航空发动机轴承预载的加载方法与工程实践

航空燃气涡轮发动机的转子具有转速高、负荷小的特点,容易引起发动机轴承打滑,进而造成滑蹭损伤,如不采取防滑措施,将对发动机的正常、可靠工作构成威胁。在某型发动机压气机部件试验过程中,试验件的辅助支点滚珠轴承由于轻载打滑造成轴承失效,导致试验件辅助支点被损坏。通过在试验件转子后与辅助支点前增加一弹簧,对滚珠轴承施加“预载”,试验验证表明,该方法能很好地解决轴承打滑问题,并且试验中轴承温度也得到明显的下降。此种对轴承施加“预载”的方法在后继的多个试验件中也得到成功运用。     

薄板孔边挤压强化对高周疲劳寿命影响的试验

为提高某压气机封严篦齿盘均压孔的疲劳强度,根据均压孔的具体结构形式,设计了三种冷挤压强化方法:单侧多次挤雎法、柱形头挤压法和T形头挤压法.用两种材料(不锈钢1Cr11Ni2W2MoV和镍基高温合金3Y1742)设计加工了带孔薄板模拟件,用上述三种强化方法对孔边进行了强化,同时进行了室温和高温两种温度下的高周疲劳对比试验...     

气量分配对轴径向旋流杯燃烧室贫熄边界的影响

针对轴径向旋流杯燃烧室,研究了头部进气面积及主燃孔布局对此类燃烧室贫熄特性的影响.实验结果表明:减小一级轴向旋流器进气面积和增加主燃孔个数对燃烧室贫熄性能有较大影响.一级进气面积减小20%可拓宽贫熄边界9.7%;增加主燃孔为4个时,燃烧室贫熄边界变宽约7.6%.此外,增加一级进气面积20%,改变二级进气面积20%及改变主燃孔个数为2个等情况对燃烧室贫熄边界影响较小.      

High energy radiation from the direction of the galactic black hole Sgr A

X-ray observations indicate that the Galactic black hole Sgr A^∗ is inactive now, however, we suggest that Sgr A^∗ can become active when a captured star is tidally disrupted and matter is accreted into the black hole. Consequently the Galactic black hole could be a powerful source of relativistic protons with a characteristic energy ∼10⁵² erg per capture. The diffuse GeV and TeV γ-rays emitted in the direction of the Galactic Center (GC) are the direct consequences of p–p collisions of such relativistic protons ejected by very recent capture events occurred ?10⁵ yr ago. On the other hand, the extended electron-positron annihilation line emission observed from GC is a phenomenon related to a large population of thermalized positrons, which are produced, cooled down and accumulated through hundreds of past capture events during a period of ∼10⁷ yr. In addition to explaining GeV, TeV and 511 keV annihilation emissions we also estimate the photon flux of several MeV resulting from in-flight annihilation process.     

Theoretical study of flow ripple for an aviation axial-piston pump with damping holes in the valve plate

Based on the structure of a certain type of aviation axial-piston pump＇s valve plate which adopts a pre-pressurization fluid path （consisting a damping hole, a buffer chamber, and an orifice） to reduce flow ripple, a single-piston model of the aviation axial-piston pump is presented. This sin- gle-piston model comprehensively considers fluid compressibility, orifice restriction effect, fluid resistance in the capillary tube, and the leakage flow. Besides, the instantaneous discharge areas used in the single-piston model have been calculated in detail. Based on the single-piston model, a multi-piston pump model has been established according to the simple hydraulic circuit. The sin- gle- and multi-piston pump models have been realized by the S-function in Matlab/Simulink. The developed multi-piston pump model has been validated by being compared with the numerical result by computational fluid dynamic （CFD）. The effects of the pre-pressurization fluid path on the flow ripple and the instantaneous pressure in the piston chamber have been studied and opti- mized design recommendations for the aviation axial-piston pump have been given out.     

机匣内间断形深孔机械加工研究

通过优化方案自主设计了一套用于深孔加工的刀具方案,用于某发动机主机匣内部关键件凸轮轴的安装孔的加工,为系列化研制该类机型积累了加工经验.     

钉载作用下层板多孔过盈配合分析

本文利用各向异性体平面弹性理论中的复势方法,以Faber级数为工具,导出层板多孔/弹性核过盈配合在钉载作用下的级数解。     

肼推进系统管路工艺孔的一种自动焊技术

介绍了氩气保护自动堵孔焊技术及其所用设备、换气焊接系统、焊接电源等。同时给出了试样焊接、模拟实样堵焊试样的检测试验数据。介绍了焊接的质量，试验表明，各项数据全部符合设计要求。实践证明，自动堵孔焊技术是完全可行的，其设备稳定可靠，重复性好。     

跨声速叶栅通道中叶片压力面簸箕孔型气膜冷却特性

在跨声速叶栅通道内,试验研究了叶片压力面气膜冷却特性,详细地对比分析了在不同主流进口雷诺数(Re=17×105,37×105,57×105)、出口马赫数(Ma=081,091,101)及多个气膜吹风比(M=05～30)条件下的压力面簸箕孔型气膜冷却效率。试验结果表明:主流出口马赫数变化对气膜孔下游冷却效率的分布与具体数值均无影响;而主流进口雷诺数的影响较大。增大主流进口雷诺数使得气膜分离再贴附对应的吹风比相应增大,Re=17×105时在吹风比M=10时出现气膜分离与再贴附现象,而Re=37×105和Re=57×105对应的临界吹风比则分别为20和25;主流进口雷诺数越大,小吹风比下近孔区域的冷却效率越高,而在孔下游区域则相反;大吹风比下,则主流进口雷诺数越大冷却效率越小。     

Black hole accretion and X-ray spectra of QSOS

Changes in Eddington accretion ratios are thought to result in X-ray spectral index changes in Galactic binary black hole systems. Objects with higher Eddington ratios have softer X-ray spectra. Can we apply this result to much more massive black hole systems such as QSOs? If so, X-ray observations will give us valuable insight into the physics of QSOs. Among QSOs, X-ray spectral index is part of a large set of correlated optical and UV observational properties, especially optical Fe II and [O III] strengths in the Hβ region. To investigate whether this set of correlations is related to Eddington ratio, we use as probes, BALQSOs that have been suggested to be youthful super-accretors. We conducted infrared spectroscopy of the Hβ rest wavelength region for a sample of BALQSOs and compared line measurements with those for high and low redshift non-BAL QSOs. Hβ line widths and bolometric luminosity are used to calculate QSO black hole masses and Eddington ratios. Our results support the hypothesis that optical Fe II and [O III] line strengths are Eddington ratio indicators in QSO central engines. A possible explanation is that strong Fe II and weak [O III] indicate abundant cold gas that could fuel near Eddington accretion.