基于Windows NT平台的光盘阵列的设计

光盘阵列在多媒体系统等巨量存储领域具有广泛的应用前景。提出设计基于ＷｉｎｄｏｗｓＮＴ平台的光盘阵列的方法。此方法采用分层结构,将整个光盘阵列的实现分为文件系统驱动程序、阵列过滤器驱动程序、光盘驱动器分类驱动程序、ＳＣＳＩ端口驱动程序和ＳＣＳＩ小端口驱动程序五个层次,实现了模块化设计。利用此方法设计出的ＴＳ Ｏ１型光盘阵列,操作简便,实际达到的数据传输率与理论值接近     

一种新型磁光盘驱动器光学头光学系统

本文叙述了一种新型磁光盘驱动器光学头的光学系统,并从理论上阐明了磁光信息读取的基本原理.该系统改善了光学系统性能,减少了系统噪声,提高了光能利用率,并用于5(1/4)时的磁光盘驱动器开发研究,获得读取信息的信噪比优于50dB的结果.     

基于傅里叶叠层显微成像的LED阵列位置校正方法

傅里叶叠层显微成像(FPM)利用LED阵列角度变化的光照来克服低数值孔径物镜的分辨率限制。在传统的FPM系统中,LED阵列的位置误差将会给图像重建过程带来严重影响。因此准确校正LED阵列的位置对于提高重建图像质量至关重要。为了解决这一问题,提出一种基于遗传退火优化算法的位置校正方法。首先分析LED阵列、样品及物镜数值孔径的相对位置给入射波矢量带来的影响;接着采用遗传退火优化算法对LED阵列的误差位置估计全局误差参数;最后在重建过程中利用全局误差参数快速、准确地对LED阵列位置进行校正。仿真结果和实验结果表明,所提方法能显著提高重建图像的质量。     

基于果蝇优化算法的三维LED光源阵列优化设计

为了在现有研究基础上使LED阵列光源的照度均匀度进一步提高,提出了一种新的LED阵列优化途径。根据Ivan Moreno提出的二维LED阵列优化设计方法,本文设计了以两种不同方式分布排列的二维优化LED阵列。利用果蝇优化算法对二维优化LED阵列芯片的位置参数进行进一步优化,实现LED阵列位置参数的三维空间的优化设计,使LED阵列光源的照度均匀度更优。使用Trace Pro对LED阵列的三维优化结果进行验证。研究结果表明,基于果蝇优化算法,经三维优化后的圆形LED阵列的照度均匀度可达到96.0%,相较于二维优化后的圆形LED阵列提高了25.3%;经三维优化后的正方形LED阵列的照度均匀度可达到97.4%,相较于二维优化后的正方形LED阵列提高了7.7%。该优化方法被证明是可行的,相较于传统优化方法,该方法节约了大量人力物力成本。     

利用协方差矩阵拟合的阵列孔径扩展方法

提出了一种协方差矩阵拟合的阵列孔径扩展方法来提高小孔径均匀直线阵的分辨力。该方法分析了具有不同阵元个数的阵列采集信号协方差矩阵之间的关系,并根据该关系构建阵列扩展的优化算法,利用小孔径实际阵列协方差矩阵拟合得到大孔径虚拟阵列的协方差矩阵。仿真分析与湖试数据处理结果表明,将拟合协方差矩阵用于现有方位估计方法中能够降低波束宽度,提高分辨力,并且随着虚拟阵元个数增加,目标分辨概率同步提高。当阵列孔径较小或环境信噪比较低时,本文方法可用于提高方位估计性能。     

