A statistical study of C IV regions in 20 Oe-stars

In this paper, using the Gauss-Rotation model (GR model), we analyse the UV C IV resonance lines in the spectra of 20 Oe-stars of different spectral subtypes, in order to detect the structure of C IV region. We study the presence and behavior of absorption clouds and analyse their characteristics. From this analysis we can calculate the values of a group of physical parameters, such as the apparent rotational and radial velocities, the random velocities of the thermal motions of the ions, the Full Width at Half Maximum (FWHM), the optical depth, as well as the absorbed energy and the column density of the independent regions of matter, which produce the main and the satellite clouds of the studied spectral lines. Finally, we present the relations between these physical parameters and the spectral subtypes of the studied stars and we give our results about the structure of the C IV region in their atmosphere.     

Effect of protrusion amount on gas ingestion of radial rim seal

In this paper, the effect of different amount of protrusion on various parameters in rotor–stator system was experimentally studied by measuring CO₂ concentration and pressure, in order to obtain the optimal protrusion amount. The parameters of different dimensionless sealing flow were measured under the condition that the annulus Reynolds number was 4.39 × 10⁵ and the rotating Reynolds number was 1.05 × 10⁶. The results show that the change of the amount of protrusions has little effect on the static pressure in the cavity, and the static pressure change near the sealing ring is almost negligible. But the total pressure and sealing efficiency increase first and then decrease with the increase of the amount of protrusion. The variation of power consumption is the same. A complex vortex structure will appear at the high radius region when the protrusion is installed. On the other hand, the protrusion can effectively reduce the minimum sealing flow of the rotor–stator cavity. Furthermore, considering the sealing efficiency and power consumption, the best range of the protrusion amount is about 36. The ratio near this range can optimally balance the alleviation of the gas ingestion and the reduction of the power consumption.     

某机第4级压气机转子叶片榫头折断故障分析

阐明了某机第4级压气机转子叶片在榫头部位断裂的故障特点。故障分析表明：经长期使用的叶片在修理厂大修时，为满足叶片摆动量要求在榫头底面涂尼龙胶，会使叶片自振频率有较大幅度下降；为排除3级叶片折断故障而提高的慢车转速又缩小了4级叶片的共振裕度，结果造成少数4级叶片落入慢车共振。共振发生时，不规则的尼龙胶和装配过程不规范引起的非正常接触容易导致微动磨损的加剧，从而大大降低了疲劳寿命，这是引起榫头断裂故障的主要原因。     

凹腔火焰稳定器阻力特性的实验研究

在超燃冲压发动机直连式实验中,模拟马赫数1.92、静温509K、静压86.6kPa来流,采用等截面燃烧室构型,利用推力测量系统对不同结构尺寸的开式凹腔火焰稳定器的冷流阻力和热试阻力进行了研究。通过对深度分别为10,15,20mm,长深比4~10,后壁倾斜角18°~60°的凹腔火焰稳定器的冷流阻力比较,实验表明凹腔火焰稳定器的冷流阻力与凹腔深度成正比;也与凹腔长深比成正比;并随后壁倾斜角的增大先减小后增大,在30°~60°范围内应存在一个角度使得冷流阻力最小。实验还以氢气为燃料,利用火花塞点火器进行点火,在燃烧模态下对不同喷注位置、不同当量比时的凹腔火焰稳定器阻力特性进行了对比,结果表明凹腔火焰稳定器的热试阻力比冷流阻力小,且受燃料喷注方式的影响较大;在实际超燃冲压发动机工况下,凹腔火焰稳定器的阻力随着当量比的增加而减小,并最终会表现为正推力。     

Alfvénic Electron Acceleration in Aurora Occurs in Global Alfvén Resonosphere Region

Auroral emission caused by electron precipitation (Hardy et al., 1987, J. Geophys. Res. 92, 12275–12294) is powered by magnetospheric driving processes. It is not yet fully understood how the energy transfer mechanisms are responsible for the electron precipitation. It has been proposed (Hasegawa, 1976, J. Geophys. Res. 81, 5083–5090) that Alfvén waves coming from the magnetosphere play some role in powering the aurora (Wygant et al., 2000, J. Geophys. Res. 105, 18675–18692, Keiling et al., 2003, Science 299, 383–386). Alfvén-wave-induced electron acceleration is shown to be confined in a rather narrow radial distance range of 4–5 R _E (Earth radii) and its importance, relative to other electron acceleration mechanisms, depends strongly on the magnetic disturbance level so that it represents 10% of all electron precipitation power during quiet conditions and increased to 40% during disturbed conditions. Our observations suggest that an electron Landau resonance mechanism operating in the “Alfvén resonosphere” is responsible for the energy transfer.     

