3D-C/SiC复合材料拉-拉疲劳模量和电阻的变化

在室温最大应力为250MPa，应力比R＝0．1和频率为60Hz条件下，对3D－C／SiC复合材料进行了拉－拉疲劳试验。用共振法和电阻增量仪分别测试了杨氏模量及电阻的变化。结果表明：随循环次数增加，杨氏模量呈显著下降，缓慢下降和突然下降的变化规律。杨氏模量的下降大部分发生在疲劳循环的前600次。缓慢降低阶段约占疲劳寿命的94％以上，此阶段杨氏模量变化率与循环次数的对数近似呈线性关系，电阻变化率除首次循环降低外，随着循环次数增加一直在增加。增加规律大致可分为缓慢增加，台阶式增加和急剧增加三个阶段。材料的电阻变化率基本反映了纤维的损伤程度和破坏形式，可作为表征复合材料纤维损伤的有效参量。     

难熔金属化合物掺杂对先驱体转化2D C/SiC复合材料抗氧化性能影响

提出在2D C/SiC复合材料基体中掺杂难熔金属化合物ZrB2,TaC,ZrC,制备了2D C/SiC-ZrB2,2D C/SiC-ZrC和2D C/SiC-TaC新型复合材料,考察了难熔金属化合物的引入对材料力学性能、抗氧化性能和微观结构的影响.结果表明,ZrB2和TaC的引入,能明显提高2DC/SiC复合材料的抗氧化性能;ZrC的引入对2D C/SiC复合材料的抗氧化性能极其不利.这归结于高温下ZrB2和TaC有助于在复合材料表层氧化形成ZrO2,B2O3和Ta2O5保护膜,阻止了材料内部的进一步氧化,从而提高了复合材料的抗氧化性能.     

Fe/O Ratios in Interplanetary Shock Accelerated Particles

It is widely accepted that diffusive shock acceleration is an important process in the heliosphere, in particular in producing the energetic particles associated with interplanetary shocks driven by coronal mass ejections. In its simplest formulation shock acceleration is expected to accelerate ions with higher mass to charge ratios less efficiently than those with lower mass to charge. Thus it is anticipated that the Fe/O ratio in shock-accelerated ion populations will decrease with increasing energy above some energy. We examine the circumstances of five interplanetary shocks that have been reported to have associated populations in which Fe/O increases with increasing energy. In each event, the situation is complex, with particle contributions from other sources in addition to the shock. Furthermore, we show that the Fe/O ratio in shock-accelerated ions can decrease even when the shock is traveling through an Fe-rich ambient ion population. Thus, although shock acceleration of an Fe-rich suprathermal population has been proposed to explain large Fe-rich solar particle events, we find no support for this proposal in these observations.     

Solar Sources of Heliospheric Energetic Electron Events—Shocks or Flares?

Electrons with near-relativistic (E≳30 keV, NrR) and relativistic (E≳0.3 MeV) energies are often observed as discrete events in the inner heliosphere following solar transient activity. Several acceleration mechanisms have been proposed for the production of those electrons. One candidate is acceleration at MHD shocks driven by coronal mass ejections (CMEs) with speeds ≳1000 km s⁻¹. Many NrR electron events are temporally associated only with flares while others are associated with flares as well as with CMEs or with radio type II shock waves. Since CME onsets and associated flares are roughly simultaneous, distinguishing the sources of electron events is a serious challenge. On a phenomenological basis two classes of solar electron events were known several decades ago, but recent observations have presented a more complex picture. We review early and recent observational results to deduce different electron event classes and their viable acceleration mechanisms, defined broadly as shocks versus flares. The NrR and relativistic electrons are treated separately. Topics covered are: solar electron injection delays from flare impulsive phases; comparisons of electron intensities and spectra with flares, CMEs and accompanying solar energetic proton (SEP) events; multiple spacecraft observations; two-phase electron events; coronal flares; shock-associated (SA) events; electron spectral invariance; and solar electron intensity size distributions. This evidence suggests that CME-driven shocks are statistically the dominant acceleration mechanism of relativistic events, but most NrR electron events result from flares. Determining the solar origin of a given NrR or relativistic electron event remains a difficult proposition, and suggestions for future work are given.     

