Q355B钢板表面星裂缺陷的研究与控制

为解决Q355B钢板材表面星状裂纹问题,采用热力学计算、金相分析、修磨、抛丸、酸洗、低倍分析、扫描电镜及能谱分析等方式对表面星状裂纹产生的原因进行了系统研究。研究结果认为,Q355B钢板表面裂纹处未发现脱碳层、氧化原点、第二相粒子、夹杂物和铜元素,说明裂纹不是源于铸坯缺陷。对铸坯分别进行热装和冷装发现冷装铸坯生产的钢板裂纹比例较低,结合两相区分析表明星状裂纹产生主要与铸坯在Ar₃～Ar₁两相区767~677 ℃内进行热装有关。通过自主设计喷淋装置,控制铸坯喷淋前温度在790 ℃以上,在入加热炉前对铸坯进行喷淋冷却至510 ℃以下从而使入炉温度低于635 ℃,Q355B钢热装星裂由攻关前的0.99%降至2021年攻关后的0.07%。     

通信电源集中监控系统网络主备用路由的实现

通过对云南玉溪电信局监控工程实现过程中的网络及双机备份中的一些关键问题的描叙,比较详细的讲解其实现过程,介绍该局网络设计原则、方案,路由器的设置,双机备份等,对其他地区监控网络的实现有一定的参考价值。     

基于IEC 61850-9-2的变电站通信网络仿真

以太网的通信能力是支撑基于IEC 61850标准的数字化变电站正常运行的重要因素。文中围绕全站统一环形网和星形网,采用仿真软件OPNET对变电站的各种典型数据流建模,采样值采用IEC 61850-9-2协议,考虑星形和环形2种网络结构、网络带宽、过程层网络传输采样值、环网断线故障、文件传输对采样值与跳闸报文的影响等因素,制定了多套仿真实验方案,针对一个实际的中型变电站进行了对比仿真实验与分析,为数字化变电站系统的构建提供一定的参考。     

利用视频判读进行白天测星方法的研究

针对测量船光测设备的电视测量系统白天测星能力的不足,提出了一种新型的白天测星方法.该方法将光测设备测星的视频图像实时记录于计算机的硬盘,并根据判读存储于硬盘中星体图像的脱靶量,完成测量船的航向修正和动态标校.应用这种方法,可以提高光测设备白天测星的能力及测量船的总体测量精度,是一种准实时的、切实可行的白天测星方法.     

Synthesis of amphiphilic heteroarm star‐shaped polymer via free radical polymerization using polyfunctional chain transfer agent and its self‐assembly behavior

Amphiphilic heteroarm star‐shaped polymers have important theoretical and practical significance. In this work, amphiphilic heteroarm star‐shaped polymer was synthesized by the use of polyfunctional chain transfer agent via sequential free radical polymerization in two steps. First, conventional free radical polymerization of methyl methacrylate (MMA) initiated by 2,2′‐azobis (isobutyronitrile) (AIBN) was carried out in the presence of polyfunctional chain transfer agent, pentaerythritol‐tertrakis (3‐mercaptopropinate) (PETMP). At appropriate monomer conversion, about two‐arm s‐PMMA having two residual thiol groups at the chain center was obtained. Second, the s‐PMMA obtained above was used as macro‐chain‐transfer agent for free radical polymerization of acrylic acid (AA). The heteroarm star‐shaped polymer with the hydrophobic PMMA segment and the hydrophilic PAA segment was obtained. The successful synthesis of heteroarm star‐shaped polymers, (PMMA)₂(AA)₂, was confirmed by ¹H‐NMR and its self‐assembly behavior in different solvents. © 2012 Wiley Periodicals, Inc. J. Appl. Polym. Sci., 2013     

基于最大能量法的白天红外星目标检测

受多种因素的影响,白天获得的红外星图像的信噪比低,且背景通常不均匀。采用一般的滤波方法无法提取出恒星目标,目前常用的形态学方法对于星图像的处理也不甚理想。首先分析背景特性,采用多帧叠加的方法消弱随机噪声,增大信噪比;然后设定阈值,对叠加后的星图进行背景消除,得到只含有目标及噪声的图像;然后用与恒星大小相近的模板按一定的规则对星图进行滤波,分割出目标。实验证明,该方法能较好地分离出恒星目标。     

基于SUSAN算子的白天红外星目标检测

受多种因素的影响,白天获得的红外星图像信噪比低,且背景通常是不均匀的,为红外星目标的提取造成了极大的困难。通过理论计算,实际白天拍摄的近红外星图信噪比极低,使用一般的滤波方法无法提取出恒星目标,目前常用的形态学方法对于星图像的处理也不甚理想。首先分析背景特性,采用多帧叠加的方法削弱随机噪声,增大信噪比;然后设定阈值对叠加后的星图进行背景消除,得到只含有目标及噪声的图像;最后基于图像的特性,使用改进的SUSAN算子对星图进行目标检测,进而分割出目标,实验证明,与传统方法相比,该方法可较好地分离出恒星目标。     

Synthesis of mid-dicarboxy polystyrene by ATRP and formation of ionic-bonded supramolecules

Dimethyl 4,6-bis(bromomethyl) isophthalate was synthesized by bromomethylation, oxidation, esterification and bromination of 1,3-dimethylbenzene. This was used to initiate the atom transfer radical polymerization of styrene successfully. Results showed that the process had some of the good characteristics of controlled/living free radical polymerization. The molecular weight of the obtained polymer increased linearly with monomer conversion, its molecular weight distribution was very narrow, and a linear relationship between ln([M]₀/[M]) and polymerization time was found. A well-defined novel structural polystyrene containing two ester groups in the mid-main chain was prepared with controlled molecular weight and narrow polydispersity. The structure of the polymer was confirmed by ¹H-NMR spectra. After being hydrolyzed, dicarboxy polystyrene was obtained and used to form ionic-bonded supramolecules with 1-dodecanamine as a model of the star-shaped supramolecules. The supramolecules formed were characterized by Fourier transform infrared (FTIR) spectrum. Translated from Acta Polymerica Sinica, 2006, (4): 597–602 [译自: 高分子学报]     

星载自适应光学系统的双导星信标理论研究

星载相机的波前畸变主要来源于两个部分:由于温度场、重力场变化引起的相机光学系统自畸变;由于大气湍流引起的波前误差。为获得高分辨率的图像,需要校正波前误差。提出一种对星载光学系统波前畸变进行有效探测的技术。星载激光器分时产生钠导星和瑞利导星,前者用于校正自畸变,后者用于校正大气湍流造成的波面像差。针对该方法对激光能量的要求,建立了双导星信标系统的数值模型,并进行仿真。结果表明,该方法对激光器的要求,在目前是可以实现的。该方法可以用于空间相机光学系统的波面畸变探测,从而为星载自适应光学的进一步研究提供依据。     

星形波长路由光网络中的波长分配

文章主要研究了网络中心与其它节点之间由两条光纤成双向传输链路的情况，给出了均匀和顾机两种业务条件下网络中所需波长数的理论下限范围，利用图着色理论构造启发式算法解决了星形网络中的波长分配问题，最后通过实际波长分配验证了算法的有效性。