现代飞机俯仰跟踪时诱发振荡预测分析

根据飞机纵向ＰＩＯ的特点，提出了预测分析ＰＩＯ所用的人－机闭环系统数学模型，其中飞机采用等效系统数学模型，驾驶员操纵采用ＭｃＲｕｅｒ模型，参数按地面人－机模拟飞行跟踪试验确定，集中介绍了四种飞机纵向ＰＩＯ预测准则，Ｓｍｉｔｈ－Ｇｅｄｄｅｓ准则，修正带宽准则，增益，相位裕度准则，Ｎｅａｌ－Ｓｍｉｔｈ原则，并提供了相应的计算方法。     

Solar flare forecasting model supported with artificial neural network techniques

Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited information from sunspots. For this reason, new measures based on solar magnetic field observations are proposed and a solar flare forecasting model supported with an artificial neural network is introduced. This model is equivalent to a person with a long period of solar flare forecasting experience.     

WL10型近红外反射式光电传感器的研制

依据光学电子学的相关原理，针对烟草行业自动生产过程中对传感器的需要，研制了ＷＬ１０型近红外反射光电传感器，并成功地应用于烟草行业的生产线上。     

层次分析法在飞机维修不安全事件影响因素评价中的应用

对飞机维修不安全事件的影响因素进行层次分解,构建层次矩阵;利用德尔菲法,导入不安全事件调查分析专家组成员对不安全事件的判断;结合层次分析法(AHP)对不安全事件影响因素进行定性和定量的评价。     

二值箝位电路的理论分析及仿真研究

在CCD焦面驱动电路设计中，经常要求产生在两个指定电平间振荡的信号，二值箝位电路以其简单的拓扑结构、稳定的性能表现而得到应用。尽管二值箝位电路的稳态输出仅受拓扑结构影响，而与初始条件无关，然而其暂态输出会随着初始条件以及拓扑结构的不同而有所差异，造成二值箝位电路设计及其应用的复杂性，文章深入地研究二值箝位电路不同的拓扑结构以及不同的输入条件对其输出的影响，给出了各种情况下的仿真结果，并针对仿真结果给出了定量和定性的分析。     

磁转速表指针摆动的故障分析

就磁转速表活动系统的动态特性以及在附加交变力矩的作用下，指针摆动随转速变化的规律，从理论上进行了分析，并结合实际探讨了指针摆动的故障原因。     

The evolution of mirror type magnetic fluctuations in the magnetosheath based on multipoint observations

Two orbits were selected in January–February 2006 when the separation between the Cluster spacecraft was large and mirror type magnetic field fluctuations were observed by all spacecraft in different regions of the terrestrial magnetosheath. Minimum variance analysis was applied to find the mirror type fluctuations, and the amplitude of the fluctuations was determined individually. Mirror mode structures are moving along the streamlines frozen in the plasma. A model was developed for the calculation of plasma flowtime from the bow shock to the observation point. The growth rate of the field strength perturbations was estimated by comparing the amplitudes of fluctuations observed simultaneously at distant locations (∼10,000 km) based on the assumption that δB ∼ exp(γt). The obtained growth rate values were about an order of magnitude smaller than those provided by linear models and they decreased in the inner regions of the magnetosheath, indicating some saturation in the growth of the waves when proceeding towards the magnetopause. The results of these two case studies suggest that mirror type fluctuations originate from the compression region downstream of the quasi-perpendicular bow shock, and the growth of the fluctuations cannot be described by linear approximations.     

Large-scale Coronal Heating, Clustering of Coronal Bright Points, and Concentration of Magnetic Flux

By combining quiet-region Fe XII coronal images from SOHO/EIT with magnetograms from NSO/Kitt Peak and from SOHO/MDI, we show that the population of network coronal bright points and the magnetic flux content of the network are both markedly greater under the bright half of the large-scale quiet corona than under the dim half. These results (1) support the view that the heating of the entire corona in quiet regions and coronal holes is driven by fine-scale magnetic activity (microflares, explosive events, spicules) seated low in the magnetic network, and (2) suggest that this large-scale modulation of the magnetic flux and coronal heating is a signature of giant convection cells. This revised version was published online in June 2006 with corrections to the Cover Date.     

某型通航飞机失速警告失效故障分析

针对某型通航飞机地面测试中发现失速警告不工作的故障,分析该失速警告系统各组成部分的结构、原理、功能、走线,制定具体排故程序逐步判断查找出故障原因电子线路故障,并对故障原因进行了分析。     

高原机场终端区飞行闭环稳定性分析

分析了高原机场终端区飞行的特殊性和影响高原机场飞行闭环稳定性的各种不利因素,指出了在高原机场缺氧条件下对飞行员数学模型修正的必要性和修正方法.采用等效闭环系统方法分析飞机在高原机场环境下的闭环稳定性,利用该思路可以用常规的分析方法研究高原机场飞行员缺氧条件下的闭环稳定性.