相变光盘的介质优选及理论计算

 本文着重论述相变光盘的存储机理、介质优选、理论计算及光存储最新进展。     

涡轮盘用变形高温合金在俄国的发展

本文简要介绍了俄国涡轮盘用变形高温合金的发展概况,列出了一些合金的成分和性能,其最高工作温度可达850℃,这个合金系列均可采用传统的熔炼加变形工艺生产涡轮盘,且其质量和性能水平可与粉末涡轮盘相比美。     

相变光盘多层膜系结构的最佳光匹配研究

论述了相变光盘最佳膜系结构的设计。采用导纳矩阵法计算膜系的能量反射率，用量优化计算方法编程计算，提出了第二大极值解作为在工艺上可行的实用光盘的膜系结构，并按这种膜系结构制作样品，其擦写循环数达１００万次上。     

Numerical study on flow fields and aerodynamics of tilt rotor aircraft in conversion mode based on embedded grid and actuator model

A method combining rotor actuator disk model and embedded grid technique is presented in this paper, aimed at predicting the flow fields and aerodynamic characteristics of tilt rotor aircraft in conversion mode more efficiently and effectively. In this method, rotor's influence is considered in terms of the momentum it impacts to the fluid around it; transformation matrixes among different coordinate systems are deduced to extend actuator method's utility to conversion mode flow fields' calculation. Meanwhile, an embedded grid system is designed, in which grids generated around fuselage and actuator disk are regarded as background grid and minor grid respectively, and a new method is presented for ‘donor searching' and ‘hole cutting' during grid assembling. Based on the above methods, flow fields of tilt rotor aircraft in conversion mode are simulated, with threedimensional Navier–Stokes equations discretized by a second-order upwind finite-volume scheme and an implicit lower–upper symmetric Gauss–Seidel(LU-SGS) time-stepping scheme. Numerical results demonstrate that the proposed CFD method is very effective in simulating the conversion mode flow fields of tilt rotor aircraft.     

The ‘soot line’: Destruction of presolar polycyclic aromatic hydrocarbons in the terrestrial planet-forming region of disks

Interstellar material is highly processed when subjected to the physical conditions that prevail in the inner regions of protoplanetary disks, the potential birthplace of habitable planets. Polycyclic aromatic hydrocarbons (PAHs) are abundant in the interstellar medium, and they have also been observed in the disks around young stars, with evidence for some modification in the latter. Using a chemical model developed for sooting flames, we have investigated the chemical evolution of PAHs in warm (1000–2000 K) and oxygen-rich (C/O < 1) conditions appropriate for the region where habitable planets may eventually form. Our study focuses on (1) delineating the conditions under which PAHs will react and (2) identifying the key reaction pathways and reaction products characterizing this chemical evolution. We find that reactions with H, OH and O are the main pathways for destroying PAHs over disk timescale at temperatures greater than about 1000 K. In the process, high abundances of C₂H₂ persist over long timescales due to the kinetic inhibition of reactions that eventually drive the carbon into CO, CO₂ and CH₄. The thermal destruction of PAHs may thus be the cause of the abundant C₂H₂ that has been observed in disks. We propose that protoplanetary disks have a ‘soot line’, within which PAHs are irreversibly destroyed via thermally-driven reactions. The soot line will play an important role, analogous to that of the ‘snow line’, in the bulk carbon content of meteorites and habitable planets.     

Growth of hydrodynamic perturbations in accretion disks: Possible route to non-magnetic turbulence

We study the possible origin of hydrodynamic turbulence in cold accretion disks such as those in star-forming systems and quiescent cataclysmic variables. As these systems are expected to have neutral gas, the turbulent viscosity is likely to be hydrodynamic in origin, not magnetohydrodynamic. Therefore, MRI will be sluggish or even absent in such disks. Although there are no exponentially growing eigenmodes in a hydrodynamic disk because of the non-normal nature of the eigenmodes, a large transient growth in the energy is still possible, which may enable the system to switch to a turbulent state. For a Keplerian disk, we estimate that the energy will grow by a factor of 1000 for a Reynolds number close to a million.     

失调叶片盘耦合振动的力学模型

借助于子结构模态综合法,为研究真实的失调叶片盘耦合振动问题提出了一种非常接近于实际叶片盘的力学模型和简便的理论分析方法;并通过对一个实际失调叶片盘的强迫振动试验,对力学模型、计算公式和程序进行了考核验证。结果表明,试验与计算相当吻合。     

碟形弹簧的弯曲效应问题

以采用壳体非线性无矩理论所确定的碟形弹簧薄膜位移与薄膜应力作为初始状态,采用壳体线性有矩理论对碟形弹簧进行了弯曲位移与弯曲应力分析.分析表明:与薄膜应力相比,弯曲应力是不能略去的;而与薄膜位移相比,弯曲位移是可以略去的.因此,对碟形弹簧而言,以壳体非线性无矩理论确定位移是合理的,而以壳体线性有矩理论确定附加弯曲应力也是可行的,同时也是必要的.     

基于主动热载荷管理技术的涡轮盘疲劳寿命

为降低航空发动机涡轮盘失效风险并提高使用寿命,将主动热载荷管理技术应用于预置裂纹的涡轮盘模型,采用通用权函数法计算裂纹应力强度因子进而分析轮盘寿命,研究经主动热载荷管理的轮盘上能量分布对轮盘寿命的影响,探索轮盘上热边界载荷与寿命的关联性和变化规律,并通过有限元仿真模拟初步分析其作用机理。结果表明:主动热载荷管理技术通过优化轮盘的温度分布,可以有效地降低裂纹附近的应力,延缓裂纹的扩展,显著的提高寿命和安全性,当热边界载荷系数分别取0.05和0.10时,轮盘相应的寿命分别增加12.2%和26.1%。     

盘轴转子系统临界转速计算的改进传递矩阵法

在用传递矩阵法分析转子系统的临界转速时,传统的方法是忽略轮盘的厚度,将轮盘的传递矩阵作为点矩阵来处理的,这样会导致转子轴的刚度比实际模型的低,进而导致临界转速的计算结果偏低。本文将通过轮盘的传递矩阵作为场矩阵来处理,对计及轮盘厚度的传递矩阵进行了推导。分别使用传统传递矩阵法和本文提出的改进传递矩阵法对2个盘在不同位置的单盘转子模型以及一个多盘转子系统的临界转速进行了计算。对比结果表明,传统传递矩阵法的计算误差很容易就会达到一个不可忽略的水平,改进的传递矩阵法解决了这一问题。