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光干涉技术与天文望远镜技术的结合是提高天文观测分辨率的一种有效方法.采用望远镜阵代替单个大口径望远镜来集光观测,利用最大基线的概念来等效传统光学望远镜的最大口径,很大程度上解决了单个望远镜集光能力不足、角分辨率不高的问题.然而对于光干涉来说,在应用中,只有满足:两束光的相位差δ必须相对稳定、存在相互平行的振动分量、频率相同、两光波在相遇点所产生振动的振幅相差不悬殊和两光波在相遇点的光程差(OPD)应在相干长度之内等这些条件时才能部分相干.光学综合孔径(OAS)望远镜产生干涉条纹的前提条件是子望远镜之间必须两两相干.推导了双光束光干涉的要求,并从双光束干涉的平行性和光程差的要求出发,研究并得出光学综合孔径望远镜子望远镜的平行性和光程差的要求.结合双光束干涉的恒星光干涉仪的光束平行性和光程差的调整方案,研究并得到了光学综合孔径望远镜子望远镜的平行性和光程差调整的光学方案,并讨论了该系统的改进措施. 相似文献
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根据激光激发声表面波的热弹运动方程及热传导方程, 采取有限元技术对方程进行求解, 得到声表面波传播波形图. 当声表面波经过近表面缺陷时, 声表面波与近表面缺陷之间产生一种振荡效应, 通过近表面缺陷的振荡波形幅值存在一个逐渐增加后又逐渐减小的过程. 当声表面波经过不同深度的近表面缺陷时, 振荡信号中心频率存在一定的变化规律. 数值仿真结果表明: 当近表面缺陷深度从0.1 mm到0.5 mm变化时, 振荡效应产生的振荡信号中心频率从0.4 MHz到0.76 MHz变化, 振荡信号中心频率与近表面缺陷深度呈近似线性关系, 这为近表面缺陷的定量检测提供了一种理论基础. 相似文献
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A driver-pickup probe possesses better sensitivity and flexibility due to individual optimization of a coil. It is frequently observed in an eddy current (EC) array probe. In this work, a tilted non-coaxial driver-pickup probe above a multilayered conducting plate is analytically modeled with spatial transformation for eddy current nondestructive evaluation. Basically, the core of the formulation is to obtain the projection of magnetic vector potential (MVP) from the driver coil onto the vector along the tilted pickup coil, which is divided into two key steps. The first step is to make a projection of MVP along the pickup coil onto a horizontal plane, and the second one is to build the relationship between the projected MVP and the MVP along the driver coil. Afterwards, an analytical model for the case of a layered plate is established with the reflection and transmission theory of electromagnetic fields. The calculated values from the resulting model indicate good agreement with those from the finite element model (FEM) and experiments, which validates the developed analytical model. 相似文献
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