遥感傅里叶变换红外光谱层析技术中的重构算法

在遥感傅里叶变换红外光谱层析技术中，对于是否能够快速、经济地得出气体空间浓度分布图及预测浓度峰位置，重构算法的选择是至重要的。理想的重构算法即使在仪器噪声较大、存在测量误差、光线数量少以及待测气体在空间的分布不稳定情况下，也能够通过有限的测量数据和非对称的光线构型，得出理想的重构图。本文对遥感傅里叶变换红外光谱层析技术中采用的几种重构算法，如ART法、MART法、SIRT法和SBFM法等，作了扼要描述。与传统的ART法相比，MART法在迭代速度和迭代精度上有较大的优越性，SIRT法克服了采用代数重构技术所带来的模糊性，SBFM法使重构结果噪声明显减小。     

傅里叶变换红外光谱在大气遥感监测中的应用

傅里叶变换红外光谱遥感技术是一门综合探测技术，它可以对气体组分分进行远距离，实时，多组分同时监测。本文介绍了遥感傅里叶变换红外谱光在遥测大气层中痕量气体，污染源排放的废气，灭火过程产生的有毒气体、气体空间分布等方面的应用现状。     

EQUINOX55型遥感傅里叶变换红外光谱系统的校正

利用遥感傅 里叶变换红外发射光谱，对红外辐射源的绝对光谱能量分布和热气体浓度进行测量时，首先必须对测得的红外辐射源的发射光谱强度进行校正，为此，需用已知温度的标准绝对黑体对系统进行校正，本文考察了黑体温度对EQUINOX55型遥感傅里叶变换红外光谱的响应函数的影响。结果表明，仪器响应函数随着温度的升高而增加，但当温度比较高时，仪器响应函数曲线变化趋小。     

遥感傅里叶变换红外光谱的大气层析技术

遥感傅里叶变换红外光谱层析技术是一项新的气体分析技术，它可用于构造气体浓度峰图形，定量分析工业污染气体总释放量等方面，随着算法的不断优化，在重构气体在空间的分布方面，遥感傅里叶变换红外光谱层析技术正在不断成长。     

污染云团红外辐射传输模型与红外光谱的计算机仿真

针对建立的三层结构污染云团红外辐射传输模型,采用实测场地背景和各种干扰物辐射光谱作为基本的辐射数据,对不同浓度的污染云团红外辐射光谱进行仿真.结果表明:利用实测场地背景辐射光谱和该模型仿真污染云团DMMP红外光谱,光谱在810 cm-1,920 cm-1和1 040 cm-1波段上有明显的特征峰.当模型考虑干扰物和背景辐射的变化影响时,污染云团在810 cm-1,920 cm-1和1 040 cm-1波段上的光谱特征明显减弱.仿真光谱与场地实测光谱有比较好的符合,两者的RMS误差约为1.0.     

子波变换及其在污染云团红外光谱监测与识别中的应用

反应离散子波变换进行污染云团红外光谱信号分析及特征提取，离散子波变换具有时－频分析特性，能将信号的细微变化反映出来，对实时遥感获取的目标云团作离散子波变换分析的结果表明：离散子波变换可明显提高目标云团的特性，十分有利于光谱的识别。     

食用菌的傅里叶变换红外光谱鉴别

利用傅里叶变换红外光谱法(FTIR)研究了担子菌木耳目、非褶菌目和伞菌目6个科9个属的10种食用菌的子实体。将光谱分为5个区S1区(3 050～2 800 cm-1),S2区(1 750～1 500 cm-1),S3区(1 500～1 200 cm-1),S4区(1 200～950 cm-1),S5区(950～700 cm-1);在5个区中,强峰出现在S4区的1 080 cm-1附近和1 040 cm-1(1 020 cm-1)附近,以及S2区的1 640 cm-1附近,1 640 cm-1附近的峰为酰胺Ⅰ振动峰,前两峰为糖类振动峰。根据5个区光谱峰值和吸收强度比,可以鉴别不同的食用菌。700～950 cm-1范围有可能作为区分不同属蘑菇间的指纹区。     

傅里叶变换红外光谱仪扫描成像系统被动遥测火焰红外图像

介绍了一种傅里叶变换红外光谱仪扫描成像系统,并用该系统测量了放在平台上的3盏普通实验用酒精灯的火焰红外发射谱,选择位于大气窗口内的波数为900～1 000 cm-1波段,利用普朗克定律,反演出了每条光谱对应的相对温度。实验中每一个光谱对应一个扫描位置即像素点,把这些温度数据通过Matlab软件绘制出了扫描范围内的红外图像。将红外图像叠加在视频图像之上,两者吻合得非常好,清楚地显示了3个火焰的位置。     