带内锥冲头挤压过程中金属变形流动行为研究

针对平模挤压过程中易产生死区、缩孔等流动缺陷,设计一种带内锥冲头用以改善成形过程中金属的变形流动行为.对冲头有、无内锥两种形式挤压过程进行数值模拟,利用罗德系数、J2应力偏量不变量等特征量进行变形分区,并利用7050铝合金进行挤压试验验证.结果表明,带内锥冲头能有效改善挤压过程中速度场的分布,显著减小死区,并避免产生缩孔缺陷.因此,带内锥冲头更利于金属的挤出成形.     

直升机尾桨/尾梁耦合稳定性分析研究

单桨带尾桨直升机的尾旋翼设计成摆振柔软型后,带来了新的动力学问题:尾桨与尾梁耦合动不稳定性问题。本文简述了它与主旋翼/机体耦合动不稳定问题的差别,主要介绍了尾桨与尾梁耦合动不稳定性问题的分析方法,通过算例分析,为消除这种不稳定性,对一些关键设计参数提出了设计要求。     

一种惯性导航用减振器的低温工作特性

使用带有环境温湿度箱的电磁振动台进行一种航空惯性导航用减振器(JZ-2）的低温动态性能测试,研究了该型减振器的低温(-70℃~20℃）工作特性,得到该减振器的谐振频率以及放大倍数在温度降低条件下的变化规律,并将谐振频率与温度的关系推广至压剪型硅橡胶减振器,为航空器用惯性导航设备在高寒地区的设计以及使用提供参数依据。研究结果表明,当温度低于室温,压剪型橡胶减振器的低温谐振频率与温度的关系符合一阶指数衰减函数。     

转静盘腔流动瞬态响应特性研究

以航空发动机转静盘腔内非稳态流动为研究对象,基于用户自定义函数编程设置进口压力按斜坡函数变化时的非稳态边界条件,利用数值模拟方法,在滞后效应、流场演化和物性参数方面,研究了不同无量纲跃升幅值下转静盘腔流动瞬态响应机理。结果表明:无量纲跃升幅值由1.05增至1.2,盘腔内部的当地响应时间延长了81.1%,相对总温的超调量增加了157.0%,其峰值时间增加了31.3%,且进口压力波动的传播方向总是由进口指向出口;瞬态过程中,转静盘腔的容积效应和旋转效应共同作用使出口流量明显滞后进口流量,且其滞留质量流量与相对总温的超调现象密切相关;冲击射流、旋转贴壁射流和静子壁面侧的涡系构成了盘腔流场演化的主体,无量纲跃升幅值越大,流场演化过程越剧烈,响应时间越长;声速和热扩散率与盘腔响应速度密切相关。     

进口流量对无管式减涡器流阻特性影响研究

为分析进口流量对压气机引气系统无管式减涡器压力损失的影响及无管式减涡器减阻效果,采用数值模拟与试验研究相结合的方法对无管式减涡器开展研究,并与直喷嘴模型进行了对比。模型试验验证了数值模拟方法的可靠性,通过数值模拟,建立了无管式减涡器流阻特性"S"形曲线三分区模型,分析了无管式减涡器各截面间压力损失及其占比随无量纲质量流量变化规律。在计算流量范围内,与直喷嘴模型相比,无管式减涡器平均可降低压气机引气系统压力损失约45.9%。在第二拐点处,共转盘腔内压力损失降低了96.44%,此时无管式减涡器减阻效果最佳,较直喷嘴模型压力损失降低了73.44%。