High Excitation ISM and Gas

An overview is given of ISO results on regions of high excitation ISM and gas, i.e. HII regions, the Galactic Centre and Supernova Remnants. IR emission due to fine-structure lines, molecular hydrogen, silicates, polycyclic aromatic hydrocarbons and dust are summarised, their diagnostic capabilities illustrated and their implications highlighted. Based on observations with ISO, an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands, and the United Kingdom), and with the participation of ISAS and NASA.     

Deep Impact: Working Properties for the Target Nucleus – Comet 9P/Tempel 1

In 1998, Comet 9P/Tempel 1 was chosen as the target of the Deep Impact mission (A’Hearn, M. F., Belton, M. J. S., and Delamere, A., Space Sci. Rev., 2005) even though very little was known about its physical properties. Efforts were immediately begun to improve this situation by the Deep Impact Science Team leading to the founding of a worldwide observing campaign (Meech et al., Space Sci. Rev., 2005a). This campaign has already produced a great deal of information on the global properties of the comet’s nucleus (summarized in Table I) that is vital to the planning and the assessment of the chances of success at the impact and encounter. Since the mission was begun the successful encounters of the Deep Space 1 spacecraft at Comet 19P/Borrelly and the Stardust spacecraft at Comet 81P/Wild 2 have occurred yielding new information on the state of the nuclei of these two comets. This information, together with earlier results on the nucleus of comet 1P/Halley from the European Space Agency’s Giotto, the Soviet Vega mission, and various ground-based observational and theoretical studies, is used as a basis for conjectures on the morphological, geological, mechanical, and compositional properties of the surface and subsurface that Deep Impact may find at 9P/Tempel 1. We adopt the following working values (circa December 2004) for the nucleus parameters of prime importance to Deep Impact as follows: mean effective radius = 3.25± 0.2 km, shape – irregular triaxial ellipsoid with a/b = 3.2± 0.4 and overall dimensions of ∼14.4 × 4.4 × 4.4 km, principal axis rotation with period = 41.85± 0.1 hr, pole directions (RA, Dec, J2000) = 46± 10, 73± 10 deg (Pole 1) or 287± 14, 16.5± 10 deg (Pole 2) (the two poles are photometrically, but not geometrically, equivalent), Kron-Cousins (V-R) color = 0.56± 0.02, V-band geometric albedo = 0.04± 0.01, R-band geometric albedo = 0.05± 0.01, R-band H(1,1,0) = 14.441± 0.067, and mass ∼7×10¹³ kg assuming a bulk density of 500 kg m⁻³. As these are working values, {i.e.}, based on preliminary analyses, it is expected that adjustments to their values may be made before encounter as improved estimates become available through further analysis of the large database being made available by the Deep Impact observing campaign. Given the parameters listed above the impact will occur in an environment where the local gravity is estimated at 0.027–0.04 cm s⁻² and the escape velocity between 1.4 and 2 m s⁻¹. For both of the rotation poles found here, the Deep Impact spacecraft on approach to encounter will find the rotation axis close to the plane of the sky (aspect angles 82.2 and 69.7 deg. for pole 1 and 2, respectively). However, until the rotation period estimate is substantially improved, it will remain uncertain whether the impactor will collide with the broadside or the ends of the nucleus.     

A lightning swept stroke model: A valuable tool to investigate the lightning strike to aircraft

In the context of lightning strike on the Dassault Falcon family of aircraft, the standard zoning of Falcon 50, 900 and 2000, inferred from FAA and EUROCAE WG31 documents [US Department of Transportation, Federal Aviation Administration, Advisory Circular AC 20-53A, 1985; US Department of Transportation, Federal Aviation Administration, Advisory Circular AC 20-53B, Draft, 1991; EUROCAE WG 31, Aircraft Lightning Zoning Standard, ED-91, 1998], has been presented. Zoning proves to be quite similar between the three types of aircraft. Thanks to the feed-back on lightning strikes to Falcon, lightning traces have been observed on the fuselage for different flight conditions and aircraft. Observations are compared with the zoning performed by Dassault. A physical model, developed by ONERA, was used to simulate the sweeping of lightning on the fuselage of a Falcon 900. The results are in good agreement with the lightning traces observed on the fuselages.     

