单组元300N发动机低温试验研究

为探究低温环境下单组元300N发动机的工作特性，揭示影响发动机低温性能的主要影响因素，以300N发动机为试验对象，开展了模拟飞行工况的发动机低温试验。给出了低温试验研究方法，分别从温度差异对发动机性能影响、催化剂活性差异对发动机低温启动特性影响和低温对电磁阀响应特性影响等方面获得研究结果。结果表明，低温是影响发动机低温性能的主要影响因素，-48℃条件催化剂无法完成推进剂的催化分解，发动机发生爆炸；-30℃条件下起活时间为80.5～87.5ms，发动机可正常启动，且启动温度与起活时间呈指数关系；催化剂批次差异也对发动机低温工作性能产生一定影响，不同批次催化剂低温起活时间的差异可达91ms；低温试验过程中，电磁阀的关闭受到低温推进剂粘性和背压的影响，产生了明显的迟滞现象，延迟时间约100ms，对发动机在轨的精准控制存在一定影响。     

中国空间探测领域40年发展

中国空间科学学会成立的40年，是中国空间探测逐渐走进世界舞台的40年，空间探测极大推动了空间科学和相邻学科的发展，也影响到经济、军事和日常生活诸多方面.本文简要回顾了从空间探测专业委员会成立的1980年至今，中国空间探测领域的主要发展历程，包括探空火箭、高空气球、科学卫星、月球与行星探测、载人航天空间探测、遥感卫星地面站等主要项目、进展和所取得的成果，对未来若干年空间探测的发展进行了展望.      

空间站燃烧科学实验系统设计

建立空间站燃烧实验系统，可满足未来空间微重力燃烧实验系统需求.通过空间站微重力燃烧实验研究，可拓展空间燃烧学研究.根据所要实现的功能及燃烧实验需求，对中国空间站燃烧柜的燃烧科学实验系统进行了设计和分析.燃烧科学实验系统由8个子系统组成，是一个适合开展气、液、固多种燃料燃烧实验的综合性实验系统.考虑到强度设计要求，在完成方案设计后，对系统进行了有限元分析，并在研制的结构件上进行了力学环境实验.实验与分析结果表明，本文设计的实验系统能够满足环模实验的要求，结构合理可行.      

Preliminary study on heat flux measurement data of TT-0 flight test

With the explosive development of aerospace science, the design of the new generation airliner at higher speeds is attracting more attentions. To achieve this goal, it is necessary to achieve accurate prediction of the aerodynamic heating / force loads and successful reduction of drag and heat flux. As a remedy for the existing studies which are based upon the CFD and wind tunnel tests, this study presents a flight test for the drag and heat reduction spike technology. The principal goals of this flight test were to provide reference for verifying the accuracy of the prediction technology on ground and promote the development of the drag and heat reduction technology. By adopting the OS-X rocket, the TT-0 test vehicle designed by Shenyang Aircraft Design & Research Institute reached a maximum Mach number of 5.8 and a maximum altitude of 38 km. Hypersonic and supersonic pressure data by pressure scanning valves and heat fluxes by gauges at different locations were obtained successfully. Also, heat fluxes obtained by in-house CFD code are illustrated in comparison with the flight data. The results indicate that the numerical errors are large in most cases. More technologies, such as more CFD codes and more numerical procedures, should be adopted to conduct studies on this issue in the future.     

一种使用Rhapsody-Simulink 工具链开发嵌入式软件的方法

描述了一种以DOORS 管理的软件需求为输入，用Rhapsody 进行软件框架建模并验证，而对部分软 件单元使用Simulink 进行详细设计、验证，然后将Simulink 模型导入Rhapsody 模型中形成完整软件配置项的 嵌入式软件开发方法。     

Case study of inclined sporadic E layers in the Earth’s ionosphere observed by CHAMP/GPS radio occultations: Coupling between the tilted plasma layers and internal waves

