were obtained using a 785‐nm excitation. The portable spectrometers display generally lower spectral resolution compared with the laboratory confocal instrument but permit the fast, unambiguous detection of minerals under field conditions. Portable Raman instruments can be advocated as excellent tools for field geological, environmental as well as exobiological applications. A miniaturized Raman instrument will be included in the Pasteur analytical package of the ESA ExoMars mission and interesting research applications can now be proposed for in situ field planetary studies. Additionally, portable Raman instruments represent an ideal tool for demonstrating possible applications of Raman spectroscopic techniques outdoor. In geosciences this approach represents a new field which could completely change classical field work. Copyright © 2009 John Wiley & Sons, Ltd.  相似文献   

9.
The effect of chemical composition on the Raman spectra of a series of natural calcalkaline silicate glasses has been quantified by performing electron microprobe analyses and obtaining Raman spectra on glassy filaments (~450 µm) derived from a magma mingling experiment. The results provide a robust compositionally‐dependent database for the Raman spectra of natural silicate glasses along the calcalkaline series. An empirical model based on both the acquired Raman spectra and an ideal mixing equation between calcalkaline basaltic and rhyolitic end‐members is constructed enabling the estimation of the chemical composition and degree of polymerization of silicate glasses using Raman spectra. The model is relatively insensitive to acquisition conditions and has been validated using the MPI‐DING geochemical standard glasses 1 as well as further samples. The methods and model developed here offer several advantages compared with other analytical and spectroscopic methods such as infrared spectroscopy, X‐ray fluorescence spectroscopy, electron and ion microprobe analyses, inasmuch as Raman spectroscopy can be performed with a high spatial resolution (1 µm2) without the need for any sample preparation as a nondestructive technique. This study represents an advance in efforts to provide the first database of Raman spectra for natural silicate glasses and yields a new approach for the treatment of Raman spectra, which allows us to extract approximate information about the chemical composition of natural silicate glasses using Raman spectroscopy. We anticipate its application in handheld in situ terrestrial field studies of silicate glasses under extreme conditions (e.g. extraterrestrial and submarine environments). © 2015 The Authors Journal of Raman Spectroscopy Published by John Wiley & Sons Ltd  相似文献   

10.
为了研究聚对苯二甲酸乙二酯(PET)分子拉曼振动模式的特性,采用拉曼光谱法对PET纤维的拉曼光谱特性进行研究,并对PET纤维分别进行酸、碱、盐处理,获得酸、碱、盐处理前后纤维的拉曼光谱,分析与比较了处理前后拉曼光谱的特性;同时,采用原子力显微镜对其形貌结构进行观察。结果表明,在200~1 750 cm-1范围,NaOH处理的PET纤维的拉曼光谱强度高于未经处理的PET纤维,当拉曼频移大于1 750 cm-1时,经碱处理的PET拉曼峰强度低于未经处理的PET拉曼峰强度,且荧光背景减弱,H2SO4处理的PET纤维强度显著低于未经处理的PET纤维,CuSO4处理的PET纤维强度较未经处理的PET纤维的强度明显增高。原子力显微镜测结果表明,碱和PET纤维分子的相互作用使化学键断裂,分子结构发生改变,经NaOH处理后的PET纤维表面较未经处理的PET纤维表面更为粗糙,H2SO4处理的PET表面相对未经处理的PET纤维表面粗糙度降低,经CuSO4处理的PET纤维表面比未经处理的PET纤维粗糙度增加。PET纤维的拉曼光谱与原子力显微镜结果相一致,表明拉曼光谱与原子力显微镜的结合有望成为高聚物物性的表征技术。  相似文献   

11.
We propose and experimentally demonstrate a novel instrument arrangement, which allows for the collection of Raman spectra with a broadband light source. This is achieved by spatially dispersing the optical spectrum in the focal plane and confocally reimaging the Raman signal, which originates from different locations, onto the entrance slit of an imaging spectrometer. Using this approach and broadband radiation derived from a commercially available LED, we acquired high signal‐to‐noise spectra with a spectral resolution limited by the spectral resolution of a spectrometer. Copyright © 2013 John Wiley & Sons, Ltd.  相似文献   

