基于ZnSe平板波导的小型光谱仪光学系统设计

一般光谱仪的小型化是通过缩小元件尺寸和元件间距离实现的,会降低仪器的性能。为实现高光通量、高光谱分辨率的红外光谱探测,提出一种基于ZnSe平板波导的小型光谱仪的设计方法。说明平板波导结构压缩光束的原理,根据介质中光栅的衍射特性,推导出光谱分辨率与各个参数的关系,给出一个小型光谱仪的具体设计。仪器的光谱范围为8~14μm,光谱分辨率为80 nm,数值孔径为0.3,光学系统是一整块ZnSe平板波导,尺寸为70 mm×70 mm×4 mm。并与相同设计指标下一般Czerny-Turner结构的光谱仪进行对比分析。结果表明基于ZnSe平板波导的小型光谱仪系统尺寸更小,光谱分辨率更高,光通量更大。     

利用四原子Cluster态概率隐形传送两原子纠缠态

为平衡光栅色散型光谱仪光通量、系统信噪比和光谱分辨率之间的矛盾,介绍了一种基于微狭缝阵列的静态双增益阿达玛光谱仪.在分析其实现静态双增益工作原理的基础上,阐述了由于阿达玛编码模板多狭缝阵列引起的光谱重叠的原因.为实现静态双增益阿达玛光谱仪光谱重叠校正,理论推导了光谱偏移量与阿达玛编码模板狭缝空间位置之间的关系,以及分光后某波长空间错位量与码元(狭缝)空间位置、波长之间的关系.仿真实验验证了此方法简单有效,无需复杂计算,修正速度快,易于编程实现.     

静态双增益阿达玛光谱仪光谱的重叠错位分析与校正

为平衡光栅色散型光谱仪光通量、系统信噪比和光谱分辨率之间的矛盾,介绍了一种基于微狭缝阵列的静态双增益阿达玛光谱仪.在分析其实现静态双增益工作原理的基础上,阐述了由于阿达玛编码模板多狭缝阵列引起的光谱重叠的原因.为实现静态双增益阿达玛光谱仪光谱重叠校正,理论推导了光谱偏移量与阿达玛编码模板狭缝空间位置之间的关系,以及分光后某波长空间错位量与码元(狭缝)空间位置、波长之间的关系.仿真实验验证了此方法简单有效,无需复杂计算,修正速度快,易于编程实现.     

微小型光栅光谱仪光学系统的特点与光谱分辨率的提高

微小型光谱仪的设计制作可以采用多种方法,其结构特点和光谱分辨率也各不相同,目前实用高光谱分辨率微小型光谱仪采用的是光栅色散型光学系统.简要回顾了微小型光谱仪的发展过程,分析了典型的光栅色散型微小型光谱仪采用的光学系统,如基于罗兰圆的光学系统,基于Czerny-Turner的光学系统的特点,总结了提高微小型光栅光谱仪光谱分辨率采用的方法和技术,特别是解决光谱仪的微小型化和光谱分辨率之间的矛盾以及测量光谱范围和光谱分辨率之间的矛盾的方法,从而为新型微小型光谱仪的研制提供经验和借鉴.     

基于平场全息凹面光栅的舌诊用光谱仪的研制

由于传统的望舌诊断法过于依赖中医师的经验判断,导致误诊的概率相对较大,而基于图像处理的舌诊法受光源、图像采集设备影响较大,同时对于病理不同而颜色相近的舌象识别率不高。为了克服上述缺点,利用舌光谱的“指纹效应”,通过使用光谱法来对不同性状的舌象进行诊断,为了实现这一目标,研制了一款用于舌象诊断的光谱仪,同时为了克服传统分光器件的不足,分光系统中采用了平场全息凹面光栅作为分光器件,能保证系统小型化、光通量利用率提高的同时,改善光谱成像的质量和分辨率。通过系统实验测试,该光谱仪的光谱范围达到340～850 nm, 分辨率优于2 nm,同时通过模拟实验充分验证了该系统的有效性。     

高光通量交叉非对称Czerny-Turner拉曼光谱仪光学系统

为克服分立式便携拉曼光谱仪光通量低的缺点,设计了一种集拉曼探头光路与分光系统于一体的光学系统。探头光路采用大数值孔径的非球面透镜实现样品的有效激发和信号的高效收集,通过胶合透镜组缩小会聚光路尺寸、消除轴向色差。分光系统基于交叉非对称Czerny-Turner结构,为获得期望的光谱分辨率和光谱范围,建立了分光系统光谱分辨率及光谱范围与交叉非对称Czerny-Turner结构参数的关系。由测得的汞灯谱图可知,分光系统的光谱分辨率优于6 cm~(-1)(0.37 nm),光谱范围为790~950 nm(200~2000 cm~(-1))。将设计的光学系统对CCL4进行测试,实验结果表明在相同积分时间内由这种整体式的光学系统检测到的CCL4光谱谱峰强度是用商业探头通过光纤连接分光系统检测到的近3倍,验证了光学系统设计的合理性。     

