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For non-Kolmogorov turbulence, the anisoplanatiam error, the angular correlation function of Zernike polynomials, the residual phase structure function and the long-exposure OTF after low-order modes correction are analyzed.

分析了非科尔莫戈罗夫湍流情况下,自适应光学系统低阶模式校正时的非等晕误差、泽尼克系数角相关函数、残余相位结构函数以及长曝光光学传递函数,并定义了一个新变量模式校正因子,用来有效评价目标非等晕误差对低阶模式校正自适应光学系统补偿效果的影响。

In part one (chapter 2-3), two new methods and systems of optical parallel logic operation are studied. Triple-in Double-out shadow-casting logic operation system is proposed and realized for the first time. Based on this, optical full adder and 3-bit decoder array logic have been obtained. It is the first time to use coding pattern and different reading-writing model to realize BSO-PROM optical parallel logic operation where the time-order operation is avoided, so that the computing speed of optical parallel logic gate which uses this kind of spatial light modulator is increased, and it is successfully used in optical symbolic substitution .

在第一部分,对两种新的并行光学布尔逻辑运算方法及系统进行了研究:首次提出并实现了三输入、双输出铸影光学逻辑运算系统及其由此得到的光学全加器,并提出一种以此为基础的3-比特译码器阵列逻辑,首次利用图形编码和不同的读写模式实现了无时序操作的BSO-PROM光并行逻辑运算,大大提高了这种空间光调制器用作光并行逻辑门的运算速度,使之成功地用于光学符号代换之中。

The small hole of the optical inducer of the traditional second-generation optical mouse used for receiving the images faces downwards, and corresponding light sources (including photoelectric diode and laser diode), optic lens and photosensitive holes are arranged at the lower part of the mouse; therefore, moving the whole mouse is a relatively convenient method for generating displacement of the mouse pointer; oppositely, the small hole of the optical inducer used for receiving the images faces upwards and corresponding light sources, optical lens and photosensitive holes (7) are arranged at the upper part of the mouse; matters on the upper surface of the photosensitive hole (7) can be moved so as to lead the mouse pointer to generate the displacement, while the moving signal transmitted by a photoelectric conversion device must be reset so as to comply with the integrated mouse of the invention.

传统的第二代光电鼠标的光学感应器接收图象的小孔是向下的,对应的光源(包括光电二极管,激光二极管)、光学透镜和感光孔都是在鼠标下部分,这样要想鼠标指针产生位移较方便的方法就是移动整个鼠标;相反,光学感应器接受图象的小孔向上,对应的光源、光学透镜和感光孔(7)在鼠标上部分,要使鼠标指针产生位移就只需移动附在感光孔(7)上面的物质,但必须重新设置光电转换装置传出的移动信号,以符合本发明。

The results of Raman, SEM and EPMA tests show that the microstructure defects of the chalcogenide glasses play an important part in their second-order nonlinear optical properties. The glasses show large SNOP because of Sb2S3 microcrystal or the mental antimony in the glasses even before they were polarized. After the electrical/thermal polarized, GeSbS glasses show larger SNOP with the increase and growth of the microcrystal. The glasses show larger SNOP because of the existence of Sb2S3 microcrystal or the mental antimony in the glasses.

通过研究玻璃的拉曼光谱、扫描电镜和电子探针显微分析后发现,硫系玻璃内部的微结构缺陷对其二阶非线性光学性能有显著影响,玻璃体系内存在的Sb2S3微晶或金属锑颗粒能使硫系玻璃在未经极化处理前就具有较大的二阶非线性光学性能;经电场温度场极化处理后,随着微晶的增多和进一步长大,导致GeSbS玻璃具有更高的非线性光学性能;由于Sb2S3微晶或金属锑的存在,导致玻璃具有较高的二阶非线性光学性能。

The first is termed aero-optic and involved optical transmission through aberrating fluid layer whose thickness, L, is smaller than or comparable with the viewing aperture dimension, A, and the turbulence scales, A , are smaller than or the order as the layers thickness:The second category, atmospheric propagation, involved optical transmission through the aberrating medium over very long propagation distance compare with the viewing aperture size, and the turbulent scales of note are generally less than or the same order as the propagation distance:Depending on the atmospheric conditions, for ground-based observatories, wave-front sensor operating at 300HZ can adequately resolved both the important spatial scales and the temporal evolution of the atmospheric-turbulence-induced aberrating wave front over viewing aperture associated with relatively large telescope.

第一类问题光学畸变发生在&近场&较短的光路上,即流层厚度L,光束直径A,以及湍流尺度Λ三者之间存在关系式:ΛA≤L≤A第二类大气传输问题光学畸变则发生在较长的一段光路上,L,A,以及Λ满足: A<<Λ≤L对于地基情况下的大气光学传输,300Hz的波前传感器就能实时地测得光波前畸变包括时间、空间频率的相关信息,为我们的自适应光学系统的设计、制造以及进行相关的自适应校正都有着相当重要的指导意义。

By adjusting the positions and angles of the two DVD optical pick-up heads, the relative distance of the two laser spots can be equivalent to one quarter of the grating pitch. When the grating moves, the surface profile of the grating can be measure directly, in order to obtain the two quadrature sinusoidal signals. Then by counting the zero crossing of these two quadrature sinusoidal signals and calculating the interpolation value of these two quadrature sinusoidal signals, the moving direction and moving displacement value of the grating can be obtained.

采用两个光学读取头,且两个光学读取头共用同一分光镜与同一聚焦物镜,於搭配光路的设计,可使两个光学读取头之光束打入同一聚焦物镜,藉由调整两个DVD光学读取头的位置与角度,使聚焦物镜聚焦的两相近聚焦光点的距离相等於四分之ㄧ光栅尺间距,当光栅尺移动时,可直接量测光栅尺的表面轮廓变化,以获得一组正交的弦波讯号,继而利用讯号四分割与细分割处理,计算出光栅尺之移动方向与移动量。

Digital laser plane interferometer is used to measure the surface of optical components and the wavefront aberration of non-confocal optical system.

数字式激光平面干涉仪是用于测量光学元件面形和无焦光学系统波像差的光学仪器。

FIG. 6 shows an optical system that includes a series of collection optics and optical concentrators.

图6显示了包括一系列收集光学器件与光学集中器的光学系统。

In this paper, the switchable optical properties, effects on optical properties and the mechanism of the rare earth films were illustrated, the corresponding properties of the epitaxial rare ea...

本文介绍了稀土光学薄膜的可转换光学性能、影响光学特性的因素以及光学特性变化的机理,并对外延稀土膜和稀土合金膜的有关性能进行了介绍

The design principle of the laser receiver with wide FOV for the laser command guidance and laser-beam riding guidance is introduced. A mathematic model of receiving light field is presented. The formula for the viewing angle of the detecting optical system was derived according to the diffraction light field of the oblique incidence parallel light. Taking a detecting optical system with the collecting objective for example, the design characteristic that the receiving optical system needs not only an extra large relative aperture but also an unvignetting receiving performance is discussed on the premise of meeting the requirement of 1064nm WFOV laser receiver.

介绍激光指令制导和激光驾束制导的大视场激光接收机的设计原理,给出接收光场的数学模型,由斜入射平行光的衍射光场推出探测光学系统的视场角公式,根据1064nm大视场激光接收机技术要求,以聚光物镜型探测光学系统为例,探讨接收光学系统既须具备特大相对孔径,又须具备无晕接收性能的设计特点,采用窄带干涉滤光镜进行光学滤波降噪。

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