航空发动机风扇叶片两种表面处理方法对比

在对激光冲击强化技术与喷丸表面强化技术比较分析之后,表明航空发动机叶片经过激光冲击强化后,能显著增加叶片表面残余压应力,提高疲劳性能,并且其效果优于喷丸表面强化技术。     

激光冲击残余应力场的有限元分析

建立模拟激光冲击残余应力场的非线性弹塑性有限元模型,预测AISI 304奥氏体不锈钢厚、薄靶材经激光冲击后表面以及内部的残余应力场分布.模拟过程中,考虑材料高应变率(106s-1)下的力学性能和激光诱导冲击波的精确加载,分析激光功率密度、激光光斑尺寸、激光脉宽、激光冲击次数、激光单面与双面冲击等激光冲击参数以及初始残余应力等因素对不锈钢靶材残余应力分布的影响.数值模拟结果与X射线衍射法测量值吻合较好.在有初始残余拉应力(250MPa)存在的情况下,激光冲击仍能使304奥氏体不锈钢靶材形成残余压应力层,说明激光冲击工艺可提高奥氏体不锈钢焊接构件的抗应力腐蚀开裂能力.     

基于大气传输软件激光透过率对比研究

简要地归纳了目前比较通用的大气传输软件LOWTRAN7、MODTRAN和FASCODE的概况和异同,分析了大气透过率的计算和激光武器选用的波长,比较了激光传输衰减和能见度的关系,重点研究对比了用LOWTRAN7和FASCODE计算1．06μm和10．6μm激光的透过率,并得出了结论。     

影响Al2O3凝相尺寸分布的因素

用激光全息装置测量含铝复合推进剂燃烧场凝聚相的分布，分辨率为5μm。分析了滞留时间、铝粉含量（2％－16％）和燃烧室压强（0.1MPa-4MPa）对凝相粒子尺寸分布的影响，实验表明，粒子总数随滞留时间减少，粒子越大，减少的相对比例越大；粒子尺寸分布不随燃烧室压强和推进剂铝粉含量变化。     

覆膜陶瓷粉末的选择性激光烧结工艺研究及参数优化

研究了选择性激光烧结成形制造过程中激光功率密度、扫描速度、预热温度和激光束扫描间距对烧结成形件致密度的影响,通过正交试验及方差分析,判定了各工艺参数的显著性及其重要性顺序,并给出覆膜陶瓷粉末烧结的最佳工艺参数。     

金属板料激光冷塑性弯曲的研究

 利用激光冲击波来成形金属板料是塑性成形领域刚刚出现的新技术，同激光热应力成形和传统的机械喷丸成形相比，具有巨大的优势。文章在分析了成形机理的基础上，用短脉冲（ns级）的强激光(GW/cm2）对LY12CZ航空铝合金材料进行了初步的激光冲击变形实验，探讨了冲击轨迹为直线情况下，激光脉冲能量、冲击次数、板料的厚度等对板料成形量的影响，实验结果表明：板料变形量随激光能量的增大而变大，随冲击次数的增加而增加，最后趋于平缓；随板料变形厚度的增加而减小。     

聚苯乙烯粉末选择性激光烧结成型机理的研究

分析了聚苯乙烯粉末材料选择性激光烧结成型机理,并通过填充改性方法提高其成型性能.结果表明,添加无机填料可提高聚苯乙烯粉末材料烧结性能,而且,多种填料同时添加,效果更明显.     

A Comparative Study of the Influence of the Active Young Sun on the Early Atmospheres of Earth, Venus, and Mars

Because the solar radiation and particle environment plays a major role in all atmospheric processes such as ionization, dissociation, heating of the upper atmospheres, and thermal and non-thermal atmospheric loss processes, the long-time evolution of planetary atmospheres and their water inventories can only be understood within the context of the evolving Sun. We compare the effect of solar induced X-ray and EUV (XUV) heating on the upper atmospheres of Earth, Venus and Mars since the time when the Sun arrived at the Zero-Age-Main-Sequence (ZAMS) about 4.6 Gyr ago. We apply a diffusive-gravitational equilibrium and thermal balance model for studying heating of the early thermospheres by photodissociation and ionization processes, due to exothermic chemical reactions and cooling by IR-radiating molecules like CO₂, NO, OH, etc. Our model simulations result in extended thermospheres for early Earth, Venus and Mars. The exospheric temperatures obtained for all the three planets during this time period lead to diffusion-limited hydrodynamic escape of atomic hydrogen and high Jeans’ escape rates for heavier species like H₂, He, C, N, O, etc. The duration of this blow-off phase for atomic hydrogen depends essentially on the mixing ratios of CO₂, N₂ and H₂O in the atmospheres and could last from ∼100 to several hundred million years. Furthermore, we study the efficiency of various non-thermal atmospheric loss processes on Venus and Mars and investigate the possible protecting effect of the early martian magnetosphere against solar wind induced ion pick up erosion. We find that the early martian magnetic field could decrease the ion-related non-thermal escape rates by a great amount. It is possible that non-magnetized early Mars could have lost its whole atmosphere due to the combined effect of its extended upper atmosphere and a dense solar wind plasma flow of the young Sun during about 200 Myr after the Sun arrived at the ZAMS. Depending on the solar wind parameters, our model simulations for early Venus show that ion pick up by strong solar wind from a non-magnetized planet could erode up to an equivalent amount of ∼250 bar of O⁺ ions during the first several hundred million years. This accumulated loss corresponds to an equivalent mass of ∼1 terrestrial ocean (TO (1 TO ∼1.39×10²⁴ g or expressed as partial pressure, about 265 bar, which corresponds to ∼2900 m average depth)). Finally, we discuss and compare our findings with the results of preceding studies.     

高能CO2激光腔镜高反介质薄膜的传输特性

为了获得适用于高能CO2激光器的高抗破坏阈值高反薄膜,以10.6μm高反膜ZnSe/YbF3,PbTe/BaF2膜系为例,数值模拟了激光在高反介质膜中的传输的场特性;给出了激光在多层介质膜中的场强分布、温度场分布及热应力分布。结果表明硅镜基体上的PbTe/BaF2膜系所需膜层厚度小、膜层数少,反射率可高达99.98%。     

激光熔敷氧化锆热障涂层微观结构研究

采用5KW连续CO_2激光器对Ni基高温合金上二次重熔NiCoCrAlY和ZrO_2陶瓷层进行了研究。结果表明:激光快速熔化和凝固获得定向外延生长、紧密堆积的柱状晶氧化锆陶瓷层。NiCoCrAlY结合层与柱状晶之间存在氧化铝层,保证了柱状晶与NiCoCrAlY层的联结。激光重熔ZrO_2层由四方相和立方相组成,经快速冷却由高温保留至室温。