CU-1型钇基重稀土对Be-Cu合金性能影响的研究

研究了CU-1型钇基重稀土对Be-Cu合金性能的影响。结果表明:Be-Cu合金经过微量CU-1型稀土的微合金化处理后,其显微硬度、耐磨性和耐腐蚀性均有不同程度的提高,热膨胀系数有所下降;随着稀土加入量的增加,Be-Cu合金的显微硬度逐渐提高,磨损量和平均腐蚀速率逐渐降低,热膨胀系数先减小后增大。     

固体发动机切割分离泄压过程分析

本文依据质点动力学和一维可压缩流体动力学原理，利用无限大容器的出流结果，在适当的简化假设基础上，建立了固体发动机切割分离泄压过程的数学模型，并对泄压过程和分离后的状态变化进行预测．通过比对分析试验容器的理论和试验结果，证明本文方法的误差在15％以内。     

航空发动机双层结构金属机匣的弹道试验

为研究航空发动机双层结构金属机匣在受叶片冲击时的包容性问题,利用滑膛炮试验系统对双层钛合金带不同间隙叠层靶板进行打靶弹道试验。通过28次有效的弹道试验发现:对比内层（迎弹面）、外层靶板厚度相同带间隙组合的试验结果,间隙越大靶板抗侵彻能力越差;对比不带间隙组合试验结果,内层较薄组合的抗侵彻能力强于内、外层厚度相同组合。采用商业有限元软件ANSYS/LS-DYNA对打靶试验进行了数值仿真,有限元仿真与试验结果吻合较好,并发现内层较薄组合的抗侵彻能力强于内层较厚组合,且两者均强于内、外层厚度相同组合;各个组合在没有间隙的情况下,弹道极限随叶片攻角增加而增加,但是速度曲线突增的攻角有所不同。无量纲靶厚决定了叶片冲击双层靶板的破坏模式。      

(TiB+TiC)/TC4复合材料电解钻孔试验研究

钛基复合材料是一种典型的难加工材料,采用传统机械加工方法存在加工效率低和加工质量差等问题。利用电解加工技术,采用直径为10mm的管状阴极,对(TiB+TiC)/TC4复合材料进行电解钻孔加工试验研究。进行了(TiB+TiC)/TC4复合材料的电化学特性研究,测量了(TiB+TiC)/TC4复合材料在10%NaNO₃溶液中的极化曲线和电流效率。探究了加工电压、电解液压力对加工精度的影响。结果表明,当加工电压为30V,电解液压力为0.6MPa时,电解钻孔可以在1mm/min的进给速度下稳定加工。当加工的盲孔深径比为3.06时,孔的圆度误差为41.1μm,锥度为0.4°,具有较高的加工精度。     

偶氮呋咱和氧化偶氮呋咱的合成及表征

介绍了高能材料二氨基偶氮呋咱(DAAF)、二氨基氧化偶氮呋咱(DAOAF)及二硝基氧化偶氮呋咱(DNOAF)的合成。其中,采用新型氧化剂制备DAAF,得率提高至65.60%。通过DSC-TG、元素分析、IR、1H NMR和MS等方法,对其结构进行了鉴定,并进行了常规的感度测试。感度数据表明,无氢炸药DNOAF的摩擦感度较大,与C-12相当,而DAAF和DAOAF为低感度炸药。     

CBERS-1卫星CCD相机像元实地分辨能力的测量及辐射特性浅析

利用CBERS - 1卫星数据、大比例尺航片和经过几何精纠正的高分辨率卫星图像进行测量、检验 ,阐述CCD相机像元实地分辨能力的测量原理和测量结果 ,并浅析其遥感图像的辐射特性     

CCSDS邻近空间链路协议的初步探究

介绍了空间数据系统咨询委员会(CCSDS)制定的邻近空间链路协议的产生背景及发展现状。     

热电偶响应对激光脉冲法测量热扩散率的影响

用激光脉冲法测量热扩散率时，作为感温元件的热电偶总有一定的响应时间。试样达到最大温升的时间比较短时，热电偶响应时间所带来的测量误差就不能忽略不计。将热电偶处理为一阶测量环节，导出了考虑热电偶响应时间的试样背面温升表达式和修正关系曲线，并据此对实验结果进行修正。结果表明：经修正后的结果和文献［１］中提供的数据相吻合。     

A study of a complete soft X-ray selected sample of AGN

We present preliminary results from analyses of hard X-ray and optical observations of a soft X-ray selected sample. We created a small but complete sample with 20 of the softest and brightest objects with low Galactic absorption from the ROSAT bright soft X-ray selected radio-quiet AGN sample. This sample consists of 10 narrow-line Seyfert 1 galaxies and 10 broad-line Seyfert galaxies. We analyze ASCA data in the 0.6–10 keV band and optical spectra from ground-based telescopes. We investigate the photon indices in the hard X-ray band, soft excesses in the ASCA band, and optical emission line properties. The photon indices in the 2–10 keV band are nominal for both narrow-line Seyfert 1 galaxies and broad-line Seyfert 1 galaxies in each class compared with other heterogeneous samples. All of the narrow-line Seyfert 1 galaxies show soft excesses, but this component seems to be less significant for broad-line Seyfert 1 galaxies. There seems to be a trend of steeper X-ray spectra to be accompanied by narrower Hβ for narrow-line Seyfert 1 galaxies, but this is not extended to the larger velocity width regime of broad-line Seyfert 1 galaxies, and no clear trend is seen among them.     

β Cephei stars from a photometric point of view

This is an observational review, with an emphasis on photometric data and their interpretation. Two lists are presented, one containing Cephei stars, and the other, Cephei suspects. These lists then serve as a basis for discussing such topics as the location of Cephei stars in the observational and theoretical H-R diagrams, the evolutionary state of these stars, the period-luminosity and period-luminosity-color relations, and observational identification of pulsation modes. The paper also includes references to recent work connected with the theoretical discovery that an opacity mechanism is responsible for the excitation of Cephei-star pulsations. Finally, observational programs for verifying the consequences of this discovery are suggested.Belgian Fund for Scientific Research (NFWO).