Evolution of the orbital elements for objects with high area-to-mass ratios in geostationary transfer orbits

A new population of uncatalogued objects in geosynchronous Earth orbits (GEO), with a mean motion of about 1 rev/day and eccentricities up to 0.6, has been identified recently. The first observations of this new type of objects were acquired in the framework of the European Space Agency’s (ESA) search for space debris in GEO and the geostationary transfer orbit (GTO) using the ESA 1-m telescope on Tenerife. Earlier studies have postulated that the perturbations due to the solar radiation pressure can lead to such large eccentricities for GEO objects with a high area-to-mass ratio (A/M). The simulations showed that the eccentricities of GEO objects with large A/M exhibit periodic variations with periods of about one year and amplitudes depending on the value of A/M. The findings of these studies could be confirmed by observations from the ESA 1-m telescope on Tenerife.     

Dynamical evolution of high area-to-mass ratio debris released into GPS orbits

A large set of simulations, including all the relevant perturbations, was carried out to investigate the long-term dynamical evolution of fictitious high area-to-mass ratio (A/M) objects released, with a negligible velocity variation, in each of the six orbital planes used by Global Positioning System (GPS) satellites. As with similar objects discovered in near synchronous trajectories, long lifetime orbits, with mean motions of about 2 revolutions per day, were found possible for debris characterized by extremely high area-to-mass ratios. Often the lifetime exceeds 100 years up to A/M ∼ 45 m²/kg, decreasing rapidly to a few months above such a threshold. However, the details of the evolution, which are conditioned by the complex interplay of solar radiation pressure and geopotential plus luni-solar resonances, depend on the initial conditions. Different behaviors are thus possible. In any case, objects like those discovered in synchronous orbits, with A/M as high as 20–40 m²/kg, could also survive in this orbital regime, with semi-major axes close to the semi-synchronous values, with maximum eccentricities between 0.3 and 0.7, and with significant orbit pole precessions (faster and wider for increasing values of A/M), leading to inclinations between 30° and more than 90°.     

Indicators of black-hole mass and Eddington accretion ratio from QSO X-ray and UV spectra

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of the host galaxy’s bulge. An important way to explore this evolution would be to measure dependences of black-hole masses and Eddington accretion ratios over a range of redshifts, i.e., with cosmological age. For low redshift QSOs (and their lower luminosity Seyfert galaxy counterparts) it has been possible to infer black-hole masses from the luminosities and velocity dispersions of their host-galaxy bulges. These masses agree with those virial black-hole masses calculated from the Doppler widths of the broad Hβ emission lines. The latter method can then be extended to more distant and luminous QSOs, up to redshifts of 0.6 with ground-based optical observations. We discuss ways to extend these explorations to higher redshifts – up to 3 using the widths of QSOs’ broad UV emission lines, and in principle, and to redshifts near 4 from ground-based infrared observations of rest-frame Hβ at 2.5 μm. We discuss the possibility of investigating the accretion history of the higher redshift QSOs using measures of Eddington accretion ratio – the soft X-ray spectral index and the eigenvectors of Principal Components Analyses of QSOs’ UV emission-line spectra.     

关于适当布置构造柱以提高墙体承载力的探讨

针对当前七、八层砖混结构住宅在不增加墙体厚度的前提下，通过适当布置构造柱，来提高墙体承载力，因而达到增大使用面积的目的。     

穿越微下冲气流的飞翼布局无人机控制方法

微下冲气流是最危险的低空风切变形式,为在起降阶段安全穿越该气流,飞翼布局的无人机控制律应具有快速响应能力和良好的鲁棒性。针对大展弦比飞翼布局无人机舵面附加升力大和低速状态俯仰操纵效能低的特点,提出了舵面附加升力和机体气动力相结合的复合控制方案,改进了以输出误差为参考量的非线性指令分配策略,设计了基于迎角保护的指令分配策略。将风干扰和模型的不确定性视为未知扰动,采用自抗扰控制(ADRC)理论设计飞翼布局无人机非线性控制律,使之对风干扰和模型的不确定性进行估计补偿。仿真结果表明,复合控制与ADRC相结合的方法加速了航迹倾角的单位阶跃响应速度,使上升时间缩短了64%,同时能够实现对风干扰的有效观测和补偿,使高度损失低于2m;能够在风切变中有效保护迎角,使其维持在5.5°以内。因此,该方法能够为飞翼布局无人机安全平稳地穿越微下冲气流提供一种参考方案。     

油气比及进口参数对三级旋流器燃烧室性能的影响

对三级旋流器燃烧室进行了常压试验研究.研究首先设计研制了三级旋流器燃烧室模型和试验系统,然后在此基础上开展了不同进口速度、进口温度和油气比等参数影响三级旋流器燃烧室的流阻特性、点火特性、贫油熄火特性和燃烧效率特性等性能的试验研究.结果表明:该三级旋流器燃烧室可以在不同试验工况下顺利点火和稳定工作,点火性能基本不受进口速度的影响;总压损失系数随进口速度的增加而增大,而流阻系数随速度的增加而减小,燃烧室流动未进入"自模状态";随着进口温度的增加,点火、贫油熄火性能变好,燃烧效率提高.     

超声速串列静叶积叠优化分析

在进口超声速、气流转折角大的高负荷条件下,静叶通道中激波强度高,激波、附面层干扰引起的损失大,且静叶中三维流动引起的径向载荷分布不均匀,易产生角区分离。叶片积叠优化是提高风扇性能的一项有效技术。采用数值模拟的方式研究了不同积叠形式对优化串列静叶沿展向激波结构,改善叶排间流动匹配的作用。三维流动对比分析可以得出:高负荷串列静叶采用正弓形积叠,叶片展向载荷分布合理,静叶端壁角区分离损失减小,前后叶片排流动匹配较好,风扇性能进一步提高。     

核翼比法进行表面粗糙度的标定及测量

介绍了一种表面粗糙度标定及测量的新方法。通过标定一组标准样块的核翼比，可以实现该标定范围内待检样块的粗糙度测量，该方法稳定可靠，试验装置简单，数据处理方便，为表面粗糙度的非接触测量提供了较好的方案。     

TiAl/IN718合金过渡液相连接

采用过渡液相TLP(Transient Liquid Phase)连接技术,以金属Ti,Cu,Ni箔构成复合焊料连接TiAl和IN718合金.研究了保温时间对接头界面结构的影响.实验结果表明:采用Ti-Cu,Ti-Ni复合焊料可以制备无缺陷的接头,但2种焊料形成液相的过程和机理不同.由于在等温凝固过程中,从IN718合金中扩散过来的合金元素可在焊缝区聚集,从而在接头中形成亚层结构.通过对接头焊缝区的组织分析和硬度测试表明,在实验条件下Ti-Ni焊料的等温凝固过程持续时间比Ti-Cu的短.     

微型脉冲推力器点火启动过程计算与点火药量选择

建立了微型脉冲推力器点火启动模型,模型中考虑了两相流动和颗粒对推进剂表面的冲击传热。根据数值计算结果,给出了不同产物颗粒含量下的点火药量选择参考范围。该参考范围对于产物颗粒含量小于50%的点火药是适用的;由于过多的颗粒含量将对装药表面产生强烈的热力冲蚀破坏作用,产物颗粒含量超过50%的点火药不适合微型火箭发动机。