中继反射镜能量特性研究

介绍了地基激光加天基中继反射镜体系的系统组成及基本工作原理, 重点对中继反射镜的能量特性进行了分析, 得出了作用距离与中继镜口径和目标辐照度的关系, 并给出了计算的实例. 其结果进一步说明了中继镜原理上的可行性, 提出了中继反射镜技术发展应该重点考虑的关键技术. 研究结果对于实际中继反射镜系统的设计有一定的参考意义.     

改善航天器反作用轮扰动实验模型参数的辨识方法

反作用轮系统是影响航天器姿控系统精度的主要扰动源之一.建立反作用轮扰动模型的目的是预测扰动对航天器产生的影响,并采取相应的控制方法和隔离系统.基于反作用轮的扰动实验模型,通过对反作用轮扰动实验数据的分析,确定出反作用轮扰动实验模型中的参数:谐波数和幅值系数,并在此基础上提出了能量补偿法,最后进行了数值仿真.结果表明,谐波数的辨识精度不超过0.04%,当采用振幅谱法计算幅值系数时,误差高达15.5%;而用能量补偿法,其幅值系数的精度不超过1.1%.可见能量补偿法提高了幅值系数的辨识精度.本文研究为改善航天器姿态控制精度和稳定度奠定了一定的基础.     

行星际扰动与不同级别磁暴强度关系的研究

利用1997-2004年间ACE卫星太阳风观测的时均值数据和相应的Dst指数,针对Dstmin≤-50 nT的磁暴,分析了行星际参数(Bz,Ey,v,Pk,|B|,ε'=vxB2zsin4(θ/2))与Dst指数的相关关系.验证了Ey,Bz与Dst指数的良好相关性;按磁暴强度的不同,发现磁暴强度越大,行星际参数与磁暴强度(Dstmin)的相关性就越好.对于中等磁暴(-100 nT＜Dstmin≤-50 nT),行星际参数与磁暴强度的相关系数不高.如果把磁暴分为两个档次,即-150 nT＜Dstmin≤-50 nT的磁暴和Dstmin≤-150 nT的磁暴,计算结果表明,ε'与Dst指数的相关性是最好的.在诸多行星际参数中,就单一因素来说,Ey对磁暴强度影响最大,Bz对磁暴强度影响次之.     

Output formation tracking for networked systems with limited energy and aperiodic silence

For leader-following networked systems with the topology switching and the aperiodic silence, limited-energy output formation tracking problems are investigated. Firstly, a new output formation tracking control protocol is proposed, which contains two components associated with the communication interactions between the leader and tracking intelligent agents and the communication interactions among tracking intelligent agents, respectively, and the aperiodic silence, the topology switching and t...     

Energy-efficiency maximization for fixed-wing UAV-enabled relay network with circular trajectory

With the development of Unmanned Aerial Vehicles (UAVs), the applications of UAVs have been extensively explored. In the field of wireless communications, the relay nodes are often used to extend network coverage. However, traditional fixed ground relays cannot be flexibly deployed due to their low heights and fixed locations. Hence, deploying UAV as relay node is a promising solution and has become a research hotspot. In this paper, we consider an UAV-enabled relaying network in which a fixed-wing UAV is deployed between the Base Station (BS) and Ground Users (GUs). We study the energy-efficiency gap between the link “BS-UAV-GUs” and the link “BS-GUs”, and jointly optimize UAV relay transmission power and flight radius to achieve the highest energy-efficiency. Firstly, the UAV/BS-GUs channels models and the UAV energy consumption model are built. Secondly, the optimization objective function is formulated to maximize the energy-efficiency gap. Then, the solution of the optimization problem is divided into a two-step iteration process, in which the UAV relay transmission power and flight radius are adjusted to maximize the energy-efficiency gap. Finally, the experimental results under different simulation scenarios (such as cities, forests, deserts, oceans, etc.) are shown to illustrate the effectiveness of the proposed algorithm. The results show that the proposed algorithm can always find the optimal UAV relay transmission power and flight radius settings, and achieve the largest energy-efficiency gap. The convergency speed of the proposed algorithm is fast, and can obtain the optimal solution within only a few iterations.     

