DFT&ET综合分析法

根据故障树(FT)和事件树(ET)之间的相互关系,动态系统的复杂性以及不同子系统之间所存在的矛盾,结合马尔可夫链的运用,提出了将动态故障树(DFT)和ET相结合的一个合理的方法,并通过实例给出证明.该方法解决了所建模型中的矛盾,且通过模块化处理提高了效率.     

整机瞬态动力特性计算及稳定性分析

采用子结构传递矩阵—模态综合法研究了航空发动机整机的瞬态动力特性及稳定性。分析了各种因素（突加不平衡大小及位置、转速、油膜间隙等）对瞬态响应和稳定性的影响规律，得到一些有价值的结论。     

材料热物理性能非稳态测量方法综述

非稳态法具有快速、准确的特点,一次测量可同时得到热导率、热扩散率和热容等多个热物性参数,测试范围可覆盖多种材料和较宽的热参数区间。阐述了目前国际上主要的六种非稳态测量方法及特点、测量原理及理论模型公式。     

Hard X-ray emission from the recurrent transient A0535+26 during its 1980 high-intensity outburst

The transient X-ray pulsar A0535+26 was observed on October 4, 1980 during a high level intensity outburst with a balloon borne hard X-ray detector. High statistical quality source spectra were determined up to 100 keV. Both blackbody and Wien laws fit well the data. Pulse phase spectroscopy shows variation of temperature index between 7.5 and 8.5 keV in the off source spectra and between 7.4 and 10.5 keV in the off pulse spectra. The time averaged luminosity above 30 keV is 8×10³⁶ erg/s.     

Invariant and energy analysis of an axially retracting beam

The mechanism of a retracting cantilevered beam has been investigated by the invariant and energy-based analysis. The time-varying parameter partial differential equation governing the transverse vibrations of a beam with retracting motion is derived based on the momentum theorem. The assumed-mode method is used to truncate the governing partial differential equation into a set of ordinary differential equations (ODEs) with time-dependent coefficients. It is found that if the order of truncation is not less than the order of the initial conditions, the assumed-mode method can yield accurate results. The energy transfers among assumed modes are discussed during retrac-tion. The total energy varying with time has been investigated by numerical and analytical methods, and the results have good agreement with each other. For the transverse vibrations of the axially retracting beam, the adiabatic invariant is derived by both the averaging method and the Bessel function method.     

航天用系列行波型超声波电机的研制

简述了超声波电机在航天领域的应用情况，并介绍了所研制的系列行波型超声波电机（直径分别为80mm、60mm、45mm和30mm）的结构形式、摩擦材料、粘结工艺、温度特性、机械特性和瞬态特性，提出了神经元自适应PID算法实现高精度的速度和位置控制。结果表明其具有良好的特性，适用于空间机器人、登月车、太阳能帆板、CCD等空间机构的驱动，并结合航天领域的应用要求，提出了下一步的研究重点。     

非线性约束的大型旋转火箭瞬态响应模拟

以大长径比、旋转无控火箭为研究对象，探讨弹-架非线性约束系统的发射动力学响应。将火箭模拟为支承、变刚度柔性转子，发射装置则简化具有弹性约束的Euler-Bernoulli，二者通过非线性弹性元件相耦联。数值模拟发射过程中的火箭瞬态响应，分析了系统特性对火箭姿态的影响。     

带环向槽环路热管主芯中流动和传热的数学模型和数值模拟

蒸发器是环路热管中最重要的部件,蒸发器主芯中的流场是设计中关注的焦点。建立了一个轴对称二维数学模型来模拟流体工质在圆柱形蒸发器主芯中的流动、传热和蒸发现象。模型充分考虑了流场和蒸发界面间相互作用对于蒸发界面的位置和孔隙中弯曲液面曲率半径的影响。模拟了瞬态和稳态流场,并研究了热负荷的影响。模拟结果在一定工况下是合理的。     

瞬态平面热源法热物理性能测量准确度和适用范围的标定——常温下标准Pyroceram 9606材料热物理性能测量

瞬态平面热源法作为一种非稳态热物理性能测试技术,其测量范围、测量准确度和试验参数的确定是正确评价和应用这种测试技术的前提条件。详细介绍了瞬态平面热源法的测量原理以及常温下的测量装置,描述了采用Pyroceram 9606热物理性能标准材料研究瞬态平面热源法在实际测试中各种试验参数对测量准确度的影响,并由此考察这种测试方法和测试装置的测量准确度。     

Dynamical characterization of the last prolonged solar minima

The planetary hypothesis of the solar cycle is an old idea in which the gravitational influence of the planets has a non-negligible effect on the causes of the solar magnetic cycle. The advance of this hypothesis is based on phenomenological correlations between dynamical parameters of the Sun’s movement around the barycentre of the Solar System and sunspots time series; and more especially, identifying relationships linking solar barycentric dynamics with prolonged minima (especially Grand Minima events). However, at present there is no clear physical mechanism relating these phenomena. The possible celestial influence on solar cycle modulation is of great importance not only in solar physics but also in Earth sciences, because prolonged solar minima have associated important climatic and telluric variations, in particular, during the Maunder and Dalton Minimum. In this work we looked for a possible causal link in relation with solar barycentric dynamics and prolonged minima events. We searched for particular changes in the Sun’s acceleration and concentrated on long-term variations of the solar cycle. We show how the orbital angular momentum of the Sun evolves and how the inclination of the solar barycentric orbit varies during the epochs of orbital retrogressions. In particular, at these moments, the radial component of the Sun’s acceleration (i.e., in the barycentre-Sun direction) had an exceptional magnitude. These radial impulses occurred at the very beginning of the Maunder Minimum, during the Dalton Minimum and also at the maximum of cycle 22 before the present extended minimum. We also found a strong correlation between the planetary torque and the observed sunspots international number around that maximum. We apply our results in a novel theory of Sun–planets interaction that it is sensitive to Sun barycentric dynamics and found a very important effect on the Sun’s capability of storing hypothetical reservoirs of potential energy that could be released by internal flows and might be related to the solar cycle. This process begins about 40 years before the solar angular momentum inversions, i.e., before Maunder Minimum, Dalton Minimum, and before the present extended minimum. Our conclusions suggest a dynamical characterization of peculiar prolonged solar minima. We discuss the possible implications of these results for the solar cycle including the present extended minimum.