Effects of Mo on the Microstructure and Hydrogen Sorption Properties of Ti-Mo Getters

The effects of Mo on the microstructure evolution, porosity and hydrogen sorption properties of Ti-Mo getters are investigated in this work. The results show that the addition of Mo prolongs the densification process of Ti-Mo getters and results in a significant amount of sintered pores. With the Mo content increasing, the porosity of getters firstly increases reaching the maximum value as it at- tains about 7.5wt.%, and then drops. At the room temperature, the hydrogen sorption property of getters increases progressively with the Mo content increasing, but the tendency is not very clear before its content lies below 2.5wt.%. When the Mo content achieves about 7.5wt.%, the hydrogen sorption property proves to be the best. The discussion is made about the above mentioned phenomena inclusive of hydrogen sorption properties of getters under different activation conditions (from 500-750 ℃).     

基于SN比试验设计法的磨削条件优化及表面粗糙度预测

通过SN比试验设计法,就各因素对磨削表面粗糙度的影响规律加以分析,并寻求能够获得最小表面粗糙度的最佳加工条件,同时提出预测表面粗糙度的方法,并通过实验加以验证。     

可压缩流动SIMPLE算法压力修正方程边界条件处理探析

可压缩粘性流体Nivier-Stokes方程SIMPLE算法求解中压力修正方程起着关键的作用.提出从连续性方程本质出发确定压力修正方程边界条件的方法.通过对双圆弧(凸包)通道内流场的计算验证了方法的正确性.     

民用飞机冰污染水平安定面失速试飞技术研究

基于CCAR-25对民用飞机冰污染水平安定面失速的合格审定试飞要求,对冰污染水平安定面失速进行了分析,针对ARJ21-700飞机,分析总结了冰污染水平安定面失速原理、改出方法、与机翼失速的差异、试飞方法和试飞结果分析,对于民用飞机合格审定试飞以及他运输类飞机具有非常重要的意义。     

腐蚀电场平面问题边界元法研究

 研究腐蚀电场平面问题的边界元理论和分析方法。首先,详细论述腐蚀电场平面问题的边界元理论。其次,针对电极极化曲线的非线性特性,提出一个求解含非线性边界条件的边界元问题的迭代解法。最后,按本文所述理论和方法,具体计算了某些电偶腐蚀电场的电位与电流密度分布,并与有关实驻结果比较,发现二者相符甚好。     

一种改进的运载火箭迭代制导方法

为提高运载火箭在大气层外当推力出现故障条件下制导算法的最优性、鲁棒性和适应性,提出了一种改进的迭代制导方法。该方法以基于最优控制理论推导的解析形式作为最优控制解,并推导出以5个轨道根数作为终端约束的横截条件,增强了算法的最优性;迭代过程中采用高斯-勒让德方法计算推力积分,并采用球极坐标系下泰勒多项式逼近方法计算引力积分,提高了故障模式下算法的积分精度;该算法采用降维迭代求解模式,并结合对控制变量的合理限幅,保障了推力故障条件下算法的实时性和收敛性。分别基于蒙特卡洛打靶和推力故障条件下进行仿真验证,结果验证了所提方法具有较强的最优性、鲁棒性和故障适应能力。     

相同设备在不同试验条件下试验图谱选择方法

同一机载设备可能安装在同一飞机的不同位置,而不同位置可能具有不同振动试验要求。为合理选择典型振动试验条件,使同状态机载设备既能经受考核验证又能满足产品互换性要求,以累计疲劳损伤理论为基础,以仿真为手段,以试验为验证,研究了不同试验条件对产品寿命的影响,并以产品寿命为依据,得出了试验条件的选择方法。     

复合材料的边界吸湿模型

在研究复合材料层合板的吸湿和退湿过程中，常常采用菲克定理来描述水分在层合板中的扩散过程中，根据层合板表面浓度逼近平衡浓度的不同响应，提出了三类不同的边界条件模型来模拟复合材料层合板在不同环境介质下的水分扩散过程，并给出了计算吸湿量的解析解和有限差分数值计算方法。     

Comparison of heliospheric conditions near the earth during four recent solar maxima

Statistical properties of the daily averaged values of the solar activity (sunspot numbers, total solar irradiance and 10.7 cm radio emission indices), the solar wind plasma and the interplanetary magnetic field parameters near the Earth’s orbit are investigated for a period from 1964 to 2002 covering the maxima of four solar cycles from 20th to 23rd. Running half-year averages show significant solar cycle variations in the solar activity indices but only marginal and insignificant changes in comparison with background fluctuations for heliospheric bulk plasma and magnetic field parameters. The current 23rd cycle maximum is weaker than 21st and 22nd maxima, but slightly stronger than 20th cycle in most of solar and heliospheric manifestations.     

Solar Wind Models from the Sun to 1 AU: Constraints by in Situ and Remote Sensing Measurements

There are three major types of solar wind: The steady fast wind originating on open magnetic field lines in coronal holes, the unsteady slow wind coming probably from the temporarily open streamer belt and the transient wind in the form of large coronal mass ejections. The majority of the models is concerned with the fast wind, which is, at least during solar minimum, the normal mode of the wind and most easily modeled by multi-fluid equations involving waves. The in-situ constraints imposed on the models, mainly by the Helios (in ecliptic) and Ulysses (high-latitude) interplanetary measurements, are extensively discussed with respect to fluid and kinetic properties of the wind. The recent SOHO observations have brought a wealth of new information about the boundary conditions for the wind in the inner solar corona and about the plasma conditions prevailing in the transition region and chromospheric sources of the wind plasma. These results are presented, and then some key questions and scientific issues are identified. This revised version was published online in June 2006 with corrections to the Cover Date.