纯磁控微小卫星姿态控制研究

针对微小卫星速率阻尼、姿态捕获及三轴稳定的不同姿态控制模式,设计了采用纯磁控的控制律.首先以轨道坐标系为参考建立卫星模型,然后在卫星能量分析和Lyapunov稳定方法基础上,应用B-dot控制进行速率阻尼,给出了全局稳定能量控制来进行姿态捕获和三轴稳定控制的新方法,同时根据线性化的卫星模型,设计了常系数LQG控制律.仿真结果表明,B-dot可以有效地进行速率阻尼,能量控制策略适用于大角度姿态捕获和三轴稳定,稳定控制时LQG与能量控制相比具有更高的精度,但稳定度略差.     

From the Solar Wind to the Magnetospheric Substorm

This paper gives a brief outline of the progression from the first substorm model developed in Ref.[4] and
[8] based on Kennel's ideas[3], to the present views about the mechanism by which solar wind kinetic energy is converted to electromagnetic energy at the Bow Shock and by which this energy is transferred to the magnetosphere in the form of current; about the transformation of the energy of this current to gas kinetic energy of convecting plasma tubes, and, finally, the back transformation of gas kinetic energy to electromagnetic energy in secondary magnetospheric MHD generators. The questions of the formation of the magnetospheric convection system, the nature of substorm break-up, and of the matching of currents in the magnetosphere-ionosphere system are discussed.     

双变量波状扰动激发重力波波包的数值研究

采用谱配置方法对双变量波状扰动激发重力波的过程及其能量传播和转换特性进行数值研究。模拟结果表明,当初始给定的两个变量的波状扰动的相对振幅和相位严格满足重力波的偏振关系时,只有水平风场扰动（u′）与温度扰动（T′）的共同作用才能抑制能量向下传输。通常情况下,两个变量的波状扰动都会激发出两支传播方向相反的重力波波包,这两支波包的相对能量明显取决于两个波状扰动之间的相对振幅关系。当两个扰动之间的相对振幅满足特定条件时,向下传播的能量几乎为零,只会有一支向上传播的重力波波包被激发。进一步的数值分析则表明,各种情况下两个变量的波状扰动所激发的重力波波包的能量传播路径和速度基本相同;与单变量波状扰动激发重力波波包的过程相比,能量传播路径几乎完全一致,扰动转化为波动的特征时间也基本相同,但能量转换效率更高。     

Core reinforcement design for improving flexural energy-absorption of corrugated sandwich composite structure

To strengthen Specific Energy-Absorption (SEA) behavior of Sandwich Composite Structure (SCS), a kind of light-weight vertical stiffener is proposed for the corrugated core. The vertical stiffener, embedded in the corrugated core, can not only absorb part of energy but also simultaneously enhance Energy-Absorption (EA) of other components. The Hashin damage model considering the shear stress and ductile damage model is adopted to predict the failure of carbon fiber face-sheets and aluminum-core, respectively. The perfect bonding is modeled for interfaces between the face-sheet and core due to little realistic debonding. The finite element model is verified by available data of conventional SCS. To obtain more design ideas, several stiffeners with different thicknesses, numbers, and positions are investigated. From the predicted results, both the flexural load and deformation of SCS correlate well with experimental results. It is highlighted that the SCSs with different vertical stiffeners exhibit 9.74%–58.48% higher SEA than the SCS without stiffener. The complex reinforcement mechanisms are extensively revealed by underlying coupling EA and deformation mechanisms. Structural parameter analysis shows that the thickness and number have significant effects on the flexural behavior and SEA of reinforced SCS.     

太阳X射线暴在地球大气中传输的Monte Carlo模拟

应用MonteCarlo方法对太阳X射线暴(1-8Å及0.5-4Å)与地球大气相互作用过程进行跟踪模拟,得到了X射线暴在电离层D层产生的电子产生率,并计算了由此产生的宇宙噪声吸收值。结果与作者在南极观测得到的X射线暴期间宇宙噪声吸收值符合较好.