振动切削——薄壁零件加工的新技术

采用三维振动试验台,对不锈钢制做的薄壁测试模型进行了加工试验,实验结果表明,振动切削方法能够加工达到薄壁测试模型各项技术要求的零件,是薄壁零件加工的新技术。     

基于DCOM技术构建分布式数控故障诊断系统

简要介绍DCOM技术的特点,对利用DCOM技术构建分布式数控故障诊断系统进行了研究,并提出了系统的组件模型结构。     

各向异性单晶叶片强度寿命研究—第I部分:晶体滑移本构模型及应用

单晶叶片技术是提高航空发动机及地面燃气轮机性能、寿命及可靠性的关键技术之一，但单晶材料机械、力学性能的各向异性特性制约了其发展和应用，对其工程应用及应用的理论基础提出了挑战。课题组开展了各向异性单晶叶片强度分析和寿命预测方面的一些研究工作。包括：建立并验证了弹塑性、蠕变滑移本构模型及蠕变持久寿命预测方法；进行了不同晶体取向DD3单晶在不同温度、不同速率或不同温度、不同应力水平下的拉伸试验及蠕变试验，这些实验数据及由其反映的单晶中、高温各向异性特性对单晶材料的应用具有重要意义。此外还进行了某种单晶叶片的实验研究。作为上述研究的应用，对某发动机单晶涡轮叶片进行了强度分析和寿命预测。本文这一部分介绍本构模型及应用，实验研究将在第II部分介绍。     

扩展的基于角色的访问控制模型

提出了一种扩展的基于角色的访问控制RBAC(Role Based Access Control)模型--RTBAC (Role & Task Based Access Control)模型.该模型在RBAC96模型之上引入了任务和任务实例的概念,形式化地定义了任务和任务实例的层次结构,界定了传统会话同任务实例之间的关系以及任务实例同权限之间的关系,并且提供了几种辅助函数.该模型可以更为自然地描述业务流程和访问控制策略,更适合分布式协作应用,特别是工作流和组合服务.基于该模型定义了一种新的动态职责分离约束--基于任务的动态职责分离约束,并且同传统动态职责分离约束进行了比较.该约束可以更准确地刻画访问控制相关的系统运行时上下文的范围,从而提高运行时访问控制的效率.     

星载GPS观测数据的模拟研究

重点分析了星载GPS观测值模拟的原理、数学模型等,并用模拟软件模拟了CHAMP卫星的星载GPS观测值情况.结果表明,根据本文提供模拟方法所模拟的CHAMP星载GPS观测值,与实测值相比,无论是在大小还是观测噪声水平上都很接近,因此能满足不同层次人员对星载GPS模拟观测值的需要.     

基于航天器解体事件的空间碎片寿命算法

研究了针对航天器解体事件所生成的空间碎片的寿命计算方法.给出了基于NASA标准航天器解体模型的航天器解体算法.该算法生成的一系列碎片参数,将作为寿命计算的初始条件.总结了现有求解碎片寿命的算法,并提出了一种半分析算法.该算法运用平均根数法的思路,计算了在J2摄动项的影响下,碎片的半长轴和偏心率的变化率;并采用微分积分法预报半长轴和偏心率随时间的变化.为了适应时变大气模型,该算法限制了计算步长.通过与数值法的比较分析了算法的计算速度和精度.选用了3种大气模型:SA76、GOST和MSIS-00,分析了不同大气模型在计算碎片寿命之间的差异.通过与P-78卫星解体事件的实测数据对比验证了整个算法的正确性.      

视觉跟踪坐标测量系统数学建模

提出了一种基于光学测头成像的单相机视觉跟踪坐标测量系统。该系统中引入了一个转动平台带动相机运动,使相机光轴始终对准运动的光学测头中某一个光点,保证光学测头成像在畸变比较小的像面中心附近。给出了系统的组成结构,通过空间变换和光学成像原理建立了系统的非线性跟踪测量数学模型,给出了利用Newton非线性迭代算法求解跟踪方程的具体算法,通过实验验证了所建立的模型和求解方法的正确性。最后,分析了转动角度误差对测量结果的影响。     

An empirical solar radiation pressure model for satellites moving in the orbit-normal mode

We present a family of empirical solar radiation pressure (SRP) models suited for satellites orbiting the Earth in the orbit normal (ON) mode. The proposed ECOM-TB model describes the SRP accelerations in the so-called terminator coordinate system. The choice of the coordinate system and the SRP parametrization is based on theoretical assumptions and on simulation results with a QZS-1-like box-wing model, where the SRP accelerations acting on the solar panels and on the box are assessed separately. The new SRP model takes into account that in ON-mode the incident angle of the solar radiation on the solar panels is not constant like in the yaw-steering (YS) attitude mode. It depends on the elevation angle of the Sun above the satellite’s orbital plane. The resulting SRP vector acts, therefore, not only in the Sun-satellite direction, but has also a component normal to it. Both components are changing as a function of the incident angle. ECOM-TB has been used for precise orbit determination (POD) for QZS-1 and BeiDou2 (BDS2) satellites in medium (MEO) and inclined geosynchronous Earth orbits (IGSO) based on IGS MGEX data from 2014 and 2015. The resulting orbits have been validated with SLR, long-arc orbit fits, orbit misclosures, and by the satellite clock corrections based on the orbits. The validation results confirm that—compared to ECOM2—ECOM-TB significantly (factor 3–4) improves the POD of QZS-1 in ON-mode for orbits with different arc lengths (one, three, and five days). Moderate orbit improvements are achieved for BDS2 MEO satellites—especially if ECOM-TB is supported by pseudo-stochastic pulses (the model is then called ECOM-TBP). For BDS2 IGSOs, ECOM-TB with its 9 SRP parameters appears to be over-parameterized. For use with BDS2 IGSO spacecraft we therefore developed a minimized model version called ECOM-TBMP, which is based on the same axis decomposition as ECOM-TB, but has only 2 SRP parameters and is supported by pseudo-stochastic parameters, as well. This model shows a similar performance as ECOM-TB with short arcs, but an improved performance with (3-day) long-arcs. The new SRP models have been activated in CODE’s IGS MGEX solution in Summer 2018. Like the other ECOM models the ECOM-TB derivatives might be used together with an a priori model.     

Numerical study of traveling ionosphere disturbances with vertical incidence data

High frequency ionosphere vertical sounding, as an important and representative application for detecting the ionosphere and studying the characteristics of radio propagation, can be utilized to monitor the ionosphere continuously variation and to acquire the ionosphere asymmetrical features of diverse scale above the ionosphere vertical sounding stations. This is a first article on real time application of numerical methods to obtain the parameters of traveling ionosphere disturbances (TIDs) using vertical incident ionograms. In this paper, the distribution of ionosphere electron density with TIDs is constructed using a background ionosphere model superimposed a perturbation theory model. The background ionosphere electron density is modelled by the inversion of vertical incident ionograms which are observed before the appearance of the disturbance. Based on the fourth order Adams-Bashforth-Moulton (the so-called ABM) predictor corrector method, instead of Runge-Kutta method, the fast digital ray tracing method is established. According to process of the disturbed trace simulation and parameters inversion, the characteristic parameters of ionosphere disturbance at different detection time can be obtained in real time. The numerical analysis of TIDs is then captured completely.