RESEARCH PROGRESS ON FULL-FREQUENCY PREDICTION TECHNIQUES OF SPACECRAFT＇S MECHANICAL ENVIRONMENT

航天器力学环境预示对于总体设计、结构与机构分系统设计是至关重要的,特别是对于首发型号,往往缺乏相似型号的遥测数据参考,使得有效的预示成为地面试验方案和试验条件确定的主要依据．航天器在发射段需要承受覆盖全频域的动态载荷,不同频段的载荷和结构振动响应特性差异很大,很难用单一的分析方法进行准确预示．本文分别针对航天器发射力学环境的低频、高频、中频3个频段,介绍了国内外航天器全频域力学环境预示的主要方法及其工程应用的研究进展,并提出了我国在该领域亟需解决的关键技术．     

磁流变加工的连续相位板波前及光强特性

对采用磁流变抛光(MRF)工艺加工的大口径连续相位板(CPP)的波前及其光强控制特性进行了分析,对由不同的加工参数(走刀间距和走刀偏置)所加工的三组CPP进行了比较,并分析了MRF加工所引入的中频误差对CPP波前和光强特性的影响。结果表明,走刀间距为2mm、对应走刀偏置范围为0.1~0.3mm时所加工CPP的波前及其光强控制能力较差,远场有一定程度的旁瓣产生;走刀间距为2mm、偏置范围为0.4~0.5mm时所加工CPP和走刀间距为1mm、偏置范围为0.1~0.3mm时所加工CPP相比较,迭代加工效率提高,CPP波前中频误差得到一定的改善。进一步分析表明MRF所引入的中频误差对CPP波前梯度及旁瓣影响较大。     

Deposition of MgO films by pulsed mid-frequency magnetron sputtering

MgO films were deposited by pulsed mid-frequency magnetron sputtering from metallic targets in the mixture of Ar and O₂ gas. The surface morphology, crystalline structure, and optical properties were characterized by using atomic force microscopy (AFM), X-ray diffraction (XRD), and spectroscopic ellipsometry, respectively. The secondary electron emission coefficients of MgO films were measured by using a self-made apparatus in He gas. A pronounced hysteresis phenomenon of target voltage, current, and deposition rate with increasing and decreasing O₂ flow rate was observed. The structure of films deposited at a metallic mode changes from Mg phase to the mixed Mg and MgO phase, and the films have a very rough surface. All the films deposited at oxide mode have high transparency and smooth surface, and show (2 2 0) preferred orientation growth. The refractive index and extinction coefficient at a wavelength of 670 nm for MgO films deposited at oxide mode with a O₂ flow rate of 3 sccm are 1.698 and 1.16×10⁻⁴, respectively. The secondary emission coefficient at a E/p of 57.8 V/(cm Torr) for MgO films deposited at a O₂ flow rate of 3 sccm is 0.16, which is higher than that of MgO films deposited by e-beam evaporation.     

被动半刚性磨盘在平滑中频误差中的应用

介绍了一种去除中频误差的有效工具被动半刚性磨盘。被动半刚性磨盘由刚性基底、变形层、薄板层以及抛光层组成。这种特殊的夹层式结构使磨盘在平滑过程中具有高通滤波特性,因而能够有效去除中频误差。基于弹性力学和滤波器理论,分析了被动半钢性磨盘的平滑机理,讨论了磨盘基本参数和误差频率之间的相互关系。以一块表面具有明显中频误差的抛物面镜为实验件,对被动半刚性磨盘的平滑能力进行验证,经过2个周期(共计75 min)的平滑后,中频误差得到了有效抑制。     

航天器全频域力学环境预示技术研究进展

航天器力学环境预示对于总体设计、结构与机构分系统设计是至关重要的, 特别是对于首发型号, 往往缺乏相似型号的遥测数据参考, 使得有效的预示成为地面试验方案和试验条件确定的主要依据. 航天器在发射段需要承受覆盖全频域的动态载荷, 不同频段的载荷和结构振动响应特性差异很大, 很难用单一的分析方法进行准确预示. 本文分别针对航天器发射力学环境的低频、高频、中频3 个频段, 介绍了国内外航天器全频域力学环境预示的主要方法及其工程应用的研究进展, 并提出了我国在该领域亟需解决的关键技术.      

中频孪生磁控溅射WO3薄膜及变色性能研究

采用先进的中频孪生非平衡磁控溅射技术,以金属钨为靶材,制备非晶态WO3电致变色薄膜。用X射线衍射(XRD)、X射线光电子能谱(XPS)、紫外分光光度计等测试手段分析薄膜的结构、表面形貌、成分以及透射光谱特性。研究了氧气流量比及热处理温度对WO3薄膜变色性能的影响。结果表明,中频孪生非平衡磁控溅射技术是制备WO3变色薄膜的一种有效方法;室温条件下沉积获得的原始态薄膜为非晶态WO3;提高氧气流量比和适当热处理温度能有效改善薄膜的电致变色性能。实验中在较高氧气流量比,200℃热处理条件下制备的薄膜在380~780 nm的可见光范围内着色态和褪色态平均透光率差值高达50%以上,表现出较好的电致变色性能。     

A PREDICTION TECHNIQUE FOR DYNAMIC ANALYSIS OF FLAT PLATES IN MID-FREQUENCY RANGE

The wave-based method (WBM) has been applied for the prediction of mid-frequency vibrations of flat plates.The scaling factors,Gauss point selection rule and truncation rule are introduced to insure the wave model to converge.Numerical results show that the prediction tech- nique based on WBM is with higher accuracy and smaller computational effort than the one on FEM,which implies that this new technique on WBM can be applied to higher-frequency range.