光刻技术在流体动力密封研究中的应用

主要介绍了流体动力密封螺旋槽动环光刻工艺的特点、原理、工艺过程、工艺流程、槽深控制方法以及应用情况，提出了采用高能束流刻蚀螺旋槽动环的新途径．结果表明，采用标准MEMS光刻工艺技术和化学铣切工艺技术，可加工出满足设计要求的螺旋槽动环．     

Lick Observatory Optical SETI: targeted search and new directions

Lick Observatory's Optical SETI (search for extraterrestrial intelligence) program has been in regular operation for 4.5 years. We have observed 4,605 stars of spectral types F-M within 200 light-years of Earth. Occasionally, we have appended objects of special interest, such as stars with known planetary systems. We have observed 14 candidate signals ("triple coincidences"), all but one of which are explained by transient local difficulties. Additional observations of the remaining candidate have failed to confirm arriving pulse events. We now plan to proceed in a more economical manner by operating in an unattended drift scan mode. Between operational and equipment modifications, efficiency will more than double.     

质量、质心测试仪适应多种战斗部测试研究

介绍了战斗部质量、质心测试原理及系统组成,通过对测试仪支撑结构与测量架的改进,提出了一种质量、质心测试仪适应多种产品测试的设计思路,经试验与应用,测试仪支撑结构的优化设计较好解决了复杂外形曲线产品质量、质心的测试。     

基于深度强化学习的机器人推拨优化装箱问题研究

三维装箱问题是指在满足容积限制、稳定性限制等条件下,将一定数量的物体放入较大容量的箱子中并使空间利用率最大的组合优化问题.三维装箱问题是典型的NP完全问题,通常采用启发式算法规划物体放置的位姿.在使用机器人完成装箱任务时,还要额外考虑机器人操作限制,如机械臂或末端执行器与物体或箱子之间的碰撞、机械臂运动轨迹的规划等,使得部分最优位姿不可行,只能将物体从更高处落下或者将物体放在最优位姿的附近.机器人在抓取、识别和放置时的不确定性也会导致最终放置位置与规划产生偏差.因此,本文提出基于深度强化学习的机器人三维装箱推拨优化方法,以最小化包装箱中物体放置位置的启发式算法分数为目标,通过推拨动作对于已放置的物体位置进行调整、归集,将物体朝角落中压缩,以腾出更多空间,提高装箱空间利用率,减小由于机器人操作不确定性对装箱结果的影响.     

A multiple-CubeSat constellation for integrated earth observation and marine/air traffic monitoring

CubeSats has evolved from purely educational tools, to useful platforms for technology demonstration and many practical applications. This paper reviews a CubeSat constellation mission involving 3 CubeSats launched into orbit on Sep. 25th 2015, aiming to demonstrate the integrated application of low-cost CubeSat technologies with distributed payloads using a group of satellites, as well as to demonstrate several new technologies. The mission scenario, the satellite system design, the innovative technologies and instruments or devices used on the CubeSats and the in-orbit experimental results and the payload data analysis, as well as some experiences and lessons learned, are presented and summaried.     

Orbit insertion error analysis for a space-based gravitational wave observatory

Constellation is required to be highly stable over several years for a space-based gravitational wave observatory. However, the stability of the constellation can be affected by orbit insertion errors. The effects of orbit insertion errors on the constellation are mainly studied in this paper. Firstly, Monte-Carlo, Unscented Transformation Covariance Analysis Method (UTCAM) and Spherical Simplex Unscented Transformation Covariance Analysis Method (SSUTCAM) are used for simulation. The results indicate that UTCAM and SSUTCAM are highly efficient in calculating, with a relative error of less than 6%. Therefore, it is concluded that because of their accuracy and high efficiency, UTCAM and SSUTCAM can be adequately used in orbit insertion error analysis for a space-based gravitational wave observatory. Secondly, SSUTCAM is used to study the effects of position and velocity errors on the constellation. For the case in this paper, when the position error does not exceed 300 km, and the velocity error does not exceed 4 cm/s, the constellation remains stable.     

基于残缺图像样本的生成对抗网络图像修复方法

针对大面积图像修复缺失严重时,需要完整且高质量训练样本的问题,提出了一种将残缺或含噪图像样本作为训练集的双生成器深度卷积生成对抗网络（DGDCGAN）模型。构建两个生成器和一个鉴别器以解决单一生成器收敛慢的问题,用残缺图像样本作为训练集,通过交叉计算、搜索损失区域类似的图像信息作为训练生成模型的样本,收敛速度更快。鉴别器损失函数改进为输出的Wasserstein距离,使用自适应估计算法优化生成器损失函数和鉴别器损失函数的模型参数,最小化两两图像之间的总距离差,使用鉴别模型和修复图像总距离变化均方差最小化两个指标优化修复结果。在4个公开数据集上进行主客观实验,结果表明:所提方法能使用残缺图像样本作为训练集,有效实现大面积失真图像的修复,且收敛速度和修复效果优于现有图像修复方法。      

卫星表面原子氧通量和遭遇量的计算及讨论

建立了一个较为理想情况下卫星表面原子氧通量和遭遇量的计算模式。在此基础上,着重讨论了轨道高度、太阳活动、飞行攻角及轨道倾角等因素对原子氧通量和遭遇量的影响。     

交会对接中的Hill制导误差

在交会对接的自动寻的阶段, Ｈｉｌｌ制导的精度受多种误差因素的影响。介绍这些误差因素,并着重研究了导航误差和控制误差与瞄准点误差之间的关系,给出了基本分析公式。根据误差公式, 研究了如何通过设计交会轨迹来减小这两项误差对终端精度的影响。结合一种典型的 Ｖ ｂａｒ 接近轨迹, 给出了仿真结果; 结果同样适用于 Ｒ ｂａｒ 接近。     

基于吸波超材料的微带天线设计

为缩减天线带内雷达散射截面,设计出一种频带较宽的超材料吸波体。该吸波体是由两层金属及其中间的有耗介质组成,上层金属是由刻蚀四个不同大小方孔的贴片形成的电谐振器,下层金属不刻蚀,作为整个金属地板。通过优化结构参数,得到了一种极化不敏感、宽入射角的超薄吸波体,吸波率达到97%,厚度只有0.3mm。仿真结果表明:通过渐变开孔,该吸波体吸波带宽大大扩展。相比普通微带天线,加载该吸波体后天线在工作频带内法向RCS减缩可达3~12.6dB,同时天线的增益也有较大提高。