三支点柔性转子系统支承不同心激励特征及振动响应分析

针对航空发动机三支点柔性转子系统的支承不同心问题,充分考虑转子结构特征和载荷特征,首次将当量刚度引入多支点柔性转子不同心问题的动力学分析,定量描述转子系统各支承间不同心度带来的转子轴段刚度非线性,并提出了多跨度柔性转子系统支承不同心激励的数学描述,建立了不同心激励下多跨度柔性转子系统的力学模型。基于Lagrange能量法,给出了转子系统动力学方程的求解方法,研究得到了支承不同心转子系统的动力响应特征。结果表明:支承不同心不仅引起转子过渡轴的刚度非线性,产生2倍频激励,还会给转子系统带来附加不平衡激励;对于三支点柔性转子系统而言,2倍频分量同样是支承不同心下转子系统振动响应的典型特征之一。转子系统2倍频分量随不同心量的增加而迅速增加,而1倍频分量基本保持不变。同时转子振动响应呈现"缓增速降"趋势,且随非线性刚度、不平衡量的增大愈加明显。     

基于加速度测量的智能桁架结构振动主动控制

加速度传感器具有频带宽、结构简单、重量轻等优点而获得了广泛使用，因此研究基于加速度测量的结构控制系统具有较大的实用价值。文中的只能获得加速度时，采用模态滤波器技术实现从物理加速度响应解耦得到单模态加速度的响应。然后改变Ｌｕｅｎｂｅｒｇｅｒ观测器的结构形式，从模态加速度响应观测得到模态们移和模态速度响应。基于模态滤波器和最优控制理论，采用独立模态空间控制策略，实现了具有密集模态的三维柔性智能桁架结构     

利用航天器分舱段振动试验数据获取整器响应的方法

未来大型组合体航天器振动试验可能难以在现有设备上进行,需要进行分舱考核。文章针对此问题开展了利用分舱段振动试验获取整器响应的方法研究。提出的方法为:根据不同界面下模态的映射关系,利用单舱段的振动试验数据辨识出舱段的两端固支模态;采用模态综合技术计算出整器组合体模态参数,拟合出结构的加速度响应传递函数;结合整器的加速度试验条件可以给出整器的试验响应曲线。仿真验证结果表明该方法合理可行,具有工程应用价值。     

TRANSIENT RESPONSE INVESTIGATION OF GIMBALLED TILTROTORS DURING ENGAGE AND DISENGAGE OPERATIONS

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Cosmic ray acceleration by supernova shocks

We analyse the results of recent measurements of nonthermal emission from individual supernova remnants (SNRs) and their correspondence to the nonlinear kinetic theory of cosmic ray (CR) acceleration in SNRs. It is shown that the theory fits these data in a satisfactory way and provides the strong evidences for the efficient CR production in SNRs accompanied by significant magnetic field amplification. Magnetic field amplification leads to considerable increase of CR maximum energy so that the spectrum of CRs accelerated in SNRs is consistent with the requirements for the formation of Galactic CR spectrum up to the energy ∼10¹⁷ eV.     

Mean energy of response to galactic cosmic ray spectrum: IMP 8 and Climax neutron monitor

Solar modulations of galactic cosmic ray (GCR) intensity contain a wealth of information about their transport in the heliosphere. To extract this information from the data one studies the dependence of the observed modulations on the mean energy of response of detectors providing data for the analyses. There is a great deal of confusion about the detector energy response to GCR spectrum in the literature. We present a preliminary report on the computations of the mean energy of response for the Climax neutron monitor (CL/NM) and IMP 8 cosmic ray nuclear composition instrument to GCR protons for 1973–1998, covering the solar cycles 21 and 22. We find that for penetrating proton channel on IMP 8 the mean energy changes by a factor of over two whereas for the neutron monitor the change is only 21%. However, the corresponding change for the computed modulation function is a factor of about 3.5.     

