一种改进的多点融合非均匀校正技术

针对空间宽幅相机在进行非均匀性校正过程中相机镜头与积分球输出口的相对位置发生变换后非均匀性校正精度下降的原因进行了分析,提出了一种改进的融合多点位置的非均匀校正新方法,即为了消除积分球的角均匀性和面均匀性的不足,采用获取多个位置的大量定标图像,融合求取平均值的方法得到校正系数来削弱这种影响,并进行试验验证分析。结果表明,多点融合的校正方法在积分球输出口光强不均匀、又无法固定相机与积分球相对位置的前提下,减少了积分球光强的不均匀性对系数可靠性的影响,相对辐射定标的非均匀校正精度得到大幅提高。     

铷频标物理系统的改进研究

物理系统是铷频标的核心部件,通过分析影响频率稳定度的因素,对物理系统内部结构进行了改进。改进后的物理系统采用分离滤光的三泡结构,增加了光学滤光技术,此外,物理系统还选用了磁控管微波腔。经测试,改进后的铷频标温度系数为9.7×10^-14/℃,频率稳定度约为1×10^-12/τ（1s≤τ≤10 000s）。     

中心进气转静系转盘风阻扭矩数值模拟

采用计算流体力学(CFD)商业软件CFX从流动参数及几何结构两个方面对中心进气转静系盘腔内转盘风阻扭矩特性进行了数值模拟研究,同时搭建一个转盘风阻扭矩实验台测量自由盘风阻扭矩.中心进气转静系转盘风阻扭矩与经典经验公式进行了对比,结果表明:利用数值模拟方法,得到的无量纲扭矩系数与经典经验关系式计算得到的数据总体相差小于10%,利用湍流参数来表征转盘转速以及叠加流流量,对于分析转盘风阻扭矩非常便利.利用湍流参数定量分析时需注意叠加流以及转速的量级同样影响着风阻扭矩的数值.几何结构对于风阻扭矩也有影响,但相比流动参数影响较小.      

运动基航天飞行训练模拟器信号缩比算法研究

当前运动基飞行模拟器对控制信号的缩比以三阶多项式缩比法为主,但其参数确定困难且当缩比幅度较大时易使信号出现较大畸变。而航天飞行模拟中常常会经历线加速度或角速度信号在较大幅值范围内的增大或减小,典型的如返回再入时的过载变化。针对此种情况,一种新的缩比算法——Hermite缩比函数法被提出。首先完善了Hermit缩比法关于最优参数理论的推导和证明;其次,引入变量“缩比度”,在实例仿真中比较了其对两种缩比方法的影响。结果表明,Hermite缩比函数法参数确定方便,其信号单调性的保持不依赖于缩比度的取值,更适合应用于缩比度变化较大的航天飞行模拟中。
     

Periodic Variations of Drag Coefficient for the ANDE Spherical Satellites During its Lifetime

A drag coefficient (C_D) inversion method is introduced to study the variations of the drag coefficient for orbital satellites with spherical geometry. Drag coefficients of the four micro satellites in the Atmospheric Neutral Density Experiment (ANDE) are compiled out with this new method. The Lomb-Scargle Periodgram (LSP) analysis of the four ANDE satellites' C_D series has shown that there are obvious 5, 7, 9, and 27 days' period in those data. Interesting results are found through comparing the LSP analysis with series of the daily solar radio flux at 10.7 cm (F_10.7 index), the Ap index, and the daily averaged solar wind speed at 1AU. All series in the same time interval have an obvious period of about 27 days, which has already been explained as the association with the 27 days' solar rotation. The oscillating periods less than 27 days are found in series of C_D, Ap and solar wind speed at 1AU, e.g., the 5, 7, 9 days period. However, these short periods disappeared in the time series of F_10.7 index. The same periodicities of 5, 7, 9 days in Ap and solar wind are presented at the same time interval during the declining phase of solar cycle 23. While in the ascending phase of solar cycle 24, these short oscillations are not so obvious as that in the declining phase of solar cycle 23. These results provide definite evidence that the C_D variations with period of 5, 7 and 9 days are produced by a combination of space weather effects caused by the solar wind and geomagnetic activity.      

节点外啮合齿轮胶合承载能力中平均摩擦因数的计算方法

分析了现有胶合承载能力计算中平均摩擦因数计算方法的不足之处,根据节点外啮合齿轮传动的啮合特点,以相关标准中渐开线圆柱齿轮的计算公式为基础,提出了一种更为合理且精度较高的平均摩擦因数计算方法,以满足节点外啮合齿轮胶合承载能力计算的需要.通过对内、外啮合副节点前啮合和节点后啮合实例的计算,得出除外啮合节点前啮合以外,利用标准计算得到的平均摩擦因数的误差都超过18.5%,而改进计算方法所得的误差都在6.5%之内,证实了这种改进的平均摩擦因数计算方法具有更高的精度,而且这一计算方法也适用于标准齿轮传动.      

分子吸附器在航天器污染控制中的应用研究

文章对分子吸附器这种新型的在轨清除航天器分子污染物的方法进行机理分析,研究分子吸附剂和基底材料的选择方法,探讨分子吸附器的吸收力和有效黏附系数的测定方案等,并简要介绍国内的研究现状,分析国内外的差距,提出发展建议。     

双层壳型冲击/气膜综合流量系数实验研究

为了研究新型高效涡轮铸冷叶片内部冷却通道中的流动特性,以铸冷叶片典型结构——双层壳型冲击/气膜复合冷却结构的平壁模型为研究对象,实验研究了该种冷却结构的综合流量系数Cd随冲击雷诺数Red(600～2800),主次流吹风比M(0.7～7),冲击间距比H/d(0.5～1.25),冲击孔和气膜孔间距比P/d(0,3,4)等参数的变化规律。研究结果表明:(1)Cd随着冲击雷诺数Red,吹风比M的增加而增大,在吹风比小于3工况下更为显著;(2)在相同的气动参数条件下,综合流量系数Cd随着孔排距比P/d的增加而增大,随着冲击间距比H/d的减小而显著降低。     

A Prediction Method for△f0F2min of a Single Station From Interplanetary Parameters Based on Statistical Study

Using 86 CME-interplanetary shock events,the correlation between the peak values of （a） the solar wind parameters(B_z,E_y,P_dyn) and the geomagnetic indices（SYM-H,ASY-H,Kp）, （b） the coupling functions（Borovsky,Akasofu,Newell） and the geomagnetic indices,（c） the solar wind parameters/coupling functions/geomagnetic indices and the ionospheric parameter(Δf₀F_2min), are investigated.The statistical results show that in group（a）,B_{z min} and SYM-H_min have the best correlation,that in group（b）,the best correlation is between the peak values of Akasofu function (A_min) and SYM-H_min,and that in group（c）,the best correlation is between K_pmax andΔf₀F_2min. Based on the statistical results,a method for predicting f₀F₂ of a single station is attempted to be set up.The input is modified B_{z min} and the outputs are SYM-H_min andΔf₀F_2min.Then 25 CME-IPS events that caused geomagnetic storms in 1998 and 2009 are used to check the prediction method. The results show that our method can be used to predict SYM-H_min andΔf₀F_2min.     

Preliminary characterization of carbon dioxide transfer in a hollow fiber membrane module as a possible solution for gas–liquid transfer in microgravity conditions

In microgravity, one of the major challenge encountered in biological life support systems (BLSS) is the gas–liquid transfer with, for instance, the necessity to provide CO₂ (carbon source, pH control) and to recover the evolved O₂ in photobioreactors used as atmosphere bioregenerative systems.