曲柄连杆机构可靠性及其关联失效控制

为了提高机械系统的整机可靠性,对机械系统的机构动作故障及其关联失效实现有效控制,在该领域对动作可靠性惟象研究基础上.在机构动作可靠性机理、失效模式、故障危害及其失效控制方面作了初步探讨;通过失效机理研究,借助集合理论,从广义变形研究出发,由Gershgorin圆盘定理及通过变形设计和组合加工对引起特征值病态的像集合中的非线性改造为线性后,提出的包容模型,实施以装配状态和实际使用状态为目标的变形控制方法,对曲柄连杆机构的实际应用表明:能够有效控制其可靠性及其关联失效.     

SiC/SiC复合材料氧化退化研究进展

针对高速推进系统温度测量传感器的设计方法、测量误差等核心问题,综述了现阶段高速推进系统接触式和非接触式温度测量的方法。其中,重点综述了辐射与红外测量、可调谐二极管激光吸收光谱(TDLAS)、相干反斯托克斯拉曼散射(CARS)及温度敏感涂料(TSP)等非接触温度测量技术在高速推进系统应用的研究进展和发展趋势,并分析了上述温度测量技术存在的问题。     

Testing the blast wave model with Swift GRBs

The complex structure of the light curves of Swift GRBs (e.g. superimposed flares and shallow decay) has made their interpretation and that of the blast wave caused by the burst, more difficult than in the pre-Swift era. We aim to constrain the blast wave parameters: electron energy distribution, p, density profile of the circumburst medium, k, and the continued energy injection index, q. We do so by comparing the observed multi-wavelength light curves and X-ray spectra of a Swift sample to the predictions of the blast wave model.     

An experimental investigation on static directional stability

A generic aircraft usually loses its static directional stability at moderate angle of attack (typically 20–30?). In this research, wind tunnel studies were performed using an aircraft model with moderate swept wing and a conventional vertical tail. The purpose of this study was to investigate flow mechanisms responsible for static directional stability. Measurements of force, surface pressure and spatial flow field were carried out for angles of attack from 0? to 46? and sideslip angles from ?8? to 8?. Results of the wind tunnel experiments show that the vertical tail is the main contributor to static directional stability, while the fuselage is the main contributor to static directional instabil-ity of the model. In the sideslip attitude for moderate angles of attack, the fuselage vortex and the wing vortex merged together and changed asymmetrically as angle of attack increased on the wind-ward side and leeward side of the vertical tail. The separated asymmetrical vortex flow around the vertical tail is the main reason for reduction in the static directional stability. Compared with the wing vortices, the fuselage vortices are more concentrated and closer to the vertical tail, so the yaw-ing moment of vertical tail is more unstable than that when the wings are absent. On the other hand, the attached asymmetrical flow over the fuselage in sideslip leads to the static directional instability of the fuselage being exacerbated. It is mainly due to the predominant model contour blockage effect on the windward side flow over the model in sideslip, which is strongly affected by angle of attack.     

对复杂平面连杆机构运动分析的研究

本文提出了用转化机构法进行单自由度复杂平面连杆机构的运动分析.基本思想是通过改变机构的原动件或机架或同时改变原动件和机架,以简化机构的运动分析.这种方法对常见的平面复杂连杆机构的运动分析非常有效,无需进行复杂的试凑或迭代.同时本文提出的这种解法有较为广泛的意义,对加深认识机构的组成以及对机构其它问题的研究都是+分重要的.     

Changes in radio emission from PSR J0737–3039B

The double pulsar system, J0737–3039, provides a unique probe of a pulsar magnetosphere due to its edge-on viewing geometry, a tight orbit and a significant rate of advance of the angle of periastron. In this paper, we report on the changes in radio emission from the long period pulsar in this system, J0737–3039B, over a period of 9 months. Observations of this system with Giant Metrewave Radio Telescope (GMRT) show that the duration of the first bright phase of the pulsar centered at 210° orbital longitude from the ascending node is shrinking. These observations will be useful to constrain the proposed models for this system.     

K4169高温合金组织细化研究

研究了 K4 1 6 9高温合金在不同浇注温度及向熔体中加入细化剂时的晶粒组织。结果表明 ,降低浇注温度可以明显细化凝固后基体的晶粒和提高铸件断面等轴晶的比例。在通常的浇注温度 1 4 0 0℃和 1 4 2 0℃下 ,并对合金熔体进行均匀化处理时 ,加入所研制的复合细化剂可使圆柱锭的晶粒分别细化至 ASTM1 .7级和 ASTMM1 0 .5级 ;断面等轴晶的比例分别达 96 %和 90 %以上。本文提出了晶粒细化的机理并分析了晶粒细化后断面等轴晶比例增大的现象     

Time variations of the total electron content in the Southeast Asian equatorial ionization anomaly for the period 2006–2011

This study presents the time variations of the total electron content in the South East Asian equatorial ionization anomaly. The time variation of the TEC is analyzed through the period 2006–2011 by using a latitudinal chain of GPS stations extending in the northern and southern hemisphere. The data shows that the shape of the diurnal variation of the TEC depends on the latitude: a plateau is observed at the stations near the equator and a Gaussian at the station distant from the equator. We observe a semiannual pattern in all the stations with maxima at equinox. In both hemispheres, the amplitude of the crest is larger in spring than autumn from 2006 to 2008 and smaller in spring than in autumn from 2009 to 2011. We also observe an asymmetry between the amplitude and the position of the two crests of ionization. There is a very high level of correlation between the amplitude of the TEC at the two crests and the sunspot number: ∼0.88. During the deep solar minimum 2008–2009, the amplitude of crests of ionization becomes small during several months in summer and winter. The results show that both crests move significantly equatorward in winter than other seasons and there is a tendency for both crests to appear earlier in winter and later in summer.     

Thermal Radiation Processes

We discuss the different physical processes that are important to understand the thermal X-ray emission and absorption spectra of the diffuse gas in clusters of galaxies and the warm-hot intergalactic medium. The ionisation balance, line and continuum emission and absorption properties are reviewed and several practical examples are given that illustrate the most important diagnostic features in the X-ray spectra.