电磁辅助激光熔化沉积的残余应力

针对激光熔化沉积内部残余应力较大的问题,对其产生的机理作了分析。基于电磁场的应用原理,提出电磁辅助激光熔化沉积以降低其残余应力的方法。利用ANSYS参数化编程语言APDL模拟了电磁辅助激光熔化沉积的过程,分析了成形件残余应力的变化规律,结果表明同步加载轴向电磁力能较好地消减成形件内部残余应力。采用X射线衍射结合电解腐蚀的方法进行深度方向的残余应力测量试验,试验结果验证了电磁辅助的有效性。     

相控阵超声检测方案设计关键技术及其在航空航天领域的应用

相控阵超声检测技术是一种多通道超声检测方法,与常规单通道水浸超声检测技术相比,检测方案的制定更加灵活也更加复杂。在针对复杂型面结构进行检测方案设计时,错误的检测方案将可能产生缺陷的误检、漏检等严重问题。为了针对航空航天领域广泛存在的复杂结构试件制定最优的相控阵超声检测方案,本文提出了一套针对复杂型面结构的相控阵超声检测方案设计流程,并对其中涉及的关键技术和应用进行介绍。首先,对流程框架进行总体概述,表明检测方案设计的重要性和必要性;然后针对其中涉及的5项关键理论方法的核心原理及用途进行介绍;最后搭建相控阵超声软硬件平台,实现上述关键理论方法,并用于航空航天典型结构件的检测研究。研究结果表明,所制定方案能够准确检出结构内部的预埋缺陷,满足被测对象的检测要求,并且所提出的检测方案设计流程及采用的关键理论方法有效地提高了检测方案的设计效率,对航空航天等重要领域复杂结构试件的检测应用具有一定的理论指导及应用价值。     

预追踪法在搭建RCS计算平台中的应用

 介绍综合不同RCS贡献机理的计算平台的搭建方法。针对射线追踪法的计算量是这类RCS计算平台计算效率的瓶颈这一现状,提出仅对多次散射区采用射线追踪计算来减小计算量的方法。给出一种通过粗略的射线追踪来确定多次散射区的方法,并用该方法获得任意目标的散射分布图。对预追踪法在RCS平台的搭建中的应用方式进行探讨,并预测效果。通过具体的计算实例验证预追踪法的效果,并给出几类典型目标的多次散射区比例系数,可供采用预追踪法时参考。计算结果表明,在不改变计算精度的条件下,预追踪法可以将RCS计算平台中射线追踪部分的计算量减少到原来的1/3以下。对散射分布的可能应用做出展望,可以作为后续工作的指导。     

用银河宇宙线判定几个引起特大磁暴CME的运动方向

利用位于南北极尖区位置的McMurdo和Thule台站的宇宙线强度的观测数据，分析了几个引起特大磁暴CME的来向．分析结果表明，所选的与4个特大磁暴相关的CME基本是朝正对磁层顶的方向运动并与磁层作用的．通过对引起第23周两个特大磁暴的CME特征分析对照，发现CME的来向是影响磁暴强弱的一个因素．同样条件下，运动方向偏向地球一侧的CME引起的磁暴比正对地球的CME引起的磁暴要弱。     

固体火箭发动机无损检测图像质量研究

详细介绍了利用工业CT进行固体火箭发动机无损检测中，提高图像质量方面的几点尝试－光轴对准、提高系统的信噪比、提高探测器效率、采用合适的硬滤手段和选用适当的图像滤波函数。给出了测试数据和处理前后的图像比较。上述几点尝度收到了较好的处理效果。     

Background-sensitive event selection in the search for gamma-ray sources

Poor angular resolution of present day gamma ray telescopes (1° at 100 MEV) together with the complicated gamma ray sky structures at compareable angular extents and poor statistics available necessitate the selection of those gammas which will increase the observable signal from a suspected source. A method for such a selection using the pre-known time signature of the source as its signal, has been developed (Özel and Mayer-Haβelwander, 1983). In an iterative procedure based on the improvement of source signal, generalized zones around the source are defined, from which gamma rays should be accepted to construct the optimum light curve of the source. These zones depend on the energy of the probed gamma rays, on the spatial structure and intensity of the background around the source, on the (estimated and/or tentative) intetnsity of the source and finally on the observing instrument's angular and energy response functions. The method, when applied to simulated and observed COS-B data demonstrated its feasibility and merits over the previonsly used circular event-acceptance cones method which was the basis of searches for gamma ray emission from radio pulsars (see for example Kniffen et al., 1974; Ögelman, et al. 1976; Kanbach, et al., 1977; and references therein). Present method does not introduce “trials” which usually reduce the significance of the results obtained, fully accounts the available knowledge on the topography of gamma ray sky, makes use of all the information about the sky, source and the instrument and therefore is the proper way of handling gamma ray data in pulsar-type searches.Presently, method is applied in the analyses of COS-B data in the context of searches for gamma ray emitting X-ray and radio pulsars. Results will be published elsewhere.     

