Protostellar Disk Formation and Early Evolution

This contribution describes the formation of circumstellar disks and their earliest evolutionary phases when self-gravity in the disk plays a crucial role in eliciting the transport of mass and angular momentum. We first discuss the formation of protostellar disks within the context of analytic infall-collapse solutions. We then discuss our efforts to understand the behavior of the newly formed disks. Our specific approach consists of performing a detailed analysis of a simplified model disk which is susceptible to the growth of a spiral instability. Using a combination of numerical simulation and semi-analytic analysis, we show how the dramatic early phase of mass and angular momentum transport in the disk can be explained by a second-order nonlinear process involving self-interaction of a dominant two-armed spiral mode. This revised version was published online in June 2006 with corrections to the Cover Date.     

Time-resolved spectroscopy of accretion disks in Algols

Time-resolved spectroscopy during the eclipse of short-period Algol systems, has shown their accretion disks to be small, turbulent structures with non-Keplerian velocity fields and asymmetries between the leading and trailing sides of the disk. These transient disks are produced by the impact of the gas stream on the mass-gaining star, and occur in systems where the star is just large enough to ensure the stream collision is complete. These emission line disks and the excess continuum emission do not always occur together. The permanent accretion disks in at least a few of the long-period Algol systems have features in common with the transient disks including non-Keplerian velocity fields.     

Time-resolved spectroscopy of accretion disks in Algols

Time-resolved spectroscopy during the eclipse of short-period Algol systems, has shown their accretion disks to be small, turbulent structures with non-Keplerian velocity fields and asymmetries between the leading and trailing sides of the disk. These transient disks are produced by the impact of the gas stream on the mass-gaining star, and occur in systems where the star is just large enough to ensure the stream collision is complete. These emission line disks and the excess continuum emission do not always occur together. The permanent accretion disks in at least a few of the long-period Algol systems have features in common with the transient disks including non-Keplerian velocity fields.     

粉末冶金涡轮盘的应用及寿命研究

介绍粉末冶金轮盘在国外的实际应用情况。以美国Ｒｅｎｅ９５粉末冶金涡轮盘为例，综述了国内外对粉末冶金盘合金材料力学特性、疲劳寿命、裂纹扩展特性研究的成果，并对涡轮盘的应力分析技术以及寿命研究发展进行了评述。提出了我国粉末冶金涡轮盘寿命研究的重点和方向。     

航空发动机失谐叶盘动态特性研究进展

航空发动机叶盘结构中不可避免存在的失谐会严重影响发动机的结构完整性和可靠性,国内外针对这一问题进行了大量深入的研究。详述了失谐叶盘建模、模型减缩、动态特性分析及评价等方面的研究现状,重点介绍多级叶盘和几何失谐叶盘的建模和动态特性分析等方面的最新研究进展,并对失谐叶盘未来研究方向进行了预测。     

具有干摩擦散乱失谐的叶盘受迫响应特性

阻尼件是叶盘结构中起减振作用的主要部件,而阻尼件的干摩擦散乱失谐会影响其在叶盘振动中的减振作用。本文利用谐波平衡法与快速傅立叶变换技术,对具有非线性干摩擦力的叶盘受迫响应进行了数学建模,仿真分析了叶盘系统在各种耦合、粘性阻尼比、干摩擦强度、干摩擦散乱失谐程度等参数影响下的受迫响应规律。研究结果显示,叶盘系统在弱耦合和粘性阻尼比较大的情况下,干摩擦散乱失谐会导致叶盘共振幅值显著增大。      

Accretion disks in stellar X-ray sources

This review presents an introduction to the theory of accretion disks. After explaining the importance of accretion disks in stellar X-ray sources, it considers observational and theoretical indications of the formation of accretion disks in close binary systems. The simple Shakura and Sunyaev model and its problems are discussed. A survey of other models that try to improve upon this model is given (in Table III), and critically discussed.     

具有非线性摩擦阻尼随机失谐的叶盘系统响应特性

针对目前含非线性摩擦阻尼失谐叶盘系统振动局部化机理研究存在的诸多困难,尤其是其非线性力学模型的建立和求解等难题.建立了具有滞迟干摩擦阻尼随机失谐的叶盘系统力学模型,并利用增量谐波平衡法分析了叶盘系统干摩擦力失谐度、耦合强度、黏性阻尼比和摩擦力强度等系统参数对叶盘系统受迫响应的影响规律.研究表明:含非线性摩擦阻尼的谐调叶...     

Resonantly Excited Non-linear Density Waves in Disk Systems

Most of the disk systems are characterized by spiral structures. A good portion of these spiral structures can be identified as waves resonantly excited by a perturber in or pertaining to the same system. For planetary rings, this is an exterior satellite; for galactic disks, a rotating bar; for proto-stellar disks (yet to be confirmed), this would be a proto-planet. These waves, not just responsible for the present morphology of the disks, also play a dominating role on evolution of the disks. Resonance excitation is a extremely effective mechanism. A relatively weak perturbation can result in a highly non-linear responses in the disk. Therefore, non-linear theory is a necessity here. We will examine the non-linear theory of resonance excitation and discuss the applications of the theory to Saturn's rings and disk galaxies in this paper.     