气动力/热与结构多场耦合试验模型方案初步设计

以多渠道、多机制交叉耦合为热防护结构特点的新一代高超声速飞行器必须采用气动力/热与结构多场耦合计算方法进行研究。目前,国外已建立较完善的耦合分析系统并用于飞行器研制,国内的中国空气动力研究与发展中心(CARDC)也已自主研发了热环境/热响应耦合计算平台(FL-CAPTER)。为验证多场耦合计算平台所用方法的有效性和计算结果的准确性,设计并开展气动力/热与结构耦合的地面试验具有十分重要的意义。本文结合气动力/热与结构多场耦合试验设计需求,以现有材料和设备能力为依托,开展了试验风洞选取、模型尺寸估算、模型材料选择、模型气动设计与模型结构设计工作。初步研究表明,模型支撑结构附近迎风面局部高温热膨胀将有利于模型前体结构产生可观的整体变形量。本文以此设计了带压缩拐角的二级压缩面结构模型,通过短时间不锈钢模型验证试验和计算对比分析初步验证了模型设计的可行性,并以此为基础预测了高温合金模型的试验结果。为下一步开展高温合金长时间风洞试验奠定了技术基础。     

Particle Acceleration Mechanisms

In this paper we review the possible mechanisms for production of non-thermal electrons which are responsible for the observed non-thermal radiation in clusters of galaxies. Our primary focus is on non-thermal Bremsstrahlung and inverse Compton scattering, that produce hard X-ray emission. We first give a brief review of acceleration mechanisms and point out that in most astrophysical situations, and in particular for the intracluster medium, shocks, turbulence and plasma waves play a crucial role. We also outline how the effects of the turbulence can be accounted for. Using a generic model for turbulence and acceleration, we then consider two scenarios for production of non-thermal radiation. The first is motivated by the possibility that hard X-ray emission is due to non-thermal Bremsstrahlung by nonrelativistic particles and attempts to produce non-thermal tails by accelerating the electrons from the background plasma with an initial Maxwellian distribution. For acceleration rates smaller than the Coulomb energy loss rate, the effect of energising the plasma is to primarily heat the plasma with little sign of a distinct non-thermal tail. Such tails are discernible only for acceleration rates comparable or larger than the Coulomb loss rate. However, these tails are accompanied by significant heating and they are present for a short time of <10⁶ years, which is also the time that the tail will be thermalised. A longer period of acceleration at such rates will result in a runaway situation with most particles being accelerated to very high energies. These more exact treatments confirm the difficulty with this model, first pointed out by Petrosian (Astrophys. J. 557:560, 2001). Such non-thermal tails, even if possible, can only explain the hard X-ray but not the radio emission which needs GeV or higher energy electrons. For these and for production of hard X-rays by the inverse Compton model, we need the second scenario where there is injection and subsequent acceleration of relativistic electrons. It is shown that a steady state situation, for example arising from secondary electrons produced from cosmic ray proton scattering by background protons, will most likely lead to flatter than required electron spectra or it requires a short escape time of the electrons from the cluster. An episodic injection of relativistic electrons, presumably from galaxies or AGN, and/or episodic generation of turbulence and shocks by mergers can result in an electron spectrum consistent with observations but for only a short period of less than one billion years.     

带止口法兰连接结构刚度特性对结构振动影响

对带有止口的法兰连接结构刚度特性进行了数值仿真研究。使用有限元软件ANSYS分析了带有止口的法兰连接结构的迟滞特性。通过对止口接触面的变形-滑移机理分析,使用一个詹金斯单元和一个弹簧单元并联模拟法兰的一个扇区,并基于法兰弯曲变形时每个扇区的不同状态建立了整个法兰结构的弯曲刚度简化模型,并对该简化模型进行了仿真,该简化模型能够较准确地模拟带止口法兰连接结构的刚度特性。基于简化模型和梁单元建立了简化转子结构模型,分析了带有止口的法兰连接结构对转子稳态动力学响应的影响。结果表明带有止口的法兰连接结构的迟滞特性能够影响峰值频率,随着止口过盈量的增加，响应峰值显著降低,具有较好的振动抑制效果。      

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.