A319飞机APU启动故障可靠性调查

本文对A319飞机131-9A型APU启动不正常事件进行可靠性调查,对APU启动故障统计分析,对影响启动的部件采取如下措施:老式启动保险6KA质量差主动更换且飞机上配备6KA;启动马达-3构型降级为-2以提高寿命,后续再升级至更高寿命的-4构型;执行改装加长启动线路以降低启动电流;点火激励器软时限控制定期拆下送厂检测。通过针对性措施,有效减少了APU启动不正常事件的发生。     

TA2/Ni+Nb中间层/1Cr18Ni9Ti扩散焊接头的组织与性能

采用50μm纯Ni箔+10μm纯Nb箔复合中间层,在焊接温度840℃,880℃和920℃,压力4MPa以及保温时间60min的工艺下,对工业纯钛TA2和1Cr18Ni9Ti不锈钢进行了真空扩散焊实验,测试了接头的抗拉强度,并利用光学显微镜(OM)、扫描电镜(SEM)、能谱(EDS)和X射线衍射(XRD)对接头的组织结构、元素分布以及断口形貌和相组成进行了分析。结果表明:Ni+Nb复合中间层的存在成功阻止了Fe,Ti互扩散,实现了TA2与1Cr18Ni9Ti的可靠连接,接头的拉伸强度达到261MPa,该强度主要受剩余Ni箔控制,且焊接温度的变化对其影响不大。接头所生成反应层自不锈钢一侧起分别为FeCrNi固溶体、剩余Ni,Ni3Nb,剩余Nb以及TiNb魏氏体。     

基于ARM下VxWorks的嵌入式车载图形系统设计

为了实现嵌入式车载系统设计,采用软硬件协同设计技术路线。研究了基于ARM9的S3C2410处理器为核心的嵌入式车载软件的运行机制,包括系统硬件初始化,VxWorks操作系统内核的配置与装载,Vxworks下的LCD显示技术和触摸屏控制技术的应用实现车载仪表信息的显示与交换功能,并通过VxWorks多任务的进行控制。通过实验测试,系统随时进行车载娱乐、自主导航、信息查询等功能。方案实时性好,操作方便。     

SiO2f/SiO2复合材料自身及其与铜、不锈钢的钎焊

采用AgCuTi活性钎料,在880℃/10min规范下成功实现了SiO2f/SiO2自身、SiO2f/SiO2与Cu和SiO2f/SiO2与1Cr18Ni9Ti三种接头的连接。实验结果表明,三种接头中靠近SiO2f/SiO2母材的界面处均形成了一层薄薄的扩散反应层组织,反应层中出现了Ti和O的富集,根据两者的原子比例推断生成了TiO2相;另外,三种接头中心区都形成了由灰色相和白色相共同组成的Ag-Cu共晶组织,其中灰色相为Cu基固溶体,白色相为Ag基固溶体。接头剪切强度结果显示,SiO2f/SiO2/Cu接头剪切强度为12.4MPa,SiO2f/SiO2/1Cr18Ni9Ti接头剪切强度为18.4MPa,接头中的残余应力是决定接头强度大小的重要因素之一。     

单层薄型双波段雷达吸收涂层的研制

研制出一种新的雷达波吸收涂层（ＲＡＣ）。涂层厚度不超过０．５ｍｍ,在Ｘ、Ｋｕ两个频段范围内具有低于－４ｄＢ的反射率。该材料综合性能优异,是一种实用型飞行器隐身材料。     

改性双基推进剂老化燃烧性能实验研究

用Ｘ射线实时荧屏分析系统对人工加速老化的改性双基推进剂的燃烧性能进行试验研究,结果表明,人工加速老化对双基推进剂的燃速影响不大,但对推进剂的装药结构性能有较大影响。试验发现在７０°Ｃ的老化温度下２４天后,推进剂的结构破坏导致异常燃烧现象明显,辅助试验表明,６０°Ｃ９０天可以认为是该种推进剂的安全界限     

Zr-Al-(Ni-Cu)合金的非晶形成能力及热学性能

采用喷射铜模铸造法研究了Ni和Cu含量对Zr-Al-(Ni-Cu)四元合金的非晶形成能力的影响.利用X射线衍射仪分析了铸态合金的相结构,利用差示扫描量热仪研究了非晶合金的热学性能.结果表明:Zr-Al-(Ni-Cu)四元合金的非晶形成能力远大于Zr-Al-Ni和Zr-Al-Cu三元合金的非晶形成能力.Zr65Al7.5Ni10Cu17.5合金显示最高的非晶形成能力,其非晶形成临界直径可以达到7 mm.相似元素Ni和Cu在一定比例下共存,使液态合金的熵值增加,自由能降低,从而有效提高了合金的非晶形成能力.