Optimal mission planning of the reconfiguration process of satellite constellations through orbital maneuvers: A novel technical framework

In this paper, a general new methodology is presented for the orbital reconfiguration of satellite constellations on the basis of Lambert targeting theorem. In view of the cost and risk reduction, it is very important to consider the problem of satellite constellation reconfiguration with the two constraints of overall mission cost minimization and the desired final configuration. Hence, the dependent non-simultaneous deployment approach is proposed to minimize overall fuel cost. Despite the fact that the satellites deploy in a non-simultaneous manner, supplementary phasing maneuvers on the target orbital pattern to achieve the desired orbital configuration are avoided. Moreover, a novel idea is presented to optimize the flight of satellites, which plays an important role in complying with the constraint of overall fuel cost minimization as much as possible. In order to achieve the global optimal solution of the satellite constellation reconfiguration problem, the efficient hybrid Particle Swarm Optimization/Genetic Algorithm (PSO/GA) technique, is implemented. Finally, to indicate the superiority of the presented method, a comparison to the simultaneous maneuver viewpoint is made on a number of representative cases. The obtained results imply significant reduction of reconfiguration costs by employing the proposed method.     

Microstructure,thermophysical property and ablation behavior of high thermal conductivity carbon/carbon composites after heat-treatment

Uni-directional carbon/carbon composites with high thermal conductivity are suitable to supply continuous thermal protection for future reentry vehicles since they could reduce surface temperature and ablation rates simultaneously in harsh environments. In this work, the high thermal conductivity carbon/carbon composites were prepared by chemical vapor infiltration. After heat-treatment, both their open porosity and internal friction increase due to the fiber/matrix thermal expansion mismatch; while their thermal conductive performance become better due to more complete carbon structure. With raising heat-treatment temperature from 1800 °C to 2450 °C, the mass and linear ablation rates of C/C composites with fibers vertical to the oxyacetylene torch for 60 s decrease from 0.66 mg/s and 2.95 μm/s to 0.51 mg/s and 2.05 μm/s respectively. The improved ablation resistance is resulted from the increased thermal conductivity from 282 to 508 W/(m·K) and more carbon fibers exposed to the flame during ablation, which have better oxidation resistance than those of carbon matrix. While such ablation rates become larger for composites with fibers parallel to the flame, from 1.02 mg/s and 3.73 μm/s to 1.28 mg/s and 5.01 μm/s respectively since the ablation occurred more easily through gaps at the fiber/matrix interfaces, which become larger and are always exposed to the flame for this case.     

复合材料MMB试件I-II混合型层间裂纹扩展分析

基于经典层合板理论及双线性黏聚区本构关系，建立了含一般分层裂纹层合板的理论模型，对I-Ⅱ混合型弯曲（MMB）断裂试件进行了裂纹扩展理论分析。提出了一种I-Ⅱ混合型断裂叠加模型，引入I型裂纹分量的刚体转动位移，同时考虑了裂纹长度超过试件半长后中部载荷分量对裂纹扩展的闭合效应，并根据黏聚区力学响应，分段获得了位移函数通解。结合叠加模型的边界条件与连续性条件，分析了MMB试件的裂纹扩展过程，求解获得了载荷-位移曲线。通过与梁模型预测以及试验结果进行对比，验证了本文模型对I-Ⅱ混合型裂纹扩展预测的有效性和准确性，并讨论了初始断裂模式混合比及闭合效应对裂纹扩展过程的影响。结果表明：初始Ⅱ型裂纹比重较大时，中部载荷的闭合效应更为明显，可能出现I型裂纹完全闭合的情况；裂纹扩展过程中，当裂纹长度小于试件半长时，断裂混合比基本保持常数；当裂纹扩展超过试件半长后，闭合效应明显，混合裂纹形式逐渐向单一型断裂模式退化。     

空域资源优化配置及调整策略研究

近年来,不断增长的空中交通需求以及有限的空域资源之间的矛盾日益突出,尤其是在飞行量密集的多机场地区。在研究如空域灵活使用等国外空域管理方面的经典理论,以及已在实践应用层面取得的成果和经验的基础上,结合中国空域自身的条件及特点,从低空空域资源、军民航协调机制、多机场地区空域资源统筹三个方面作为切入点,提出了相应的空域资源配置及调整的构想,并详细阐述了实施的方法,得出了采用更科学优化和共享模式的空域资源使用方式才是解决中国空域紧缺的有效手段。     