12.
The polarized Raman spectroscopy is capable of giving confirmation regarding the crystalline phase as well as the crystallographic orientation of the sample. In this context, apart from crystallographic X‐ray and electron diffraction tools, polarized Raman spectroscopy and corresponding spectral imaging can be a promising crystallographic tool for determining both crystalline phase and orientation. Sub‐micron sized hexagonal AlGaN crystallites are grown by a simple atmospheric pressure chemical vapor deposition technique using the self catalytic vapor–solid process under N‐rich condition. The crystallites are used for the polarized Raman spectra in different crystalline orientations along with spectral imaging studies. The results obtained from the polarized Raman spectral studies show single crystalline nature of sub‐micron sized hexagonal AlGaN crystallites. Optical properties of the crystallites for different crystalline orientations are also studied using polarized photoluminescence measurements. The influence of internal crystal field to the photoluminescence spectra is proposed to explain the distinctive observation of splitting of emission intensity reported, for the first time, in case of c‐plane oriented single crystalline AlGaN crystallite as compared with that of m‐plane oriented crystallite. Copyright © 2016 John Wiley & Sons, Ltd.  相似文献   

13.
The application of polarization‐sensitive (PS) coherent anti‐Stokes Raman scattering (CARS) spectroscopy for the investigation of highly luminescent free‐base porphyrins under Qx band resonance is discussed. For coproporphyrin I tetramethyl ester (CP‐I‐TME), PS CARS spectra involving resonances with the electronic Qx absorption band as well as polarized spontaneous Raman spectra involving B band resonance are presented. A quantitative evaluation of the CP‐I‐TME spectra is performed and the results are compared to our previously presented data on free‐base octaethylporphine (OEP) and mesoporphyrin IX dimethyl ester (MP‐IX‐DME), which were obtained under identical excitation conditions. This comprehensive analysis reveals several spectral differences that can be attributed to the different β–substitution pattern of the porphyrin macrocycle. Additionally, the strong resonance enhancement of totally symmetric modes under Qx band excitation is identified as a common property for OEP, CP‐I‐TME, and MP‐IX‐DME; this enhancement selectivity distinguishes the investigated substances from what is generally observed for metallo porphyrins. Copyright © 2008 John Wiley & Sons, Ltd.  相似文献   

14.
One of the most common minerals in the Earth's crust, quartz, is stable across a wide range of temperature and pressure conditions. As its microstructure is sensitive to diverse deformation mechanisms, quartz may provide valuable information regarding the structural evolution of many different rock types. Using Raman microspectroscopy, single quartz grains and monomineralic domains characterized by different deformation conditions can be identified and separated. In this study, three microstructurally extreme quartz grain types were discriminated from a subsurface shear zone: grains with undulose extinction (T0), grains with subgrains (T1), and grains with recrystallized grains (T2). Moreover, several microstructurally transitional grains were measured, which represent combinations of the aforementioned extremes. Statistical analysis revealed that the microscopically identified extreme grains possess significantly different spectral attributes and as such can be divided on the basis of certain variables of their respective Raman spectra. The three extreme quartz grain types were formed by different deformation mechanisms and thus represent distinct deformation conditions. The T0‐T1‐T2 spectral space can therefore also be considered a virtual deformational space. Although each complex quartz grain measured also appears elsewhere in the deformation process defined by T0‐T1‐T2 extreme conditions, they together represent a successive deformation path. This combined pathway is assumed to be characteristic for the whole rock volume under study. Finally, the computed Raman spectroscopy‐based virtual deformational space enabled the determination of the structural evolution of the analyzed shear zone. Copyright © 2014 John Wiley & Sons, Ltd.  相似文献   

15.
Non‐degenerate second‐order scattering due to interaction of infrared and ultraviolet pulses is observed in picosecond infrared‐pump/anti‐Stokes Raman‐probe experiments under electronic resonance conditions. We detected resonance hyper‐Rayleigh scattering at the sum frequency of the pulses as well as the corresponding frequency‐down‐shifted resonance hyper‐Raman lines. Nearly coinciding resonance hyper‐Raman and one‐photon resonance Raman spectra indicate conditions of A‐term resonance Raman scattering. Second‐order scattering is distinguished from transient anti‐Stokes Raman scattering of v = 1 to v = 0 transitions and v = 1 to v′ = 1 combination transitions by taking into account their different spectral and temporal behaviour. Separating these processes is essential for a proper analysis of transient vibrational populations. Copyright © 2007 John Wiley & Sons, Ltd.  相似文献   

