Fast approximate maximum likelihood period estimation from incomplete timing data

 To estimate the period of a periodic point process from noisy and incomplete observations, the classical periodogram algorithm is modified. The original periodogram algorithm yields an estimate by performing grid search of the peak of a spectrum, which is equivalent to the periodogram of the periodic point process, thus its performance is found to be sensitive to the chosen grid spacing. This paper derives a novel grid spacing formula, after finding a lower bound of the width of the spectral mainlobe. By employing this formula, the proposed new estimator can determine an appropriate grid spacing adaptively, and is able to yield approximate maximum likelihood estimate (MLE) with a computational complexity of O(n²). Experimental results prove that the proposed estimator can achieve better trade-off between statistical accuracy and complexity, as compared to existing methods. Simulations also show that the derived grid spacing formula is also applicable to other estimators that operate similarly by grid search.     

氮化硼陶瓷前驱体的制备及表征

以三氯化硼和六甲基二硅氮烷为原料制备了聚硼氮烷预聚体,再经高分子化制备了可溶的氮化硼陶瓷前驱体—聚硼氮烷.该法合成工艺简单,反应温和.采用凝胶渗透色谱、核磁共振氢谱、傅里叶红外光谱、热失重分析仪、元素分析等对预聚体高分子化过程中的分子量变化、高分子化机理、聚硼氮烷的裂解过程、所得陶瓷的元素组成进行了研究.结果表明,高分子化过程中主要发生了六甲基二硅氮烷脱除和转氨基反应.所得聚硼氮烷重均分子量为7 582,氮气下1 000℃时的陶瓷产率为41.6 wt％,陶瓷化转变主要发生在400～600℃,800℃时陶瓷化转变基本进行完毕,800℃氨气下裂解得到低C含量的白色氮化硼陶瓷,进一步在1 500℃氩气中裂解可得到结晶度较高的氮化硼陶瓷.     

一种无人机罗差修正方法

栽体磁场的干扰是导致地磁导航精度较低的主要因素,在对无人机载体磁场干扰地磁场产生的地磁测量误差简要分析的基础上,将小姿态时地磁匹配导航采用的12系数误差补偿模型引入一种无人机地磁定向导航的罗差修正.在静态条件下,利用无磁转台分别获取无人机在±30°姿态角范围内有无干扰源的磁测数据.实验数据分析表明,通过补偿,栽体航向角在±5°范围内其误差均方差由2.174°下降到0.350°,其余角度下航向角误差均方差则由2.282°下降到0.732°,满足无人机在大角度姿态飞行时航向稳定度优于±3°的要求.     

Interaction of single-pulse laser energy with bow shock in hypersonic flow

Pressure sensing and schlieren imaging with high resolution and sensitivity are applied to the study of the interaction of single-pulse laser energy with bow shock at Mach 5. An Nd:YAG laser operated at 1.06 lm, 100 mJ pulse energy is used to break down the hypersonic flow in a shock tunnel. Three-dimensional Navier–Stokes equations are solved with an upwind scheme to simulate the interaction. The pressure at the stagnation point on the blunt body is measured and calculated to examine the pressure variation during the interaction. Schlieren imaging is used in conjunction with the calculated density gradients to examine the process of the interaction. The results show that the experimental pressure at the stagnation point on the blunt body and schlieren imaging fit well with the simulation. The pressure at the stagnation point on the blunt body will increase when the transmission shock approaches the blunt body and decrease with the formation of the rarefied wave. Bow shock is deformed during the interaction. Quasi-stationary waves are formed by high rate laser energy deposition to control the bow shock. The pressure and temperature at the stagnation point on the blunt body and the wave drag are reduced to 50%, 75% and 81% respectively according to the simulation. Schlieren imaging has provided important information for the investigation of the mechanism of the interaction.     

激光焊接夹层喷管的技术现状

激光焊接冷却通道壁技术是适应商业需要(降低制造费用和缩短开发时间)开发的科研成果.沃尔沃公司(VOLVO)已经研究出其核心技术,即应用于焊接通道壁技术的激光焊接法和X射线辅助连接系统.此项技术最初的开发目的是应用于一次性使用发动机,但是现在发现其应用于可重复使用发动机上也很有优势.使用寿命、热负荷、最小内壁厚度和材料疲劳特性等综合决定了此项技术的适用范围.目前,已经进行了夹层喷管热试,并且制造出了具有典型尺寸的用于演示的夹层喷管.正在研究应用于非再生冷却系统的激光焊接夹层技术.研究成果表明,这项技术可用于各种发动机,即从助推级到上面级均适用.现在,欧洲和美国正在讨论应用此项技术加工Vulcain和RL60发动机的喷管夹层结构.本文对下面内容进行了叙述激光焊接夹层技术概况;目前激光焊接夹层技术在一次性使用发动机上的应用情况;可重复使用发动机用激光焊接夹层技术的一些特性.     

TypeⅡ试验下ε（λ,μ）分布位置参数的EB估计

讨论了在ＴｙｐｅⅡ（无替换定数截尾）试验方案下，当产品寿命为双参数指数分布时，位置参数μ的经验Ｂａｙｅｓ（简记ＥＢ）估计及其收敛速度问题。设受试验产品有ｎ个，试验中前ｒ个产品依次出现的失效时间为     

Up-to-date observations of space energetic particles made by the Chinese satellite Fengyun-1 (B).

This paper presents the observational results of space energetic particles obtained by the Cosmic Ray Composition Monitor (CRCM) onboard the Chinese satellite, Fengyun-1(B). These results, including those of a few solar proton events, the geomagnetically trapped particles and the anomalous cosmic ray components, were obtained from 3 September 1990 to 15 February 1991. The observed elements include H, He, C, N, O and Fe of energies from 4-23 MeV/u. It was found that the proton fluxes of the inner Radiation Belt (IRB) increased obviously during the period of solar proton event (SPE). A few kinds of heavy ions (Z > or = 6) were also detected in the IRB. As to the anomalous cosmic ray component (ACRC), in addition to C, N and O, anomalous iron particles were also recorded.     

单片微机用于陀螺参数辨识

简要介绍一种用伪随机信号对陀螺进行参数辨识的方法，及单片微机的应用。     

半导体器件铝腐蚀的判别方法研究

半导体器件内部铝腐蚀是卫星用半导体器件主要的失效模式之一,快速准确地判断铝腐蚀具有重要意义。文章给出了判别方法和程序,并对方法中的关键技术进行研讨。