Influence of longitudinal-torsional ultrasonic-assisted vibration on micro-hole drilling Ti-6Al-4V

As Ti-6Al-4V is a typical hard to machine material, especially in micro drilling aviation parts, chip breaking difficulty is of increasing interest to explore its further development. In this study, Longitudinal-Torsional Ultrasonic Assisted Drilling (LTUAD) was employed to machine Ti-6Al-4V, and its feasibility was evaluated by comparing with Conventional Drilling (CD). By combining periodical characteristics and vibration models (the separated or the unseparated ultrasonic elliptical vibration), the influence of ultrasonic frequency on the intersection characteristics of trajectories were analyzed. And the intersection characteristics were divided into four categories: even periodicity, odd periodicity, non-odd and even periodicity and composite periodicity, indicating different capability for chip breaking. By applying the longitudinal-torsional compound vibration horn, the micro-hole drilling experiment was carried out on machining center. The chip morphology, the thrust force, and the burr height were discussed. Experimental results showed that the morphology of chips presented as smaller and more fragmentary ones in LTUAD compared with continuous helical conical ones and fold-shaped ones in CD. Compared with CD, the average values of the thrust force in LTUAD reduced by 1.98% to 24.9%. According to the burr around the hole exit in both LTUAD and CD, the height of the latter was greatly affected by the drilling parameters. And the burr around the exit of the hole were distributed rather evenly with smaller extension in LTUAD. Consequently, the LTUAD employed in micro-hole drilling was effective.     

含稀土TiCx增强钛基激光熔覆层组织与耐磨性

采用同轴送粉激光熔覆技术在Ti6Al4V合金表面成功制备了含稀土CeO₂的碳化钛增强钛基激光熔覆层。运用渗透探伤、光学显微镜、X射线衍射仪、扫描电镜、能谱分析仪、电子探针、显微硬度计、摩擦磨损试验机等分析和测试方法研究了碳化钛增强钛基激光熔覆层的成形质量、微观组织、元素分布、硬度和摩擦磨损性能。结果表明,涂层内无裂纹缺陷,仅在层间过渡区分布有少量气孔（孔隙率为1.65%）。涂层中物相主要包括富Ti、Cr元素的β固溶体（CrTi₄）、缺位型碳化钛（TiC_x）和稀土氧化物（CeO₂）。熔覆层各微区的碳化钛形貌存在显著差异,熔覆层顶部和中部区域呈发达树枝晶状和针状,而结合区由针状和小尺寸不发达枝晶组成。碳化钛枝晶中碳元素分布不均匀,一次枝晶含碳量高于二次枝晶。基体相中Ni和Cr元素呈现明显偏析,而Al和V元素分布相对均匀。此外,稀土氧化物CeO₂主要分布于TiC_x与CrTi₄相界以及CrTi₄晶粒边界处。与基材相比,尽管TiC_x增强钛基复合涂层具有较高的摩擦系数,但其耐磨性显著增加（提高近52%）。熔覆层和基材磨损机制均为黏着磨损和磨粒磨损的复合磨损模式,但熔覆层的磨损程度较轻。     

双(口恶)唑啉化合物改性热固性树脂的研究

采用自制2,2′-(1,3-苯)双(4,5-二氢)(口恶)唑分别与热塑性酚醛树脂或二氨基二苯甲烷(DADPM)进行聚合反应制得了聚醚酰胺树脂(PEAR)和聚氨基酰胺树脂(PAAR).实验表明PEAR的冲击强度达到6 kJ/m2以上,弯曲强度达到100MPa以上,且电绝缘性能优良,可作为H级绝缘材料使用;PAAR的冲击强度最高达到22kJ/m2,弯曲强度达到202 MPa,电绝缘性能较PEAR稍差,但仍然可作为H级绝缘材料使用,另外还可望作为无卤阻燃材料使用.以这两种高性能热固性树脂为基体可制备出性能优良的玻璃布复合材料.     

30CrMnSiNi2A和GC4（40CrMnSiMoVA）钢裂纹扩展性能比较分析研究

在分析30CrMnSiNi2A和GC4力学性能的基础上,在相同裂纹长度条件下,对两种材料的裂纹扩展寿命和裂纹扩展速率的统计特性进行了统计研究。经比较分析后认为,由于30CrMnSiNi2A钢的裂纹扩展速率较慢,故裂纹扩展寿命较长,但由于其分散性较大,在裂纹长度较大时,99.9%的安全寿命尽管仍比GC4钢大,但两者已很接近。     