Compression Creep Behavior of High Volume Fraction of SiC Particles Reinforced AI Composite Fabricated by Pressureless Infiltration

The compression creep deformation of the high volume fraction of SiC particles reinforced AI-Mg-Si composite fabricated by pressure-less infiltration was investigated. The experimental results show that the creep stress exponents are very high at temperatures of 673 K, 723 K and 773 K, and if taking the threshold stress into account, the true stress exponent of minimum creep strain rate is still approximately 5, although the volume fraction of reinforcements is very high. The creep strain rate in the high volume fraction reinforced aluminum alloy matrix composites is controlled by matrix lattice diffusion. It is found that the creep-strengthening effect of high volume fraction of silicon carbide particles is significant, although the particles do not form effective obstacles to dislocation motion.     

孔隙预置技术制备多孔C/SiC复合材料及其性能表征

以玻璃纤维为成孔剂,采用孔隙预置技术制备了发汗多孔C/SiC复合材料.对孔隙结构进行了表征,并研究了材料的力学性能和渗透行为.研究结果表明,采用孔隙预置技术能够有效地实现多孔 C/SiC材料开孔率和孔隙结构控制,该材料具有良好的力学性能和渗透性能.     

C/SiC复合材料紧固件拉-拉疲劳行为研究

为了研究C/SiC复合材料紧固件的拉-拉疲劳行为,在疲劳应力比为0. 1、加载频率为10 Hz的条件下对不同应力水平的疲劳寿命进行统计。采用断口分析和金相分析方法对C/SiC复合材料螺钉疲劳破坏的细观机制进行了研究。结果表明:C/SiC复合材料螺钉拉-拉疲劳包含拉断疲劳及拉脱疲劳两种失效形式;基于双参数幂指数形式的寿命模型,两种失效形式的疲劳寿命经验公式相似;C/SiC复合材料螺钉的疲劳极限约为拉伸强度的65%～70%,若最大疲劳应力大于0. 7σmax,其材料损伤随循环次数增多而明显增大。     

C/SiC复合材料螺旋铣削与钻削制孔效果对比

采用PCD刀具对C/SiC复合材料螺旋铣削与钻削制孔的制孔效果进行了对比研究。在同等加工效率条件下测量了两种制孔方法产生的切削力及切削热,并观察制孔质量。试验结果表明:螺旋铣孔产生的轴向力小于钻孔,约为钻孔的56.9%;孔壁粗糙度及孔径差均小于钻削;钻孔产生的切削热少于螺旋铣削制孔,约占螺旋铣的58.7%,但螺旋铣产生的切削热对材料及刀具的影响小。     

熔融渗硅工艺制备的SiCf/SiC复合材料微观结构与性能

SiC纤维增强SiC陶瓷基复合材料（SiC_f/SiC复合材料）在航空发动机热端部件方面具有重要应用。本文以第二代碳化硅纤维为增强材料,采用熔融渗硅工艺制备出SiC_f/SiC复合材料,测试复合材料的基本物理性能及常规力学性能,并利用Micro-CT、SEM对试样的微观结构和断面进行了表征分析。结果显示：SiC_f/SiC复合材料的体积密度为2.78 g/cm³,开气孔率小于2.0%,基体较为致密,1 200 ℃时热导率（厚度方向）为14.30 W/（m?K）,室温~1 200 ℃厚度方向和面内方向的线胀率分别为0.59%、0.56%,平均热胀系数分别为5.02×10^-6、4.73×10^-6/K;室温面内拉伸强度典型值为317 MPa,SEM显示试样断面具有明显的纤维拔出效应,弯曲强度和层间拉伸强度典型值分别达794和49 MPa。     

C/SiC复合材料反射镜研究进展

反射镜在空间光学系统中起着非常关键的作用,目前已发展到第四代C/SiC复合材料。C/SiC复合材料具有低密度、高模高强、结构设计灵活等优点,已成为非常重要的新型反射镜材料。本文对四代反射镜的特点进行了归纳和对比,对C/SiC复合材料反射镜的结构设计、几种常用的制备工艺进行了整理和总结,并对目前国内外的研究进展进行了综述。