Constructions of pairs of orthogonal latin cubes

A pair of orthogonal latin cubes of order $q$ is equivalent to a maximum distance separable code with distance 3 or to an ${\mathit{OA}}_1\left(3,5,q\right)$ orthogonal array. We construct pairs of orthogonal latin cubes for sequences of previously unknown orders $q_i=16\left(18i?1\right)+4$ and $q_i^{\prime }=16\left(18i+5\right)+4$. The minimal new obtained parameters of orthogonal arrays are ${\mathit{OA}}_1\left(3,5,84\right)$.     

光机械式红外探测器中镜面弯曲对探测灵敏度的影响

光学读出式红外成像技术是近年来研究的热点，本文讨论了镜面弯曲对光学检测灵敏度的影响。由双材料微悬臂梁组成的非致冷焦平面阵列通过体刻蚀工艺加工而成，由于残余应力的影响，制成的焦平面阵列将会发生弯曲，应力导致的镜面弯曲将会降低光学探测灵敏度。本文通过傅立叶光学模拟了镜面弯曲对光学探测灵敏度的影响，并通过实验验证了该模型。实验和模拟结果表明，在镜面曲率为0．1mm-1时，光学探测灵敏度将会降低到理想情况的40％。最后我们用这个模型评价了通过表面修饰来提高光学性能的效果。     

Integrable models associated with Myers–Perry–AdS–dS black hole in diverse dimensions

Myers–Perry–AdS–dS black hole exhibits $SO(2,1)\times U\left(n\right)$ symmetry in the near horizon limit in the special case that all rotation parameters are equal. We consider a massive relativistic particle propagating on such a background and reduce it to superintegrable angular mechanics with $U\left(n\right)$ symmetry. A complete set of functionally independent $u\left(n\right)$ generators realized in the model is given.     

基于MEMS线阵的便携式中红外水中油浓度速测仪

针对传统光谱测油仪存在的环境适应能力弱、分析速度慢、测量重复性差等问题,研制了一种便携式中红外水中油浓度速测仪。其核心光路采用典型的非对称折叠式M型Czerny-Turner光学结构,有效缩小仪器体积;使用周期性转动的斩光器调制红外光源,并对斩光器转速进行数字PID控制,调制精度达到±0.5%;采用固定光栅作为分光元件,无需光栅扫描装置且不存在转动误差;利用新型MEMS红外线传感器阵列探测调制后的光谱信号,显著提高光谱采集速度。光学仿真及实验结果表明仪器光谱范围为2 800~3 200cm-1,光谱分辨率达到6cm-1(@3 130cm-1),信噪比达到5 200∶1,谱图采集速度为13ms·幅-1,吸光度标准偏差优于3×10-3,满足了水中油测定国家标准要求。与已有红外光谱测油仪相比,该仪器小型便携,分析速度快,测量精度高,抗震防潮性能好,特别适用于环境监测部门对水中油浓度的现场实时测量,因此在水质监测领域具有广阔的应用前景。     

Uncertainty of array-based measurement of radiated and absorbed sound intensity

Patch near-field acoustic holography (NAH) coupled with an array of sound intensity probes allows separating the sound field incident on a surface from the one radiated by the surface itself. Although the measurement principle has been successfully used to separate the noise source contribution from disturbing sources and/or noise reflections, the method accuracy has not been investigated in the literature. We describe the results of experiments meant to evaluate the uncertainty in the identification of noise radiated by vibrating panels with different absorption characteristics in presence of an incident acoustic radiation using the statistically optimized near-field acoustic holography. Measurement errors were evaluated through tests performed in controlled acoustic conditions. Results evidenced that the measurement uncertainty depends on the accuracy of the microphone array positioning and on the incident sound field. These conclusions were in agreement with the results obtained by simulations in the phase of instrument optimization.     

