全权限数字电子控制器雷电试验方法研究

在分析机载设备雷电感应敏感度试验相关标准的基础上,对全权限数字电子控制器雷电间接效应试验方法进行研究。对雷电间接效应耦合方式进行了分类,并以某型全权限数字电子控制器为例,介绍了数字电子控制器雷电感应瞬态敏感度试验波形组、试验电平选择方法及试验过程。并对空客和波音公司机载设备雷电感应瞬态敏感度试验方法做了初步介绍。研究成果可供制定机载设备雷电防护要求及试验方案时参考。     

电子辐照对聚乙烯热缩套管力学性能的影响

利用45 keV,1 MeV和2 MeV电子分别对聚乙烯热缩套管进行辐照实验,研究不同能量电子辐照对聚乙烯热缩套管力学性能的影响,并分析电子辐照下材料的损伤效应机理,建立力学性能退化规律。结果表明：实验选定的3种能量电子辐照都会造成聚乙烯的降解,材料脆化产生裂纹,从而导致其力学性能下降;但是由于这3种能量电子穿透深度不同,45 keV电子只能造成聚乙烯热缩套管表层材料损伤,力学性能最大下降量只有30%~40%,而1 MeV和2 MeV电子却会导致套管力学性能完全丧失,力学性能下降接近100%。     

航空发动机燃烧室出口高温热电偶校准技术

在高温校准风洞上,对测量航空发动机燃烧室出口温度气冷式和非气冷式这两种形式的高温热电偶进行校准,确定了高温热电偶的辐射修正系数.校准实验结果表明:高温热电偶的辐射误差随气流速度和压力的增加而降低,而且气流温度与航空发动机机匣壁面温度的温差越大,辐射误差也越大.比较两种结构形式的高温热电偶,非冷却式高温热电偶的测量误差比气冷式高温热电偶的相对较小.      

Advances and trends in plastic forming technologies for welded tubes

With the implementation of environmental protection, sustainable development and conservation-oriented policies, components and parts of thin-walled welded tubes have gained increasing application in the aircraft and automotive industries because of their advantages: easily achieving forming and manufacturing process at low cost and in a short time. The current research on welded tube plastic forming is mainly concentrated on tube internal high-pressure forming, tube bending forming, and tube spinning forming. The focuses are on the material properties and characterization of welded tubes, finite element modeling for welded tube forming, and inhomogeneous deformation behavior and the mechanism and rules of deformation coordination in welded tube plastic forming. This paper summarizes the research progress in welded tube plastic forming from these aspects. Finally, with a focus on the urgent demand of the aviation, aerospace and automotive industries for high-strength and light-weight tubes, this paper discusses the development trends and challenges in the theory and technology of welded tube plastic forming in the future. Among them,laser tailor-welded technology will find application in the manufacture of high-strength steel tubes.Tube-end forming technology, such as tube flaring and flanging technology, will expand its application in welded tubes. Therefore, future studies will focus on the FE modeling regarding how to consider effects of welding on residual stresses, welding distortions and microstructure, the inhomogeneous deformation and coordination mechanism of the plastic forming process of tailor-welded tubes, and some end-forming processes of welded tubes, and more comprehensive research on the forming mechanism and limit of welded tubes.     

高能电子对地球同步轨道卫星的影响分析

为了厘清在轨GEO(Geosynchronous Earth Orbit,地球同步轨道)卫星不时出现异常的原因,提高卫星执行任务的可靠性,首先从机理上介绍了空间环境中的地球辐射带及高能电子的情况,引出GEO卫星所处恶劣空间环境的现实;其次基于我国SEPC(Space Environment Prediction Center,国家空间环境预报中心)以及NSMC(National Satellite Meteorological Center,国家卫星气象中心)的空间环境月报资料,结合某GEO环境业务卫星故障的实际数据,经统计归纳,分析得出了地球辐射带中的高能电子是导致GEO卫星发生故障的主要原因;最后按照事例技术分析、常规按需预报和特殊情况下的实时预报等3个层次对高能电子预报方法进行了初步探讨。通过分析可以看出,为提高卫星完成任务的可靠性、降低长期管理风险,需要加强GEO卫星所处空间环境高能电子的预报工作。     