纳米铁酸铜的制备及对RDX热分解的催化作用

以CuCl2·2H2O和Fe(NO3)3·9H2O为原料,采用室温固相化学反应法制备出三种不同铜、铁摩尔质量比的纳米CuFe2O4粉体,产物的粒径约为5nm。采用差示扫描量热法(DSC)测试了纳米CuFe2O4对RDX热分解的催化作用。结果表明:纳米CuFe2O4对RDX热分解有明显的催化效果。在三种纳米CuFe2O4中,铜、铁摩尔质量比为1∶1的纳米CuFe2O4的催化效果最好,它使RDX的分解峰温前移了17 8℃,放热量增加了250J/g,活化能降低了21 9kJ/mol。纳米CuFe2O4的用量增加对RDX热分解的催化效果显著增大。     

利用金属间化合物增强陶瓷钎焊接头强度

研究了Ag-Cu-Ti/加Ti/N i/Ti复合层钎焊S i3N4陶瓷的接头组织与性能。结果表明,钎缝中形成了以金属间化合物为高熔点相和Ag-Cu作为基体的组织。对界面反应层的观察表明,反应层分为两层结构。保温时间、连接温度、Ti箔和N i箔厚度及Ag-Cu-Ti钎料厚度均能影响接头组织和强度。在本实验范围内,其它参数一定的条件下,分别在30m in,970℃,Ti箔30μm和N i箔60μm及Ag-Cu-Ti片150μm时取得了最大强度值。     

Cr4M04V钢表面预制缺陷对滚动接触疲劳性能的影响

用推力片实验研究了表面预制缺陷对Cr4Mo4V高温轴承钢滚动接触疲劳性能的影响。应用洛氏硬度计和维氏硬度计预制不同形状、不同大小的表面缺陷,通过扫描电镜记录滚动疲劳裂纹的萌生、发展乃至试样失效的全过程。结果表明,表面预制缺陷对Cr4Mo4V钢滚动接触疲劳性能有很大的影响。不同形状的预制缺陷对疲劳性能有不同的影响,且疲劳性能有明显的缺陷尺寸效应。     

基于概率模型运动检测技术的视频对象分割技术研究

MPEG-4最重要的特点是用音频-视频对象来描述内容和进行编码。这就需要按照视频对象进行视频图像分割,而视频对象具有时域和空域这两大特点,而时域分割又占主要的地位。研究了一种时域分割算法,即研究了一种运动检测技术方案,采用Til Aach,Andre Kaup提出的基于概率模型的运动检测技术,用Gauss模型描述噪声引起的像素值变化,将运动目标和有噪声的背景区别开来。最后,采用二值开闭重建滤波器来去除前景和背景中的“小洞”,从而获取了最终的运动检测掩码。     

SiC纤维CVD涂层工艺研究

对SiC纤维的CVD涂层工艺进行研究.实验发现采用BCl3,H2及CH4作为反应气体,采用与SiC纤维生产工艺相匹配的走丝速度并控制一定的工艺参数,在1350℃左右可得到厚度2～3mm且表面致密的B4C涂层,纤维涂层后性能基本保持不变.仅采用BCl3及CH4作为CVD涂层工艺反应气体,在1180～1250℃即可沉积出表面光滑致密,厚度2～3mm的富碳B4C涂层,涂层后纤维性能可提高10%左右,且涂层与纤维结合强度很高,优于B4C涂层与SiC纤维的结合强度.实验还发现SiC纤维涂覆B4C及富碳B4C涂层后,能有效阻隔界面反应,可大幅提高SiC/Ti基复合材料的性能.     

The primordial Helium-4 abundance determination: systematic effects

By extrapolating to O/H = N/H = 0 the empirical correlations Y–O/H and Y–N/H defined by a relatively large sample of 45 Blue Compact Dwarfs (BCDs), we have obtained a primordial ⁴Helium mass fraction Y _p=0.2443±0.0015 with dY/dZ=2.4±1.0. This result is in excellent agreement with the average Y _p=0.2452±0.0015 determined in the two most metal-deficient BCDs known, I Zw 18 (Z /50) and SBS 0335–052 (Z /41), where the correction for He production is smallest. The quoted error (1) of 1% is statistical and does not include systematic effects. We examine various systematic effects including collisional excitation of hydrogen lines, ionization structure and temperature fluctuation effects, and underlying stellar Hei absorption, and conclude that combining all systematic effects, our Y _p may be underestimated by 2–4%. Taken at face value, our Y _p implies a baryon-to-photon number ratio =(4.7^+1.0 _–0.8)×10^–10 and a baryon mass fraction _b h ² ₁₀₀=0.017±0.005 (2), consistent with the values obtained from deuterium and Cosmic Microwave Background measurements. Correcting Y _p upward by 2–4% would make the agreement even better.