Automatic 3D scanning surface generation for microphone array acoustic imaging

This work presents a new technique for automatically generating the 3D scanning surface for acoustic imaging using microphone arrays. Acoustic images, or maps, of sound coming from spatially distributed sources, may be generated from microphone array data using algorithms such as beamforming. Traditional 2D acoustic maps can contain errors in the near-field if the object being imaged has a 3D shape. It has been shown that using the 3D surface geometry of an object as a scanning surface for beamforming can provide more accurate results. The methods used previously to generate this 3D scanning surface have either required existing CAD (Computer-Aided Design) models of the object being acoustically imaged or have required separate equipment which is generally bulky and expensive. The new method uses one or more cameras in the array, a data projector, and structured light code to automatically generate the 3D scanning surface. This has the advantage that it is inexpensive, can be incorporated as an add-onto existing microphone arrays, has short scan time, and is capable of being extended to imaging dynamic scenes. This technique is tested using beamforming and CLEAN-SC (CLEAN based on spatial Source Coherence) algorithms for a spherical array and an Underbrink multi-arm spiral array. For sound sources located about 1.2 m from the array, the mean position errors obtained are 6 mm. This is a quarter of the diameter of the mini-speakers being used as a sound sources.     

Automatic defect recognition of TFT array process using gray level co-occurrence matrix

This study proposed an automatic optical inspection (AOI) system for detection of thin-film transistor (TFT) array defects. gray level co-occurrence matrix (GLCM) and MATLAB regionprops function were used to calculate 53 TFT array defect features, which were inputted into the neural network to train the defect classifier. The images to be inspected were compared with a standard image first, in order to judge whether the TFT array samples have defects. For defective images of a TFT array, the proposed defect classifier can successfully recognize five kinds of defects in the process. According to the experimental results, the defect recognition rate of proposed system is verified to be 83.3%, which can replace manual inspection and reduce the risks of false inspections due to long duration manual work. Moreover, the proposed AOI system can improve testing efficiency and reduce manufacturing costs.     

Optical bistability in a single-bus InGaAs micro-ring resonator array

In this paper, we investigate the optical bistability induced by optical nonlinearity in a compact parallel array of micro-ring resonators with radius of 5 μm. Due to the nature of perfect light confinement in this structure, resonance and accumulation process in a ring resonator and optical nonlinear effects, are observable even at small optical power (a few milliwatts). Different optical applications such as all-optical switching, optical memory devices, logic gates and modulators are possible, due to optical bistability in a ring resonator. Using alternative semiconductor compounds, instead of silicon that have weak nonlinear optical properties, we improve the performance of ring-resonator based devices. Here we use a polymer cladding layer with negative thermo-optic coefficient. Using this structure we can eliminate the temperature created nonlinearity which is a very slow process. Therefore, the switching speed increases from a few MHz to several tens of GHz. By plotting the transfer function of the resonator, a hysteresis loop is observed in a few milliwatts. Although, using a ring resonator array the bandwidth reduces, however, the width of the hysteresis loop and resolution between both steady state increases.     

Aerodynamic heating of the dome on imaging quality degradation of conformal optical systems

The aerodynamic flow field surrounding the conformal dome was calculated. The thermal response of the aerodynamically heated conformal dome was analyzed. Gradient refractive index method was used to rebuild the non-uniform refractive index field of the conformal dome. Zernike polynomial fitting method was employed to establish the deformed surfaces of the conformal dome. Zernike aberration theory and modulation transfer function were adopted to evaluate the imaging quality of the conformal optical system. The results show that the aerodynamic heating of the dome severely affects the imaging quality of the conformal optical system.     

Optimization of multilayer radial beam array in weak turbulent atmosphere

The on-axis scintillation index of multilayer radial beam array with incoherent combination propagating through weak turbulence is studied. The results indicate that for large beam number, the scintillation index can be reduced by adjusting beams on different concentric circles. Further studies manifest that optimum radii arrangement of the three-layer array can be adopted to get the smallest scintillation index.