某型机化铣零件成形工艺

化铣是一种能使表面形状复杂、加工精度要求高的零件达到加工要求的表面处理方法。铝合金的化学铣切已经成为航空工业零件成形的可靠加工方法,尤其是在加工飞机蒙皮时要比用传统的机械加工方法优越得多。本文对某型机零件表面出现锤痕现象进行了技术分析,发现其锤痕原因是由于成形零件用榔头校形而造成。同时,提出了采用钣金"一步成形法"即在淬火时效期内进行零件成形后再化铣的工艺方法。     

Testing the blast wave model with Swift GRBs

The complex structure of the light curves of Swift GRBs (e.g. superimposed flares and shallow decay) has made their interpretation and that of the blast wave caused by the burst, more difficult than in the pre-Swift era. We aim to constrain the blast wave parameters: electron energy distribution, p, density profile of the circumburst medium, k, and the continued energy injection index, q. We do so by comparing the observed multi-wavelength light curves and X-ray spectra of a Swift sample to the predictions of the blast wave model.     

The Radio Observatory on the Lunar Surface for Solar studies

The Radio Observatory on the Lunar Surface for Solar studies (ROLSS) is a concept for a near-side low radio frequency imaging interferometric array designed to study particle acceleration at the Sun and in the inner heliosphere. The prime science mission is to image the radio emission generated by Type II and III solar radio burst processes with the aim of determining the sites at and mechanisms by which the radiating particles are accelerated. Specific questions to be addressed include the following: (1) Isolating the sites of electron acceleration responsible for Type II and III solar radio bursts during coronal mass ejections (CMEs); and (2) Determining if and the mechanism(s) by which multiple, successive CMEs produce unusually efficient particle acceleration and intense radio emission. Secondary science goals include constraining the density of the lunar ionosphere by searching for a low radio frequency cutoff to solar radio emission and constraining the low energy electron population in astrophysical sources. Key design requirements on ROLSS include the operational frequency and angular resolution. The electron densities in the solar corona and inner heliosphere are such that the relevant emission occurs at frequencies below 10 MHz. Second, resolving the potential sites of particle acceleration requires an instrument with an angular resolution of at least 2°, equivalent to a linear array size of approximately 1000 m. Operations would consist of data acquisition during the lunar day, with regular data downlinks. No operations would occur during lunar night.     

一种基于三正交主轴平面的快速星图模拟方法

为在地面上进行星图模拟以测试星图识别算法和星敏感器性能, 提出了一种新的快速星图模拟方法. 该方法利用截面圆和固定区域的性质, 将单位天球按照三个正交主轴平面进行等分, 根据赤纬值求解恒星矢量与主轴平面夹角来确定选星条件, 进而根据坐标变换原理进行星图模拟. 为验证所提方法与现有方法相比的优势, 进行了大量的仿真实验. 实验结果表明, 与现有星图模拟方法相比, 本文方法在保证星图模拟精度的条件下, 选星速度提高了3倍以上.      

Effects of Atomic Oxygen Irradiation on Transparent Conductive Oxide Thin Films

作为一种功能薄膜,透明导电氧化物(TCO)薄膜在飞行器的抗原子氧(AO)涂层和太阳能电池领域有着巨大的应用价值。ZnO:Al(ZAO)和In2O3:Sn(ITO)薄膜是目前研究和应用最广泛的TCO。本文对ITO薄膜和ZAO薄膜进行了不同通量的AO辐照。通过对辐照前后样品的X射线衍射、扫描电镜及霍耳效应的表征及测试,研究了AO辐照对这两种TCO薄膜的结构、性能及电学特性的影响。研究表明AO辐照对ZAO薄膜表面有明显的侵蚀作用,但对其结构和导电性能没有明显影响。对于ITO薄膜,随着AO通量的增大,其载流子浓度逐渐下降从而导致了电阻率的提高,电阻率的最大变化达到了21.7%。     

先进云纹测量技术及应用

本文着重介绍了高灵敏度云纹法的发展及其在结构和材料力学行为测量方面的应用,包括云纹干涉法、微米云纹法、纳米云纹法及其相移技术。介绍了清华大学工程力学系光测实验室近年来利用云纹干涉法在材料科学、激光焊接、微电子封装等力学行为测量方面的应用成果。讨论了微米/纳米云纹法分别在微电子封装、微机械系统(MEMS)、纳观变形场测量中的应用。     

战斗机座舱动态温度快速计算软件开发

座舱温度是开展座舱舒适性评估的设计输入,飞机结构的复杂性和飞行工况的多变性为座舱温度的精确计算带来了一定困难,为解决复杂飞机结构,不同工况下的座舱温度快速、精确计算问题,采用集总参数法,结合传统传热学理论,构建了座舱动态温度快速计算数学模型,并基于 VB编程语言,开发了战斗机座舱动态温度快速计算软件,并对设定的飞行任务剖面进行了座舱热载荷数值模拟,结果表明软件计算结果与实测结果较为吻合,同时软件具有较好的通用性和可操作性,为后续开展座舱热舒适性的快速评估提供了工具支撑。     

油门杆角度相同时发动机推力不相等的几种修正方法

多发飞机要求油门杆角度相同时,发动机产生相等的推力,但由于发动机本体和油门系统的个体差异导致相同油门角度时发动机产生的实际推力大小不一样。对于电传油门系统,发动机本体通过引人推力修正参数消除个体差异,通过油门杆角度传感器校正消除油门推力指令差异。对于随动形式的自动油门,通过总线弓人推力修正指令消除因自动油门执行机构精度不足引起的推力差异。对于机械式油门系统,飞机设计发动机同步修正系统,以一侧发动机推力为基准,自动控制装置跟随微调另一侧发动机的推力,消除机械式发动机本体和油门系统的差异产生的推力不一致。     

Radio emission from coronal streamers

Different models of coronal streamers are used to calculate the radio brightness temperature at the wavelengths of observation of the Nançays Radioheliograph. Calculation are performed assuming the location of the streamer both on the disk and at the limb. Their comparison with observations show that a satisfactory agreement with a particular model can be found in the shape and in the relative enhacement of the streamer with respect to the quiet Sun, although the absolute values of the computed brightness temperatures are much higher than the observed ones.