Periodic X-ray outbursts from A0535+26, 2S1145-619 and GX301-2

We report Ariel V(SSI) observations of three X-ray pulsars A0535+26, 2S1145-619 and GX301-2 (2S1223-624). These sources exhibit X-ray outbursts which appear, on the basis of observations extending over 5 years, to have recurrence periods of 110 days, 187.5 days and 41.4 days respectively. If these periods are orbital in origin, the observed X-ray modulation may be explained in terms of an appreciable orbital eccentricity giving rise to time variable accretion. (In the case of GX301-2 published pulse timing data already provide independent evidence for a 41.4 day orbital period and an eccentricity e 0.4). The optical counterparts are all early-type stars; A0535+26 and 2S1145-619 are identified with Be main sequence stars and GX301-2 with a B2 supergiant which also shows an emission line spectrum. The implications of the observations in relation to possible mass transfer mechanisms in such systems are discussed.     

EXOSAT observations of the bright X-ray source GX9+1

We present the results of the spectral and timing analysis of an observation of GX9+1/4U1758-205 performed with the Medium Energy Experiment aboard EXOSAT. During our observation the source flux varied irregularly in time scales from minutes to hours. No periodic emission in the period range from 16 msec to 2000 sec was found with an upper limit of around 1% (3 ) for the pulsed fraction. The hardness ratio shows a correlated change with the flux intensity (Sco X-1 behaviour). The spectrum could be fitted by a double component model, a black body component (kT=1.16–1.26 keV) together with a thermal bremsstrahlung law (kT=13–15keV). The black-body temperature-black-body flux relation follows a Stefan Boltzmann law with R_BB=15.3 km^*D/10 kpc. No iron line was detected. The upper limit for the line equivalent width of a 6.7 keV iron emission line is 40 eV (1). The X-ray spectral behaviour of GX9+1 indicates, that this source belongs to the class of Low-Mass X-ray Binaries (LMXB).     

Ariel 5 observations of GX 339-4

Observations of GX 339-4 with the Ariel 5 spectrometer are reported. The spectrum of the source is very steep, possibily a low temperature blackbody or Bremsstrahlung distribution. Differences and similarities with the related sources Cyg X-1 and Cir X-1 are discussed.     

Observation of X-ray spectrum of GX301-2

X-ray source GX301-2 was observed with scintillation proportional counters in binary phase 0.90 to 0.05. Intense iron fluorescent emission and sharp iron K absorption edge appeared in all spectrum including flare, which occured on JD 2445814.6. The equivalent width are linearly correlated with column density and this can be interpreted by a simple model that cold isotropic gas surround compact source. Pulse fraction also changed inversely correlated way with column density which suggest smearing by scattering of x-rays in the reprocessing medium. Averaged iron K absorption edge energy was 7.36±0.02 keV.     

微动疲劳损伤试验设计研究

研制了微动桥式试验装置及试验方法。高低周复合加载由改装过的PW3-10型疲劳试验机来实现。使用应变片弓形元件测量微位移幅值。用弹性环实现微动桥和板状试件上法向接触压力的加载,利用本文中的方法及装置,已成功地完成了钛合金TC-11对高温合金GX8的微动疲劳损伤试验。     

Spectra and time variability of GX 5-1

From a short observation of GX 5-1 with EXOSAT we have derived information on spectral and temporal behaviour in the energy range 1–20 keV. The source was found to be variable on time scales from 10 s to 1 h. Describing the spectrum one is forced to assume at least two spectral components. The best fit is reached using a spectrum composed of two blackbody functions with typical temperatures 1 keV and 2 keV, corresponding to apparent blackbody radii of 43 km and 11 km, respectively (for a distance of 10 kpc). With respect to the hot component there is evidence for variability in temperature as well as in apparent blackbody radius. No periodic variability has been found over the period range 0.25 s to 2000 s. There is no evidence for an iron emission line.     

Mg/Al合金粉末热压烧结中相变扩散过程研究

利用OLYMPUS GX71金相显微镜及EDS对Al-15％Mg热压烧结样品进行金相显微组织观察与成分分析,探讨烧结过程中组织演变过程。实验结果表明：热压烧结过程中两种粉体发生互扩散,首先在Mg颗粒边缘形成γ（Al12Mg17）相,而后随扩散的进行γ相转变为β（Al3Mg2）相,Mg颗粒由外向内不断的形成γ相,而后不断的转变为β相,直到全部生成β相。随温度的降低,β相会以极其细小的颗粒形式析出;利用真空热压烧结方法在420℃,150Mpa下保压3—4h进行固相烧结获得密度低于2．5g／cm^3致密度达98％以上的Al—15％Mg合金。     

CT5ATP在GTCP131-9BAPU管理中的作用

针对波音737NG机型GTCP131—9B辅助动力装置（APU）出现涡轮叶片移位的故障,分析了叶片移位对APU的影响,提出7CT5ATP方法．并结合南航的经验将其应用于GTCP131—9BAPU的管理中．确定了以CT5ATP作为启动值,结合修后使用时间（TSR）、孔探结论和后中心体盖裂纹检查作为完整性能监控的手段,为APU拆换提供了可信的实践依据,实现7APU单位维修成本的有效降低。     

