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。     

A review on the upper atmospheric sodium observations from India: Insights

This review article briefly brings out the historical development of atmospheric sodium (Na) measurements over India and the importance of coordinated measurements with multiple techniques to address physical processes in the Earth's upper atmosphere. These measurements were initiated in the early 1970s by observing Na airglow emission intensities with broad band airglow photometer from Mt. Abu, a low-latitude hill station in India. Considerable amount of night-to-night variations in nocturnal emission intensities of the Na airglow were observed. Later, investigations regarding the dependence with the magnetic activities from the equatorial and low latitudes were carried out and double-humped structures in the nocturnal variation of intensities were reported. With the advent of Na lidar at Gadanki around 2005, the measurements of atmospheric neutral Na atom concentration became possible and more frequent occurrences of sporadic Na layers over the magnetic low latitude station compared to other latitudes were detected indicating the role played by electrodynamics. Later, a possible relationship between E-region field aligned plasma irregularities and the concentration of neutral Na atoms was investigated using coordinated measurements of VHF radar and Na lidar. Further, simultaneous measurements with Na lidar and a narrow band airglow photometer with narrow field of view brought out the importance of coordinated observation wherein the characterization of gravity waves could be carried out and also revealed the importance of collisional quenching due to ambient molecules in the Na airglow emission processes. In addition, combining the ground based measurements of Na lidar and meteor wind radar along with satellite measurements made possible to hypothesize the over-turning Kelvin–Helmholtz billow in the Na layer manifests “C-type” or inverted lambda shape structures in the height-time-concentration map of neutral Na atoms. This review paper presents a synoptic view mostly based on the previously reported observations of Na airglow emission, Na lidar and coordinated Na airglow and Na lidar observations from the Indian sector and highlights the importance of simultaneous measurements of mesospheric Na and its emissions along with satellite-borne measurements to address interesting geophysical processes in the Earth's upper atmosphere.     

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.     

等值线绘制简易算法

本文首先介绍了等值线的相关知识,然后重点讨论了一种不需要抽象数学理论和复杂数学模型做支撑的等值线追踪方法和相关数据存储结构,最后简单讨论了基于GDI+的等值线平滑技巧。实践表明该算法具有较高的运行效率。     

The radio recombination lines of hydrogen

The impact theory of spectral line broadening is used to obtain complete profiles for radio recombination lines broadened by electron and proton impact. Electron impact dominates but proton impact becomes increasingly significant as Δn$\mathrm{\Delta }n$ increases. Thus these new calculations essentially confirm previous results and so a longstanding discrepancy between observation and theory remains unresolved.