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.     

存储系统中两级纠错编码方案设计与验证

针对恶劣空间环境设计了一种两级存储编码方案，以应对航天系统中存储单元发生多个单粒子翻转（SEU）错误的问题。方案设计的主要思想是根据简单低纠错编码组合出高容错编码，通过编码组合，使用字间编码来纠正字内编码无法纠正的错误，从而使存储系统更加可靠；对两级编码方案提出若干优化策略，以提高编解码性能，使得两级冗余编码效率接近于原始字内编码。实验结果表明，提出的两级冗余编码方案能够较好解决存储系统中发生多个单粒子翻转错误的问题。即与单一的字内编码相比，两级纠错编码方案能够大大降低星上存储系统出现不可修复的概率，保证了星上存储系统的可靠运行。     

航空制造领域移动机器人加工系统研究综述

移动机器人加工系统在航空大部件装配领域应用广泛。由于移动机器人加工系统脱离定点作业模式进行移动加工,在实际加工过程中,其大部件待加工部分的高精度定位以及切削加工过程的加工稳定性问题必须要得到研究和解决。通过对国内外先进移动机器人加工系统的研究综述,重点研究移动状态下大部件高精度定位技术以及加工过程中的振动抑制问题,以实现移动机器人的稳定切削加工,并对有待解决的问题及未来的研究方向进行了讨论和展望。     

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.     

一种柔性空间双臂机器人的协同控制和避障方法

针对柔性空间机械臂在轨服务应用需求，提出一种基于刚体运动与柔性振动相耦合的空间双臂机器人协同控制方法.首先引入空间位姿变量的概念，构造出面向协同控制目标的Jacobian矩阵，建立柔性空间机器人系统的刚柔耦合动力学模型，基于指定的最小距离得到其运动学逆解，并根据系统动量矩守恒关系及系统的Jacobian矩阵，并根据机械臂末端的运动速度,然后采用阻尼最小二乘法得出关节角度，使柔性空间机器人能够有效完成协同控制和空间避障任务，并基于RecurDyn V7R5软件环境验证算法的正确性.最后，基于SolidWorks和ADAMS虚拟样机建立柔性空间机器人系统的立体CAD模型，并结合空间在轨搬运任务进行模拟仿真，柔性空间机器人关节操作和运动轨迹的仿真结果图验证了本文算法的有效性.     

Global ionospheric scintillations revealed by GPS radio occultation data with FY3C satellite before midnight during the March 2015 storm

Global observations of S4 amplitude scintillation index by the GPS Occultation Sounder (GNOS) on FengYun-3 C (FY3C) satellite reveal global dynamic patterns of a strong pre-midnight scintillations in F-region of the ionosphere during the St. Patrick’s Day geomagnetic super storm of 17–19 March 2015. The observed strong scintillations mainly occurred in the low latitudes, caused by equatorial plasma bubbles. During the main storm phase (March 17), the scintillations were first triggered in the New Zealand sector near 160°E longitudes, extending beyond 40°S dip latitude. They were also enhanced in the Indian sector, but significantly suppressed in East Asia near 120°E longitude and in Africa around 30°E longitude. During the initial recovery phase (March 18–19), the global scintillations were seldom observed in GNOS data. During the later recovery phase (after March 19), the scintillations recovered to the pre-storm level in Indian, African, and American sectors, but not in East Asian and any of Pacific sectors. These results closely correlate with observations of the density depletion structures by the Communication/Navigation Outage Forecasting System (C/NOFS) satellite, and ground-based instruments. Such consistency indicates reliability of our scintillation sensing approach even in a case-by-case comparison study. The prompt penetration electric field and disturbance dynamo electric field are suggested as the main factors that control the enhancement and inhibition of the scintillations during the storm, respectively.