波纹板夹层结构高温钎焊焊缝X射线影像分析

为检测波纹板夹层结构高温钎焊焊缝质量,对其进行了X射线照相检查。波纹板夹层钎焊缝与一般熔焊焊缝不同,无论焊缝本身以及焊缝缺陷都有其特有的特点。本文通过对钎焊焊缝结构特点及焊缝X射线影像的分析,总结了获得高清晰X射线照片的方法及焊缝缺陷的识别特征。     

Delineation of possible influence of solar variability and galactic cosmic rays on terrestrial climate parameters

The present paper has investigated the associations of solar activity (SA), represented by total solar irradiance (TSI), galactic cosmic rays (GCR) and terrestrial climate parameters in particular the global cloudiness and global surface temperature. To that end, we have analysed thirty five years (1983–2018) data of these parameters and have applied the Granger-causality test in order to assess whether there is any potential predictability power of one indicator to the other. The correlations among the involved parameters are tested using Vector Auto Regression (VAR) model and variance decomposition method. As a result of the above analysis, we have found that the TSI is an important factor and has contributed about 8.77 ± 0.42% in the cosmic ray intensity variations. In case of cloud cover variations, the other three parameters (TSI, cosmic ray and global surface temperature) have played a significant role. Further, the TSI changes have contributed 1.68 ± 0.03% fluctuations in the variance of the cloud cover while the cosmic ray intensity and global surface temperature have contributed about 4.89 ± 0.08% and 10.87 ± 1.41% respectively. In case of the global surface temperature anomaly both TSI and cloud covers have contributed about 5.07 ± 0.47% and 14.42 ± 2.13% fluctuations respectively. Additionally, we have also assessed the impact of internal climate oscillations like multivariate ENSO index (MEI), north Atlantic oscillations (NAO) and quasi biennial oscillations (QBO) on cloud cover variations. The contribution of these internal oscillations e.g. ENSO, NAO and QBO in cloud cover variation were reported as 7.48 ± 1.02%, 5.51 ± 0.16% and 1.36 ± 0.43% respectively.     

低RCS齿形挂架参数选择研究

常规飞机的机翼与外挂架构成90°的二面角,成为飞机侧向的重要散射源.为求在不改变机体结构的前提下减缩飞机侧向RCS,采用齿形方案改变了挂架外形,消除了直角二面角结构,削弱了耦合效应.计算结果显示,改形的国产某型战斗机的机翼-外挂架结构的RCS在侧向重点姿态角内降低了9~13dBsm,证明了齿形改形方案能明显改善飞机侧向的耦合散射效应.在计算过程中使用了射线追踪法.      

Empirical model of cosmic ray spectrum in energy interval 1 MeV–100 GeV during 11-year solar cycle

The galactic cosmic rays (GCR) are the main ionization source at altitude of ∼3–35 km in the atmosphere. For high latitude anomalous cosmic ray (ACR) component has also a significant influence on the atmospheric ionization. We propose an empirical model for differential spectra D(E) of galactic and anomalous cosmic rays in energy interval 1 MeV–100 GeV during solar cycle. In the model data are used which cover three solar cycles: 20, 22 and 23. The LEAP87, IMAX92, CAPRICE94, AMS98 and BESS experimental spectra for protons and alpha particles are fitted to the proposed empirical model. The modulated GCR differential spectra are compared with force-field approximation to the one-dimensional transport equation and with solutions of two-dimensional cosmic ray transport equation. For experimental spectra, the calculation of the model parameters is performed by Levenberg–Marquardt algorithm, applied to the special case of least squares. Algorithm that combines the rapid local convergence of Newton–Raphson method with globally convergent method for non-linear systems of equations is applied for theoretically obtained differential spectra. The described programmes are realized in algorithmic language C++. The proposed model gives practical possibility for investigation of experimental data from measurements of galactic cosmic rays and their anomalous component.