滑动轴承—转子系统Hopf分岔分析计算方法

基于Hopf分岔定性理论、周期系统Floquet理论,针对流固耦合系统力函数计算特点,并考虑系统规模大小对算法的不同要求,提出了一套新的转子-轴承系统Hopf分岔分析计算方法。这套方法主要包括自激周期解计算的边值方法、周期解稳定性判别算法、周期解预测-校正延续算法、自激振动的稳定裕度准则等,可以有效地确定转子-轴承系统Hopf分岔临界点及分岔方向,可以研究分岔解的发展、变化,包括研究实践中关注的“跳跃”、“迟滞”等典型非线性现象。      

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.     

高温超导磁悬浮助推缩比试验系统动态测试分析

基于磁悬浮助推技术概念研究方案建立了一套悬浮加速缩比试验系统.从整体缩比模型振动试验出发,主要研究悬浮质量以及悬浮刚度对整体系统动态性能的影响,并在进行缩比单元动态试验结论的基础上,建立试验模型的加速试验动态采集系统,对整体模型进行运行性能试验.在试验基础上提出了提高磁悬浮推进系统运行稳定性的依据,并据此提出相应可行的解决方案设想.通过模型加速试验并采集试验数据定性分析磁浮系统的综合运动性能,以更好地评估系统稳定特性和品质,也为进一步研究磁悬浮助推发射的气动、分离系统稳定性和可靠性提供参考.     

更替某型飞机电压限定器的研究

文章在介绍某型电压限定器工作原理的基础上,阐述了利用集成电路技术和自动控制技术进行该型电压限定器国产化研制的方法,给出了电压限定器探测及延时电路、均衡控制电路、防止误动作保护电路的详细设计方案,解决了激磁控制、均衡控制、故障鉴别等国产化研制过程中遇到的问题,保证了新研制产品与原有进口产品的可互换使用,提高了设备的工作可靠性。     

磁悬浮火箭发动机推力测试台

将电磁悬浮技术用于火箭发动机推力测试试验台是一次新的尝试。本文给出了应用电磁悬浮技术的发动机推力测试试验台的结构,推导了系统的运动方程,并对试验台进行了系统仿真。最后对整个试验台成功进行了多发现场试验,仿真结果和试验结果都表明电磁悬浮技术用于火箭发动机推力测试是成功的,提高了测试系统的性能和推力测试精度。     

On the Coronal Magnetic Field Configuration and Solar Flare/CME Process

The coronal magnetic field configuration is important for understanding the energy storage and release processes that account for flares and/or CMEs. Here we present a model which is based on the work for potential magnetic field problems that only applies the condition at infinity with the boundary condition on the solar surface specified. We also discuss some recent progress on general force-free field models. For some event analyses, we have employed MDI/SOHO longitudinal magnetogram insected into the synoptic magnetogram to obtain whole boundary condition over the solar surface. Globally, the extrapolated global magnetic field structures effectively demonstrate the case for the disk signature of the radio CMEs and the evolution of the radio sources during the CME/flare processes.     

高速圆柱滚子轴承保持架动力学特性分析

建立了高速圆柱滚子轴承动力学微分方程,采用精细积分法和预估-校正Adams-Bashforth-Moulton多步法相结合的算法,对高速圆柱滚子轴承动力学微分方程进行求解,并对保持架的动力学特性进行了理论分析.结果表明:过大的保持架间隙比不利于保持架稳定运转;在一个套圈固定、另一个套圈工作状态下,保持架引导方式采用旋转套圈引导时,保持架打滑率较低;保持架采用外引导方式时保持架质心运动较为稳定;在内外圈同向旋转且外圈转速高于内圈转速条件下,保持架采用外引导方式时,保持架打滑率较低;在内外圈反向旋转且外圈转速高于内圈转速条件下,保持架质心轨迹变得不规则;保持架采用外引导方式时,保持架打滑率为负值.      

主动冷却燃烧室燃烧与传热耦合过程迭代分析设计方法

为了对主动冷却超燃冲压发动机进行研究与设计,采用实验与计算相结合的方法,对主动冷却超燃冲压发动机燃烧室内传热与燃烧的耦合过程进行了分析。该方法采用燃烧室静压分布的测量值作为输入条件,开展燃气-结构-燃料耦合传热分析,获得经过冷却系统后燃料的状态参数;将燃料的状态参数作为实验参数,开展直联式超声速燃烧实验,得到新的静压分布,如此反复迭代,直至燃料状态不再变化,最终确定主动冷却燃烧室的各种传热与燃烧特性参数。利用该分析方法,初步开展了不同飞行马赫数条件下主动冷却燃烧室闭环运行状态研究,得到了冷却煤油温度与燃烧室壁温同飞行马赫数的关系。     

基于库伦摩擦效应的箔片轴承极限承载力理论与试验

基于有限单元法建立了考虑库伦摩擦的波箔型径向气体箔片轴承的箔片结构模型,采用有限差分法和有限单元法耦合求解Reynolds方程和气膜厚度方程,通过求解轴颈达到极限偏心率时的轴承极限承载力,研究了箔片结构库伦摩擦效应对轴承极限承载力的影响规律,并搭建了轴承极限承载力测试试验台,利用温度法测量了两个具有不同轴承壳内表面粗糙度的波箔型径向气体箔片轴承的轴承极限承载力.通过对比分析仿真结果与试验结果表明:轴承壳圆柱孔内表面粗糙度为0.4μm的轴承在10000r/min和20000r/min下,轴承极限承载力分别为15.5N和42.3N;而表面粗糙度为1.6μm的轴承极限承载力为10.9N和29.6N,这是由于波纹箔片和轴承壳体之间的库伦摩擦力增大了波纹箔片的刚度,因此增大箔片结构摩擦因数使得轴承极限承载力降低,并且仿真结果变化趋势和试验结果变化趋势吻合.