聚酰亚胺/无机氧化物复合薄膜的制备与耐原子氧性能

分别以锆酸四丁酯、钛酸四丁酯和正硅酸乙酯为氧化物前驱体,利用溶胶凝胶法制备了一系列聚酰亚胺/无机氧化物复合薄膜,在原子氧地面模拟设备中进行了原子氧暴露实验,原子氧累计通量约为3.1×10²⁰ atom/cm².分别考察了无机氧化物种类和含量对复合薄膜力学性能和耐原子氧性能的影响.结果表明,无机氧化物在聚酰亚胺基体中的分散形态对其力学性能影响很大;原子氧暴露后,聚酰亚胺薄膜表面分别形成了富锆、富钛和富硅的保护层,质量损失率减小,耐原子氧性能明显提高.     

Kalman滤波的铷原子钟控制算法

以GPS接收机输出的1pps信号为参考信号,采用Kalman滤波算法对铷原子钟的参数进行估计,计算铷原子钟的频率调整量,对铷原子钟进行调整,使其和UTC时间保持同步。实验结果表明,受驯铷原子钟输出1pps与UTC（NTSC）钟差的标准差优于3.5 ns,钟差峰峰值优于15 ns,100 s采样的Allan方差为1.83×10 -12 ,10000 s采样的Allan方差为6.1×10 -13 。实验证明了基于Kalman滤波的铷原子钟控制算法,使铷钟获得了较好的准确性和长期稳定性,且对其短期稳定性影响最小,是一种可靠稳定的铷钟控制方法。     

Vertical distribution of the power of short- and long-period oscillations in a sunspot and in surrounding magnetic elements

We present the results of processing three 256-min series of observations of quasi-periodic oscillations of the field of line-of-sight velocities in three sunspots. The Doppler shifts were determined simultaneously for six spectral lines formed at different heights in the solar atmosphere. In addition to the well-known high-frequency (periods of 3–5 min) oscillations, a band of low-frequency oscillations with periods of 60–80 min is revealed in the spectra of the sunspot umbra and magnetic elements located in immediate proximity of the sunspot. Unlike the short-period modes, the power of the long-period mode of line-of-sight velocity oscillations in the sunspot decreases sharply with height: these oscillations are distinctly seen in the line formed at a height of 200 km and almost are not seen in the line with the formation height of 500 km. This is indicative of different physical nature of the short-period and long-period oscillations of a sunspot. If the former are caused by slow magnetosonic waves within the field tube of the spot, the latter are representative of global vertical-radial oscillations of a magnetic element (spot, pore) as a whole near the position of a stable equilibrium.     

基于用户自定义变更的本体进化

提出一种基于用户自定义变更的本体进化方法。首先给出了该方法的形式化描述,建立了本体一致性模型和原子变更及冲突消解方法,然后对用户自定义变更模型进行语义描述,将用户自定义变更转换成原子变更,并对其进行了优化。最后给出了用户自定义变更及优化的实例。结果表明:本方法可以很好地满足本体进化过程中用户的复杂需求,并实现了本体变更的形式化描述,解决了各种变更中的冲突问题。     

原子谱线参数的辨识方法

在一种原子谱线参数测量的辨识方法基础上编制了一套原子港线参数辨识的标准软件。用此软件对纯氩和氩、氮混合非平衡电弧等离子体射流的原子谱线进行了处理，获得了射流的电子温度、气体平动温度、电子和原子数密度。状态诊断表明；实验条件下的等离子体射流除中心点为ＬＴＥ外非平衡效应是非常显著的。     

IIR滤波器在芯片原子钟中的应用

芯片原子钟是具有小体积,低功耗特点的原子钟。本文采用了IIR滤波器方案对芯片原子钟物理系统输出信号进行处理,该方案有利于减小芯片原子钟的体积、提高芯片原子钟短期频率稳定度。实验结果表明,与FIR滤波方案相比,IIR滤波器使用的FPGA资源减小了约58%;与现有模拟滤波方案相比,使用IIR滤波器方案的芯片原子钟频率稳定度提高了1.4×10~(-10)τ~(-1/2)(τ=1s-100s),电路面积减小了10%。     

多元高温合金固溶极限预测

综合考虑了溶质元素与基体元素的原子半径、电负性以及外层电子数的立方根对溶质元素固溶度的影响，推导出二元合金的固溶度定量方程，提出了多元高温合金固溶极限曲线的预测新方法，并将其应用于计算镍基和钴基三元合金相图的γ／（γ＋σ）相界和γ（γ＋μ）相界。结果表明，计算的固溶极限曲线与已知相图的固溶极限曲线较吻合，与Ｍｄ值法计算的相界比较，该方法具有较高的精度。     

Loop Models from SOHO Observations

The Coronal Diagnostic Spectrometer (CDS) on SOHO is a grazing/normal incidence spectrograph, aimed to produce stigmatic spectra of selected regions of the solar surface in six spectral windows of the extreme ultraviolet from 150 Å to 785 Å (Harrison et al. 1995). In the present work, CDS, EIT, MDI and Yohkoh observations of active region lops have been analyzed. These observations are part of JOP 54. CDS monochromatic images from lines at different temperatures have been co-aligned with EIT and MDI images, and loop structures have been clearly identified using Fe XVI emission lines. Density sensitive lines and lines from adjacent stages of ionization of Fe ions have been used to measure electron density and temperature along the loop length; these measurements have been used to determine the electron pressure along the loop and test the constant pressure assumption commonly used in loop modeling. The observations have been compared with a static, isobaric loop model (Landini and Monsignori Fossi 1975) assuming a temperature-constant heating function in the energy balance equation. Good agreement is found for the temperature distribution along the loop at the coronal level. The model pressure is somewhat higher than obtained from density sensitive line ratios.     

相对测量在编队卫星自主定轨中的应用

针对编队卫星自主定轨问题进行了研究,设计了一种完全不依赖于地面站和GPS系统的自主导航方案。利用星间测量信息进行卫星编队相对轨道状态的自主确定;并在利用磁强计进行卫星绝对轨道自主确定的基础上,引入星间测量信息提高绝对定轨精度;设计扩展卡尔曼滤波器进行卫星编队轨道状态估计,数学仿真结果验证了这种导航方案和算法的有效性。     

原子氧对Kapton侵蚀及ZnO-有机硅涂层防护效应研究

在原子氧(AO)侵蚀地面模拟试验设备中对聚酰亚胺(Kapton)和涂ZnO-有机硅防护层的样品进行原子氧剥蚀效应试验。用LAMBDA-9分光度计、光电子能谱(XPS)、红外光谱(FTIR)和扫描电镜(SEM)等对试验前后试样的表面形貌、质量及化学结构进行表征研究。AO对Kapton表现了较严重的侵蚀作用,其化学结构、元素百分含量和表面形貌都发生明显变化。而所施用的ZnO-有机硅涂层对AO辐照有较强的防护效果,并具有较好的空间稳定性。因腐蚀产物为SiO2,这对抑制AO的进一步侵蚀起到了关键作用。