基于区间分析法的防冰引气管路系统故障树分析

针对防冰引气管路系统故障树分析中底事件故障率和概率统计信息的不确定性,基于区间分析法开展某型飞机防冰引气管路系统可靠性评估。根据防冰引气管路系统原理和故障发生机理建立系统的故障树,并采用区间概率来描述底事件失效概率的不确定性。计算结果表明:区间分析法在分析防冰引气管路系统故障树时只需要底事件失效概率的取值范围,而不要求其详细的概率统计信息,因而其适用面更广,更适合实际工程问题的需要。     

Form-finding methods for deployable mesh reflector antennas

Deployable high-frequency mesh reflector antennas for future communications and obser- vations are required to obtain high gain and high directivity. In order to support these new missions, reflectors with high surface accuracy are widely required. The form-finding analysis of deployable mesh reflector antennas becomes more vital which aims to determine the initial surface profile formed by the equilibrium prestress distribution in cables to satisfy the surface accuracy requirement. In this paper, two form-finding methods for mesh reflector antennas, both of which include two steps, are pro- posed. The first step is to investigate the prestress design only for the cable net structure as the circum- ferential nodes connected to the supporting truss are assumed fixed. The second step is to optimize the prestress distribution of the boundary cables connected directly to the supporting truss considering the elastic deformation of the antenna structure. Some numerical examples are carried out and the simulation results demonstrate the proposed form-finding methods can warrant the deformed antenna reflector surface matches the one by design and the cable tension forces fall in a specified range.     

基于FFT含有饱和环节的非线性等效系统的方法研究

基于快速傅里叶变换(FFT)方法,对系统的输入和输出信号进行快速傅里叶变换,对含有高次谐波的输出信号进行滤波,得到期望主频率的傅里叶频谱,然后进行傅里叶反变换,求得在各主频率下的幅值和相位.利用MATLAB中的非线性最小二乘拟配方法得到含有非线性环节的飞机纵向飞行控制系统的频域等效线性模型.这种方法也为含有非线性环节的飞机纵向飞行控制系统的飞行品质评估提供了一种可行的方法.     

Ionospheric electron density over Resolute Bay according to E-CHAIM model and RISR radar measurements

In this study, predictions of the E-CHAIM ionospheric model are compared with measurements by the incoherent scatter radars RISR at Resolute Bay, Canada, in the northern polar cap. Reasonable coverage was available for all seasons except winter for which no conclusions were drawn. It is shown that ratios of the model-to measured electron densities are close to unity in the central part of the F layer, around its peak. This is particularly evident for summer daytime. Distributions of the ratios are wider for other seasons indicating larger number of cases when the model underestimates or overestimates. E-CHAIM underestimates the electron density at ionospheric topside and bottomside by ～ 10–20 %. At the bottomside, the underestimations are strongest in summer and equinoctial nighttime. At the topside, the underestimations are strongest in autumn nighttime. Model overestimations are noticeable in the middle part of the F layer during dawn hours in autumn. Overall, the model tends to not predict highest-observed peak electron densities and the largest-observed heights of the peak.     

Improved interpretation of solar wind ion measurements via high-resolution magnetic field data

The Wind   spacecraft’s Faraday cups (FC) continue to produce high-quality, in situ observations of thermal protons (i.e., ionized hydrogen) and α$\alpha$-particles (i.e., fully ionized helium) in the solar wind. By fitting a Wind/FC ion spectrum with a model velocity distribution function (VDF) for each particle species, values for density, bulk velocity, and temperature can be inferred. Incorporating measurements of the background magnetic field from the Wind Magnetic Field Investigation (MFI) allows perpendicular and parallel temperature components to be separated. Prior implementations of this analysis averaged the higher-cadence Wind/MFI measurements to match that of the Wind/FC ion spectra. However, this article summarizes recent and extensive revisions to the analysis software that, among other things, eliminate such averaging and thereby account for variations in the direction of the magnetic field over the time taken to measure the ions. A statistical comparison reveals that the old version consistently underestimates the temperature anisotropy of ion VDF’s: averaging over fluctuations in the magnetic field essentially blurs the perpendicular and parallel temperature components, which makes the plasma seem artificially more isotropic. The new version not only provides a more accurate dataset of ion parameters (which is well suited to the study of microkinetic phenomena), it also demonstrates a novel technique for jointly processing particle and field data. Such methods are crucial to heliophysics as wave-particle interactions are increasingly seen as playing an important role in the dynamics of the solar wind and similar space plasmas.     