成像光谱仪一体化设计

随着超光谱成像技术的发展,超光谱成像光谱仪的要求也随之提高,小型化、高光谱分辨率和高空间分辨率成为发展趋势,这就要求设计者在进行仪器设计的过程中不断完善和优化设计。提出了成像光谱仪一体化设计的方法,即不单纯地进行光谱仪分光系统的设计,而是将光谱仪分光系统置于整体结构中进行整体系统设计和优化,从而实现超光谱成像光谱仪的最佳设计结果,并以近年来应用较为广泛的凸面光栅成像光谱仪为例,较为详细地阐述了成像光谱仪一体化设计方法在系统研制过程中的应用,并通过对该凸面光栅成像光谱仪的测试验证了该方法的正确性。     

Offner型成像光谱仪波长使用范围和光谱分辨率研究

研究了Offner型成像光谱仪消像差结构的参量和性能.用几何法推导出Offner型成像光谱仪的波长使用范围、系统线色散以及光谱分辨率的计算公式;在理想像差条件下,分析了Offner型成像光谱仪光谱分辨率与入射狭缝的宽度、凸面光栅分辨率和探测器像元尺寸各个因素之间的关系;探讨了提高光谱分辨率采用的方法和技术,解决了光谱仪的各个参量和光谱分辨率之间的矛盾.研究表明:当系统像差很小可忽略时,通过减小狭缝宽度,有利于提高光谱分辨率;Offner型成像光谱仪的分辨率由入射狭缝宽度、光栅和CCD像元尺寸三者中分辨本领最低的参量确定.     

室外高光谱BRDF自动测量系统的设计

室外BRDF(Bidirectional reflectance distribution function)测量随着遥感的发展越来越重要。室外测量要求测量周期短、测量点多、光谱分辨率高。为了满足这一要求,设计了室外高光谱BRDF自动测量系统。系统主要由自动测量架和光谱仪器组成。测量架半径为2m,主要由天顶弧轨道、方位圆轨道、伺服电机、PLC组成。光谱仪器包括一台亮度计和一台照度计,亮度计测量反射亮度,被固定在测量架小车平台上,照度计测量入射照度。两台光谱仪器采用相同的平场凹面光栅分光、线阵列探测器探测。光谱测量范围为400~2500nm,光谱分辨率为3.5nm(400~1000nm)、12nm(1000~2500nm)。系统在工控机的控制下完成自动测量。在自动默认状态下测量周期大约为10min。     

近红外微型光谱仪光学系统设计与模拟

基于光谱仪基本工作原理和光学设计理论,以系统微型化、且能满足一定光谱范围和分辨率要求为具体设计目标,提出了基于平面衍射光栅分光的交叉式C-T结构的近红外微型光谱仪光学系统结构方案。采用ZEMAX软件对近红外微型光谱仪的分光系统、成像系统进行了优化设计与模拟分析。最终设计与模拟分析结果表明,该光学系统光谱范围为900～1 700 nm,分辨率<10 nm,谱面展宽为12.74 mm,F数为8.128 388,系统体积为51.26 mm×41.81 mm×22 mm。     

Compact Fourier-transform volume holographic spectrometer for diffuse source spectroscopy

We present a new idea for diffuse source spectroscopy using a Fourier-transform volume holographic spectrometer formed by a Fourier-transform lens, a volume hologram, and a CCD. We show that this spectrometer can operate well under spatially incoherent light illumination. Furthermore, this spectrometer is less bulky, less sensitive to input alignment, and potentially more appropriate for implementation of highly sensitive spectrometers than conventional spectrometers.     

光栅光谱仪的整体建模与分析

理论模型是研究光谱技术,开发光谱仪器的重要工具。文章提出了一种对现代光栅光谱仪进行整体建模与分析的方法。与现有方法仅局限于光学成像等局部环节不同,该方法从光谱信息传递和变换的角度将光栅光谱仪分割为光学成像、探测、重建和显示4个功能模块,分析各个模块对光谱信息的影响,建立光栅光谱仪的整体模型并导出它的传递函数。进一步,又利用它们分析了各模块对仪器整体性能的影响规律,并揭示出要获得高质量的光谱图必须增加基带响应,抑制假响应,而重建模块将是重要途径。     

Transform spectrometer based on measuring the periodicity of Talbot self-images

We demonstrate a compact transform spectrometer based on measuring the periodicity of Talbot self-images. The system has no moving parts; it contains only a tilted absorption grating that is imaged onto a CCD camera. The linear architecture of the system makes it possible to use this design in imaging arrays of spectrometers. Unlike other transform spectrometers, its resolution is independent of wavelength.     

Multidimensional spectroscopy of cascades of photons emitted by quantum objects

In the paper we describe the capabilities of the multidimensional (multidetector) spectroscopy of photon cascades. Attention is paid to a considerable increase in the resolution of multidetector spectrometers compared to one-detector spectrometers. We give a derivation of the radiation intensity detection limit, which relates all the basic characteristics of a multidetector spectrometer, and present examples of calculation of spectrometer characteristics. Translated from Zhurnal Prikladnoi Spektroskopii, Vol. 65, No. 2, pp. 278–283, March–April, 1998.     

