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.      

利用平滑约束复原方法处理CCD相机遥感图像

重点研究了频域平滑约束复原方法以及该方法对遥感领域中的实际应用，文章先介绍了平滑约束复原方法的理论基础，然后用该方法对CCD相机的遥感图像进行了复原处理，讨论了遥感器系统调制传递函数（MTF）曲线的拟合，遥感器系统MTF矩阵的构造以及复原参数的选择。可以得出结论，在一定条件下，利用平滑约束复原方法可以有效地改善整个系统的调制传递函数，从而使图像变得清晰。     

CCSDS图像无损压缩标准在恒速信道中的应用研究

在CCSDS建议的无损数据压缩的基本原理上 ,结合基于局域纹理特征的处理方法 ,给出数据输入输出在恒速信道条件下一种有效的面向空间应用的遥感图像无损压缩方案。该方案包括去相关处理、熵编码以及压缩缓存控制三部分。去相关操作是在局域纹理分析方法的基础上 ,通过提取两种有效的预测模型并自适应选择最佳的模型进行处理 ;然后采用快速有效的CCSDS熵编码器对最佳去相关模型的预测误差编码。在压缩方案中充分考虑了输入输出恒速信道条件下应用的特殊性 ,设计了相应的压缩码流控制方法 ,从而给出了一套有效的针对恒速输入输出信道条件下的图像无损压缩的应用方案     

厘米-分米波段Ⅲ型爆发的统计分析

统计分析了太阳第23周期间(2000年7月至2004年9月)在625~1500,MHz,2600~3800,MHz和5200~7600,MHz范围频谱仪观测到的Ⅲ型射电爆发. 给出了Ⅲ型爆发的分布、寿命、频率漂移率、偏振度和频率带宽. 结果显示, 频率漂移率和频率带宽的平均值随频率的增加而增大, 寿命和偏振度的平均值既不是常数也不是在宽频延伸上保持均匀不变的.最多的Ⅲ型爆发分布在625~3800,MHz范围内, 且随频率的增加而增多. 分析表明, 电子加速和能量释放地点主要是在分米波范围内, 这个频率范围的特征可能与分米波段上的磁位形有关, 并且与主耀斑地点附近磁重联区中的电子加速有关. 然而, 还有相当数量的Ⅲ型爆发发生在5200~7600,MHz范围内, 这个特征表明电子加速的地点是在一个日冕的宽范围中. 关于厘米relax-relax 分米波段Ⅲ型爆发的辐射机制最可能包含相干的等离子体辐射或电子回旋脉泽辐射过程.     

基于黑盒测试环境的交会对接软件时序分析技术及应用

航天器空间交会对接难度大,GNC软件对任务的完成起到重要作用.由于交会对接控制软件功能复杂,时序要求严格,这对软件测试提出了很高的要求.基于黑盒测试环境,利用FPGA设计方法和时序分析技术,实现了对交会对接软件重要数据运行时序的捕获和对上下行信号相位关系的跟踪,完善了故障触发和上行注入手段.该测试环境在交会对接软件研制过程中起到重要作用.     

Investigating gamma-ray burst data reduction techniques with Swift’s instruments

The amount of data on gamma-ray bursts (GRBs) and the detected afterglows observed by the Swift satellite contributed significantly to the understanding of the phenomenon. The behavior of the early afterglow rises some interesting questions. With the early afterglow localizations of gamma-ray burst positions made by Swift, the clear delimitation of the prompt phase and the afterglow is not so obvious any more. There are hints of a canonical X-ray afterglow lightcurve with segments of different slopes. Not all bursts necessarily show all the segments. It is important to see if the prompt phase and the afterglow has the same origin or they stem from different parts of the progenitor system. We will combine the of gamma-ray burst data from BAT and XRT and compare the extrapolated gamma-ray flux to the X-ray in a sample of bursts and find that there is a good agreement between the two measurements. This indicates that the physical process shaping burst and the early afterglow are the same.     

Non-stationarity and cross-correlation effects in the MHD solar activity

The analysis of turbulent processes in sunspots and pores which are self-organizing long-lived magnetic structures is a complicated and not yet solved problem. The present work focuses on studying such magneto-hydrodynamic (MHD) formations on the basis of flicker-noise spectroscopy using a new method of multi-parametric analysis. The non-stationarity and cross-correlation effects taking place in solar activity dynamics are considered. The calculated maximum values of non-stationarity factor may become precursors of significant restructuring in solar magnetic activity. The introduced cross-correlation functions enable us to judge synchronization effects between the signals of various solar activity indicators registered simultaneously.     

Accurate approximation of in-ecliptic trajectories for E-sail with constant pitch angle

Propellantless continuous-thrust propulsion systems, such as electric solar wind sails, may be successfully used for new space missions, especially those requiring high-energy orbit transfers. When the mass-to-thrust ratio is sufficiently large, the spacecraft trajectory is characterized by long flight times with a number of revolutions around the Sun. The corresponding mission analysis, especially when addressed within an optimal context, requires a significant amount of simulation effort. Analytical trajectories are therefore useful aids in a preliminary phase of mission design, even though exact solution are very difficult to obtain. The aim of this paper is to present an accurate, analytical, approximation of the spacecraft trajectory generated by an electric solar wind sail with a constant pitch angle, using the latest mathematical model of the thrust vector. Assuming a heliocentric circular parking orbit and a two-dimensional scenario, the simulation results show that the proposed equations are able to accurately describe the actual spacecraft trajectory for a long time interval when the propulsive acceleration magnitude is sufficiently small.