复合材料旋翼桨叶剖面扭转刚度计算

本文对Krahula,J.L.等人提出的“圣维南扭转的有限元解”作了合理的改进,使改进后的公式能很方便地编成计算程序,作复合材料旋翼桨叶的扭转刚度计算。还应用改进后的公式计算了两种型号直升机旅翼桨叶的扭转刚度,计算值和试验值有很好的一致性。     

砂垫层刚度对地面地震反应的影响研究

我国是一个多地震国家，地震区分布范围广，发震频繁。因此减震、隔震技术对国民经济基本建设具有重要意义。随着科学技术的进步、计算机的运用等，减震、隔震方法的研究与应用取得了很大的发展，但仍有许多问题有待解决，特别是就我国目前中、低层房屋较多的实际状况而言，这一问题显得尤为突出。采用在基础与地基之间设置砂垫层的方法，减小或不放大地震对地面的影响，最终达到减震、隔震的目的。在提出砂垫层隔震概念及其与《建筑抗震设计规范》(GB50011—2001)的区别之后，研究了砂垫层刚度对地面地震反应的影响，得到了一些有益的结果。     

平显成像抖动问题分析与解决方法

简述了某型直升机选装的平显系统的组成和功能．针对在实际应用中遇到的平显在飞行中成像抖动现象进行了分析和总结，并给出了解决问题的方法。     

套筒式张线天平的研制

根据民机张线测力试验的特殊要求,研制了一台套筒结构形式的张线天平。详细介绍了该天平在研制中遇到的难点、关键技术的解决措施以及研制的结果。天平元件布置在58mm的外套筒上,内杆直径为44mm,外套筒和内杆通过楔块焊接在一起。法向力、俯仰力矩和滚转力矩为拉压变形,横向力和偏航力矩为＂S＂形变形,轴向力为弯曲变形,元件支撑部分受拉压变形且刚度较强。通过对天平进行有限元分析,在法向力和俯仰力矩作用下,得出的应变结果与实际输出基本吻合。风洞试验结果表明：天平设计合理,天平外套筒、内杆及张线支撑系统刚度好,天平各分量测量精度高。     

Effect of “Noisy” sun conditions on aircrew radiation exposure

In computer codes used to estimate the aircrew radiation exposure from galactic cosmic radiation, a quiet sun model is usually assumed. A revised computer code (PCAIRE ver. 8.0f) is used to calculate the impact of noisy sun conditions on aircrew radiation exposure. The revised code incorporates the effect of solar storm activity, which can perturb the geomagnetic field lines, altering cutoff rigidities and hence the shielding capability of the Earth’s magnetic field. The effect of typical solar storm conditions on aircrew radiation exposure is shown to be minimal justifying the usual assumptions.     

Variations of geomagnetic cutoff rigidity in the southern hemisphere close to 70°W (South-Atlantic Anomaly and Antarctic zones) in the period 1975–2010

We report the existence of rapid variations in (effective) geomagnetic cutoff rigidity (Rc) between the equatorial and Antarctic zones adjacent to the Andes Mountains, revealed by the variation rate of geomagnetic cutoff rigidity (VRc) in the period 1975–2010. Our analysis is based on empirical records and theoretical models of the variations in cosmic rays and on the structure of geomagnetic fields. These have given us a different view of variations in Rc in time and space along the 70°W meridian, where secular variations in the geomagnetic field are strongly influenced by the proximity of the South Atlantic Magnetic Anomaly (SAMA), one of the most important characteristics of the terrestrial magnetic field that affects our planet, close from the equator to the 50°S parallel and from South America to South Africa. The VRc presents rapid changes in mid-latitudes where SAMA exerts its influence despite the existence of smooth changes in the geomagnetic field. This shows that these changes occur mainly in the spatial configuration, rather than in the temporal evolution of Rc. The analysis was performed using measurements from the Chilean Network of Cosmic Rays and Geomagnetism Observatories, equipped with BF-3 and latest generation He-3 neutron monitors, Fluxgate magnetometers, geomagnetic reference field (IGRF) and Tsyganenko 2001 model (just for completeness).     

Shape control of spacecraft formation using a virtual spring-damper mesh

This paper derives a distance-based formation control method to maintain the desired formation shape for spacecraft in a gravitational potential field. The method is an analogy of a vir-tual spring-damper mesh. Spacecraft are connected virtually by spring-damper pairs. Convergence analysis is performed using the energy method. Approximate expressions for the distance errors and control accelerations at steady state are derived by using algebraic graph representations and results of graph rigidity. Analytical results indicate that if the underlying graph of the mesh is rigid, the convergence to a static shape is assured, and higher formation control precision can be achieved by increasing the elastic coefficient without increasing the control accelerations. A numerical exam-ple of spacecraft formation in low Earth orbit confirms the theoretical analysis and shows that the desired formation shape can be well achieved using the presented method, whereas the orientation of the formation can be kept pointing to the center of the Earth by the gravity gradient. The method is decentralized, and uses only relative measurement information. Constructing a distributed virtual structure in space can be the general application area. The proposed method can serve as an active shape control law for the spacecraft formations using propellantless internal forces.     

机动飞行飞行器内具有初始弯曲和刚度不对称的转子运动模型

本文建立了位于机动飞行飞行器内且同时具有初始弯曲、不对称刚度和质量不平衡的单盘Jeffcott转子的动力学模型。当飞行器静止时,设相关参数为零后该模型与相应地面转子系统的数学模型完全相同。应用该模型可数值仿真研究飞行器运动时位于飞行器内的等转速、等加速、等减速运行转子的动态特性,研究飞行器不同飞行速度和加速度对转子动力学特性的影响,分析飞行器飞行时转子出现故障时的响应特性,从而为机动飞行器内转子的动力学分析和故障诊断提供依据。     

具有接触接合面的篦齿封严组件振动特性分析

运用弹性力学理论研究了篦齿封严组件及其减振结构之间过盈装配压力和接触刚度的求解方法,在此基础上给出了具有接触接合面的封严环/阻尼片组合结构动力特性的分析方法,并且研究了阻尼片厚度、阻尼片周向分布数量、装配过盈量等参数对结构动力特性的影响规律.转动情况下封严环离心应力与阻尼片厚度近似成线性关系;阻尼片的周向分布数量影响封严环的固有频率和振型;阻尼片沿周向分布数量越多,应力分布越均匀,封严环的离心应力越小.