An IR,optical and X-ray study of the two state behaviour of GX 339-4

We review results of correlated IR, optical and X-ray observations of GX 339-4 made from March 1981 through May 1984. In the soft X-ray state, the object does not show outstanding optical and X-ray variability. Night-to-night smooth optical variations of 0.3 magnitudes were however present during one observing run. In contrast, the hard X-ray state is characterised by strong erratic optical and X-ray fluctuations on time scales from 20 milliseconds to seconds, as well as 7 to 20 second quasi-periodic oscillations. The optical counterpart appears much redder in the IR during the hard state. Particular attention is drawn to the hard to soft X-ray transition which occured in June 1981. The shape of the IR to X-ray energy distribution is discussed. The unusual features of this black hole candidate are examined in the framework of the current theories of accretion.Based partly on observations obtained at the European Southern Observatory, La Silla, Chile.     

飞机退租管理及改进措施研究

结合5架空客飞机退租的经验,对退租管理工作中的不足,围绕结构修理管理、工程管理和附件控制三方面进行了分析和探讨．并给出了有效的改进建议。     

信息融合技术在飞机发动机油液故障诊断中的应用研究

详细介绍了信息融合技术中的D-S证据理论,并运用该理论能够处理不确定信息能力的特点,对油液分析的光谱数据和铁谱数据进行了有效的融合,解决了单独分析方法难以得到综合信息的问题,提高了飞机发动机油液故障诊断的准确性.     

基于QAR数据的关联规则挖掘算法能研究

介绍和分析了关联规则的概念和Apriori算法,针对Apriori算法需要多次扫描数据库而导致运算效率不高的缺点．设计并实现了基于事务标识列表的频繁项集的产生算法——TagList Apriori。对比实验证明,新方法可以有效减少数据库扫描次数,节省运算时间．提高算法的运算效率,提高OAR数据关联规则挖掘的效率。     

AS35083直升机发动机控制系统的检查与排故方法

通过分析AS35083直升机装备的阿赫耶ARRIEL281发动机控制系统的原理，深入研究发动机控制系统引起的故障，从外场维护的角度提出快速确认故障部件的具体方案。     

民机在役构型管理思路和方法研究

基于国内某型号民用飞机在研阶段构型管理工作,结合民机在役运营的适航要求和客户的安全经济运营需求,阐述了民机在役构型管理的重要性．分析了在役构型管理的目标范围和管理重点,提出了民机在役构型管理标识方法．并讨论了在役构型的分类更改控制方法。该研究将填补国内民机在役构型管理领域的空白。     

浅谈老龄飞机外场维护对策

通过对一定时期内6架某型老龄飞机的故障统计分析,根据飞机的技术状况以及故障的多发部位,从故障原因、故障预防和维护特点等方面提出了相应的维修预防措施。     

Paral lel VLSI Implementation of the Kalrman Filter

The problem of parallel implementation of the square-root Kalman filters is addressed. At the system level, our approach is to apply systolic-type VLSI processor arrays as basic building blocks to accelerate the matrix operations required in each iteration. To maximize the parallelism, we also exploit an inter-array pipelining scheme through the overlapping of execution between successive processor arrays. We estimate that with (5n2 + r2 + 8nr + n + 3r)/2 processors, it would take max[(4n + 2r, 2n + 4r-2)] time units to complete one Kalman filter iteration, where n is the dimension of the underlying state space model and r is the dimension of the input vector.     

民用航空器的修理、改装和其他的研究

就美国联邦航空局、欧洲航空安全局、中国民用航空局各种法规、条例以及波音和空客等航空器制造厂和国外航空公司对民用航空器维护过程中的修理、改装和其他的定义进行了比较、分析和研究．结合国内法规条例和工作认识,对民用航空器维修过程中的修理、改装及其他进行了精确定义,对判断某项修理、改装或其他是否属于重要、是否需要局方批准等提供了借鉴。     

波音767飞机翼尖小翼改装的技术分析

波音767飞机执行融合型翼尖小翼改装后可获得一系列飞行性能的提升,显著降低燃油成本,可为航空公司创造巨大的经济效益。本文介绍了实施改装中的关键技术以及一些技术问题的解决方案。     

老龄波音757飞机结构损伤特性分析

通过对老龄波音757飞机结构损伤特性的分析和隐蔽性等特点,建议实施有针对性、及时性、扩展性、构的安全。得出其具有集中性、蔓延性、严重性、重复性彻底性和双重性的维修,以确保老龄757飞机结     

三维立体相位扫描测量技术在发动机孔探中的应用

介绍了工业视频内窥镜测量技术的发展历程及民航孔探工作的常用测量方式,并从工作质量、工作效率以及安全角度考虑．推荐使用高精度、单视窗的三维测量技术。