基于模块级流水和并行处理的CAVLC编码器实现

基于上下文的自适应变长编码(CAVLC)是高清视频压缩标准H.264的关键模块。CAVLC编码器设计的优劣直接影响系统实时性。本文设计的编码器整体采用模块级流水线架构,关键子模块内部采用并行处理,提高了实时性。设计在Xilinx公司的xc5vlx330t芯片上实现,综合后时钟频率可达222MHz。视频数据的实际测试显示,编码器可满足系统实时性需求。     

Towards development of a consistent orbit series for TOPEX,Jason-1, and Jason-2

The TOPEX/Poseidon, Jason-1 and Jason-2 set of altimeter data now provide a time series of synoptic observations of the ocean that span nearly 17 years from the launch of TOPEX in 1992. The analysis of the altimeter data including the use of altimetry to monitor the global change in mean sea level requires a stable, accurate, and consistent orbit reference over the entire time span. In this paper, we describe the recomputation of a time series of orbits that rely on a consistent set of reference frames and geophysical models. The recomputed orbits adhere to the IERS 2003 standards for ocean and earth tides, use updates to the ITRF2005 reference frame for both the SLR and DORIS stations, apply GRACE-derived models for modeling of the static and time-variable gravity, implement the University College London (UCL) radiation pressure model for Jason-1, use improved troposphere modeling for the DORIS data, and apply the GOT4.7 ocean tide model for both dynamical ocean tide modeling and for ocean loading. The new TOPEX orbits have a mean SLR fit of 1.79 cm compared to 2.21 cm for the MGDR-B orbits. These new TOPEX orbits agree radially with independent SLR/crossover orbits at 0.70 cm RMS, and the orbit accuracy is estimated at 1.5–2.0 cm RMS over the entire TOPEX time series. The recomputed Jason-1 orbits agree radially with the Jason-1 GDR-C orbits at 1.08 cm RMS. The GSFC SLR/DORIS dynamic and reduced-dynamic orbits for Jason-2 agree radially with independent orbits from the CNES and JPL at 0.70–1.06 cm RMS. Applying these new orbits, and using the latest altimeter corrections for TOPEX, Jason-1, and Jason-2 from September 1992 to May 2009, we find a global rate in mean sea level of 3.0 ± 0.4 mm/yr.     

圆锥螺纹塞规测量方法综述

随着现代工业的发展,对圆锥螺纹塞规的加工精度提出了更高的要求,如何提高圆锥螺纹塞规的测量准确度成为必须解决的重要课题.本文以接触式测量和非接触式测量分类方法为例,对比分析了国、内外现有的多种圆锥螺纹塞规基面中径测量方法及研究现状,认为利用CCD作为螺纹几何要素探测器件的视觉检测技术将是未来的发展趋势,随着模式识别、图像处理等相关技术的进步,随着机器视觉技术自身的成熟和发展,视觉检测技术将得到更为广泛的应用.     

基于改进层次分析法的民用飞机修理级别非经济性分析

修理级别分析（level of repair analysis,简称LORA）是飞机保障性分析的一个重要内容,是在设计阶段评估维修对飞机成本影响的一种系统分析方法。在缺乏相关修理级别经济性分析数据的前提下,经过对多种国际主流机型维修大纲和维修手册的研究,分析了飞机修理级别分析的影响因素,建立了层次化的综合评价指标体系,同时又通过专家打分法将定性评价指标进行量化。在此基础上,运用灰色关联分析对修理级别方案进行综合排序,从而选出最优的修理基地。最后通过实例分析说明了本文所提模型的合理性。     

腔体闭式流动控制的实验和数值模拟

利用数值模拟和风洞实验相结合的方法,研究了闭式流动腔体的流动特征及其设置圆柱控制杆后腔体内声压级(SPL, Sound Pressure Level)和压力分布的变化.数值模拟求解三维N-S方程,采用AUSM+计算格式,湍流模型采用Wilcox k-ω模型.实验在0.6 m×0.6 m超音速风洞中进行,在腔体底部布置了40个常规静压测量点和15个动态测压点.研究表明,在外流为超音速流时,闭式流动的腔体底部压力变化梯度较大,腔体底部和后缘的测压点的SPL值和频率关系曲线中没有明显的SPL峰值.实施控制后,腔体底部的压力变化梯度减缓,在腔体后缘分离区内的测压点SPL值降低,而前缘分离区内的测压点SPL值增加.      

