O形圈密封载荷衰减研究

对两种硅橡胶材料O形圈的载荷衰减规律进行了试验研究,结果发现,O形圈的载荷衰减规律与O形圈材料的性能有关;温度对O形圈的衰减规律也有很大影响,温度越高,O形圈的载荷衰减速度越快.在试验的基础上对O形圈载荷衰减的理论模型进行了研究,采用无穷多个Maxwell模型并联的方式,找到了一个能较好地表示O形圈载荷衰减规律的模型.      

改进FDTD／集总源模型分析航天器场线耦合

针对典型的电磁脉冲对航天器电缆耦合问题,建立了航天器场线耦合分析模型。在场分布计算方面,采用基于平均电参数和分析目标与 Yee网格不重合的边缘部分修正的改进时域有限差分法。在场线耦合方面,建立基于集总等效源模型的多导体传输线瞬态响应模型,将外场在传输线上激励的分布电压源和电流源与传输线指数矩阵解耦,建立了集总等效电压源和电流源模型。采用分析模型分析运载内一根电缆受电磁脉冲影响的响应,结果表明,即使存在屏蔽作用,电磁脉冲在电缆上耦合的干扰足以损毁设备。     

仪器设备间距对空间实验室机柜内部流动和传热的影响分析

为充分利用机柜内有限空间并改善仪器设备的散热环境,建立了空间实验室机柜的模型,运用数值计算方法,对不同仪器设备间距下机柜内流场和温度场进行求解,研究了不同布局仪器层平均风速和仪器表面平均对流换热系数的变化规律。结果表明,合理地选择仪器设备间距可以有效地改善其表面的散热状况,为空间实验室机柜的热设计提供了依据。     

电子设备热分析软件应用研究

应用热分析技术,能在产品的设计阶段获得其温度分布,从而优化设计,提高产品可靠性.介绍了现在流行的电子设备热分析软件,阐述了电子设备热分析软件在应用中面临的一些问题,并结合一简单实例,展示了电子设备热分析的全过程,对热分析软件应用中的部分难题提出了解决方案.结果表明:妥善处理好主要问题,则能够达到较高的热分析精度,满足工程需求.      

数字地球中实时地形晕渲的实现方法

通过使用法线贴图的模式,不增加地面网格数的前提下,在三维数字地球仿真系统中实现了对全球地形的高精度实时晕眩效果的地形浏览.首先通过对高程数据进行分层分块处理,制作级地块法线贴图,再通过绘图芯片用可程序化像素着色器流程计算法线贴图的光照效果,最后将纹理贴到对应的分层三维地形网格上.根据光源的入射方向、色调、饱和度及亮度,计算中考虑了顶点的环境光、漫反射光、镜面反射光,在低地形网格数的前提下,实现了如高精度地形网格般的明显光影变化.      

A regional tropospheric model for airborne GPS applications

A regional tropospheric model can be constructed using surveys from GPS ground networks. Using this model the tropospheric delays of a kinematic station within the region can be interpolated. However, such a model is generally not suitable for an airborne platform high above the ground networks. In this paper, a method of constructing a regional tropospheric model for airborne GPS applications is described. First, the kinematic station in the air is projected onto the ground. Then the tropospheric delays at projected point are interpolated from those of the ground networks. Finally, the tropospheric delays at projected point are extended upward to the airborne platform using pressure and temperature gradients and humidity exponential function. For validation of this method, the data of airborne campaign carried out by BKG in cooperation with GFZ and BGR 2008 in the northern Alps are used. The results show that GPS kinematic positioning precision in height component can be improved using this method.     

Geometric calibration of Colour and Stereo Surface Imaging System of ESA’s Trace Gas Orbiter

There are many geometric calibration methods for “standard” cameras. These methods, however, cannot be used for the calibration of telescopes with large focal lengths and complex off-axis optics. Moreover, specialized calibration methods for the telescopes are scarce in literature. We describe the calibration method that we developed for the Colour and Stereo Surface Imaging System (CaSSIS) telescope, on board of the ExoMars Trace Gas Orbiter (TGO). Although our method is described in the context of CaSSIS, with camera-specific experiments, it is general and can be applied to other telescopes. We further encourage re-use of the proposed method by making our calibration code and data available on-line.     

Orbital stability close to asteroid 624 Hektor using the polyhedral model

We investigate the orbital stability close to the unique L4-point Jupiter binary Trojan asteroid 624 Hektor. The gravitational potential of 624 Hektor is calculated using the polyhedron model with observational data of 2038 faces and 1021 vertexes. Previous studies have presented three different density values for 624 Hektor. The equilibrium points in the gravitational potential of 624 Hektor with different density values have been studied in detail. There are five equilibrium points in the gravitational potential of 624 Hektor no matter the density value. The positions, Jacobian, eigenvalues, topological cases, stability, as well as the Hessian matrix of the equilibrium points are investigated. For the three different density values the number, topological cases, and the stability of the equilibrium points with different density values are the same. However, the positions of the equilibrium points vary with the density value of the asteroid 624 Hektor. The outer equilibrium points move away from the asteroid’s mass center when the density increases, and the inner equilibrium point moves close to the asteroid’s mass center when the density increases. There exist unstable periodic orbits near the surface of 624 Hektor. We calculated an orbit near the primary’s equatorial plane of this binary Trojan asteroid; the results indicate that the orbit remains stable after 28.8375?d.