块菌的傅里叶变换红外光谱研究

块菌是珍稀野生食用菌,其蛋白质和糖类含量较高,块菌多糖具有潜在的药用价值。文章利用傅里叶变换红外光谱技术(FTIR)对五种云南野生块菌作了研究。结果表明,块菌属真菌有其独特的光谱特征,全谱最强峰为出现在1 042和1 077 cm-1附近的强双峰。在脂分子的羰基峰1 742 cm-1及糖类异构体的指纹区1 200～750 cm-1,不同种类、不同产地块菌的光谱有明显差异,另外,正常块菌和霉变块菌的光谱亦有明显差异,主要体现在谱峰吸收强度的变化上,部分谱峰吸收强度比的变化表明,块菌样品变质前后,其蛋白质和糖类物质的含量发生了变化。FTIR光谱提供了块菌成分的有关化学信息,为鉴别块菌和区分块菌的种类、质量提供了简便快捷的手段。     

几种花粉的傅里叶变换红外光谱研究

本文利用傅里叶变换红外光谱技术(FTIR)对7种植物[玉兰、香水百合、天竺葵(粉红,红色)、兰花、菊花、马蹄莲]花粉进行了研究。结果显示,花粉样品的红外光谱主要由蛋白质、多糖、脂类物质的特征吸收峰组成。不同种花粉的红外光谱的差异表现为脂类物质的特征吸收峰强度的变化,多糖特征吸收峰峰形的区别,以及蛋白质和多糖的特征峰强度比的不同。不同颜色的天竺葵光谱差异较小,仅脂类特征吸收峰略有差异。研究表明,利用红外光谱建立数据库,有可能依据花粉的傅里叶变换红外光谱鉴别植物。     

Raman and infrared spectra of tere-phthalaldehyde

The laser Raman spectrum of tere-phthalaldehyde powder has been recorded on a Jobin Yvonhg 2S spectrophotometer with a~100 mW Argon-Ion laser. The infrared spectrum of the solid substance has been recorded on a Perkin-Elmer 621 spectrophotometer in the region 300–4000 cm^-1 using KBr and nujol mull techniques. The observed frequencies have been assigned in terms of the fundamentals, overtones and combinations assumingD _2h point-group symmetry.     

A fast infrared radiative transfer model for overlapping clouds

A fast infrared radiative transfer model (FIRTM2) appropriate for application to both single-layered and overlapping cloud situations is developed for simulating the outgoing infrared spectral radiance at the top of the atmosphere (TOA). In FIRTM2 a pre-computed library of cloud reflectance and transmittance values is employed to account for one or two cloud layers, whereas the background atmospheric optical thickness due to gaseous absorption can be computed from a clear-sky radiative transfer model. FIRTM2 is applicable to three atmospheric conditions: (1) clear-sky, (2) single-layered ice or water cloud, and (3) two simultaneous cloud layers in a column (e.g., ice cloud overlying water cloud). Moreover, FIRTM2 outputs the derivatives (i.e., Jacobians) of the TOA brightness temperature with respect to cloud optical thickness and effective particle size. Sensitivity analyses have been carried out to assess the performance of FIRTM2 for two spectral regions, namely the longwave (LW) band (587.3-1179.5 cm⁻¹) and the short-to-medium wave (SMW) band (1180.1-2228.9 cm⁻¹). The assessment is carried out in terms of brightness temperature differences (BTD) between FIRTM2 and the well-known discrete ordinates radiative transfer model (DISORT), henceforth referred to as BTD (F−D). The BTD (F−D) values for single-layered clouds are generally less than 0.8 K. For the case of two cloud layers (specifically ice cloud over water cloud), the BTD (F−D) values are also generally less than 0.8 K except for the SMW band for the case of a very high altitude (>15 km) cloud comprised of small ice particles. Note that for clear-sky atmospheres, FIRTM2 reduces to the clear-sky radiative transfer model that is incorporated into FIRTM2, and the errors in this case are essentially those of the clear-sky radiative transfer model.     

Fourier transform infrared emission spectra of MnH and MnD

Fourier transform infrared emission spectra of MnH and MnD were observed in the ground X⁷Σ⁺ electronic state. The vibration-rotation bands from v = 1 → 0 to v = 3 → 2 for MnH and from v = 1 → 0 to v = 4 → 3 for MnD were recorded at an instrumental resolution of 0.0085 cm⁻¹. Spectroscopic constants were determined for each vibrational level and equilibrium constants were found from a Dunham-type fit. The equilibrium vibrational constant (ω_e) for MnH was found to be 1546.84518(65) cm⁻¹, the equilibrium rotational constant (B_e) is 5.6856789(103) cm⁻¹ and the eqilibrium bond distance (r_e) was determined to be 1.7308601(47) Å.     