DORIS processing at the European Space Operations Centre

This paper gives an overview of the DORIS related activities at the Navigation Support Office of the European Space Operations Centre. The DORIS activities were started in 2002 because of the launch of the Envisat satellite where ESOC is responsible for the validation of the Envisat Precise Orbits and a brief overview of the key Envisat activities at ESOC is given. Typical orbit comparison RMS values between the CNES POE (GDR-C) and the ESOC POD solution is 6.5, 18.8 and 23.1 mm in radial-, along- and cross-track direction. In the framework of the generation of the ITRF2008 ESOC participated in the reprocessing of all three space geodetic techniques; DORIS, SLR, and GPS. Here the main results of our DORIS reprocessing, in the framework of the International DORIS Service (IDS), are given. The WRMS of the weekly ESOC solution (esawd03) for the 2004–2009 period compared to the IDS-1 combined solution is of the order of 12 mm. Based on the long time series of homogeneously processed data a closer look is taken at the estimated solar radiation pressure parameters of the different satellites used in this DORIS analysis. The main aim being the stabilization of the Z-component of the geocentre estimates. We conclude that the ESOC participation to the IDS ITRF2008 contribution has been beneficial for both ESOC and the IDS. ESOC has profited significantly from the very open and direct communications and comparisons that took place within the IDS during the reprocessing campaign.     

小型电磁辐射敏感度自动测试系统的设计

介绍电磁辐射敏感度自动测试系统组成、工作原理和设计方法，叙述了硬件配置、系统控制、数据采集处理等软件设计。其中较详细地介绍了光纤式场强数据采集部分的设计。     

UVCS/SOHO Observations of Spectral Line Profiles in Polar Coronal Holes

Ultraviolet emission line profiles have been measured on 15-29 September 1997 for H I 1216 Å, O VI 1032, 1037 Å and Mg X 625 Å in a polar coronal hole, at heliographic heights ? (in solar radii) between 1.34 and 2.0. Observations of H I 1216 Å and the O VI doublet from January 1997 for ? = 1.5 to 3.0 are provided for comparison. Mg X 625 Å is observed to have a narrow component at ? = 1.34 which accounts for only a small fraction of the observed spectral radiance, and a broad component that exists at all observed heights. The widths of O VI broad components are only slightly larger than those for H I at ? = 1.34, but are significantly larger at ? = 1.5 and much larger for ? > 1.75. In contrast, the Mg X values are less than those of H I up to 1.75 and then increase rapidly up to at least ? = 2.0, but never reach the values of O VI.     

Spectroscopic Constraints on Models of Ion-cyclotron Resonance Heating in the Polar Solar Corona

Using empirical velocity distributions derived from UVCS and SUMER ultraviolet spectroscopy, we construct theoretical models of anisotropic ion temperatures in the polar solar corona. The primary energy deposition mechanism we investigate is the dissipation of high frequency (10-10000 Hz) ion-cyclotron resonant Alfvén waves which can heat and accelerate ions differently depending on their charge and mass. We find that it is possible to explain the observed high perpendicular temperatures and strong anisotropies with relatively small amplitudes for the resonant waves. There is suggestive evidence for steepening of the Alfvén wave spectrum between the coronal base and the largest heights observed spectroscopically. Because the ion-cyclotron wave dissipation is rapid, even for minor ions like O⁵⁺, the observed extended heating seems to demand a constantly replenished population of waves over several solar radii. This indicates that the waves are generated gradually throughout the wind rather than propagated up from the base of the corona. This revised version was published online in June 2006 with corrections to the Cover Date.     

The relationship between plasma effects and cosmic radiation studied with TriTel-LMP measurements during the ESEO mission

The main point of the paper is to use the simultaneous measurements of the energetic particle flux by TriTel and those of electron density by a Langmuir probe to study the question of to what extent solar electromagnetic and corpuscular radiation (galactic cosmic rays, particle precipitation from the radiation belts) are responsible for the ionization of the atmosphere. The electron density measured by the Langmuir probe is the sum of the ionization produced by the solar electromagnetic radiation and that due to the corpuscular radiation. The ionization produced by the solar electromagnetic radiation may be computed. The flux of energetic particles in an energy range may be determined by taking the difference between the threshold energy of the TriTel telescopes and the energy corresponding to the local cut-off rigidity. As the ESEO satellite will have a quasi-polar and circular orbit, the cut-off rigidity will change from low to high latitudes, thus enabling the assignment of different energy bands for the telescopes. Thus, it will be possible to determine which energy bands of particle produce ionization at different latitudes.