IRCT下对数正态和正态分布参数的MLE

在文［１－４］的基础上进一步研究了带有不完全信息的随机截尾试验模型（ＩＲＣＴ）。着重讨论了对数正态分布参数的统计分析问题，建立了参数所满足的似然方程组，给出并证明了似然方程组解即参数的极大似然估计（ＭＬＥ）的存在唯一性定理，所得的结论对于正态分布也同样适用。文末给出了随机模拟数值解例子，结果表明，参数的ＭＬＥ具有较高的精度。     

一种微型仿昆扑翼飞行器扑翼操控机制

提出了一种扑翼操控机制,用于解决微型仿昆扑翼飞行器悬停飞行的飞行动力问题。通过对扑翼运动参数对气动力及空气动力矩的作用进行理论和仿真分析,设计了一种采用可变幅值的周期函数调节扑翼运动的扑打角和旋转角变化的方法,实现对气动力和气动力矩进行独立控制的操控机制。仿真结果验证了此操控机制可以较好地解决仅一对翼的仿昆扑翼飞行器飞行动力问题。     

军用飞机结构耐久性设计的细节疲劳额定值方法

 为满足军用飞机研制初步设计阶段对结构耐久性(疲劳)快速设计与评估的迫切需求,在全面分析军用飞机与民用飞机主要区别的前提下,针对军用飞机结构与使用载荷特点,以民用飞机细节疲劳额定值(DFR)方法的基本思想和技术途径为基础,从寿命服从对数正态分布的假设出发,对随机载荷谱的当量等幅化方法、结构DFR许用值的确定技术以及标准S--N曲线的建立等关键问题进行深入研究,建立了适用于军用飞机的DFR方法及相应的工程实施技术。初步应用表明方法可行且偏保守,能明显缩短研制周期、降低研制成本,具有重要的工程意义和应用价值,可用于军用飞机研制的初步耐久性设计。     

常用卫星通信信号数字调制方式的自动识别

针对常用的卫星通信信号的调制方式识别问题,提出了一种新的自动识别算法.该算法基于统计特性分类原理,通过建立一组统计特征参数,在无需先验信息的条件下,实现对信号调制方式的自动识别.对实际采集数据进行了实验验证,结果表明该算法在低信噪比环境下仍有较高的识别率,简单易用,具有较强的工程可行性和良好的扩展性.     

航空发动机振动环境谱统计归纳方法及振动试验台复现

为满足航空发动机及机载产品研制过程贴近使用环境的振动考核试验需求,需根据发动机实测振动数据给出振动考核试验所需的输入谱图。依据GJB/Z 126-99中给出的环境测量数据归纳方法,建立了发动机实测振动环境谱统计归纳方法并通过程序实现。利用发动机多架次实测试飞振动数据统计归纳得到发动机测点位置的振动实测谱。基于能量等效及信号频域特征分布一致原则,将归纳得到的实测谱转化为可用于振动台输入的振动环境谱,并在振动台上进行了振动信号的复现试验。结果表明：振动台输出信号与发动机实测振动信号频域分布特征一致,在统计频率带宽范围内振动总量最大相差5.7%,证明了转化方法是合理的,为航空发动机机载设备贴近使用环境的振动考核试验方法提供了真实的输入谱图。     

Statistical study of radio drifting pulsation structures with associated CMEs and other observations

Solar radio burst, especially the fine structures (FSs) and the drifting pulsation structures (DPSs), may be used as an important diagnostics tool to draw the evolution map of the flare loop in the initial phase of solar flares. In this work, 52 radio events were found accompanying with DPSs. They were all observed with the Solar Radio Spectrometers (0.625–7.6 GHz) of China during 1998–2004. Combining the radio observations with LASCO-C2, Goes-8 SXR, H_α, EUV and Trace observations, we analyzed all these events and obtained some statistic conclusions: First, 88% DPSs take place at the initial phase of the radio burst, and their rich spectrum characteristics are helpful to understand the events further. Second, 83% DPSs are associated with CMEs or ejection events, and all the events are accompanied by Goes SXR flare. Third, for CMEs and DPSs, which take the first step, there is no significant predominance of either of them. The relationship between the DPSs and CMEs is still not clear in this study because of the lack of spatial resolution in the centimeter–decimeter band. However, the EIT or Trace ejection happened during the onset/end time of DPSs. They are signatures of the initial phase of CMEs. Two events will be illustrated to explain this.     

A question raised from the observation of dynamic cusp formation: When and where does particle acceleration occur?

We present observations of a C9.4 flare on 2002 June 2 in EUV (TRACE) and X-rays (RHESSI). The multiwavelength data reveal: (1) the involvement of a quadrupole magnetic configuration; (2) loop expansion and ribbon motion in the pre-impulsive phase; (3) gradual formation of a new compact loop with a long cusp at the top during the impulsive phase of the flare; (4) appearance of a large, twisted loop above the cusp expanding outward immediately after the hard X-ray peak; and (5) X-ray emission observed only from the new compact loop and the cusp. In particular, the gradual formation of an EUV cusp feature is very clear. The observations also reveal the timing of the cusp formation and particle acceleration: most of the impulsive hard X-rays (>25 keV) were emitted before the cusp was seen. This suggests that fast reconnection occurred during the restructuring of the magnetic configuration, resulting in more efficient particle acceleration, while the reconnection slowed after the cusp was completely formed and the magnetic geometry was stabilized. This observation is consistent with the observations obtained with Yohkoh/Soft X-ray Telescope (SXT) that soft X-ray cusp structures only appear after the major impulsive energy release in solar flares. These observations have important implications for the modeling of magnetic reconnection and particle acceleration.     

Abundances of Light Elements

This paper briefly reviews a few relevant features about the abundances of light elements (D, ⁴He, ⁶Li, ⁷Li, ⁹Be) in the Milky Way. It places special emphasis on metal-poor stars. Observational concerns are discussed. The use of ⁷Li and ⁶Li as cosmological probes and of ⁹Be as a chronometer for the early evolution of our Galaxy are discussed.     

统计过程控制研究领域及趋势概述

本文首先介绍了质量工程技术的主要内容。在此基础上，概述了统计过程控制技术的研究现状及其发展趋势。最后，讨论了与此相关的几个问题。