包米勒PLC在蛇形造波机设计中的关键技术研究

蛇形造波机是一种在海洋工程研究领域中,用于模拟大范围海浪的阵列式实验设备。为了进一步提高大范围海浪模拟的精度,蛇形造波机同步控制性能的提高具有十分重要的意义。针对包米勒PLC的运动控制技术进行研究,提出了基于其具有多级主从式结构的蛇形造波机同步运动控制系统,实现所有造波单元的严格同步控制。针对上位机和各PLC间数据量大、传输速度慢的问题,采用无损数据压缩和线性数据插值降低数据量,并应用多线程以太网通讯方式提高数据传输速率。另外由于该系统机械结构惯量大和总体负载大的特点,存在启停过程中电机过流问题。为此提出了一种基于余弦函数的拟合算法优化造波机启动和停止过程。在各个性能指标的验证实验中,该系统运行稳定,数据传输速度快,同步性能高,完全满足大范围海浪模拟要求。     

任意几何形状和阵元指向性的传感器阵列优化波束形成方法

针对常规波束运用到实际传感器阵列时旁瓣较高这一缺点,提出了适用于任意几何形状和阵元指向性的传感器阵列的两种旁瓣约束优化波束形成方法。一种是主瓣宽度约束条件下的最低旁瓣波束形成,另一种是在所能允许的最高旁瓣约束条件下的高增益波束形成。通过对加权向量范数进行约束,提高波束形成的稳健性。这两种优化波束形成问题都可以写成二阶锥(Second-OrderCone)约束优化的形式,然后利用已有的内点方法(Interior-PointMethods)求出其数值解。计算机仿真和湖上实验数据处理结果表明,该低旁瓣波束形成方法相比于常规波束和其它基于自适应波束形成的旁瓣控制方法,在同等主瓣宽度的情况下可以获得更低的旁瓣级;该高增益波束形成方法在同等旁瓣级约束条件下可以获得更高的阵增益,而且旁瓣级能够满足设定要求。     

电磁超构表面与天线结构一体化的低RCS阵列

提出一种电磁超构表面与天线一体化设计以实现低散射阵列的新方法.该方法利用传输线将超构表面部分单元串联,并采用同轴馈电激励,以此得到新型天线阵列,该阵列的辐射性能和传统阵列几乎相同;当外来雷达波照射该阵列时,利用超构表面和其周围天线结构散射场的差异,将能量在空间重新分配,从而实现天线工作频带内的雷达散射截面(radar cross section,RCS)减缩.基于该方法,以2 × 1阵列为例,构建了天线模型,数值分析了其性能,验证了该阵列的良好辐射和低RCS特征,并详细阐述了天线的工作机理,进一步的分析还揭示了超构表面结构对天线辐射和散射性能的影响规律.遵循该规律,可以灵活设计满足需求的天线阵列.该方法不仅简单易行、集成度高,还可以拓展至更大规模的阵列天线设计.     

基于哈特曼波前传感器的非制冷红外成像光学读出系统

提出了一种新的基于哈特曼波前传感器(SHWS)的光学读出系统.该系统利用SHWS探测焦平面阵列(FPA)单元在受热前后反射波前斜率的变化量重构被探测物体的红外辐射图像.在理论上详细讨论其成像性能后,实验获得了单元尺寸为60 μm×60 μm,阵列大小为34 pixel×38 pixel的高温物体红外图像,其噪声等效温度差(NETD)约为3.8 K.优化系统参数设计,可以提高哈特曼波前传感器对到达角的测量精度进而获得更小的噪声等效温度差.     

多阶光盘系统中帧同步信号的自适应检测

多阶光存储是提高光盘存储容量和数据传输率的重要途径。帧同步信号在多阶光盘的重放系统中起着很重要的作用。分析了实际多阶存储系统中帧同步信号的特征和信号检测的特点,提出了一种自适应检测帧同步码的方法。实验结果表明,该方法的精度可以满足系统的需求。     

Spot Shape on Super-Resolution Optical Disks with a Photon-Mode Mask Layer

The spot shape on super-resolution optical disks with a photon-mode mask layer was theoretically analyzed. The spot shape was found to depend on the lifetime of the bleached state of the dyes, the light power, and the disk rotation speed. When the lifetime is short, the super-resolution spot shape is not produced at high disk speeds. On the other hand, a dye mask layer with long lifetime, such as a photochromic mask, can produce a sharp spot shape in the higher disk speed region, and therefore is suitable for obtaining a super-resolution disk with a high data transfer rate.     

