原子氧对Kapton／Al薄膜性能影响研究

模拟空间环境下原子氧辐照条件,通过采用固定的原子氧束流密度进行不同时间辐照试验,研究了温控涂层材料Kapton/Al薄膜的质量损失、光学性能、表面形貌和表面粗糙度的演化规律.试验结果表明,原子氧对材料的剥蚀量与原子氧的作用时间成正比例关系.材料辐照后太阳吸收率发生明显变化,而辐射率几乎不发生变化.辐照后试样表面的粗糙度,是影响太阳吸收率变化主要因素.随着辐照时间的增长,材料表面粗糙度增加,导致太阳吸收率增大.     

高低温箱运行及故障分析探讨

通过对高低温箱的运行记录进行整理，分析其运行状况及故障，判断故障产生的原因，有针对性地提出故障排除的方法和设备维护保养措施，以延长设备的使用寿命。     

启动过程推力器喷注管内推进剂流的温降

根据空间发动机的总体结构、环境特点和能量守恒原理,提出推进剂在推力器喷注管内流动降温的简化数理模型,研究启动时单元推进剂在推力器喷注管内的流动降温现象.耦合求解推进剂流和喷注管能量方程,可以获得单元推力器喷注管单推三流整体温度的沿程分布规律.用推进剂模拟液实际考察和验证推力器喷注管的流动特点和理论模型的计算结果,分析推进剂流速、喷注管长度和内径对推进剂流温度变化的影响,导出推进剂流前缘出口温度和这3个物理参量间的拟合关系式.研究结果对推力器的热控设计有参考价值.     

超高负荷低压涡轮叶型边界层被动控制

应用商用流体计算软件求解定常雷诺平均N-S方程组耦合Lantry-Menter转捩模型,对来流湍流度1.5%,不同进口雷诺数下,前加载超高负荷低压涡轮叶型进行了数值模拟。在与相关实验数据对比的基础上,研究了三种被动控制方式的控制效果与控制机理。结果表明:弧形凹槽的最佳开槽位置在分离点,最佳深宽比为0.15,表面拌线和矩形条的最佳加载位置在速度峰值点与分离点的中点;控制方式能否有效与其增加的掺混损失和减少的分离损失有关;三种控制方式均通过产生小漩涡来增加低能流体与高能流体之间的交换,从而加速转捩减小分离泡降低叶型损失。     

吸附式低反动度超、跨音速轴流压气机气动设计原理及其验证

当增加动叶转角以进一步提升超、跨声速轴流压气机级负荷时,为解决其内部流动问题,提出了吸附式低反动度超、跨声速轴流压气机气动设计原理。分析了在该气动设计原理指导下,级内参数的演变规律与相互影响。利用该气动设计原理完成了一高负荷超声速轴流压气机气动设计,三维粘性数值模拟结果表明,在叶尖切线速度370m/s的前提下,实现了一级压比2.5,效率87%的压气机级设计。      

Type II Solar Radio Bursts: Theory and Space Weather Implications

Recent data and theory for type II solar radio bursts are reviewed, focusing on a recent analytic quantitative theory for interplanetary type II bursts. The theory addresses electron reflection and acceleration at the type II shock, formation of electron beams in the foreshock, and generation of Langmuir waves and the type II radiation there. The theory's predictions as functions of the shock and plasma parameters are summarized and discussed in terms of space weather events. The theory is consistent with available data, has explanations for radio-loud/quiet coronal mass ejections (CMEs) and why type IIs are bursty, and can account for empirical correlations between type IIs, CMEs, and interplanetary disturbances. This revised version was published online in August 2006 with corrections to the Cover Date.     

Real-Time Specifications of the Geospace Environment

We report the recent progress in our joint program of real-time mapping of ionospheric electric fields and currents and field-aligned currents through the Geospace Environment Data Analysis System (GEDAS) at the Solar-Terrestrial Environment Laboratory and similar computer systems in the world. Data from individual ground magnetometers as well as from the solar wind are collected by these systems and are used as input for the KRM and AMIE magnetogram-inversion algorithms, which calculate the two-dimensional distribution of the ionospheric parameters. One of the goals of this program is to specify the solar-terrestrial environment in terms of ionospheric processes, providing the scientific community with more than what geomagnetic activity indices and statistical models provide. This revised version was published online in August 2006 with corrections to the Cover Date.     

Modelling of the electromagnetic field in the interplanetary space and in the Earth's magnetosphere

A magnetohydrodynamic model of the solar wind flow is constructed using a kinematic approach. It is shown that a phenomenological conductivity of the solar wind plasma plays a key role in the forming of the interplanetary magnetic field (IMF) component normal to the ecliptic plane. This component is mostly important for the magnetospheric dynamics which is controlled by the solar wind electric field. A simple analytical solution for the problem of the solar wind flow past the magnetosphere is presented. In this approach the magnetopause and the Earth's bow shock are approximated by the paraboloids of revolution. Superposition of the effects of the bulk solar wind plasma motion and the magnetic field diffusion results in an incomplete screening of the IMF by the magnetopause. It is shown that the normal to the magnetopause component of the solar wind magnetic field and the tangential component of the electric field penetrated into the magnetosphere are determined by the quarter square of the magnetic Reynolds number. In final, a dynamic model of the magnetospheric magnetic field is constructed. This model can describe the magnetosphere in the course of the severe magnetic storm. The conditions under which the magnetospheric magnetic flux structure is unstable and can drive the magnetospheric substorm are discussed. The model calculations are compared with the observational data for September 24–26, 1998 magnetic storm (Dst _min=−205 nT) and substorm occurred at 02:30 UT on January 10, 1997. This revised version was published online in August 2006 with corrections to the Cover Date.     

现代飞机制造成本控制方法研究

介绍了作业成本法(Activity-BasedCosting-ABC)及其全新的成本管理和控制思想。通过对工业工程(IndustryEngineering-IE)的技术特性与ABC算法内在联系的探讨,建立了一个IE+ABC成本控制体系,目的是对飞机制造过程的成本实施有效控制。企业实证初步表明了这个成本控制体系的实际应用效果及其研究推广价值。