16.
G‐quadruplexes (G4s) are four‐stranded DNA structures formed within nucleic acid sequences that are rich in guanines. G4 formation within DNA strands is believed to have significant biological relevance for the control of cell replication and gene expression. Therefore, the development and validation of experimental techniques that can easily and reliably characterize G4 structures under biologically relevant measurement conditions, like Raman spectroscopy, are desirable for G4‐targeted structure based drug design. Here we report Raman and polarized Raman studies of solutions of three oligonucleotides, thrombin binding aptamer (TBA) 5′‐GGTTGGTGTGGTTGG‐3′, human telomeric (HT) 5′‐(TTAGGG)4‐3′, and a modified c‐Myc NHE‐III1 sequence (MycL1) 5′‐TGAGGGTGGGTAGGGTGGGTAA‐3′, which were previously reported to form four distinct intramolecular G4 structures in the presence of Na+ or K+, as determined by NMR. Our results support the previously proposed antiparallel (TBA), antiparallel and hybrid (HT), and parallel with double‐chain reversal (DCR) loop (MycL1) structures. Large sample‐dependent variations in the intensity of bands associated with deoxyribose backbone modes in the 840–930 cm−1 and 1420–1460 cm−1 spectral regions were observed. Most notably, a highly polarized deoxyribose ring symmetric stretch (~930 cm−1) appeared strongly in the solution spectra for HT and TBA, but was very weak or absent in the solution spectrum for MycL1 and the drop deposition (dried sample) spectra for all three oligonucleotides. It is hypothesized that the intensity of this band is likely controlled by furanose ring structure uniformity and/or solvent accessibility to certain nucleotide binding sites. Raman depolarization ratios measured for the G4s in solution were generally very similar to those previously reported for canonical B DNA, with the possible exception of base ring modes that consistently yielded slightly lower depolarization ratios for G4s compared to B DNA. The results further underscore the utility of Raman and polarized Raman spectroscopy for G4 structure elucidation under biologically relevant solution conditions. Copyright © 2015 John Wiley & Sons, Ltd.  相似文献   

17.
Raman spectroscopy has been effectively applied to clinically differentiate normal and cancerous mucosal tissues. Micro‐Raman spectroscopy provides a tool to better understand the molecular basis for the Raman clinical signal. The objective of the current study was to utilize micro‐Raman spectroscopy to define the molecular/spectral differences between normal and abnormal squamous cell carcinoma (SCC) in oral mucosa (in vitro). Understanding this may help in identifying unique spectra or may be useful for in vivo application of this technology. Micro‐Raman (confocal) spectroscopy was used to obtain molecular images of normal and SCC cells of human oral mucosa. Four fresh flashed‐frozen tumor and four matched normal tongue specimens were studied. The spectra covered a wavenumber range from 300 to 4000 cm−1 with a spectral resolution of 8 cm−1 and a spatial resolution of 1.0 µm. The cells were located within thin sections of tongue mucosa biopsies. The excitation wavelength of 515 nm was used. We were able to obtain Raman images with rich information about the spectroscopic and structural features within the cytoplasm, cell membrane, and cell nuclei. Significant spectral differences were observed between the Raman images of normal and malignant squamous cells. The heterogeneity of tumor cells within the abnormal tissue was also demonstrated. Spectral differences demonstrated between both tissue types have provided important information regarding the origins of specific signals within the cells of each tissue type. In our search for specific spectral biomarkers, we believe that a cell surface protein, greatly upregulated in SCC cells, was discovered at 1583 cm−1. Copyright © 2010 John Wiley & Sons, Ltd.  相似文献   

