环氧树脂基复合材料加筋板结构吸湿行为研究

环氧树脂基复合材料的性能对湿热环境敏感，掌握该材料所组成结构的吸湿行为对其实际应用具有重要意义。通过以碳纤维环氧树脂基复合材料层合板的non-Fickian吸湿模型为基础，建立环氧树脂基复合材料加筋板结构的non-Fickian吸湿模型，在70℃/85% RH湿热条件下开展加筋板结构的吸湿实验，对所建立模型进行验证，并与已有的加筋板吸湿模型进行对比，通过所建立模型给出了加筋板沿厚度方向的吸湿量分布规律。结果表明:所建立加筋板non-Fickian吸湿模型的计算结果与实验结果吻合良好，在整个吸湿阶段相对误差小于5%，模型的预测精度高于传统Fick模型。所建立的加筋板non-Fickian吸湿模型可用于环氧树脂基复合材料加筋板层合结构吸湿量的准确预测。      

仿壁虎刚毛阵列对卫星表面吸附能力模型与计算

壁虎脚的粘着机理对航天机器人脚掌的研制和开发具有重要启发意义.通过单根刚毛与光滑表面黏着力模型与计算、卫星粗糙表面分布模型与接触概率与计算、刚毛阵列与卫星粗糙表面黏着力模型与计算等，分析仿壁虎刚毛阵列对卫星表面的吸附能力，发现在一定条件下仿壁虎刚毛阵能够在太空失重环境中黏着在卫星表面，对航天舱内爬行机器人、管道机器人的研制和开发具有重要的启示意义.     

Simulation and Analysis of Electromagnetic Force in Laser Melting Deposition by Electromagnetic Impact

Magnetic field was introduced in laser melting deposition to reduce the pores in workpieces.Finite 3-D model of the coil-deposition layer-substrate was established.Simulation results show that the electromagnetic force in deposition layer mainly concentrates in the projection area of the coil.Axial electromagnetic force shows repulsion in one cycle.The experimental results indicate that the magnetic field is beneficial for grain refinement,microhardness increasement and decline of quantities and average sizes of pores.     

Ionospheric F2-Layer critical frequency retrieved from COSMIC radio occultation: A statistical comparison with measurements from a meridional ionosonde chain over Southeast Asia

In this paper, we compared the F2-Layer critical frequency (foF2) derived from FORMOSAT-3/COSMIC radio occultation (RO) and ionosondes at Chiang Mai, Chumphon and Kototabang during the years 2008–2015 to evaluate the performance of COSMIC RO over Southeast Asia region. The results show that the time development of foF2 values derived from COSMIC RO generally agrees well with those from ionosonde measurements. However, the differences between the foF2 derived from COSMIC RO and that derived from ionosonde observations display latitudinal dependence. COSMIC RO tends to underestimate foF2 at Chiang Mai and Kototabang, which is near to the north EIA crest and the south one, respectively, while a little overestimate foF2 at Chumphon, which is close to the geomagnetic equator. COSMIC RO agrees best with ionosonde at Chumphon and worst at Chiang Mai. At each ionosonde station, the quality of COSMIC RO data degrades with the increase of solar activity. In addition, at the station Chiang Mai and Kototabang, COSMIC RO performs better in summer than in equinox and winter. Furthermore, the differences in foF2 derived from COSMIC RO and that from ionosonde measurements vary with local time, i.e., the differences in foF2 are generally smaller at night and larger in noontime when equatorial ionization anomaly (EIA) is well developed.     

一种基于深度学习的电磁信息泄漏检测方法

电子信息设备工作时无意发射的电磁波中包含有用信息，会导致电磁信息泄漏，从而威胁设备的信息安全。现有的电磁信息泄漏检测方法，在复杂现场环境下，难以从具有不确定性的电磁泄漏信号中提取有用信息。面向电磁信息安全问题，开展了电磁信息泄漏检测研究，提出了一种基于深度学习的检测方法。设计了一个适用于电磁泄漏信号的一维卷积神经网络，并结合改进的梯度加权类激活映射方法，在未知电磁信息泄漏特征的前提下，通过深度学习实现电磁信息泄漏特征的智能标定和自动提取，从而解决了现场环境下电磁信息泄漏检测难以提取有用信息的问题。分别通过实测和仿真对比实验，验证了所提方法的有效性。      

Research on navigation of satellite constellation based on an asynchronous observation model using X-ray pulsar

Pulsar navigation is a promising navigation method for high-altitude orbit space tasks or deep space exploration. At present, an important reason for restricting the development of pulsar navigation is that navigation accuracy is not high due to the slow update of the measurements. In order to improve the accuracy of pulsar navigation, an asynchronous observation model which can improve the update rate of the measurements is proposed on the basis of satellite constellation which has a broad space for development because of its visibility and reliability. The simulation results show that the asynchronous observation model improves the positioning accuracy by 31.48% and velocity accuracy by 24.75% than that of the synchronous observation model. With the new Doppler effects compensation method in the asynchronous observation model proposed in this paper, the positioning accuracy is improved by 32.27%, and the velocity accuracy is improved by 34.07% than that of the traditional method. The simulation results show that without considering the clock error will result in a filtering divergence.     

激光动态液位测量技术研究

如今,运载火箭大量使用液氧、煤油等液体推进剂,其液位测量技术主要有浮子式、激光式、电容式、雷达式等。介绍并实现了一种激光液位测量系统,该系统体积小、功耗低,可适应多种测量环境,能满足航天燃料液位测量高精度、高动态、连续稳定测量的要求。系统利用相位式激光测距技术,通过测量激光回波信号的相位延迟,计算激光光程从而得到距离数据并通过客户端进行直观展示和数据存储。系统最大测量距离可达100 m,精度为±1 mm。该系统为非接触测量,耐腐蚀,通过加入反射板可实现透明、非透明液体测量。