XILINX的FPGA芯片架构剖析

从芯片结构原理上分析了XILINX的Virtex系列芯片.结合微电子学相关知识,详细分析了芯片的基本结构、可配置功能逻辑、输入输出模块、可编程内连等方面.最后将该芯片与XILINX其它系列芯片相关内容进行了比较分析,给出了该芯片与其它各类不同芯片之间结构与性能上的差异.     

基于气/固耦合非定常流动的叶栅颤振分析

采用二维N-S方程／结构振动方程组耦合数值方法，分析计算了二维非定常气动力强迫振动条件下振动能量及气动力对叶栅所做的功，分别根据振动能量和气动力做功分析了叶栅的颤振特性。NACA0012和PROF叶栅在不同折合频率下气动参数随时间的变化表明，折合频率是影响叶栅颤振的重要因素。气固耦合方法得到的NA-CA0012叶栅颤振折合频率比非耦合的结果高，而对PROF叶栅则相反。这表明叶栅结构动力参数对其发生颤振时的折合频率影响很大且很复杂，要准确预测颤振应该考虑叶栅结构动力与气动力的耦合因素。     

基于Client/Server模式的敏捷制造信息系统方法

客户/服务器(Client/Server)采用并发服务器和socket编程方法,巧妙地解决了网络通信的同步问题。基于Client/Server模式,根据动态联盟的组织原则,提出了开放性的敏捷制造信息系统结构。这种结构实现了动态联盟中分散的制造资源的共享;维护了联盟单元在解决问题时的自主性;通过联盟单元间的双向委托协议,可以保证信息数据的一致性;保证了联盟单元组织不同结构的兼容性。解决了在组织动态联盟时的几个关键问题,为进一步开展敏捷制造方法奠定了基础。     

The Coma of Comet 9P/Tempel 1

As comet 9P/Tempel 1 approaches the Sun in 2004–2005, a temporary atmosphere, or “coma,” will form, composed of molecules and dust expelled from the nucleus as its component icy volatiles sublimate. Driven mainly by water ice sublimation at surface temperatures T > 200 K, this coma is a gravitationally unbound atmosphere in free adiabatic expansion. Near the nucleus (≤ 10² km), it is in collisional equilibrium, at larger distances (≥10⁴ km) it is in free molecular flow. Ultimately the coma components are swept into the comet’s plasma and dust tails or simply dissipate into interplanetary space. Clues to the nature of the cometary nucleus are contained in the chemistry and physics of the coma, as well as with its variability with time, orbital position, and heliocentric distance. The DI instrument payload includes CCD cameras with broadband filters covering the optical spectrum, allowing for sensitive measurement of dust in the comet’s coma, and a number of narrowband filters for studying the spatial distribution of several gas species. DI also carries the first near-infrared spectrometer to a comet flyby since the VEGA mission to Halley in 1986. This spectrograph will allow detection of gas emission lines from the coma in unprecedented detail. Here we discuss the current state of understanding of the 9P/Tempel 1 coma, our expectations for the measurements DI will obtain, and the predicted hazards that the coma presents for the spacecraft. An erratum to this article is available at .     

Deep Impact Mission Design

The Deep Impact mission is designed to provide the first opportunity to probe below the surface of a comet nucleus by a high-speed impact. This requires finding a suitable comet with launch and encounter conditions that allow a meaningful scientific experiment. The overall design requires the consideration of many factors ranging from environmental characteristics of the comet (nucleus size, dust levels, etc.), to launch dates fitting within the NASA Discovery program opportunities, to launch vehicle capability for a large impactor, to the observational conditions for the two approaching spacecraft and for telescopes on Earth.     

The History and Dynamics of Comet 9P/Tempel 1

Since its discovery in 1867, periodic comet 9P/Tempel 1 has been observed at 10 returns to perihelion, including all its returns since 1967. The observations for the seven apparitions beginning in 1967 have been fit with an orbit that includes only radial and transverse nongravitational accelerations that model the rocket-like thrusting introduced by the outgassing of the cometary nucleus. The successful nongravitational acceleration model did not assume any change in the comet’s ability to outgas from one apparition to the next and the outgassing was assumed to reach a maximum at perihelion. The success of this model over the 1967–2003 interval suggests that the comet’s spin axis is currently stable. Rough calculations suggest that the collision of the impactor released by the Deep Impact spacecraft will not provide a noticeable perturbation on the comet’s orbit nor will any new vent that is opened as a result of the impact provide a noticeable change in the comet’s nongravitational acceleration history. The observing geometries prior to, and during, the impact will allow extensive Earth based observations to complement the in situ observations from the impactor and flyby spacecraft.     

碳纤维涂层结构与性能的关系

 本文用抗氧化数Φ(无量纲)的概念来衡量碳纤维涂层的抗氧化能力。依据化学动力学导出了涂层抗氧化数与涂层结构参数的关系:Φ=KX/D。通过实验,研究了SiO_2及sic涂层结构及碳纤维上涂覆SiO_2及SiC涂层后的热失重及抗拉强度,求得涂层抗氧化数并与计算结果进行了比较。由此分析了涂层结构对抗氧化能力的影响。     

HRS定向凝固过程中固/液界面位置控制

 本文通过在计算机上模拟固/液界面位置受到控制的整个HRS定向凝固过程、求出使固/液界面稳定在隔热板及其附近时抽拉速度的调节规律。依此规律,利用一个以TP 801 B单板机为核心的控制系统对铸件的HRS定向凝固过程进行实时控制。用Al—4.5％Cu合金试样进行了验证试验。结果表明:受控HRS定向中、固/液界面很快趋近于隔热板并在定向过程中稳定在隔热板附近。对界面位置实行控制能有效提高固/液界面前沿温度梯度及其稳定性明显改善定向凝固显微组织。     

TiC/Al复合材料在锌液中均匀化机理分析

采用自蔓延高温合成（SHS）法制备高TiC颗粒含量的TiC／Al复合材料。利用自制的实验装置研究复合材料中TiC颗粒在静止锌液中的均匀化过程。结果表明：当锌液温度低于铝的熔点时，TiC／Al复合材料置于锌液后，锌向其内部扩散，引起复合材料表层内液相线温度降低，当表层内Al-Zn合金的液相线温度等于或低于锌液温度时，Al-Zn合金便处于熔融状态，TiC颗粒随其一起从TiC／Al复合材料块上脱落，并不断地向锌液内部传输，最终均匀分布在锌液中；而当锌液温度高于铝熔点时，TiC／Al复合材料置入后，锌和铝同时进行扩散，但是当复合材料表面温度达到铝熔点时，铝开始熔化，铝的熔化导致TiC颗粒的脱落，脱落下来的TiC颗粒不断向锌液内部传输，最终均匀分布在锌液中。     

基于宽带综合业务数字网／ATM的航天测控网管理系统组成及性能研究

本文根据宽带综合业务数字网／ATM的特点、功能及发展前景，针对我国航天测控网的现状和未来测控任务的需求，提出了我国航天测控网管理系统的构成、管理模式等思想。这些对航天测控网管理系统的发展具有一定的参考价值。