风扇出口导向叶片低噪声设计Ⅰ:方法与优化

作为"风扇出口导向叶片（Outlet Guide Vanes，OGV）低噪声设计"系列文章的第1篇，本文在现有压气机气动设计流程的基础上，加入了噪声评估过程，建立了基于通流设计的气动/声学一体化设计方法。为提高设计阶段的评估速度，以三维升力面理论与管道声学理论为基础，从通流设计和造型设计输出中提取参数，结合转子尾迹模型，建立了转/静干涉噪声的解析预测模型。以现代大涵道比涡扇发动机风扇/增压级为对象，采用该模型系统分析了OGV轴向掠形与周向倾斜对转/静干涉噪声的影响，获取了轴向掠形角与周向倾斜角等三维设计参数与风扇噪声的关系图谱，初步确定了低噪声设计较优降噪量的掠和倾组合方案。以此为基础，在保持叶尖子午投影位置和弦长不变的前提下，将叶片前缘和径向积叠进行参数化，采用遗传算法进一步开展了OGV的低噪声优化设计，最终获得了2个优化方案，预估的降噪量达到了8 dB。     

分布式数据采集控制系统的现状及发展趋势

综述了ＤＣＳ系统的形成，现状及今后的发展方向，阐明了应用远智能Ｉ／Ｏ改进ＤＣＳ系统的优越性及向ＦＣＳ系统的过渡。     

生长在Si上的GaAs外延膜中有关深能级缺陷与其形貌间的关联研究

由于在GaAs和Si单晶材料间有着很大的格子常数及线性热膨胀系数差别，所以在St上生长的GaAs异质外延薄膜（GaAs／Si）中会存在着界面失配形变与高密度的结构缺陷。我们的实验显示，GaAs／Si外延膜的无序与其生长条件有关，尤其与其［As］／［Ga］比密切相关。与GaAs／Si无序相关的失配位错、线位错及畴区的形貌已用扫描电子显微镜作了观察;与深能级相关的缺陷与其形貌间的关联也已用实验说明。对于高有序GaAs／Si外延膜来说，其与离域相关的主发光峰的强度对温度的变化服从阿兰纽斯方程，而对低有序的GaAs／Si外延膜来说，其与局域相关的主发光峰的强度对温度的变化关系则遵循对无定型半导体才成立的另一种方程。     

Composition of the Volatile Material in Halley's Coma from In Situ Measurements

The investigation of the volatile material in the coma of comets is a key to understanding the origin of cometary material, the physical and chemical conditions in the early solar system, the process of comet formation, and the changes that comets have undergone during the last 4.6 billion years. So far, in situ investigations of the volatile constituents have been confined to a single comet, namely P/Halley in 1986. Although, the Giotto mission gave only a few hours of data from the coma, it has yielded a surprising amount of new data and has advanced cometary science by a large step. In the present article the most important results of the measurements of the volatile material of Halley's comet are summarized and an overview of the identified molecules is given. Furthermore, a list of identified radicals and unstable molecules is presented for the first time. At least one of the radicals, namely CH₂, seems to be present as such in the cometary ice. As an outlook to the future we present a list of open questions concerning cometary volatiles and a short preview on the next generation of mass spectrometers that are being built for the International Rosetta Mission to explore the coma of Comet Wirtanen. This revised version was published online in June 2006 with corrections to the Cover Date.     

Comparison of Polar and Equatorial Coronal Holes Observed by UVCS/SOHO: Geometry and Physical Properties

We analyzed UVCS/SOHO data and compared the H I Lyα (121.6 nm) and O VI (103.2 nm, 103.7 nm) emission in the polar and equatorial coronal holes. We found that the emission lines have similar characteristics in these two types of coronal holes. Both types show evidence for superradially diverging boundaries. The latitudinal distribution of the O VI line ratio may indicate that the equatorial coronal hole has O⁺⁵ outflow velocities lower than in the polar coronal holes. This revised version was published online in June 2006 with corrections to the Cover Date.     

Multi-point observations and modeling of subauroral polarization streams (SAPS) and double-peak subauroral ion drifts (DSAIDs): A case study

While subauroral polarization streams (SAPS) are well recognized as representatively one of the most important features of magnetosphere-ionosphere (M-I) coupling processes in the subauroral region, the double-peak subauroral ion drifts (DSAIDs) is a newly recognized ionospheric phenomenon, categorized as a subset of subauroral ion drifts (SAIDs). In this study, we investigate both SAPS and DSAIDs that appear during the storm main phase of the 17 March 2015 event through a combination of multi-point observations and numerical simulations. We find that when SAPS/DSAIDs are observed by the DMSP spacecraft near the dusk subauroral region, strong electric fields are detected minutes later by the Van Allen Probes almost in the same conjugate region near the equatorial plane. Numerical simulations are carried out not only to reveal the global context and dynamic evolution of the SAPS in both the magnetospheric and ionospheric systems, but also to aid the understanding of the effect of conductance on the DSAIDs. Our results confirm that SAPS are indeed associated with Region 2 field-aligned currents (FACs) flowing into the low conductance region. On the other hand, the DSAIDs may be related to the double-conductance-trough in the subauroral region.