考虑维修效能的修理级别优化

修理级别分析(LORA)是在装备研制阶段为建立使用维修制度而进行产品维修决策的重要方法,而修理级别分析无法决策每级站点的备件配置数量.为此,相对于传统研究,提出了一种在装备保障系统中重点考虑维修时间的库存与修理级别分析联合优化方法,并对该方法作了系统的分析, 确定了修理级别优化模型的目标函数和建模条件,解析了故障送修数量、备件需求、备件短缺等随机变量在多级多站点保障组织中的传递耦合关系,将维修时间参数引入到传统的只考虑维修费用的修理级别量化分析中,建立了联合修理级别和备件库存的单层三级优化模型;分析了优化问题的特点,设计了高效率的多变量凸优化算法,使得该模型能够高效地应用于多级多站点多类型备件的复杂保障系统;最后构建了优化方法应用案例,并利用仿真验证了该算法和模型的正确性,为修理级别分析工作的开展提供了一套可行的优化方法.      

中段目标高分辨距离像姿态敏感性影响度量方法

高分辨距离像（HRRP）存在散射中心模型改变、越距离单元走动、闪烁现象三个方面的姿态敏感性,同时影响距离像预处理、特征选择、模板生成等方面。为了区分不同姿态敏感性对距离像识别的影响,从而研究针对性的解决办法,首先在识别理论框架下,建立了“HRRP姿态敏感性影响水平统计模型”作为姿态敏感性对目标识别性能影响的定量分析工具。其次,针对弹道中段目标识别问题,定量分析了中段目标HRRP的姿态敏感性。暗室实测数据表明,闪烁现象与越距离单元走动对HRRP识别的影响程度相近。最后,通过比较聚类模板生成算法和邻近姿态角模板生成算法,验证了基于姿态敏感性影响水平分析方法的有效性。此分析方法对于弹道中段目标识别具有一定的参考价值。     

一种高声强校准装置的高声强级测量不确定度评定方法

介绍了一种高声强级发生及测量方法、数学模型及其测量不确定度的评定方法,并给出了不确定度评定实例及验证结果。     

快船式飞行器参数化建模及高超声速气动计算

针对快船式飞行器概念研究和总体设计的需要,将已知几何构型截面划分为三个形状控制函数,并基于圆锥曲线拼接的思想将其封闭为统一的参数化截面形状函数。通过动态调整形状函数的少量控制参数,可获得一簇连续的形状截面,实现了飞行器几何外形的快速参数化建模。基于三角面元划分,进行了高超声速气动特性工程计算,并给出了数据的4阶多项式拟合公式。设计了一种中长航程任务,采用全数值预测校正再入制导算法对快船式飞行器和阿波罗飞船进行了相同条件的再入仿真。仿真表明,相比传统飞船,快船式飞行器升阻比增大,机动性增强,过载环境改善,着陆精度更高。     

Computation of radiation environment during ground level enhancements 65, 69 and 70 at equatorial region and flight altitudes

The radiation environment in the troposphere of the Earth is governed by cosmic rays of galactic and solar origin. During major solar energetic particles events the radiation environment changes dramatically. As a results the risk of biological effects due to exposure to ionizing radiation of aircrew increases. Here we present a numerical model for computation of absorbed dose in air due to cosmic rays of galactic and solar origin. It is applied for computation of radiation environment at flight altitude in the equatorial region during several major ground level enhancements, namely GLE65 on 28 October 2003, GLE69 on 20 January 2005 and GLE70 on 13 December 2006. The model is based on a full Monte Carlo simulation of cosmic ray induced atmospheric cascade. The cascade simulation is carried out with CORSIKA 6.990 code with corresponding hadron generators FLUKA 2011 and QGSJET II. The contribution of different cascade components, namely electromagnetic, hadron and muon is explicitly obtained. The spectra of arriving solar energetic particles are calculated from ground level measurements with neutron monitors and satellite data from GOES. The obtained results are discussed.