利用M1.4喷管和开孔壁试验段实现低超声速流场实验研究

在FL-26y风洞中利用M1.4喷管和开孔壁试验段进行了实现低超声速流场的实验研究工作.通过实验研究验证了利用M1.4喷管在开孔壁试验段上建立起的低超声速流场的流场品质能够满足国军标合格指标的要求.实验还考察了不同稳定段总压、驻室抽气量等开车参数以及不同试验段扩开角、主流引射缝开度和开孔壁开孔率等洞体条件对流场的影响,为2.4m×2.4m跨声速风洞增设M1.4喷管,拓展该风洞试验马赫数的范围,使其具备M1.4的低超声速试验能力提供了技术支持,同时也为该风洞在下一阶段正式开展M1.4流场调试提供了可供参考的调试参数.     

300M钢超音速火焰喷涂WC／17Co涂层的疲劳性能

夹杂物尺寸对超高强结构钢的疲劳寿命有明显影响.疲劳断口分析表明,300M超高强钢中的疲劳裂纹源主要由其中的夹杂物所造成.而超音速火焰喷涂WC/17Co处理后300M钢裂纹源全部来自于基体中的夹杂,夹杂组成均为Al2O3.xCaO.ySiO2.分别采用统计极值法和广义Pareto分布对不同质量300M钢中的最大夹杂物进行估计,与实际疲劳断裂的最大夹杂物尺寸进行对比,并对不同质量300M钢的疲劳极限进行估算.HVAF处理使300M钢中次表面的残余压应力增大,对抑制裂纹萌生和扩展有利.试验结果表明,在低载荷下HVAF提高了基体疲劳寿命,而在高载荷下由于压应力作用有限,以及喷砂氧化铝对300M钢表面造成损伤带来负面作用而降低300M钢的疲劳寿命.     

粉末高温合金研究进展与应用

粉末高温合金由于特有的组织与性能已成为制造先进航空发动机涡轮盘的优选材料.为提升航空发动机的使用性能及可靠性,对粉末高温合金从材料、制造技术到涡轮盘的工程化应用进行全面和深入的研究,在粉末盘相应的关键技术上取得突破性进展,确立粉末盘制备的工艺路线,并制定工艺与检测的技术文件.为缩短研制周期,优化工艺过程.数值模拟技术也在粉末盘制备过程中得到广泛应用,并取得初步验证实验结果.     

FL－7风洞计算机综合测控系统的可靠度仿真计算

依据Ｍｏｎｔｅｃａｒｌｏ法，对系统基本部件统计抽样，按故障树模型，确定系统平均失效时间，计算系统可靠度各项指标，进行可靠性设计。经２８００多条气动实验曲线测定表明，在控制精度、燃料消耗、系统可靠度等方面均达到国内高速风洞的先进水平。     

面向任务的单武器系统平均修复时间模型

平均修复时间(MTTR,Mean Time To Repair)作为一个重要的维修性定量指标,目前其预计方法及算法立足于大量的试验结果和经验估计.通过对任务—装备—维修组成的面向任务的队列模型的研究,将任务需求、武器系统的可靠性及维修性综合考虑,针对故障率和修复率均服从指数分布的可修系统,建立了一种基于M/G/1可修排队模型的武器系统MTTR的模型,并给出了定量预计方法.此模型符合基于可靠性基础上的维修理论的基本结论,避免了设计初期对大量维修统计数据的依赖,为订购方在装备采购中提出维修性定量的要求提供了依据.      

高性能M40J/BADCy复合材料的研究

对E51环氧树脂改性双酚A型氰酸酯(BADCy)体系的力学性能及热性能进行了研究,发现当E51环氧树脂的质量含量为5%时,改性体系的弯曲强度和冲击强度分别由原来的95.6MPa和9.24kJ/m²提高到了117.8MPa和12.6kJ/m²,而热变形温度仅下降8℃。以该改性体系为基体制作的M40J复合材料,其弯曲强度、模量和剪切强度分别高达:1270MPa,172GPa,68 9MPa。消泡剂BYK141能提高M40J/BADCy复合材料的力学性能,层间剪切强度可提高到77.1MPa。M40J/BADCy复合材料还具有良好的耐环境能力,是一种理想的航空航天结构材料。     

300M 超高强钢起落架外筒模锻件锤锻工艺

利用Gleeble-1500热模拟试验机对300M超高强钢进行了热压缩试验,建立了材料流变应力模型;采用DEFORM 3D有限元软件对300M超高强钢起落架外筒模锻件锤锻成型过程进行了数值模拟,研究了不同工艺参数对锻件成型的影响.结果表明:模锻件在1100℃始锻温度下,经三火成型填充完全,锻件平均应力228 MPa,平均应变1.51.     

粉末高温合金FGH96惯性摩擦焊接头室温CTOD测试与分析

FGH96是采用损伤容限设计思想研制的新型粉末高温合金,是满足高推比、高燃效发动机使用要求的涡轮盘、环形件和其他热端部件的理想材料。FGH96惯性摩擦焊接头的CTOD值小于母材,其断口的韧窝小于母材。母材和接头断裂路径均为穿晶断裂。     

Involvement of nitric oxide in the mechanism of biochemical alterations induced by simulated microgravity in Microcystis aeruginosa

Simulated microgravity (SMG) can inhibit proliferation and enhance microcystin production of Microcystis aeruginosa. We investigated the role of nitric oxide (NO) in regulating the SMG induced changes of proliferation, photochemical system II photochemical activity, pigment, soluble protein and microcystin production in M. aeruginosa. M. aeruginosa was exposed to 0.1 mM sodium nitroprusside (SNP, NO donor) or 0.02 mM 2-(4-carboxyphenyl)-4, 4, 5, 5-tetramethylimidazoline-1-oxyl-3-oxide (c-PTIO, NO scavenger) alone or in combination with SMG for 48 h. SMG and SNP inhibited the growth of M. aeruginosa while c-PTIO had no effect on cell number. As to yield, the negative effect of SMG was augmented by SNP and suppressed by c-PTIO. The intracellular concentrations of chlorophyll a, carotenoid, phycocyanin, soluble protein and microcystin were increased by SMG after 48 h. The effects of SMG on these metabolic processes could be enhanced by SNP and be partly eliminated by c-PTIO. Moreover, SNP and c-PTIO only functioned in these biochemical processes under SMG, unlike in the regulation of cell proliferation and yield. These results showed that the effects of SMG could be enhanced by adding exogenous NO and be mitigated by scavenging endogenous NO, revealing the involvement of NO in the changes in biochemistry processes induced by SMG in M. aeruginosa.     

The role of ultraviolet imaging in studies of resolved and unresolved young stellar populations. M31 and M33

We discuss the relevance of UV data in the detection and characterization of hot massive stars and young stellar populations in galaxies. We show results from recent extensive surveys in M31 and M33 with Hubble Space Telescope (HST) multi-wavelength data including UV filters, which imaged several regions at a linear resolution (projected) of less than half a pc in these galaxies, and from GALEX far-UV and near-UV wide-field, low-resolution imaging of the entire galaxies. Both datasets allow us to study the hierarchical structure of star formation: the youngest stellar groups are the most compact, and are often arranged within broader, sparser structures. The derived recent star-formation rates are rather similar for the two galaxies, when scaled for the respective areas. We show how uncertainties in metallicity and type of selective extinction for the internal reddening may affect the results, and how an appropriate complement of UV filters could reduce such uncertainties, and significantly alleviate some parameter degeneracies.