稀土钇提高离子镀TiN膜层与基体结合力的研究

研究了稀土钇不同含量时对离子镀ＴｉＮ膜层与基体结合力的影响．用扫描电镜，俄歇谱仪，Ｘ射线衍射等手段，对加入稀土钇的ＴｉＮ膜层作了分析。结果表明，加适量稀土钇后，ＴｉＮ膜层与基体的结合力大大提高。其微观机制是，加稀土钇后，膜层相组成发生变化，在膜－基之间形成一过渡层，塑性相（Ｔｉ相）增加，脆性相（Ｔｉ２Ｎ）减少，从而减小了膜－基界面间的应力。此外，结果还表明，稀土钇能明显提高镀膜过程中钛料蒸发率，使成膜速率增加，在相同镀膜时间内ＴｉＮ膜层加厚。     

SiCP/Al复合材料脉冲氩弧焊接研究

研究在脉冲氩弧焊条件下铝基复合材料SiCp／2124Al的可焊性。通过正确选择填充材料和在焊接过程中加入微量脉冲，大大减弱了增强体SiC颗粒与基体Al之间的界面反应。拉伸实验和显微硬度测试表明，接头质量良好，与母材强度相比，接头的抗拉强度未见有大幅度下降；金相组织观察显示，焊缝组织致密、无夹杂和裂纹等缺陷。对接头进行X射线衍射相结构分析和拉伸断口扫描电镜观察等微观分析，并从热力学角度探讨焊接过程中抑制SiC／Al界面反应发生的机理，提出了在氩弧焊条件下获得高质量SiCp／Al焊接接头应采取的措施。     

Rapid short-term pulse-period variations in Vela X-1 (4U 0900-40)

Results are presented of an analysis of 83 days of 2–12 keV X-ray observations of Vela X-1 (4U 0900-40) obtained during three separate pointings with the ESA COS-B satellite. The pulsation period is shown to undergo very rapid intrinsic changes, at a rate of up to during intervals of a few days. The lower values of which were previously observed over longer intervals, appear to result from an averaging-out of these rapid changes. It is argued, that the transfer of angular momentum to the neutron star by the accreting matter is very unlikely to be sufficient to explain these pulsation-period changes. An alternative explanation is suggested.     

An identification for GEMINGA: A review of all the available data

Dedicated X-ray, optical and radio observations aimed at the identification of the bright γ-ray source 2CG195+04 (GEMINGA) are presented. A very promising candidate is found and its properties are discussed in the context of possible astrophysical scenarios.     

CLF-1钢X数字射线照相等效系数的确定

针对聚变堆结构材料拟采用的新材料CLF-1(low-activated ferritic/martensitic steel)钢在进行射线检测过程中没有特定标准参考的问题,采用等效法在相同透照条件开展了不同厚度CLF-1钢和Q235钢的X数字射线等效透照实验研究。基于相同成像条件下两种材料对应的X射线图像具有相同灰度即透照系数相同,通过对比拥有相同图像灰度值的两种材料的厚度,得出CLF-1钢对应于Q235钢的等效透照系数。试验设计了4~20 mm,递增0.5 mm的阶梯厚度的CLF-1钢和Q235钢在100~400 kV(递增50 kV)管电压条件下进行了透照实验,获得了对应电压下CLF-1钢相对于Q235钢的X射线透照等效系数为1.10~1.13。该研究结果对CLF-1钢在进行X射线检测时的检测技术参数的确定具有指导意义。     

2219合金TIG补焊接头亮线影像成因及其力学性能

针对2219合金TIG补焊接头X射线底片亮线影像,开展2219合金不同坡口面角TIG补焊接头组织及性能研究。通过X射线、扫描电镜及能谱仪分析接头底片亮线影像位置对应的微观形貌及成分,并通过拉伸试验评价补焊接头力学性能。结果显示:在0～20°随坡口面角α值的增大,X射线底片上亮线影像的黑度逐渐降低;Cu含量较高的α(Al)+θ非平衡共晶组织对X射线的散射与吸收作用较强,是X射线底片亮线影像的成因;坡口面角α角侧受电磁搅拌作用弱于β角侧,其固-液界面前沿的边界层宽度大于β角侧,且温度梯度及边界层内的成分过冷度均大于β角侧,促进了α角侧枝晶的生长。当β角为20°时,在0°～20°随着α角度值增大,接头的抗拉强度与延伸率逐渐增大,20°时获得了优良的室温力学性能。X射线底片上存在亮线影像的补焊接头力学性能满足型号使用要求,亮线影像结构可不按焊接缺陷处理。     

天基X射线掠入射式成像望远镜发展现状

阐述了太阳X射线成像观测在空间天气预报中的地位和作用，叙述了掠入射式X射线聚焦成像的基本原理，简要介绍了在轨成功运行的天体X射线成像望远镜和太阳X射线成像望远镜的基本设计和技术指标，并介绍了国内正开发研制的专门服务于空间天气预报的太阳X射线成像望远镜基本设计和主要特点．     

X-ray broad line emission in Seyfert galaxies: Mrk 766 and NGC 4051

Long (>100 ks) observations of the bright Seyfert galaxies Mrk 766 and NGC 4051 have been obtained using XMM-Newton. The RGS 5–38 Å spectra reveal evidence of broad features. These can be modelled with relativistic emission lines coming from the immediate vicinity of a massive rotating black hole. Lines of OVIII, NVII and CVI are required to reproduce the spectrum of Mrk 766, whereas the spectrum of NGC 4051 can be modelled using a single, even broader OVIII line. Both Seyferts also exhibit broad iron line emission in the 2–8 keV range, and the data available thus far suggest that the strength of the low-energy emission lines and the strength of the iron line may be correlated.     

Differential emission measure distributions in X-ray solar flares

X-ray spectrometer RESIK has observed spectra in the four wavelength bands from 3.3 Å to 6.1 Å. This spectral range contains many emission lines of H- and He-like ions for Si, S, Ar and K. These lines are formed in plasma of coronal temperatures (T > 3 MK). Analysis of their intensities allows studying differential emission measure distributions (DEM) in temperature range roughly between 3 MK and 30 MK. The aim of present study was to check whether any relationship exists between the character of DEM distribution, the event phase and the X-ray flare class. To do this we have calculated and analyzed the DEM distributions for a set of flares belonging to different GOES classes from the range B5.6–X1. The DEM distributions have been calculated using “Withbroe–Sylwester” multiplicative, maximum likelihood iterative algorithm. As the input data we have used absolute fluxes observed by RESIK in several spectral bands (lines + continuum). Respective emission functions have been calculated using the CHIANTI v. 5.2 atomic data package.     

Pre-correction X-ray pulsar navigation algorithm based on asynchronous overlapping observation method

In order to shorten the data update period and further improve the accuracy, a pre-correction X-ray pulsar navigation algorithm based on asynchronous overlapping observation method is proposed. The asynchronous overlapping observation method partially overlaps the two adjacent observation periods, so that the data update period depends on the minimum pulsar observation period rather than the maximum like the other algorithms. The number of sampling points is also reduced to 2, which will effectively reduce the calculation burden. The proposed pre-correction extended Kalman filter uses observation data of adjacent sampling points to achieve a two-fold correction and makes up for the problem of insufficient observations on some sampling points caused by the observation method. Finally, simulations show that the proposed algorithm reduces the position and velocity errors by 21.55% and 19.13% compared to the EKF based on asynchronous observation method when using three detectors to observe the corresponding pulsars simultaneously. At the same time, the running time of one data update calculation is only 6.6% more than that of the EKF algorithm based on synchronous observation method.