大口径望远镜结构热分析

为了评估温度对望远镜的影响,针对某地基光电望远镜,建立了包括光学组件,跟踪架结构以及电控设备等在内的有限元热模型.在传导、对流、辐射以及热流等不同热环境下进行热分析,计算了望远镜光机结构的时间和空间温度分布.根据温度分布进行了热-弹性分析,得出了望远镜结构的热变形.分析表明:温度变化对望远镜跟踪架以及主光学系统的影响很大,对主次镜造成的相对位移达到毫米级,必须进行严格控制.最后从防护圆顶、跟踪架以及主镜等方面入手给出了热控设计方案.     

球面反射镜镜面热变形的数值分析

对热环境下球面反射镜的镜面热变形进行了数值模拟分析,应用光机热(TSO)集成分析方法,在对光机结构进行有限元分析的基础上,以Zernike多项式为接口工具拟合镜面变形,评估了环境载荷对光机系统光学性能的影响,最后还分析了硅橡胶层对光机系统结构应变能的吸收效用。     

空间太阳望远镜主镜精密温度控制方案介绍

通过光-机-热集成分析，用简单可靠的热控方法，对空间太阳望远镜直径为1m的主镜进行了热设计：采用周边绝热、将热量从正面传导到背面，再设计装有控温回路和热管的集热板，以及与卫星平台辐射器冷板连接散热，保证了主镜的温度水平和稳定性；在主镜压紧结构前设置挡光板，减少压紧结构引起的主镜温度不均匀．结果表明，利用智能型高准确度控温仪和加热回路的优化设计实现主构架均匀性热设计，采用高传热性能热管排散准直镜热反射面极高热流密度，可以消除主镜周围热环境对主镜温度影响的结论．     

700mm光学望远镜结构设计与分析北大核心CSCD

针对某700mm口径高分辨率光学成像望远镜,提出了一种结构设计方案。对主镜支撑采用9点whiffle-tree底支撑加球头芯轴侧支撑的结构方案,保证主镜具有高面形精度;望远镜镜筒采用碳纤维桁架式结构,既满足望远镜整体重量较轻,又可以保证系统刚度;建立了望远镜有限元模型,分析主镜支撑面形、主次镜相对偏心及系统整体模态特性,其中主镜支撑面形精度可达到λ/40,主、次偏心为0.015mm(水平状态)、0.008mm(竖直状态);使用激光干涉仪及平行光管对望远镜光学指标进行定量检测,光学系统RMS可达到λ/14,鉴别率板检测望远镜分辨率可达到46lp/mm,均接近光学极限水平。为同类望远镜的结构设计提供一定参考价值。     

激光器光学系统光机热集成分析方法

论述了光机热集成分析方法原理及接口多项式,并将其应用于某激光器光学系统进行光机热集成分析。该分析方法首先对光学系统进行热分析、结构有限元分析计算,获取激光辐照下光学元件表面的结构变形;其次,对有限元计算的光学元件变形结果数据进行Zernike面形拟合处理;最后将变形后的光学表面导入到通用光学设计分析软件,分析激光器光学系统变形后产生的各类光学像差。结果表明:利用集成分析方法能够分析光学元件产生热变形对激光系统成像质量造成的影响,为光学系统设计提供参考。     

700mm光学望远镜结构设计与分析

针对某700mm口径高分辨率光学成像望远镜,提出了一种结构设计方案。对主镜支撑采用9点whiffle-tree底支撑加球头芯轴侧支撑的结构方案,保证主镜具有高面形精度;望远镜镜筒采用碳纤维桁架式结构,既满足望远镜整体重量较轻,又可以保证系统刚度;建立了望远镜有限元模型,分析主镜支撑面形、主次镜相对偏心及系统整体模态特性,其中主镜支撑面形精度可达到λ/40,主、次偏心为0.015mm(水平状态)、0.008mm(竖直状态);使用激光干涉仪及平行光管对望远镜光学指标进行定量检测,光学系统RMS可达到λ/14,鉴别率板检测望远镜分辨率可达到46lp/mm,均接近光学极限水平。为同类望远镜的结构设计提供一定参考价值。     

