基于CATIA V5的自动钻铆机托架变形研究

探讨了大型自动钻铆机托架系统的变形机理及其影响.研发了基于CATIA V5的托架变形补偿技术及变形模拟系统,可对变形量在加工过程实施实时修补,有效地解决了自动钻铆机大型托架的变形问题并已成功应用于ARJ21的机翼壁板的生产.     

等离子体涡电磁散射特性及隐身性能

 针对非均匀等离子体在飞行器隐身中的应用,采用分段线性电流密度递归卷积时域有限差分（PLJERC-FDTD）方法计算等离子体涡及涡串电磁散射特性,分析等离子体涡对飞行器隐身性能影响。计算表明,等离子体涡在很大频率区间对电磁波吸收效果显著,RCS降低很大,具有明显的隐身效果。等离子体涡表现出一定规律性的极化特性,对L,S和C波段电磁波具有不同的吸收、反射特性。     

A Satellite-borne Miniature Ion Mass Spectrometer for Space Plasma

The miniature design technology is an important trend in space exploration. Mass spectrometer is used extensively in the space environment detection. The miniature ion mass spectrometer utilizes a 127° cylindrical electrostatic analyzer accompanied with a Time of Flight (TOF) unit based on ultrathin carbon foil to measure the energy spectra and composition of space plasma. The Time of Flight technique has been used broadly in space plasma measurement. A new type of miniature method for the ion mass spectrometer is introduced. The total mass of the instrument is 1.8 kg and the total power consumption is 2.0W. The calibration results show that the energy measurement range is 8.71～43550eV, the energy resolution is 1.86% and the ion mass from 1 amu (1 amu = 1.67 × 10^-27 kg) to 58 amu can be resolved by the miniature mass spectrometer. The miniature ion mass spectrometer also has a potential to be increased in the field of view by an electrostatic deflecting system to extend its application in space plasma detection. The miniature ion mass spectrometer has been selected for pre-study of Chinese Strategic Priority Research Program on Space Science.     

中地球轨道高能电子辐射环境特性分析

采用中国中地球轨道卫星在太阳活动下降相到上升相的高能电子探测数据, 首次分析研究了该轨道高能电子环境的空间分布、通量强度、时序变化以及对地磁暴活动响应的特性. 结果表明, 中地球轨道高能电子的空间分布 范围稳定, 电子通量强度随能量升高而下降; 中地球轨道高能电子环境是 一个在不同时间尺度上剧烈变化的动态系统, 该系统可能间歇性地出现27天重 现性变化, 该系统变化受地磁暴事件调制, 但其对磁暴的响应呈现出非线性特征.     

高强高模聚乙烯纤维对大掺量矿物掺合料高强混凝土抗冻性的影响

用快冻法研究高性能的高强高模聚乙烯(High elasticity module polyethylene,HEMP)纤维对大掺量矿物掺合料高强混凝土(High strength concrete,HSC)抗冻性的影响.结果表明,大掺量矿物掺合料HSC具有较好的抗冻性,但是其抗冻性对养护环境RH非常敏感,干燥养护条件下的冻融寿命仅有标准养护的38%～40%.掺加0.1%HEMP纤维虽然降低了大掺量矿物掺合料HSC的抗冻性,但能够显著改善其抗冻性对养护环境RH的敏感性,在30%RH～50%RH养护条件下的冻融寿命高达标准养护时的81%～90%.     

基于传输矩阵法的等离子体鞘套传输特性分析

引入分层模型传输矩阵法,分析高速临近空间飞行器等离子体鞘套传输特性.通过对典型飞行器模型进行纳维-斯托克斯方程组数值求解,仿真了等离子体鞘套的流场电子密度分布,分析了电磁波在等离子体鞘套内传输时的衰减常数,给出信号传输的反射系数和透射系数.基于传输矩阵法的仿真结果与理论分析结果和时域有限差分法仿真分析结果有良好的一致性,同时,该方法有效降低了计算复杂度,适用于任意电子密度分布和厚度的等离子体鞘套传输特性的数值求解.     

GTEM电磁敏感度测试系统的研制

90年代以来 ,GTEM以其独特的优越性在电磁兼容测试领域中得到了广泛的应用。许多先进国家的军用工业标准均推荐采用此项技术。文中给出了一套适合我航天型号电磁兼容测试要求的 GTEM电磁敏感度测试系统。该测试系统由 GTEM、双定向耦合器、功率计、功率放大器、射频开关矩阵、信号源、计算机组成。其工作原理是 ,按照辐射电磁敏感度的测试要求 ,系统应在试样所在区域产生幅度和频率均已知的连续波电磁场 ,当系统集成完成后 ,只需调整GTEM端口的馈入信号功率、频率以及试样安放的位置 ,即可在试样所在区域产生测试所需的连续波电磁场。系统测控软件兼顾系统的安全性及可操作性 ,采用人机对话的方式 ,在WINDOWS3.1环境下运行。该系统测试操作直观简便 。     

Low-latitude storm time ionospheric predictions using support vector machines

The electromagnetic drift plays an important role in low-latitude storm time ionospheric dynamics. In this study we attempt to utilize the electric field data into ionospheric predictions by using support vector machine (SVM), a promising algorithm for small-sample nonlinear regressions. Taking the disturbance electric field data as input, different SVMs have been trained for three seasonal bins at two stations near the north crest of the Equatorial Ionization Anomaly (EIA). Eighteen storm events are used to check out their predicting abilities. The results show fairly good agreement between the predictions and observations. Compared with STORM, a widely used empirical correlation model, the SVM method brings a relative improvement of 23% for these testing events. Based on this study we argue that the SVM method can improve the storm time ionospheric predictions.     

Evaluation and improvement of coastal GNSS reflectometry sea level variations from existing GNSS stations in Taiwan

Global sea level rise due to an increasingly warmer climate has begun to induce hazards, adversely affecting the lives and properties of people residing in low-lying coastal regions and islands. Therefore, it is important to monitor and understand variations in coastal sea level covering offshore regions. Signal-to-noise ratio (SNR) data of Global Navigation Satellite System (GNSS) have been successfully used to robustly derive sea level heights (SLHs). In Taiwan, there are a number of continuously operating GNSS stations, not originally installed for sea level monitoring. They were established in harbors or near coastal regions for monitoring land motion. This study utilizes existing SNR data from three GNSS stations (Kaohsiung, Suao, and TaiCOAST) in Taiwan to compute SLHs with two methods, namely, Lomb–Scargle Periodogram (LSP)-only, and LSP aided with tidal harmonic analysis developed in this study. The results of both methods are compared with co-located or nearby tide gauge records. Due to the poor quality of SNR data, the worst accuracy of SLHs derived from traditional LSP-only method exceeds 1?m at the TaiCOAST station. With our procedure, the standard deviations (STDs) of difference between GNSS-derived SLHs and tide gauge records in Kaohsiung and Suao stations decreased to 10?cm and the results show excellent agreement with tide gauge derived relative sea level records, with STD of differences of 7?cm and correlation coefficient of 0.96. In addition, the absolute GNSS-R sea level trend in Kaohsiung during 2006–2011 agrees well with that derived from satellite altimetry. We conclude that the coastal GNSS stations in Taiwan have the potential of monitoring absolute coastal sea level change accurately when our proposed methodology is used.     

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.