动磁式线性电机理论研究与测试技术

本文以昆明物理研究所的SC100H线性斯特林制冷机为研究对象,对该制冷机采用的动磁式线性振荡电机磁路特性进行了理论与实验研究。建立了电机理论模型,对模型进行了结构简化以便于分析计算,利用等效磁路法和机电能量转换原理,分析电机推力特性与动子相对位置等的关系,利用拉力测试系统对电机在不同输入电流的推力特性进行了测试,测试结果与理论值很好的吻合,从而为电机结构参数和运行参数的设计优化提供了设计参考与依据。     

Sandwich module prototype progress for space solar power

Space solar power (SSP) has been broadly defined as the collection of solar energy in space and its wireless transmission for use on earth. This approach potentially gives the benefit of provision of baseload power while avoiding the losses due to the day/night cycle and tropospheric effects that are associated with terrestrial solar power. Proponents have contended that the implementation of such systems could offer energy security, environmental, and technological advantages to those who would undertake their development. Among recent implementations commonly proposed for SSP, the modular symmetrical concentrator (MSC) and other modular concepts have received considerable attention. Each employs an array of modules for performing conversion of concentrated sunlight into microwaves or laser beams for transmission to earth. While prototypes of such modules have been designed and developed previously by several groups, none have been subjected to the challenging conditions inherent to the space environment and the possible solar concentration levels in which an array of modules might be required to operate. The research described herein details our team's efforts in the development of photovoltaic arrays, power electronics, microwave conversion electronics, and antennas for microwave-based “sandwich” module prototypes. The implementation status and testing results of the prototypes are reviewed.     

示波器输入电容对上限截止频率测量的影响

单管放大电路是模拟电路中的一个经典实验。通过这个实验,学生可以更好地掌握静态工作点的调整和测试方法,并通过测量放大电路的主要性能指标,体会静态工作点对动态特性的影响。实验电路的上限截止频率仿真值和实测值存在较大差异,本文针对这个问题进行了详细的分析,指出示波器的输入电容是引起差异的主要原因,并进一步讨论了可有的改进测试...     

非稳定动态过程非定常气动力建模

现有的大迎角非定常气动力建模方法，通常是以一个或多个频率的稳定振动试验数据来预测稳定滞环。然而，飞机快速机动如过失速机动的过程，不可能是持续的稳定振动，而是一个非稳定的动态过程。因此，这个过程中的气动力不会达到稳定滞环，而是始终处于进入滞环的初始非稳定过程中。基于振动理论分析得出，非定常气动力的动态响应过程存在非稳定和稳定两个阶段，传统建模方法着眼于稳定阶段，而飞机的真实机动过程在非稳定阶段。设计了一种适于非线性系统辨识的激励输入，并以最小二乘支持向量机（LS-SVM）方法为例，实现了在大迎角区幅值和频率范围内任意运动的非定常气动力建模。模型训练完成后，用来预测某机翼在不同基准状态下大迎角范围内做俯仰运动时的升力系数、阻力系数和俯仰力矩系数。结果表明，不仅稳定滞环实现了准确预测，进入滞环的初始非稳定过程也得到了准确预测；此外，基准状态对气动力在初始非稳定过程中的特性存在明显影响。进一步的验证还表明，基于稳定滞环数据只能预测到稳定滞环，无法预测进入滞环的非稳定过程。     

利用质子强度变化对太阳质子事件进行短期预报方法初步研究

采用GOSE-10卫星4～9 MeV(P2),9～15 MeV(P3),15～40 MeV(P4),40～80 MeV(P5)能段上的质子通量数据,结合质子能谱,对太阳质子事件发生前各能谱参数的变化特征进行分析,详细介绍利用能谱参数的变化特征及能量E>10 MeV的质子通量数据对太阳质子事件进行预报的新方法,并运用这种方法对2002-2006年期间太阳质子事件进行了预报.预报结果显示,预报提前量最多达到100 h以上,对质子事件的报准率达97.5%,预报方法具备一定的有效性和实用性.      