We have used the radio occultation (RO) satellite data CHAMP/GPS (Challenging Minisatellite Payload/Global Positioning System) for studying the ionosphere of the Earth. A method for deriving the parameters of ionospheric structures is based upon an analysis of the RO signal variations in the phase path and intensity. This method allows one to estimate the spatial displacement of a plasma layer with respect to the ray perigee, and to determine the layer inclination and height correction values. In this paper, we focus on the case study of inclined sporadic E (E_s) layers in the high-latitude ionosphere based on available CHAMP RO data. Assuming that the internal gravity waves (IGWs) with the phase-fronts parallel to the ionization layer surfaces are responsible for the tilt angles of sporadic plasma layers, we have developed a new technique for determining the parameters of IGWs linked with the inclined E_s structures. A small-scale internal wave may be modulating initially horizontal E_s layer in height and causing a direction of the plasma density gradient to be rotated and aligned with that of the wave propagation vector k. The results of determination of the intrinsic wave frequency and period, vertical and horizontal wavelengths, intrinsic vertical and horizontal phase speeds, and other characteristics of IGWs under study are presented and discussed.     

多航天器协同探测效能影响参数不确定性分析

为解决传统基于蒙特卡洛仿真的探测效能不确定性分析评价方法中时间效率低，参数关系映射单一的问题，提出一种基于神经网络的不确定性分析方法，利用人工神经网络在拟合回归分析上的非线性特性，设计了能够替代复杂系统的神经网络结构，能够通过少量仿真计算结果作为训练样本实现模型的收敛并能有效反映被替代系统的原有特性。选择以一个多航天器的天文观测任务作为典型用例，建立了仿真分析模型，并与蒙特卡洛仿真方法结果进行了对比，验证了此方法的准确性和计算效率。     

Global ionospheric scintillations revealed by GPS radio occultation data with FY3C satellite before midnight during the March 2015 storm

Global observations of S4 amplitude scintillation index by the GPS Occultation Sounder (GNOS) on FengYun-3 C (FY3C) satellite reveal global dynamic patterns of a strong pre-midnight scintillations in F-region of the ionosphere during the St. Patrick’s Day geomagnetic super storm of 17–19 March 2015. The observed strong scintillations mainly occurred in the low latitudes, caused by equatorial plasma bubbles. During the main storm phase (March 17), the scintillations were first triggered in the New Zealand sector near 160°E longitudes, extending beyond 40°S dip latitude. They were also enhanced in the Indian sector, but significantly suppressed in East Asia near 120°E longitude and in Africa around 30°E longitude. During the initial recovery phase (March 18–19), the global scintillations were seldom observed in GNOS data. During the later recovery phase (after March 19), the scintillations recovered to the pre-storm level in Indian, African, and American sectors, but not in East Asian and any of Pacific sectors. These results closely correlate with observations of the density depletion structures by the Communication/Navigation Outage Forecasting System (C/NOFS) satellite, and ground-based instruments. Such consistency indicates reliability of our scintillation sensing approach even in a case-by-case comparison study. The prompt penetration electric field and disturbance dynamo electric field are suggested as the main factors that control the enhancement and inhibition of the scintillations during the storm, respectively.     

Homologous flare–CME events and their metric type II radio burst association

Active region NOAA 11158 produced many flares during its disk passage. At least two of these flares can be considered as homologous: the C6.6 flare at 06:51 UT and C9.4 flare at 12:41 UT on February 14, 2011. Both flares occurred at the same location (eastern edge of the active region) and have a similar decay of the GOES soft X-ray light curve. The associated coronal mass ejections (CMEs) were slow (334 and 337 km/s) and of similar apparent widths (43° and 44°), but they had different radio signatures. The second event was associated with a metric type II burst while the first one was not. The COR1 coronagraphs on board the STEREO spacecraft clearly show that the second CME propagated into the preceding CME that occurred 50 min before. These observations suggest that CME–CME interaction might be a key process in exciting the type II radio emission by slow CMEs.     

齿轮槽头型新型标准件安装工艺与试验研究

航空制造领域大量采用了如螺栓连接的标准件连接,随着新型飞机性能的提高,长寿命、高疲劳强度和高振动环境等指标对标准件的使用提出了更高的要求.本文通过开展齿轮槽头型新型标准件安装工艺与试验研究,一方面确定了该型标准件安装力矩等关键工艺参数及对复合材料的适用性,为其装机和使用提供理论依据及数据支持;另一方面,也对开展新型标准件安装工艺与试验的研究方法进行了有益的探索,对逐步形成一套完善的试验方法规范具有很好的指导作用.