Theoretical Analysis of Super-Resolution Optical Disk Mastering Using a Photoreactive Dye Mask Layer

The super-resolution mastering of read-only optical disks using a photoreactive bleachable dye mask layer was theoretically analyzed. Equations have been derived which describe the photoreactions of the resist layer and mask layer. A numerical simulation based on these equations showed that the transmittance of the mask directly affects the quality of the formed pit shape. A high-quality pit shape is obtained by using a low transmittance mask.     

Pressure-sensitive paint measurement on co-rotating disks in a hard disk drive

There is much demand for improvement in the performance of a hard disk drive (HDD) along with recent rapid developments of information technology. While high-speed disk rotation of a HDD is necessary to accommodate such needs, it causes disk flutter induced by pressure fluctuation on disks and degrades reliability of a HDD. In order to understand the mechanism of the fluttering phenomenon, it is important to know pressure field on the rotating disk. However, it is impossible to measure the pressure by ordinary methods such as pressure taps. Pressure-sensitive paint (PSP) is a pressure measurement technique based on the oxygen quenching of luminescence and enables us to measure the pressure non-invasively. In general, however, the temperature sensitivity of PSP makes it difficult to measure the precise pressure on the surface with temperature distribution. We measured the time-averaged pressure on the disk rotating at 10 000-20 000 rpm for the first time by adopting a temperature-insensitive PSP composed of pyrene sulfonic acid (PySO₃H) as a luminophore. It was found that the pressure forms a concentric circular distribution and decreases toward the center of the disk. Additionally, we elucidate how disk rotational speed and spacing between co-rotating disks influence on the pressure field.     

一种面向编译器的数据访问节能技术研究

当前针对磁盘功率管理的大部分研究都是把重点放在磁盘空闲周期的利用上。人们相继研究了硬件功率节约机制(比如降速磁盘和多速磁盘)和补充性的软件策略(比如改变代码和数据布局,以提高空闲周期的长度)。然而,硬件功率节约机制无法处理高能耗并行应用的短空闲周期,而代码/数据重组策略往往要求大规模的代码更改。在本文中,我们提出一种面向编译器的数据访问(I/O调用)调度技术,以节约磁盘能量,在更短的周期内聚集了尽可能多的数据请求,进而延长了磁盘空闲周期,提升硬件功率管理机制的有效性。与先前基于软件的策略相比,该技术不需重组代码或数据。在基于集群的仿真环境下结合6种应用程序对本文方法进行评估。结果表明,本文方法提升了降速磁盘和多速磁盘的性能,将功率节约平均效果提升了一倍。     

Dual Focus Optical Head for 0.6 mm and 1.2 mm Disks

We propose a dual focus optical head with a holographic optical element (HOE) which corrects spherical aberrations in order to read both 0.6 mm disks and 1.2 mm disks. The thin disks are read using transmitted light and the thick disks are read using +1st order diffracted light of the blazed HOE. The good quality of the focused spots and the focusing error signals was experimentally confirmed. No influence of unnecessary diffracted light was observed.     

Laser heterodyne cross-polarized technique for inspection of magnetic disks

A new optical technique for observation of service magnetic tracks on magnetic disks is developed. Weak depolarization of the probe beam due to longitudinal magneto-optical Kerr effect is detected by means of heterodyne mixing of the two cross-polarized and frequency shifted waves generated by Zeeman-type laser. In comparison with the traditional homodyne method the proposed technique has better sensitivity and spatial resolution. Experimental results obtained with standard sample magnetic disks showed the signal-to-noise ratio of about 10, and the spatial resolution of about 30 μm. A possibility of the phase-contrast super-resolution is discussed.     