Fast radiative transfer modeling for infrared imaging radiometry

Fast radiative transfer codes have been developed for simulating the outgoing radiance (and corresponding brightness temperature) to be measured by the Infrared Imaging Radiometer (IIR) of the space Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) mission. Two simple codes (FASRAD and FASAA), for which scattering is neglected, as well as an accurate code (FASDOM), accounting for scattering and absorption with the Discrete Ordinate Method (DOM), are presented. Their accuracy has been estimated with a reference code including a line-by-line model and the DOM. Simulations have shown that the accuracy is generally better than 0.3 K on the brightness temperature for clear or cloudy atmospheres. This accuracy agrees with the expected one of future IIR measurements. In addition, the impact of scattering on the brightness temperature has been evaluated for semi-transparent liquid clouds in the IIR spectral range. Especially, simulations have shown that cloud microphysics retrieval might be possible with the Brightness Temperature Difference (BTD) between two IIR bands, using the couple of wavelengths (8.7-) or (10.6-). However, scattering strongly influences the radiation for shorter wavelengths. The error on the BTD with (8.7-) can reach 4 K when scattering is neglected, leading to large uncertainties in the retrieval of droplet effective radius.     

The high-resolution, jet-cooled infrared spectrum of pentafluoroethane

The jet-cooled spectrum of pentafluoroethane (C₂HF₅) has been recorded between 1100 and 1325 cm⁻¹ at a resolution of 0.0022 cm⁻¹. A rotational temperature of approximately 10 K was achieved by expanding 50 Torr of C₂HF₅ in 500 Torr of helium. Transitions belonging to five different fundamental vibrations have been assigned and fit to a Watson Hamiltonian: the ν₃ band at 1309.880494(189) cm⁻¹, ν₄ at 1200.734645(67) cm⁻¹, ν₅ at 1142.78147(33) cm⁻¹, ν₁₃ at 1223.334098(115) cm⁻¹, and ν₁₄ at 1147.394185(163) cm⁻¹. The fit of the ν₄ band has an rms deviation of 0.000436 cm⁻¹ compared to the uncertainty in the experimental line position of 0.0002 cm⁻¹. Satisfactory fits were achieved for the other four bands (ν₃, ν₅, ν₁₃, ν₁₄) at this cold temperature, with most of the centrifugal distortion constants fixed at the ground state values. Joint fits with previous work were attempted for the ν₄ and ν₁₃, successfully in the former case and unsuccessfully in the latter.     

Polarised raman and infrared spectra and vibrational analysis forα-naphthylamine

The Raman spectrum of polycrystalline α-naphthylamine was recorded in the region 100–4000 cm⁻¹. Polarisation measurements were made in CS₂ and CHCl₃ solutions. The infrared spectrum was recorded in nujol mull in the region 200–4000 cm⁻¹. The resolution was better than 2 cm⁻¹ and the accuracy of the measurements was within ± 2 cm⁻¹ for all the spectra. Vibrational assignments have been proposed for the observed frequencies. Out of the 54 normal modes of vibrations, 51 modes could be observed experimentally.     

污染气体扫描成像红外被动遥测系统实时数据处理研究

使用红外被动遥测技术可实现污染气体的远程监控和预警. 该技术应用过程中, 获取背景辐射是进行定量解析的关键, 在已有的应用中, 多采用同条件测量法和上风口测量方法获取背景光谱和环境光谱, 但这些方法均需要提前或者同时测量无目标物的背景光谱, 难以在实际应用中满足快速响应的需求. 本文基于红外辐射传输模型分析, 通过研究在800–1200 cm^-1波段内的实测光谱中同时包含目标、背景和环境辐射的基本原理, 采用了一种不需要事先测量背景的目标特征的背景光谱实时提取算法, 通过将该方法应用于自主研制的污染气体扫描成像红外被动遥测系统, 以六氟化硫为示踪气体, 开展了遥测验证实验. 将获取的浓度数据与应用同条件测量法获取的数据进行了比较, 结果显示两者的相关系数平方值达到0.99, 表明该方法切实可行, 可有效提高系统的响应速度和适用范围. 关键词： 傅里叶变换红外光谱 被动遥测 实时光谱提取算法     

High-resolution infrared spectra of NCCN and NCCN

High-resolution spectra of ¹⁵N¹²C¹²C¹⁵N and ¹⁴N¹³C¹³C¹⁴N have been measured and analyzed from 200 to 3600 cm⁻¹. All the vibrational levels below 900 cm⁻¹ have been observed and characterized. The Fermi resonance between ν₂ and 2ν₄ has been studied and the resonance constant has been determined for several cases. Several Σ⁻ states have been directly observed for the first time for each isotopomer, the (0001111)0f, (0011111)0f, and (0002222)0f states. The pattern of the energy levels for clusters of l-type resonance coupled levels, such as 0001131,3, has been determined for cyanogen for the first time. Among other things this involved the determination of the vibrational l-type resonance constant, r₄₅. Many of the power series constants, α_i and x_ij, and higher order constants have been determined.     

Temperature dependence of infrared reflectance spectra of InN

To investigate both the optical and electrical properties of InN, we have measured the infrared reflectance spectra of InN thin films and performed the fitting analyses of the infrared spectra to obtain not only phonon frequencies and the damping factors but also the carrier concentration of InN. In this paper, we extend the aim of those analyses to the electron mobility and demonstrate that the temperature dependence of the electron mobility can be discussed using the infrared reflectance spectra analyses.