计算轮盘破裂转速的大变形解析法

本文为轮盘破裂转速研究课题组的研究报告之一。文中提出的大变形解析法是计算轮盘破裂转速的一种新方法, 首先推导了基本方程, 其次叙述了计算步骤, 并对几个试验盘作了数值计算。最后将计算结果与试验结果作了对比, 误差均在 4 %以内。作者认为, 此法简便易行, 准确度符合工程需要, 适应范围较大, 可以在发动机轮盘研制工作中应用。      

某型发动机涡轮转子温度和应力测试研究

为确保某型发动机的安全使用,通过对该发动机涡轮转子的温度和动应力进行实测,据此对涡轮转子叶片和盘进行强度和寿命计算。对涡轮转子的叶片和盘进行强度初步计算,确定应力最大点,在发动机实际工作状态下,得到测试部位的实际温度和动应力;利用测试结果,计算确定涡轮转子叶片和盘的疲劳寿命。该研究首次得到了涡轮转子叶片和盘的温度和动应力数据。计算结果表明:涡轮转子叶片的寿命不低于2000 h,涡轮盘的寿命不低于5000 h。     

油液冷却航空湿式摩擦离合器热特性分析

为了研究航空高功率密度湿式摩擦离合器在油液冷却作用下的温度特性,基于计算流体动力学（computational fluid dynamics,CFD）方法建立了华夫槽湿式摩擦离合器的热特性分析模型;研究了湿式摩擦离合器中摩擦副上热流密度的计算方法和施加方式;运用热流耦合方法,考虑了油液的散热作用,分析了离合器内各对摩擦副上的油液分布及温度分布。研究结果表明:钢片上和摩擦片上的油液分布不均造成钢片和摩擦片上温度分布不均;不同钢片和摩擦片上的温度分布受片上油液分布及该片热传导性能的影响,呈现出不同的温度分布规律。      

A probabilistic assessment of cycle life of GTE disks made of granular materials

A technique of assessing cycle life and fracture probability for disks made of granular nickel alloys is presented. The technique makes it possible to take into account the probability of detecting inherent metallurgical anomalies available in disks. The calculation results are verified by experimental data.     

多谐波法研究带有叶间干摩擦阻尼失谐叶盘系统的共振特性

提出一种高效的多谐波分析方法,以用于研究失谐对带有叶间干摩擦阻尼的叶盘系统共振特性的影响规律.该方法可准确预测叶盘系统在频域的受迫响应,其有效性用数值积分法进行了验证.利用该方法对带有叶间干摩擦阻尼的叶盘受迫振动响应进行了仿真计算,分析了叶盘系统在谐调和失谐两种情况下受耦合强度、黏性阻尼和干摩擦阻尼等系统参数影响下的共振特性.结果表明,提出的多谐波分析法能够高效地研究失谐对带有叶间干摩擦阻尼的叶盘系统共振响应的影响特征,尤其适合考虑各种系统参数的综合影响.     

同向旋转盘间换热特性的实验研究

本文将实际发动机高、低压涡轮盘简化成几何形状相对简单的中心轴向进气、径向出气、两盘以不同速度同向旋转的旋转盘系统。用实验方法研究了冷气流量、转速以及两盘间隙对旋转盘间换热的影响规律,并对结果进行了相应的分析。     

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。     

粉末涡轮盘力学性能的计算机预测

通过对采用直接热等静压工艺制备的粉末高温合金涡轮盘的性能与淬火冷速的关系分析,建立了盘件淬火计算机模拟分析的基本技术,可用于盘件的淬火冷速分析和组织性能预测.与实际比较,力学性能预测结果达到了很高的精度,为盘件材料的研制提供了强有力的工具.     

韩国高性能C/C刹车盘的开发

介绍了韩国国防开发署与大宇重工合作开发的飞机C/C刹车盘的制造工艺和动力矩试验结果。韩国使用专门设计的预形体通过沥青浸渍和化学气相沉积工艺制备了具有要求的摩擦磨损性能、密度、热性能及机械性能的C/C刹车盘,在无损检测、机械加工、金属夹组装和防氧化处理等工序之后进行鉴定试验。包括动力矩试验和服役寿命试验的全部鉴定试验根据MIL—W—5013规范和洛克希德公司的GD16ZL001B规范在惯性动力仪上进行。全部鉴定试验结果显示新的刹车装置与已鉴定过的现役C/C刹车盘相比具有良好的刹车性能,达到了全部要求。     

Flow between finite and infinite disks with consideration of surface mobility

A problem of modeling the incompressible viscous flow between two disks taking into account the rotation of one of them is considered. We study the effect of the disk angular velocity (flow regimes) in the interdisk spacing, finiteness (infiniteness) of disk radiuses, calculation region configuration as well as distances between disks on the flow characteristics, particularly, on the resistance moment coefficient. Numerical simulation is performed with the aid of Maple and ANSYS Fluent software.     

考虑尺寸效应的轮盘应力疲劳概率寿命分析方法

针对基于应变寿命模型的体方法对中、长寿命轮盘及模拟件寿命预测精度不准的缺陷,提出了考虑尺寸效应基于应力寿命模型的体方法,将最大应力比作为寿命可靠性计算的一个参数.对轮盘模拟试件进行了考虑尺寸效应的疲劳寿命可靠性分析,计算概率寿命与试验中值寿命相差14％,吻合良好.而传统的应变寿命点方法中值寿命预计结果误差达15倍之多.表明考虑尺寸效应的应力寿命体方法可以用来预估中、长寿命轮盘及模拟件的概率寿命.