基于低体分SiC/Al主镜框的空间相机主支撑结构热特性分析与验证

基于微小卫星平台对高分辨相机的重量约束,以高分微纳卫星CX6-02数字超分辨相机研制为例,提出一种基于低体分SiC/Al主镜框的空间相机主支撑的结构形式,并开展主镜框一体拓扑优化设计分析和试验验证。Zernike多项式计算及光机热集成仿真结果验证了低体分SiC/Al主镜框作为空间相机主支撑结构的有效性。热光试验数据及在轨成像结果表明,兼具主支撑功能的低体分SiC/Al主镜框的空间相机试验数据与仿真数据基本吻合,且性能稳定,可为未来采用低体分SiC/Al主镜框作为主支撑的航天相机轻量化设计和研制提供理论与技术参考。     

月基望远镜热设计及热分析

为了利用月球观测地球等离子体层的优势,开展了月基望远镜的研究,并对其进行了热设计和热分析.分析了月基望远镜所处的空间环境.对望远镜各个部分进行了热设计;采用被动热控措施控制望远镜的温度水平,降低空间环境的影响;采用热疏导的方式对探测器进行散热.根据月基望远镜的空间环境、结构特点,以及采取的热控措施,在I-DEAS/TM...     

大口径折反射式光学系统的光机结合分析

大口径折反射式光学系统在空间遥感仪器中广泛应用,反射镜的支撑结构直接关系镜面面形变化从而影响光学遥感器的成像质量.建立了光学系统的光机结合分析方法,使得在设计阶段就能评测光学元件支撑结构是否满足要求,得到支撑结构对成像质量的影响的直观结果.这一方法也可用于光学系统的光机热结合分析.     

空间光学遥感器光机热集成分析技术综述

介绍了光机热集成分析技术的基本原理及其关键技术———数据传输技术的研究现状和最新进展。通过接口工具Zernike多项式进行数据传输的基本过程是:数据处理,即将有限元分析中得到的变形结果转换成基于弧矢坐标系或基于波前坐标系的数据形式;多项式拟合,即利用最小二乘法或Gram_Schmidt正交化方法进行拟合。提出了自动数据转换接口程序,它能够简化光机热集成分析的过程,可提高工作效率。     

Speckle characteristics of a broad-area VCSEL in the incoherent emission regime

We present a technique to reduce the speckle contrast of a NIR broad-area VCSEL based on the spatially incoherent emission regime that can be obtained when using the proper driving conditions. We evaluate the efficiency of this technique to reduce the speckle contrast by comparing it with the speckle characteristics in multimode emission under cw operation. Depending on the illumination setup, the incoherent emission regime can lead to a strongly reduced speckle contrast down to 1.3%. This is in agreement with estimates of the expected speckle contrast reduction when three contrast reducing effects are taken into account. These low contrast values make the investigated sources attractive for several applications that suffer from speckle noise.     

XYZ particles at Belle

In this paper, I review recent progress in the study of the XYZ particles at Belle. I only focus on studies with charmonium and one or more light mesons in the final states. This covers the X(3872), X(3915),Y(4140), X(4350), and the charged Z states.     

Beyond the LAN: Ethernet’s Evolution into the Public Network

This article details the evolution of Ethernet into Gigabit Ethernet and how this LAN-based technology has undergone major transformations over time. From its data rates and distances to supported media and functionality, Ethernet has greatly improved, enabling it to surmount many of its former limitations and in so doing to expand beyond the LAN into the MAN and now even the WAN. In this article, Pioneer Consulting explores the evolution further by focusing on some of the major technological directions in the Ethernet equipment industry.     

带有碳杂质的钨中氢稳定性的第一性原理研究

应用第一性原理计算方法研究了碳(C)原子对钨(W)中氢(H)原子稳定性的影响. 本征W中, 当C-H间距离为～2.5 Å时, H的溶解能出现最低值, 此时为H最稳定的位置. W中存在空位时, 由于C的影响, H占据的最佳电子密度面值为0.10 Å^-3. 研究发现, W中单空位最多能容纳10个H原子, 且不能形成H分子, 不同于没有C存在的情况, 表明C对W中H稳定性存在很大影响. 此外, 当两个C原子存在于空位中时, H占据的最佳电子密度面值变为0.13 Å^-3.     

Optical transmission through an interface between subwavelength slits

This paper studies optical transmission through an interface between two slits with different widths in a sheet composed of an ideal conductor. Such a structure is of potential use in fabricating optical diode and may be the simplest one compared to other designs. Our calculations show that there is a critical wavelength. When the light wavelength is below the critical wavelength, the transmissivity is unidirectional. The expression of the stable transmissivity as a function of the ratio of the widths of the two slits was obtained analytically. Particularly, at the critical wavelength, the transmissivities are zero. This phenomenon has great potential for application in the manufacture of wavelength blockers.     