采用变速控制力矩陀螺的一种姿态/能量一体化控制研究

本文研究采用变速控制力矩陀螺（VSCMG）的航天器姿态／能量一体化控制技术。首先建立了以变速控制力矩陀螺为执行机构的航天器姿态动力学模型，并给出了全局稳定的姿态反馈控制律。以控制力矩陀螺群的构型奇异量度为依据，分别考虑了VSCMG的控制力矩陀螺（CMG）工作模式和反作用飞轮（RW）工作模式。在陀螺群接近奇异时启用转子的反作用飞轮工作模式来补偿控制力矩陀螺采用鲁棒伪逆操纵律时所引起的力矩误差；在陀螺群远离奇异状态时，用控制力矩陀螺来补偿转子储能带来的干扰力矩。在姿态控制的同时利用转子的变速特性，完成按照给定的功率存储／释放能量，并在陀螺群远离奇异状态时对储能过程中转子的转速进行调节，以保持良好地动量包络外形。最后以某航天器的姿态控制为例，给出了数值仿真结果。     

一种基于NOMA的Q学习卫星通信随机接入方法

基于非正交多址接入(NOMA)的Q学习(Q-Learning)随机接入方法(NORA-QL)是实现物联网中海量设备泛在接入的一项有效技术.为了解决NORA-QL方法仍存在的传输能效和过载容量较低的问题,提出了一种适合卫星通信网络的改进方法(I-NORA-QL).针对传输功耗高的问题,I-NORA-QL利用卫星广播的全局...     

运载火箭故障模式及制导自适应技术应用分析

为提高制导控制系统在运载火箭全发射任务周期中的智慧水平，提高运载火箭完成任务的鲁棒能力，从不同角度阐述了运载火箭故障模式，创新提出了基于能量属性的故障分类方法。针对不同级别的能量故障提出了对制导控制系统的功能、性能需求。尤其针对小、中级别能量故障，简述了运载火箭故障飞行制导自适应方法应用，包含案例及任务目标变更原则等，并分析了制导自适应技术后续工程化应用的实施途径。基于能量属性的故障分类方法及制导自适应方法可应用于后续中国运载火箭工程研制。     

Drag and energy accommodation coefficients during sunspot maximum

Conditions appropriate to gas-surface interactions on satellite surfaces in orbit have not been successfully duplicated in the laboratory. However, measurements by pressure gauges and mass spectrometers in orbit have revealed enough of the basic physical chemistry that realistic theoretical models of the gas-surface interaction can now be used to calculate physical drag coefficients. The dependence of these drag coefficients on conditions in space can be inferred by comparing the physical drag coefficient of a satellite with a drag coefficient fitted to its observed orbital decay. This study takes advantage of recent data on spheres and attitude stabilized satellites to compare physical drag coefficients with the histories of the orbital decay of several satellites during the recent sunspot maximum. The orbital decay was obtained by fitting, in a least squares sense, the semi-major axis decay inferred from the historical two-line elements acquired by the US Space Surveillance Network. All the principal orbital perturbations were included, namely geopotential harmonics up to the 16th degree and order, third body attraction of the Moon and the Sun, direct solar radiation pressure (with eclipses), and aerodynamic drag, using the Jacchia-Bowman 2006 (JB2006) model to describe the atmospheric density. After adjusting for density model bias, a comparison of the fitted drag coefficient with the physical drag coefficient has yielded values for the energy accommodation coefficient as well as for the physical drag coefficient as a function of altitude during solar maximum conditions. The results are consistent with the altitude and solar cycle variation of atomic oxygen, which is known to be adsorbed on satellite surfaces, affecting both the energy accommodation and angular distribution of the reemitted molecules.     

基于快速极坐标格式算法的MIMO雷达虚拟孔径成像

针对共址多输入多输出（Multiple Input Multiple Output,MIMO）雷达在单次快拍下的虚拟孔径成像问题,分析了MIMO雷达虚拟合成阵列,建立了MIMO雷达极坐标格式波数域回波模型,分析了基于距离向和方位向尺度变换的空间谱转化,指出MIMO雷达方位向尺度变换不再是Keystone变换,提出了一种新的MIMO雷达快速极坐标格式成像算法。仿真表明了该文方法的有效性。