SMP2仿真引擎的多核并行化

仿真模型可移植性规范2（SMP2）是由欧洲航天局制定并得到广泛应用的仿真模型开发与集     

视觉导引的无人直升机自主着舰系统仿真

对于无人直升机着舰问题,提出了基于视觉导引的自主着舰方案;建立了一套无人直升机自主着舰仿真系统;建立了舰船运动模型,无人直升机六自由度非线性全量模型;设计了着舰特征图案,通过摄像机模型获取舰船上的特征图案;提出快速四点算法实现3D位姿估算,并以此构建视觉信息识别系统,识别直升机与舰船相对运动参数;通过分层控制思想,实现基于视觉信息导引着舰。在此基础上形成仿真闭环,对无人直升机定点自主着舰的全过程进行仿真验证。     

空间飞行器的对接分离与地面模拟试验的仿真分析研究

对两对接飞行器的分离过程和地面模拟试验过程进行了理论分析,论述了两飞行器在分离瞬 间空间分离过程与地面模拟试验过程之间的对应比拟关系;依据地面试验中给出的多种工况 ,利用多体动力学软件ADAMS仿真分析并比对了地面和空间零重力两种环境条件下两飞行器 分离时的运动特性,讨论了地面五自由度对接分离气浮平台模拟两飞行器在空间实际分离时 带来的原理误差影响。     

基于数字化仿真技术的模块化装配单元应用

传统航空机电产品尤其是液压产品的装配工艺复杂,总装工艺流程长,生产过程控制困难,装配质量难以保证。利用数字化仿真技术实现模块化部件装配单元规划,有利于提升装配专业化水平,缩短总装周期,实现产品的快速产出。     

无人机仿真测试系统设计应用研究

仿真测试系统可以对无人机控制规律进行有效的检测和评估,在无人机研制中起到重要作用。通过研究无人机仿真测试系统工作原理,建立了无人机动力学和运动学数学模型,采用四阶龙格-库塔法进行解算,得到了无人机位置、高度和姿态等信息,对无人机飞行控制的稳定性进行有效验证和评估,并成功运用于某型无人机的研制中。     

某型无人机运动学建模与分析CSCD

采用运动学建模方式对无人机进行总体设计,并通过数字风洞仿真实验对其进行验证,结果表明设计指标正确、合理。     

进口圆度仪智能化改造

以Talyrond73型圆度仪为例，介绍了圆度仪智能化改造的基本原理，圆度测量软件的主要功能以及回度误差评定方法的优化，探讨了保证检测精度的若干措施，并给出了检定结果。     

Temporal and spatial stochastic behaviour of high-frequency slant tropospheric delays from simulations and real GPS data

In this paper, a turbulence theory-based simulation procedure for slant tropospheric delay variations is presented. Based on this procedure tropospheric delay variations are simulated for three different geometric scenarios. The stochastic behaviour of the generated time series is assessed in terms of temporal structure functions. It is shown that the temporal structure functions – in general – follow a 5/3 to 2/3 power-law behaviour. Deviations from this behaviour due to the complex interaction between varying observation geometry and atmospheric/turbulent conditions are discussed.     

A simulation analysis of systematic errors in ion arrival angle and drift velocity from the satellite borne ion drift meter

As one payload of a Chinese seismic satellite program, an ion drift meter (IDM) will measure drift velocity of thermal ions at an altitude of 500 km. Previous works have shown that such instruments use biased grids to create nonuniform potential in the grid planes, which brings systematic errors to the inferred parameters. A commercial finite element analysis software is used to simulate this instrument in the exact size. The error sources from thermal velocity, nonuniform transparency of real grids and potential depression in the grid planes are explained. The simulation results show that the arrival angle and drift velocity will be underestimated in all the conditions and the maximal error will be about −0.87° and −121 m/s, respectively. Furthermore, the relative error of the inferred arrival angle and the drift velocity will be inversely correlated with the arrival angle because of the lensing effect of the potential depression. This simulation provides a quantificational method of evaluating and correcting the data during in situ operation.     

Real-time global MHD simulation of the solar wind interaction with the earth’s magnetosphere

We have developed a real-time global MHD (magnetohydrodynamics) simulation of the solar wind interaction with the earth’s magnetosphere. By adopting the real-time solar wind parameters and interplanetary magnetic field (IMF) observed routinely by the ACE (Advanced Composition Explorer) spacecraft, responses of the magnetosphere are calculated with MHD code. The simulation is carried out routinely on the super computer system at National Institute of Information and Communications Technology (NICT), Japan. The visualized images of the magnetic field lines around the earth, pressure distribution on the meridian plane, and the conductivity of the polar ionosphere, can be referred to on the web site (http://www2.nict.go.jp/y/y223/simulation/realtime/).The results show that various magnetospheric activities are almost reproduced qualitatively. They also give us information how geomagnetic disturbances develop in the magnetosphere in relation with the ionosphere. From the viewpoint of space weather, the real-time simulation helps us to understand the whole image in the current condition of the magnetosphere. To evaluate the simulation results, we compare the AE indices derived from the simulation and observations. The simulation and observation agree well for quiet days and isolated substorm cases in general.