Effect of swift heavy ion irradiation on photoluminescence properties of ZnO/PMMA nanocomposite films

We report a study on the SHI induced modifications on structural and optical properties of ZnO/PMMA nanocomposite films. The ZnO nanoparticles were synthesized by the chemical route using 2-mercaptoethanol as a capping agent. The structure of ZnO nanoparticles was confirmed by XRD, SEM and TEM. These ZnO nanoparticles were dispersed in the PMMA matrix to form ZnO/PMMA nanocomposite films by the solution cast method. These ZnO/PMMA nanocomposite films were then irradiated by swift heavy ion irradiation (Ni⁸⁺ ion beam, 100 MeV) at a fluence of 1×10¹¹ ions/cm². The nanocomposite films were then characterized by XRD, UV-vis absorption spectroscopy and photoluminescence spectroscopy. As revealed from the absorption spectra, absorption edge is not changed by the irradiation but the optical absorption is increased. Enhanced green luminescence at about 527 nm and a less intense blue emission peak around 460 nm were observed after irradiation with respect to the pristine ZnO/PMMA nanocomposite film.     

Grain boundary potential and charge density at grain boundaries of chemically prepared thin silver sulfide films

The grain boundary potential and interface state charge density at the grain boundaries of silver sulfide (Ag₂S) thin films prepared by chemical conversion of cadmium sulfide (CdS) films have been determined from the dc resistance of the material and are found to be sensitive to annealing. A reduction in the grain boundary potential and the grain boundary charge density of the film has been noticed when the source CdS film is annealed at different temperatures prior to chemical conversion. The variation in the grain boundary charge density of the grown Ag₂S film with source annealing temperature has been found to be similar to that of thin cadmium sulfide film, reported earlier. An additional low temperature heat treatment of the sample results in an enhancement in the charge density at the grain boundaries. The change in the silver vacancy and/or oxygen and sulfur content of the films as revealed from the energy dispersive spectra of the films suggests possible role of film composition on the grain boundary charge density.     

Reflections from polished single mode fiber ends

Abstract

The performance of a wavelength division multiplexing (WDM) system with optical cross-connects (OXCs) and in the presence of polarization and nonlinear effects was analyzed. We determined the effect of PMD and PDL; nonlinearity such as XPM, SPM, and FWM; and CD on the system performance. We found that the system outage probability is highest at DGD threshold for the respective maximum eye closure (EC). We showed that the allowable DGD depends on the time slot for one bit T, which is the inverse of the network bit rate. Wider T is more immune to large PMD with the EC still maintained at the same level since DGD/T is unchanged. Our analysis also indicated that as DGD increases, BER increases. The BER also increases with increase in PDL and further increases with the presence of XPM, SPM, FWM, and CD.     

The Effects of Polarization and Non-Linearity on the Performance of WDM System with Optical Cross-Connects

The performance of a wavelength division multiplexing (WDM) system with optical cross-connects (OXCs) and in the presence of polarization and nonlinear effects was analyzed. We determined the effect of PMD and PDL; nonlinearity such as XPM, SPM, and FWM; and CD on the system performance. We found that the system outage probability is highest at DGD threshold for the respective maximum eye closure (EC). We showed that the allowable DGD depends on the time slot for one bit T, which is the inverse of the network bit rate. Wider T is more immune to large PMD with the EC still maintained at the same level since DGD/T is unchanged. Our analysis also indicated that as DGD increases, BER increases. The BER also increases with increase in PDL and further increases with the presence of XPM, SPM, FWM, and CD.     

化学发光法测定巯嘌呤的含量

在流动注射系统中,利用巯嘌呤在碱性Luminol-K₃Fe(CN)₆化学发光体系中发光信号强的特点,建立了一种测定巯嘌呤的新方法。在优化条件下,方法的线性范围是1.02×10-7～1.02×10-9mol·L-1, 回归方程是Y=36.315c+140.72(Y是相对发光强度,c是巯嘌呤浓度与10-8 mol·L-1的乘积), 相关系数是0.998 2,检出限(S/N=3)是6.33×10-10mol·L-1,RSD为3.54%（c_i=2.0×10-9mol·L-1, n=12）。该法用于合成样品的测定,简便、灵敏、快速,结果令人满意。文章简要地探讨了巯嘌呤在碱性Luminol-K₃Fe(CN)₆化学发光体系中的化学发光机理：在反应过程中,产生大量的过氧自由基和羟基自由基,自由基与鲁米诺反应,形成激发态的鲁米诺分子,鲁米诺分子由激发态回到基态产生化学发光现象。