18.
实现了一套实验室环境下的LIBS-Raman测试系统的设计,并验证激光诱导击穿光谱技术(LIBS)和拉曼(Raman)光谱技术在火星模拟环境下矿物样品的综合检测能力。该系统使用卡塞格林望远镜结构进行远程的LIBS激发,使用旁路反射光路进行远程脉冲Raman光谱的激发,其激发光源的波长分别为1 064和532 nm。之后统一使用卡塞格林望远镜进行二者光谱信号的收集。为了充分模拟火星表面矿物所处的物理条件,设计与实现了一套气体腔体,通过将样品放置在气体舱中,可以实现对火星表面条件进行最大程度的模拟。为了验证使用该LIBS-Raman系统进行火星矿物分析的能力,利用8种典型矿物(孔雀石、蓝铜矿、雄黄、雌黄、文石、方解石、硬石膏和石膏等)样品展开实验分析。在这些样品中存在巨大的元素和分子成分上的差异,其中孔雀石、蓝铜矿分子具有不同的价态和原子比例;雄黄、雌黄分子的各原子的个数均不相同;文石、方解石虽具有相同的分子式,但是晶体结构明显不同;硬石膏和石膏矿物的差异则体现在其分子有无含有结晶水上。利用LIBS和Raman技术对这些差异性进行研究,以此来验证在火星条件下使用此组合仪器分析矿物种类和成分的有效性,并研究激光诱导击穿光谱技术和拉曼光谱技术在物质成分分析中的优缺点。实验结果表明,该系统可以在火星条件下有效分析矿物种类和成分。该对比实验还验证了在分析火星物质中的特定矿物元素组成这一问题上,LIBS技术可快速区分元素种类,但针对分子信息探测存在明显局限性;Raman光谱技术则可以在一定程度上对这种局限性进行补偿。二者结合将有效提高极端条件下具有不同分子组成和结构的矿物的识别效能。该系统的成功验证可为进一步火星探测计划提供有力补充,并对实验室建立有价值数据库提供帮助。  相似文献   

19.
This paper presents a methodology conceived as a support system to identify unknown materials by means of the automatic recognition of their Raman spectra. Initially, the design and implementation of the system were framed in an artistic context where the Raman spectra analyzed belong to artistic pigments. The analysis of the pigmentation used in an artwork constitutes one of the most important contributions in its global study. This paper proposes a methodology to systematically identify Raman spectra, following the way analysts usually work in their laboratory but avoiding their assessment and subjectivity. It is a three‐phase methodology that automates the spectral comparison, which is based on one of the most powerful paradigms inmachine learning: the case‐based reasoning (CBR) systems. A CBR system is able to solve a problem by using specific knowledge of previous experiences (well‐known spectral library of patterns) and finding the most similar past cases (patterns), reusing and adapting them to the new problem situation (unknown spectrum). The system results in a global signal processing methodology that includes different phases such as reducing the Raman spectral expression by means of the principal component analysis, the definition of similarity measures to objectively quantify the spectral similarity and providing a final value obtained by a fuzzy logic system that will help the analyst to take a decision. The major benefit of a Raman spectral identification system lies in offering a decision‐support tool to those who are not experts or under difficult situations with respect to Raman spectroscopy. Copyright © 2011 John Wiley & Sons, Ltd.  相似文献   

20.
Recently, we have reported on the characterization of various carbonaceous materials including multiwalled carbon nanotube (MWCNT) filters, which have specific molecular filtering capabilities and good mechanical strength and can be produced in bulk as highly aligned arrays of bundles of CNTs. We have extended our studies using Fourier transform‐Raman spectroscopy with 1064 nm excitation wavelength and a rotating sample holder in the region 1000–2800 cm−1, in addition to 532 and 785 nm, which were used for Raman excitation in our previous study. Raman spectra were analyzed for band positions and line shape with special emphasis on the D‐, G‐ and G′‐ bands. For the single‐walled species, Carbotrap and graphite spectra were also recorded with 488 nm excitation. A dispersion study has been made from the Raman data available with the different excitation wavelengths. Slight band shifts and band broadening could be observed under the two sample conditions, one with the stationary sample and the other with sample rotation. The spectral changes are related to the excessive heating caused in a stationary sample by laser irradiation. Based on our findings in this study combined with our earlier study, we can state that only a careful line shape analysis and study of intensity pattern of the D‐ and G‐Raman bands under well‐defined measurement conditions lends itself as a good measure of degree of alignment in the MWCNT bundles. Copyright © 2010 John Wiley & Sons, Ltd.  相似文献   

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