Disk Noise Measurement System for Optical Disks

We developed a system to measure disk noise as a function of both radial and angular position. In order to obtain an accurate disk noise measurement, crosstalk and intersymbol interference were avoided by recording regularly repeating pit patterns and the influence of electronic and laser noise was removed by averaging techniques. We found the system’s mapping ability and its high sensitivity to be very useful in investigating disk noise phenomena in the mastering process. We used the system to assess the accuracy and reproducibility of the photopolymerization replication and Al vapor deposition processes. Also, we investigated the choice of photoresist and found that photoresists with the combination of the narrowest molecular weight distribution and the highest photo-active compound content resulted in the lowest disk noise levels. Our system can, in principle, be adapted to evaluate magneto-optical and phase change disks.     

Differentially Rotating Disks of Dust: Arbitrary Rotation Law

In this paper, solutions to the Ernst equation are investigated that depend on two real analytic functions defined on the interval [0,1]. These solutions are introduced by a suitable limiting process of Bäcklund transformations applied to seed solutions of the Weyl class. It turns out that this class of solutions contains the general relativistic gravitational field of an arbitrary differentially rotating disk of dust, for which a continuous transition to some Newtonian disk exists. It will be shown how for given boundary conditions (i.e. proper surface mass density or angular velocity of the disk) the gravitational field can be approximated in terms of the above solutions. Furthermore, particular examples will be discussed, including disks with a realistic profile for the angular velocity and more exotic disks possessing two spatially separated ergoregions.     

基于微束X射线荧光光谱的新型铸&锻GH4096合金涡轮盘成分分布解析

铸&锻GH4096高温合金涡轮盘拥有高承温能力、高强度、低裂纹扩展速率、高抗疲劳性能等优异性能,是航空发动机的关键热端部件。但由于其合金化程度较高、零件尺寸大、制备工艺复杂等,不可避免会出现成分和组织分布不均匀,一定程度影响涡轮盘的服役性能。微区X射线荧光光谱（μ-XRF）具有微区分辨率高、分析速度快、多元素同步分析、非破坏性等优点,被广泛应用于考古、地质、生物等领域,但对大尺寸高温合金构件的成分分布的研究较少,对于材料各原始位置处的成分定量分布表征也未见报道。本试验通过选择合适的测量条件、优化仪器定量方法,建立了基于微束X射线荧光光谱的新型铸&锻GH4096合金涡轮盘成分分布定量分析方法,并引入了原位统计分析方法对涡轮盘中Cr,Co,Mo,W,Ti,Al,Nb和Ni八种主要元素进行了定量统计分布解析。发现涡轮盘厚度的中心区域内Co,Mo和Ti三种元素从轮毂至轮缘存在较明显的弧形负偏析带,而Ni和Cr两种元素存在弧形正偏析带。另外,涡轮盘径向也存在一定的成分梯度分布,Co,Cr和W三种元素含量从轮毂到轮缘的呈现逐渐降低的趋势,而Mo,Ti和Nb三种元素含量则呈现逐渐上升趋势。对各元素最大偏析度、统计偏析度、统计符合度计算分析后可知,Cr,Co,Mo,W,Ti,Nb和Ni七种元素测量区域内整体偏析程度较小、统计符合度大,在材料元素设计值允许范围内具有较好的成分均匀性。使用火花源金属原位分析仪（OPA-200）对相同测试区域的元素进行了线分布分析,其分析结果与微束荧光光谱得到的分析规律具有较好的一致性,说明大尺寸涡轮盘在热处理过程中存在温度场分布,导致了各元素扩散行为以及显微组织分布的差异,因此不同部位的成分也存在一定偏析。通过对大尺寸的涡轮盘成分进行定量统计分布解析,对于评价新型铸&锻变形GH4096高温合金涡轮盘的成分分布均匀性,解析制备工艺与大尺寸构件成分、组织结构分布的相关性具有重要意义。