线纹尺安装方式对空气折射率实时修正效果的影响

根据三种实际测量情况进行分析,介绍了在使用激光干涉法测量线纹尺过程中,空气折射率实时修正技术对测量结果的影响与仪器布局和线纹尺安装方式的关系,并得出了相应的结论.     

八工位聚氨酯注塑回转自动生产线回转盘系统结构设计

本文介绍了八工位聚氨酯注塑回转自动生产线中回转盘系统的总体设计思路及各部件的结构设计，该系统具有运行平稳，定位准确和制造简单的特点。     

Intrinsic parameters of massive OB stars

We present the results of our observations of stars of type O5 and earlier and show that inclusion of the line blocking between 228 and 912 A solves the problem found by Herrero et al. (1992) in the determination of their stellar parameters. We study the influence of the line blocking and other effects on the mass and helium discrepancies and show that the first one is reduced by the use of spherical, non hydrostatic model atmospheres and that the second one is probably due to exposure of CNO material.The INT is operated on the island of La Palma by the RGO in the Spanish Observatorio de El Roque de los Muchachos of the Instituto de Astrofsica de Canarias     

基于核心零部件聚类的飞机现场可更换单元划分

为研究军用飞机测试性设计过程中现场可更换单元（LRU）划分工作，以功能独立性和结构独立性为基本原则，以降低飞机维修保障成本和时间为主要目标，设计了一种军用飞机LRU划分方案。方案在首先实现了飞机从整机到零部件的功能结构分层划分基础上，从设备零部件层级出发，以综合重要度作为各零部件的定量化指标，运用帕累托（Pareto）原则筛选出核心零部件。然后基于核心零部件开发了一种LRU划分聚类算法，该算法以军用飞机设计研制阶段、使用保障阶段、退役处置阶段全寿命周期内成本和时间为优化目标构造综合评判因子，实现了非核心零部件与LRU模块之间的聚类组合，得到最优的LRU划分结果。最后以某型军用飞机上蒸发循环制冷装置为例，运用本文设计的方案实现了该装置LRU的划分，并将划分结果与该装置的实际LRU清单进行对比，通过维修保障成本和时间综合评判因子对两种划分结果的优劣性进行分析，得出本文设计方案得到的LRU划分结果对飞机维修保障成本和时间的优化效果较为均衡的结论。     

公务机预见性航线维修管理

持续分析和监督系统（CASS）是持续适航维修方案（CAMP）的十大要素之一，目的是监督和改进持续适航维修方案的效能，属于安全管理范畴。本文阐述了持续分析与监督系统在公务机航线维修管理的应用与实践效果。     

飞机着陆操纵指令模型设计与仿真

针对某型飞机进场着陆完全靠目视飞行的现状,分析了该飞机加装着陆指令驾驶系统的可行性,分别设计了下滑线、基准线和下滑速度操纵指令模型。对人机闭环系统进行了飞机全量运动方程数值仿真。仿真结果表明所设计的着陆操纵指令模型可用于实现飞机着陆指令驾驶任务。     

非匀速弹道SAR成像方法研究

非匀速直线弹道成像是弹载SAR领域的核心问题之一。首先构建三维空间中的非匀直弹道模型,通过泰勒近似公式分析运动偏差的来源,并将运动偏差分解成方位偏移、地距偏移和俯仰偏移等三个部分。推导了横向运动和俯冲运动分别引起的地距偏移和俯仰偏移函数,从而得到了对应的运动补偿函数。方位偏移表现为SAR平台在方位向作变速直线运动,回波的数据格式可看成空间非均匀采样的结果。为此,提出了一种利用空间非均匀采样模型替代时域变多普勒模型的成像方法。该算法将变速运动等间隔时间采样的回波数据等效为匀速运动中非等间隔时间采样数据,然后通过方位向非均匀离散傅立叶变换将数据变换到均匀频率域,再完成其它后续的成像操作。完整地推导了非匀直弹道SAR成像的全过程,点目标仿真结果清晰可见,表明了算法的有效性。
     

EWIS介绍以及维护管理要求

电气导线互联系统(EWIS)是航空器适航管理中的一项重要内容,而且与老龄飞机的工程管理和维护工作的要求密切相关。本文从EWIS的定义和内容,以及在适航管理、维护指南和培训方面的要求进行阐述,对工程管理人员和飞机维护人员均有一定的指导作用。     

基于产品结构和CATIA的作战飞机易损性建模方法

介绍了作战飞机易损性建模的基本步骤和主要建模方法,分析了不同易损性建模方法的优点和不足,在此基础上,提出了一种基于产品结构和CATIA的易损性建模方法,该方法采用CATIA软件直接构建飞机的外形和部件模型,通过产品结构树对部件进行组织和管理,并利用CATIA二次开发在CATIA环境中直接生成三维射击线,有效提高了易损性模型的精度和易损性分析中各项操作的效率,为进一步的易损性定量计算提供了基础。以捕食者无人机为例,建立了全机易损性模型,生成了全机射击线,验证了文章所提方法的有效性和模型的可用性。     

Particle acceleration and gamma rays in solar flares: Recent observations and new modeling

Experiments on SMM, GAMMA, Yohkoh, GRANAT, Compton GRO, INTEGRAL, RHESSI and CORONAS-F satellites over the past three decades have provided copious data for fundamental research relating to particle acceleration, transport and energetics of flares and to the ambient abundance of the solar corona, chromosphere and photosphere. We summarize main results of solar gamma-astronomy (including some results of several joint Russian–Chinese projects) and try to appraise critically a real contribution of those results into modern understanding of solar flares, particle acceleration at the Sun and some properties of the solar atmosphere. Recent findings based on the RHESSI, INTEGRAL and CORONAS-F measurements (source locations, spectrum peculiarities, ³He abundance etc.) are especially discussed. Some unusual features of extreme solar events (e.g., 28 October 2003 and 20 January 2005) have been found in gamma-ray production and generation of relativistic particles (solar cosmic rays, or SCR). A number of different plausible assumptions are considered concerning the details of underlying physical processes during large flares: (1) existence of a steeper distribution of surrounding medium density as compared to a standard astrophysical model (HSRA) for the solar atmosphere; (2) enhanced content of the ³He isotope; (3) formation of magnetic trap with specific properties; (4) prevailing non-uniform (e.g., fan-like) velocity (angular) distributions of secondary neutrons, etc. It is emphasized that real progress in this field may be achieved only by combination of gamma-ray data in different energy ranges with multi-wave and energetic particle observations during the same event. We especially note several promising lines for the further studies: (1) resonant acceleration of the ³He ions in the corona; (2) timing of the flare evolution by gamma-ray fluxes in energy range above 90 MeV; (3) separation of gamma-ray fluxes from different sources at/near the Sun (e.g., different acceleration sources/episodes during the same flare, contribution of energetic particles accelerated by the CME-driven shocks etc.); (4) asymmetric magnetic geometry and new magnetic topology models of the near-limb flares; (5) modeling of self-consistent time scenario of the event.