A point-wise least squares spectral analysis (LSSA) of the Caspian Sea level fluctuations,using TOPEX/Poseidon and Jason-1 observations

The Caspian Sea has displayed considerable fluctuations in its water level during the past century. Knowledge of such fluctuation is vital for understanding the local hydrological cycles, climate of the region, and construction activities within the sea and along its shorelines. This study established a point-wise satellite altimetry approach to monitor the fluctuations of the Caspian Sea using a complete dataset of TOPEX/Poseidon for the period 1993 to the middle of 2002, and its follow-on Jason-1 for the period 2002 to August 2009. Therefore, 280 virtual time-series were constructed to monitor the fluctuations. The least squares spectral analysis (LSSA) method is, then employed to find the most significant frequencies of the time-series, while the statistical method of principle component analysis (PCA) is applied to extract the dominant variability of level variations. The study also used the observations of TOPEX/Poseidon and Jason-1 over the Volga River along with 5 years of Volga’s water discharge to study its influence on the Caspian Sea level changes. The LSSA results indicate that the lunar semidiurnal (M2) and the Sun semidiurnal (S2) frequencies are the main tidal frequencies of the Caspian Sea with the mean amplitude of 4.2 and 2.8 cm, respectively. A statistically significant long-term frequency (12.5-years period) is also found from altimetry and tide gauge observations. A phase lag, related to the inter-annual frequencies of the Volga River was detected from the point-wise time-series showing level propagation from the northwest to the southeast of the sea. The cross-correlation between the power spectrum of Volga and that of the northern-most, middle, and southern-most points within the Caspian Sea were respectively 0.63, 0.51 and 0.4 of zero-lag correlation, corroborating the influence of the Volga River. The result of PCA also shows that different parts of the Caspian Sea exhibit different amplitudes of level variations, indicating that the point-wise approach, when employing all available satellite measurements could be a suitable method for a preliminary monitoring of this inland water resource as it gives accurate local fluctuations.     

时间触发AFDX网络的设计和实时性分析

时间触发机制可以近一步提高航空电子全双工交换式以太网(AFDX,Avionics Full Duplex Switched Ethernet)的确定性,保障时间关键消息具有完全的时间确定性.将时间触发机制引入了AFDX网络,设计了时间触发ADFX网络(TTAFDX,Time-Triggered AFDX)的体系结构,包括协议栈、虚拟链路类型、端系统调度、交换机调度、透明通信机制和降级通信机制,并且设计了端系统和交换机的时刻调度算法.对TTAFDX网络从理论和仿真实验两方面进行了分析,验证了TTAFDX网络对时间关键消息的完全时间确定性的保障.     

卫星星体对多波束天线的散射影响分析

地球静止轨道(GEO)移动通信卫星,多采用大反射面天线及多馈源组成的空间可展开多波束天线系统,具有更高的天线增益,并提高了整体系统性能,但由于过于庞大的天线反射面和馈源阵列,在整星结构构型布局中难免由于卫星星体或其它机构部件的存在而造成散射.文章主要针对GEO移动通信卫星星体对多波束天线散射影响问题,利用仿真分析软件,...     

卫星贮箱故障时液体燃料运动特性仿真分析

不少在轨卫星都使用半管理液体燃料贮箱,贮箱内的液体收集器上安装有表面筛网,可阻止贮箱内气体在发动机工作时通过收集器进入到液体燃料管路中.文章假设卫星液体燃料贮箱的底部收集器出现故障,无法阻止气体进入发动机管路.为确保卫星正常在轨运行,利用计算流体动力学数值仿真方法,对液体燃料贮箱在卫星姿态控制发动机工作时的运动规律进行...     

空间电子设备意外跌落冲击响应分析

文章针对空间部件意外跌落事件,利用冲击分析原理,结合具体跌落时的路面和部件包装箱刚度,对空间部件的冲击加速度载荷进行了分析,为评价意外冲击事件是否影响产品性能提供了数值依据。