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131.
132.
基于OSG的飞行仿真系统视景平台的研究与开发 总被引:2,自引:1,他引:2
分析了飞行仿真系统的特征,并对其应用需求进行分析,在此基础上完成了系统视景平台的规划与设计。采用OpenSenceGraph(OSG)开源场景图形库对视景平台进行开发,针对需求分析实现了飞行仿真系统视景平台各模块的基本功能。 相似文献
133.
134.
针对民用飞机故障的动态特性及维修体制,在符号有向图(SDG)模型中引入动态元素,并融合系统结构模型,提出一种结构和参数能随工况变化而调整的增强型有向图(ESDG)模型。进而提出基于故障依赖矩阵的相容根树搜索算法与分层诊断策略,能解决实际排故中常常因部分状态未测量而造成诊断信息缺失的问题。该方法能满足分级维修中不同诊断精度的要求。多个工况的综合诊断进一步提高了推理分辨率。最后以某民机发动机引气系统为实例说明了该方法的有效性。 相似文献
135.
《中国航空学报》2016,(6):1730-1739
This paper derives a distance-based formation control method to maintain the desired formation shape for spacecraft in a gravitational potential field. The method is an analogy of a vir-tual spring-damper mesh. Spacecraft are connected virtually by spring-damper pairs. Convergence analysis is performed using the energy method. Approximate expressions for the distance errors and control accelerations at steady state are derived by using algebraic graph representations and results of graph rigidity. Analytical results indicate that if the underlying graph of the mesh is rigid, the convergence to a static shape is assured, and higher formation control precision can be achieved by increasing the elastic coefficient without increasing the control accelerations. A numerical exam-ple of spacecraft formation in low Earth orbit confirms the theoretical analysis and shows that the desired formation shape can be well achieved using the presented method, whereas the orientation of the formation can be kept pointing to the center of the Earth by the gravity gradient. The method is decentralized, and uses only relative measurement information. Constructing a distributed virtual structure in space can be the general application area. The proposed method can serve as an active shape control law for the spacecraft formations using propellantless internal forces. 相似文献
136.
137.
具有接触接合面的篦齿封严组件振动特性分析 总被引:2,自引:2,他引:2
运用弹性力学理论研究了篦齿封严组件及其减振结构之间过盈装配压力和接触刚度的求解方法,在此基础上给出了具有接触接合面的封严环/阻尼片组合结构动力特性的分析方法,并且研究了阻尼片厚度、阻尼片周向分布数量、装配过盈量等参数对结构动力特性的影响规律.转动情况下封严环离心应力与阻尼片厚度近似成线性关系;阻尼片的周向分布数量影响封严环的固有频率和振型;阻尼片沿周向分布数量越多,应力分布越均匀,封严环的离心应力越小. 相似文献
138.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(9):2119-2130
The aim of this work is the analysis of the mid-latitude ionospheric trough (MIT) using the Global Ionospheric Maps from IGS (GIMs) during the solar minimum, year 2008. This study was performed for different local times, 22, 00, 02 and 04 LT on the Northern and Southern hemisphere simultaneously. In the two hemispheres the MIT show asymmetric pattern. The high-latitude troughs are clearly distinguished in autumn and winter. Another feature is the longitudinal development towards the west of the geomagnetic pole covering a wider area in the Northern Hemisphere. Five empirical reference models were tested and compared with the MIT minimum position obtained from GIMs at different local times for both hemisphere. The results show a better agreement with the observations for the Northern Hemisphere specially with the Köehnlein & Raitt model. Fluctuations of 9 days and 27 days of the MIT minimum position are found, which could be related with the solar wind oscillations, especially for 00 and 02 LT in both hemisphere, suggesting a link between them. 相似文献
139.
《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2020,65(5):1402-1413
The present paper reports coordinated ionospheric irregularity measurements at optical as well as GPS wavelengths. Optical measurements were obtained from Tiny Ionospheric Photometer (TIP) sensors installed onboard the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) satellites. GPS radio signals were obtained from a dual frequency GPS receiver operational at Calcutta (22.58°N, 88.38°E geographic; geomagnetic dip: 32.96°; 13.00°N, 161.63°E geomagnetic) under the SCIntillation Network Decision Aid (SCINDA) program. Calcutta is located near the northern crest of Equatorial Ionization Anomaly (EIA) in the Indian longitude sector. The observations were conducted during the unusually low and prolonged solar minima period of 2008–2010. During this period, four cases of post-sunset GPS scintillation were observed from Calcutta. Among those cases, simultaneous fluctuations in GPS Carrier-to-Noise ratios (C/No) and measured radiances from TIP over a common ionospheric volume were observed only on February 2, 2008 and September 25, 2008. Fluctuations observed in measured radiances (maximum 0.95 Rayleigh) from TIP due to ionospheric irregularities were found to correspond well with C/N0 fluctuations on the GPS links observed from Calcutta, such effects being noted even during late evening hours of 21:00–22:00 LT from locations around 40° magnetic dip. These measurements indicate the existence of electron density irregularities of scale sizes varying over several decades from 135.6 nm to 300–400 m well beyond the northern crest of the EIA in the Indian longitude sector during late evening hours even in the unusually low solar activity conditions. 相似文献
140.
在发射带宽严格受限的约束下连续函数波形信号较传统矩形波形表现出了较高的频谱利用率优势和优良性能,很有可能应用到未来的全球卫星导航系统(GNSS,Global Navigation Satellite System)信号体制中.在建立导航信号波形设计准则的理论模型基础上,研究了7种可能适用于未来GNSS系统的新型信号波形,在典型的宽/窄发射带宽条件下,通过仿真评估了传统GNSS信号和新型GNSS信号的精度、抗多径、抗干扰等性能,优选出BOCc和MSK两种适用于不同环境的信号波形: 在频谱资源充足的情况下,BOCc信号具有最优的导航性能;在频率资源受限的情况下,MSK信号兼容性好,抗干扰能力强,拥有较好的导航性能.最后,结合两类信号波形的优缺点提出了我国新一代卫星导航系统信号波形设计的建议. 相似文献