模型修正中一种特殊广义逆的性质与功能

本文对一种特殊的广义逆矩阵在模型修正中使用时可能具有的性质与功能给予了间接的论证,从而为这种广义逆的进一步应用给予了提示。该论证表明,这种广义逆不仅具有增补方程个数的作用,而且还具有对修正模型的参考基增补高阶理论模态信息的功能。通过本文论证,文[2][4]之解的唯一性问题明确解决了,即为一个实用完备模态空间中的确定解。     

再入体激波层和近尾流热辐射实验研究

本文介绍了在弹道靶设备上对再入速度下模型的热辐射进行的实验研究工作。铝、高硅氧和聚碳酸酯三种材料的模型在速度为4.5～6.0(km/s),压力为600—8000Pa条件下做了实验,在258nm—1100nm光谱范围内完成了九个波段的辐射测量,给出了三种材料模型的辐射光谱分布曲线。结果表明辐射量除了受环境条件影响外,还强烈地依赖于模型材料;由烧蚀产物引起的辐射通量主要在可见光和近红外区(465nm以上)。估算了烧蚀产物引起的辐射加热率,对头部和近尾流辐射通量做了比较。     

宇航科学文献情报源初析

本文通过对《宇航学报》1981～1988年322篇论文中2466条参考文献的统计分析,得出以下结论,(a)宇航科学的文献情报源重在期刊类文献。(b)以《宇航学报》、《航空学报》、《AIAA,Jourual》等六种期刊类文献为重点文献。(c)中文的引文作者和论文作者相对集中。(d)期刊类文献的半衰期为8～10年。     

数值模拟高超音速化学非平衡流的隐式格式

针对高超音速化学非平衡流提出了两种隐式格式.一种是近似因子分解算法对角化形式在隐式TVD(全变差递减)格式上的推广,另一种可视为隐式TVD格式的LU分解形式.数值试验表明,本文给出的算法保持了TVD格式的高分辨率特性,同时计算量大大减少,是高超音速化学非平衡流数值模拟的有效方法.     

带滑移铰空间机械臂惯性空间轨迹的复合自适应跟踪控制

讨论了载体的位置与姿态均不受控制的漂浮基带滑移铰空间机械臂的控制问题。动力学分析表明，结合系统动量及动量矩守恒关系得到的运动Jacobi关系及系统动力学方程将是系统惯性参数的非线性函数，借助于增广变量法，我们得到了与惯性参数呈线性关系的系统广义Jacobi矩阵及系统控制方程，以此为基础，针对系统中存在未知惯性参数的情况，设计了一种末端抓手惯性空间期望轨迹跟踪的复合自适应控制方案，此控制方案的优点在于不需要测量空间机械臂载体的位置及移动的速度，加速度，仿真运算证实了方法的有效性。     

SPACE LIFE SCIENCE IN 2000-2001

Chinese scientists studied some of the problems in the field of space life science and achieved success in the area during 2000-2001. Space biological experi ments were carried out in the orbit and the results of ground studies on protein crystallization, space radiation, space motion sickness were introduced in this paper. The influences of simulated weightlessness on the brain-function, the car diovascular, endocrine hormones, immunity, skeletal and muscle systems were presented. In addition, gravity medicine and space environment medicine, as well as countermeasures to space deconditioning, such as the traditional Chinese medicine, were also reported.     

KuaFu Mission

The KuaFu mission-Space Storms, Aurora and Space Weather Explorer-is an "L1+Polar" triple satellite project composed of three spacecraft: KuaFu-A will be located at L1 and have instruments to observe solar EUV and FUV emissions, and white-light Coronal Mass Ejections (CMEs), and to measure radio waves, the local plasma and magnetic field,and high-energy particles. KuaFuB1 and KuaFu- B2 will bein polar orbits chosen to facilitate continuous 24 hours a day observation of the north polar Aurora Oval. The KuaFu mission is designed to observe the complete chain of disturbances from the solar atmosphere to geospace, including solar flares, CMEs, interplanetary clouds, shock waves, and their geo-effects, such as magnetospheric sub-storms and magnetic storms, and auroral activities. The mission may start at the next solar maximum (launch in about 2012), and with an initial mission lifetime of two to three years. KuaFu data will be used for the scientific study of space weather phenomena, and will be used for space weather monitoring and forecast purposes. The overall mission design, instrument complement, and incorporation of recent technologies will target new fundamental science, advance our understanding of the physical processes underlying space weather, and raise the standard of end-to-end monitoring of the Sun-Earth system.     

部分开放多极磁场中的日冕磁绳灾变

采用球坐标下二维三分量理想MHD模型，研究部分开放多极背景磁场中日冕磁绳的灾变现象．背景磁场由含3个闭合双极场的冕流和带赤道中性电流片的开放场构成，磁绳位于中心双极场的下方，其特性由环向磁通和轴向磁通表征．对给定的环向磁通，存在轴向磁通的一个临界值；对给定的轴向磁通，也存在环向磁通的一个临界值．在该临界值以下，磁绳附着于太阳表面，系统处于平衡状态；该临界值一旦被超越，磁绳将脱离太阳表面向上喷发，说明部分开放多极背景磁场中的日冕磁绳系统存在灾变现象．本文算例表明，灾变点对应的磁能阈值超过对应部分开放场(中心双极场开放，两侧的双极场仍维持闭合)能量约15％，其超过部分可为日冕物质抛射一类太阳爆发提供能源．