运载火箭中电子设备的阻尼隔振

本文叙述了用国产9050粘弹性高阻尼材料制成的阻尼垫式的三向隔振器来代替JPZ三向等刚度减震器附加阻尼器组成的三向隔振系统。当用在5.8kg设备中,阻尼垫隔振器的低频共振频率为45±3Hz,放大率小于3。当激励频率大于67Hz时,即起隔振作用。     

大型航天产品冲击响应谱试验方法探讨

文章对目前国內外冲击响应谱的试验方法进行了简要的描述,重点探讨了利用谐振的方法来完成大型航天产品的冲击响应谱试验的可行性,为大型谐振板冲击响应谱模拟装置的研制及大型航天产品的冲击响应谱试验,提供了很有价值的参考。     

固体火箭发动机推力终止过程的数值分析

本文指出,在大、中型固体火箭发动机的推力终止过程中,打开反向喷管(或辅助排气孔)必定导致产生一系列强度相当大的压力脉冲,而现有的理论分析均不能预估和解释这一现象。本文提供了一组冷模拟实验结果,讨论了产生压力脉冲的原因,提出了估算其强度的方法,并且应用特征线法和激波拟合法进行一维非定常流动的数值计算,发展了一种能够同时预估压力脉冲强度的内弹道计算程序。预估结果与实验曲线吻合良好。     

带反喷管发动机地面实验数据分析

带反喷管固体火箭发动机地面实验时，在其反向喷管打开后，激波进入主喷管情况下，会给数据处理带来困难。文中介绍了根据地面实验数据分析反喷管在高空提供的反推力，为带反喷管发动机地面实验数据处理提供了简便的分析方法。     

康普顿散射对X射线热激波破坏效应的影响

本文应用ＧＲＡＹ三相物态方程及Ｌａｇｒａｎｇｅ数值模拟方法，计算并讨论了康普顿散射对Ｘ射线热激波及其破坏效应的影响。计算结果表明，对较硬的Ｘ射线谱（１５ｋｅＶＰｌａｎｃｋ谱），康普顿散造成量沉积与热击波峰压明显下降，在ＬＹ－１２铝中，能量沉积的相对差△Ｅ（ｘ）／Ｅ（ｘ）可达９％－２２％，热击波峰压的相对差△ｐｍ（ｘ）／ｐｍ（ｘ）约为１２％。     

基于单CPU的通用微机冲击振动控制技术

基于单ＣＰＵ的通用微机冲击振控制技术的独到之处在于，冲击驱动信息的生成、修正以及冲击响应信号的采样、分析等操作均由微机软件进行控制。主要介绍实现该技术的软件设计原理，并给出相应控制实验结果。     

Reflected shock/turbulent boundary layer interaction structure analysis based on large eddy simulation

In order to understand the physical phenomenon of the reflected shock/turbulent boundary layer interaction, the Large Eddy Simulation (LES) is conducted to investigate shock wave and turbulent boundary layer interaction in a $12°$ compression ramp with inlet high Mach number of 2.9. Rescaling/recycling method is used as inflow turbulence generation technique and validated on a supersonic flat plate turbulent boundary layer. The flow field of recycling plane in the plate computation domain is obtained to give the inlet boundary condition for the LES computation. This paper focuses on the reflected shock/turbulent boundary layer interaction region, where the fine flow structure and instantaneous flow field are analyzed in detail. It is found that the unsteady motion of the shock wave leads to the increase of wall pressure fluctuation.     

Aeroelastic stability analysis of heated flexible panel subjected to an oblique shock

The critical conditions for aeroelastic stability and the stability boundaries of a flexible two-dimensional heated panel subjected to an impinging oblique shock are considered using theoretical analysis and numerical computations, respectively. The von-Karman large deflection theory of isotropic flat plates is used to account for the geometrical nonlinearity of the heated panel, and local first-order piston theory is employed in the region before and after shock waves to estimate the aerodynamic pressure. The coupled partial differential governing equations, according to the Hamilton principle, are established with thermal effect based on quasi-steady thermal stress theory. The Galerkin discrete method is employed to truncate the partial differential equations into a set of ordinary differential equations, which are then solved by the fourth-order Runge-Kutta numerical integration method. Lyapunov indirect method is applied to evaluate the stability of the heated panel. The results show that a new aeroelastic instability (distinct from regular panel flutter) arises from the complex interaction of the incident and reflected wave system with the panel flexural modes and thermal loads. What’s more, stability of the panel is reduced in the presence of the oblique shock. In other words, the heated panel becomes aeroelastically unstable at relatively small flight aerodynamic pressure.     

Evolution of the temporal and the spectral properties in 2010 and 2011 outbursts of H 1743-322

The Galactic black hole candidate H 1743-322 exhibited two X-ray outbursts in rapid succession: one in August 2010 and the other in April 2011. We analyze archival data of this object from the PCA instrument on board RXTE (2–25 keV energy band) to study the evolution of its temporal and spectral characteristics during both the outbursts, and hence to understand the behavioral change of the accretion flow dynamics associated with the evolution of the various X-ray features. We study the evolution of QPO frequencies during the rising and the declining phases of both the outbursts. We successfully fit the variation of QPO frequency using the Propagating Oscillatory Shock (POS) model in each of the outbursts and obtain the accretion flow parameters such as the instantaneous shock locations, the shock velocity and the shock strength. Based on the degree of importance of the thermal (disk black body) and the non-thermal (power-law) components of the spectral fit and properties of the QPO (if present), the entire profiles of the 2010 and 2011 outbursts are subdivided into four different spectral states: hard, hard-intermediate, soft-intermediate and soft. We attempt to explain the nature of the outburst profile (i.e., hardness-intensity diagram) with two different types of mass accretion flow.     

Direct numerical simulation of impinging shock wave and turbulent boundary layer interaction over a wavy-wall

The interaction of an impinging oblique shock wave with an angle of 30° and a supersonic turbulent boundary layer at Ma_∞=2.9 and Re_θ = 2400 over a wavy-wall is investigated through direct numerical simulation and compared with the interaction on a flat-plate under the same flow conditions. A sinusoidal wave with amplitude to wavelength ratio of 0.26 moves in the streamwise direction and is uniformly distributed across the spanwise direction. The influences of the wavy-wall on the interaction, including the characterization of the flow field, the skin-friction, pressure and the budget of turbulence kinetic energy, are systematically studied. The region of separation grows slightly and decomposes into four bubbles. Local peaks of skin-friction are observed at the rear part of the interaction region. The low-frequency shock motion can be seen in the wall pressure spectra. Analyses of the turbulence kinetic energy budget indicate that both diffusion and transport significantly increase near the crests, balanced by an amplified dissipation in the near-wall region. Proper orthogonal decomposition analyses show that the most energetic structures are associated with the separated shock and the shear layer over the bubbles. Only the bubbles in the first two troughs are dominated by a low-frequency enlargement or shrinkage.