多维动态参数的多层Bayes融合估计

在多维动态参数的分层模型下，运用多层Bayes估计方法和离散线性模型状态估计方法，给出了动态参数的Bayes融合估计，并以飞行器试验分析的一些例子，说明方法的运用。     

Genesis on-board determination of the solar wind flow regime

Some of the objectives of the Genesis mission require the separate collection of solar wind originating in different types of solar sources. Measurements of the solar wind protons, alpha particles, and electrons are used on-board the spacecraft to determine whether the solar-wind source is most likely a coronal hole, interstream flow, or a coronal mass ejection. A simple fuzzy logic scheme operating on measurements of the proton temperature, the alpha-particle abundance, and the presence of bidirectional streaming of suprathermal electrons was developed for this purpose. Additional requirements on the algorithm include the ability to identify the passage of forward shocks, reasonable levels of hysteresis and persistence, and the ability to modify the algorithm by changes in stored constants rather than changes in the software. After a few minor adjustments, the algorithm performed well during the initial portion of the mission. This revised version was published online in August 2006 with corrections to the Cover Date.     

Summary of quantitative interpretation of IMAGE far ultraviolet auroral data

Direct imaging of the magnetosphere by instruments on the IMAGE spacecraft is supplemented by simultaneous observations of the global aurora in three far ultraviolet (FUV) wavelength bands. The purpose of the multi-wavelength imaging is to study the global auroral particle and energy input from the magnetosphere into the atmosphere. This paper describes the method for quantitative interpretation of FUV measurements. The Wide-Band Imaging Camera (WIC) provides broad band ultraviolet images of the aurora with maximum spatial resolution by imaging the nitrogen lines and bands between 140 and 180 nm wavelength. The Spectrographic Imager (SI), a dual wavelength monochromatic instrument, images both Doppler-shifted Lyman-α emissions produced by precipitating protons, in the SI-12 channel and OI 135.6 nm emissions in the SI-13 channel. From the SI-12 Doppler shifted Lyman-α images it is possible to obtain the precipitating proton flux provided assumptions are made regarding the mean energy of the protons. Knowledge of the proton (flux and energy) component allows the calculation of the contribution produced by protons in the WIC and SI-13 instruments. Comparison of the corrected WIC and SI-13 signals provides a measure of the electron mean energy, which can then be used to determine the electron energy flux. To accomplish this, reliable emission modeling and instrument calibrations are required. In-flight calibration using early-type stars was used to validate the pre-flight laboratory calibrations and determine long-term trends in sensitivity. In general, very reasonable agreement is found between in-situ measurements and remote quantitative determinations.     

Heliosphere-Geosphere Interactions Using Low Energy Neutral Atom Imaging

Development of the low energy neutral atom (LENA) imager was originally motivated by a need to remotely sense plasma heating in the topside ionosphere, with the goal of greatly enhanced temporal resolution of an otherwise familiar phenomenon. During ground test and calibration, the LENA imager was found to respond to neutral atoms with energies well above its nominal energy range of 10–750 eV, up to at least 3–4 keV, owing to sputtering interactions with its conversion surface. On orbit, LENA has been found to respond to a ubiquitous neutral atom component of the solar wind, to the neutral atoms formed by magnetosheath interactions with the geocorona during periods of high solar wind pressure, and to the interstellar neutral atoms flowing through the heliosphere during the season of maximal relative wind velocity between spacecraft and interstellar medium. LENA imaging has thus emerged as a promising new tool for studying the interplanetary medium and its interaction with the magnetosphere, in addition to the ionospheric heating and outflow that result from this interaction. LENA emissions from the ionosphere consist of a fast component that can be observed at high altitudes, and slower components that evidently create a quasi-trapped extended superthermal exosphere. The more energetic emissions are responsive to solar wind energy inputs on time scales of a few minutes.     

加力用气冷与气动雾化喷油杆的性能研究

本文提出了一种新型加力用喷油杆方案—气冷与气动雾化喷油杆。该方案既可降低喷油杆壁温,又可将冷却排气用于雾化而具有气动雾化的特点。本文用示温漆和红外热像仪对新型喷油杆的冷却效果进行了研究,用 PDA对其雾化性能进行了研究,并将其与 V型稳定器进行匹配燃烧试验,探讨了其对燃烧性能的影响。试验表明该新型喷油杆的冷却方案初步可行,并且它对雾化和燃烧性能的改善也表明将冷却气用于雾化是可行的。      

现代飞机制造成本控制方法研究

介绍了作业成本法(Activity-BasedCosting-ABC)及其全新的成本管理和控制思想。通过对工业工程(IndustryEngineering-IE)的技术特性与ABC算法内在联系的探讨,建立了一个IE+ABC成本控制体系,目的是对飞机制造过程的成本实施有效控制。企业实证初步表明了这个成本控制体系的实际应用效果及其研究推广价值。     

飞机谱载荷下裂纹扩展的三维约束效应

研究裂纹端部三维应力约束、塑性约束和位移约束等对谱载疲劳裂纹扩展的影响。用适于三维应力状态的修正条带屈服模型 ( Modified Strip Yield Model)计算与裂纹扩展有关的三维约束因子。利用所得约束因子的理论解改进 NASA多年来发展的 FASTRAN-II寿命预测软件 ,使其避免了依赖经验确定的约束因子进行寿命预测的局限 ,仅利用一组常幅疲劳裂纹扩展数据和材料的常规机械性能便可预测飞机谱载下的裂纹扩展寿命。对多种谱型、应力水平、过载比和材料的组合情况进行了分析 ,预测寿命与试验结果吻合很好 ,证明本文方法和改进软件可以用于实际结构的寿命预测。     

含椭圆分层复合材料层板三维问题的三角级数能量解法

根据叠加原理将含有椭圆形内部分层的层板在横向载荷作用下的受力状态进行分解 ,从而将分层问题归结为在分层表面上的附加剪切载荷作用下层板附加位移与附加应力的分析 ,并据此建立了一个仅包含分层区的力学模型。然后利用双三角级数构造满足层板分层区位移边界条件的位移模态。最后 ,应用最小势能原理确定位移解。计算结果收敛 ,挠度收敛尤为迅速。     

NEW DYNAMIC SLOT ASSIGNMENT SCHEME OF SELF-ORGANIZED TDMA VHF DATA LINK

Self- organized TDMA ( S- TDMA ) protocolproposed by Johnsson[1] in aeronautical VHF-band is the representation of the new generationVHF aeronautic data communication system.　　 A mobile station or a ground station can oc-cupy one time slot. A group of slots that span aperiod of one minute constitute one superframe.Each station broadcasts current and future slotreservation information periodically.A stationwill build up and maintain a reservation tablethrough receiving the periodic bro…     

支架的主动约束层阻尼处理

利用主动控制和约束层阻尼处理优势互补,构成既有主动控制高效智能、又有约束层阻尼处理稳定可靠特点的主动约束层阻尼振动控制系统。采用一阶剪切理论,利用有限元方法,研究了航天结构中常用构件支架的振动控制,为改进支架的动态特性提供可靠的理论指导。