Effect of the size of experimental channels of the lead slowing-down spectrometer SVZ-100 (Institute for Nuclear Research, Moscow) on the moderation constant

Lead slowing-down (LSD) spectrometers have a low energy resolution (about 30%), but their luminosity is 10³ to 10⁴ times higher than that of time-of-flight (TOF) spectrometers. A high luminosity of LSD spectrometers makes it possible to use them to measure neutron cross section for samples of mass about several micrograms. These features specify a niche for the application of LSD spectrometers in measuring neutron cross sections for elements hardly available in macroscopic amounts—in particular, for actinides. A mathematical simulation of the parameters of SVZ-100 LSD spectrometer of the Institute for Nuclear Research (INR, Moscow) is performed in the present study on the basis of the MCNPX code. It is found that the moderation constant, which is the main parameter of LSD spectrometers, is highly sensitive to the size and shape of detecting volumes in calculations and, hence, to the real size of experimental channels of the LSD spectrometer.     

Electron spin-echo spectroscopy at 95 GHz

An electron spin-echo spectrometer operating at 94.9 GHz is described. The experimental details of the microwave circuit are discussed and the performance is compared with that of more conventional spectrometers at 9.5 GHz.     

Decay Pion Spectroscopy of Electro-Produced Hypernuclei

The investigation of light hypernuclei is quite important for understanding the basic YN interaction and the mechanism of hypernuclear structure. We started the commissioning of the decay pion spectroscopy of light hypernuclei at MAMI-C in 2011. In order to realize the K⁺ tagging efficiently, some detectors on KAOS spectrometer were upgraded or newly installed. The existing and well-studied spectrometers, SpekA, SpekC were used as pion spectrometers. The analysis is ongoing to estimate the detectors performance and develop the spectrometers for future experiments with higher beam intensity. The preliminary results of the particle identification are presented in this article.     

基于银膜孔阵列超强透射效应的相敏表面等离子体共振传感器的仿真研究(英文)

We present an ultra compact and high resolution free space optical spectrometer and demonstrate it by using FDTD simulations. The miniature interferometer-based spectrometer is a series of submicron phase objects on a polymethyl methacrylate(PMMA) film with a CCD as the detector. The spectrum is obtained by solving a system of simultaneous linear equations. The Tikhonov regularization method is used to achieve a resolution at the picometer level. Compared with conventional spectrometers, the proposed device...     

X-radiography of cultural heritage materials using handheld XRF spectrometers

This study investigated the feasibility, repeatability, and limitations of using handheld X-ray fluorescence spectrometers to perform radiography with thorough safety measures. Radiography is a well-established nondestructive technique commonly used in the field of cultural heritage preservation but not easily accessible to many. Equipped with X-ray generating tubes, handheld spectrometers could potentially assist performing radiographic tasks off-site due to their portability and increasing availability. These spectrometers are designed to work at close range within a limited voltage range and wattage, so the exposure settings should be modified for the spectrometers to generate big enough X-ray beams to irradiate the artifacts and enough radiation to penetrate through them to produce useful radiographs. Using a Bruker Tracer 5i, the effective beam spread angle, which was computed from several test shots, was used to determine the constant relation between the area of irradiation and the X-ray source to image-receptor distance. Based on inverse square law and the total wattage limitation of the spectrometer, current and exposure time were recalculated to produce informative radiographs. Because of the limitations of the tested spectrometer, this method is best applicable to an area smaller than 9 cm, with the scanning distance shorter than half a meter. The spectrometer cannot be used to radiograph materials that require higher voltage than it can produce.     

Analysis of the tuning and operation of reflection resonator EPR spectrometers

This paper investigates basic characteristics of the electron paramagnetic resonance (EPR) signal obtained from spectrometers employing reflection resonators. General equations are presented which reveal the phase and amplitude dependence on instrumental parameters of both components of the continuous wave (CW) EPR signal (absorption and dispersion). New phase vector diagrams derived from these general equations are presented for the analysis of the EPR response. The dependence of the phase and absolute value of the CW EPR signal on the local oscillator (LO) phase and on resonator offset and coupling is presented and analyzed. The EPR spectrometer tuning procedures for both balanced and unbalanced heterodyne receivers are analyzed in detail using the new phase diagrams. Extraneous signals at the RF input of the microwave receiver (resulting from circulator leakage and reflections in the resonator transmission line) have been taken into account and analyzed. It is shown that a final tuning condition that corresponds to an extremum of the receiver output as a function of the resonator frequency is necessary and sufficient for the acquisition of pure absorption signal. This condition is universal: it applies to all spectrometer configurations in all frequency ranges. High Frequency EPR spectrometer (130 GHz) data are used to generate experimental phase diagrams that illustrate the theoretical concepts presented in the paper. Conditions are presented under which the absorption signal can be measured with complete suppression of the dispersion, independent of the mutual frequency offset between the microwave source and the EPR sample resonator. Equations describing the approximate relationship between changes of the resonator properties (Q-factor and frequency) and paramagnetic susceptibility are derived and analyzed.