纸基蜂窝模块化固持方法研究

 基于磁场与摩擦学蜂窝芯材料固持原理,提出复杂型面纸基蜂窝零件固持平台的模块化设计思想。运用移动模块、固定模块、模块夹具以及导磁体和隔磁体解决了该原理中磁路控制问题,实现了复杂曲面零件在模块化固持平台上的加工固持。通过理论分析和有限元仿真研究了固持系统中蜂窝孔格的受力,分析了固持系统的特点和可靠性,以及永磁体厚度、固定平台高度、铁粉填充高度和平台间隙对磁场力的影响规律。实验与仿真结果表明,模块化固持平台能够满足复杂曲面蜂窝铣削加工的固持要求。     

气膜孔内置扰动条作用下的射流-横流流场

为改善气膜冷却效率,提出了在倾斜气膜孔前缘内置扰动条的结构。通过与典型的圆柱形气膜孔流场的对比研究,总结出内置扰动条对流场的影响规律。研究结果表明,在射流-横流流场中,内置扰动条减小了射流向主流的穿透,使反向旋转涡对向壁面靠拢,穿透顶点下移;扰动条使下游反向涡对的强度增大;随着吹风比的增大,气膜孔下游同一位置处的流向涡强度增大,这一方面增加了主次流的相互掺混,另一方面也增大了流体沿展向的相互掺混。     

构件低周疲劳损伤的金属磁记忆检测试验研究

对18CrNi4A钢缺口试件在三级应力水平下进行了低周疲劳试验和磁记忆信号检测,研究应力集中、疲劳损伤及疲劳应力对磁信号的影响规律。结果表明,利用磁信号Hp(y)曲线突变特征和磁信号梯度K曲线异变峰特征可表征试件损伤位置;采用H′p(y)=Hp(y)N-Hp(y)0的磁信号处理方式,磁信号H′p(y)曲线过零点与试件断裂位置重合,处理后的磁信号过零法可更有效的表征试件损伤位置;磁信号梯度Kmax值随疲劳损伤程度的增加而逐渐增加,反映了构件疲劳损伤程度,可表征试件疲劳损伤程度;磁信号与疲劳应力水平存在强烈的相关性,应力水平越大,磁信号值也越大。     

磁悬浮反作用飞轮速率模式控制系统设计

针对磁悬浮反作用飞轮干扰力矩对输出力矩精度的影响,提出了一种速率模式数字控制方法,实现了正向加速、正向减速、反向加速、反向减速的四象限高精度稳定的转速跟踪控制,减速时,高速段利用飞轮储存的动能进行能耗制动,低速时进行反接制动,从而实现磁悬浮反作用飞轮速率模式控制.     

异种金属材料磁脉冲焊接技术

通过对磁脉冲焊接技术结合机理的阐述,采用5A03Al-5A06Al、1050Al-AZ31Mg异种金属材料进行焊接试验.对所得的焊接接头进行气密性试验和剥离试验,检测其结合质量;结合光学显微镜,对比分析Al-Al、Al-Mg焊接接头的微观形貌特点;并采用SEM/EDS分析界面附近的元素分布;最后通过硬度试验,检测接头界...     

高精度光纤IMU的磁屏蔽方法及实验研究

惯性测量单元(IMU)是位置姿态系统(POS)的核心部分,IMU的精度很大程度上决定着POS精度.由于高精度光纤陀螺(FOG)的光纤线圈对磁场敏感,基于高精度FOG的IMU精度会受磁场影响而降低.本文研究了FOG磁敏感性机理,通过实验得出高精度光纤IMU对磁场敏感的结论.采用电磁场有限元分析软件Ansoft Maxwe...     

端弯叶片通道出口二次流的研究

实验并且采用考虑粘性的涡传输方程计算端弯压气机叶片通道出口二次流。给出了３种端弯叶片及对应的原始直叶片通道出口气流偏转角的实验值和计算预测值。研究表明：采用上述方程能比较准确地预测出口气流偏转角；叶片后缘减弯可减小流向二次涡强度。     

考虑顶隙的压气机单转子内三维跨音速粘性流场结构的数值模拟

借助于考虑叶片顶部间隙的压气机转子内跨音速湍流流场的三维数值解,得到了该转子流场中的复杂涡系与波系结构。给出了叶片表面及轮毂面上的壁面流型,分析并揭示了转子叶道内的马蹄涡、通道涡、角涡、尾涡等复杂涡系及其与激波的相互干涉;特别是,分析并揭示了转子叶道内顶隙射流的特点,得到了顶隙附近激波与泄漏流动的干涉形态及泄漏流动的发展,并着重给出了其与激波的干涉形态。     

Relationship Between Substorm Auroras and Processes in the Near-Earth Magnetotail

Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for monitoring of substorm intensity in terms of the magnetic flux and energy dissipation.     

Geoeffectivity of Coronal Mass Ejections

Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity, magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour high-latitude activity.