混沌理论在尾桨气动噪声信号分析中的应用

研究剪刀式尾桨气动噪声的混沌特性,并应用混沌理论进行了直升机尾桨气动噪声信号分析。本文通过利用多频调制方法对尾桨噪声进行理论分析,得出相对声压值随剪刀变化的规律;然后将混沌运动的特征参数——关联维数用于剪刀式尾桨气动噪声信号的分析。分析结果表明剪刀式尾桨引起的气动噪声含有混沌特性,同时对比理论和试验结果表明剪刀尾桨构型的参数对气动噪声有明显的影响。     

高精度非接触磁浮机构电磁干扰特性分析

针对因双超平台姿态控制引入非接触磁浮机构这一关键执行机构,而可能引起的卫星平台新的电磁兼容问题,开展了非接触磁浮机构的电磁干扰特性研究。首先,介绍了非接触磁浮机构及其驱动器的工作原理;其次,分别对非接触磁浮机构驱动器的脉冲宽度调制(PWM)控制信号高频干扰特性和传导电磁干扰特性进行了理论和仿真分析,并将其频率特性与星上其他典型单机的工作频率进行了比对。对比分析结果表明:非接触磁浮机构的电磁干扰频率与星上其他典型单机之间间隔较大,其相互之间产生的电磁干扰可忽略,磁浮机构的引入不会产生新的电磁兼容问题。     

Radial distribution of galactic cosmic rays at solar maximum

In this paper we analyze the spatial distribution of galactic cosmic rays during periods of maximum solar activity of the cycles 21, 22 and 23. We have used a two dimensional model to solve the cosmic ray transport equation. This model includes all relevant physical processes: diffusion, convection, drift and shock effects on cosmic ray propagation inside the heliosphere. We focused on the study of the radial distribution of galactic cosmic rays, and compare our results with the spacecraft observations for two energies (175 MeV H and 265 MeV/n He). Although the radial intensities of galactic cosmic rays can be explained qualitatively with all three local interstellar spectra (LISs) used in this work, we applied a reduced chi-squared analysis to investigate the best LIS that could fit the data.     

Change in the rigidity dependence of the galactic cosmic ray modulation in 2008–2009

Observations of charged particle fluxes in the stratosphere of the polar regions represent the cosmic rays variations with energy above 100 MeV. At the end of 2009 these fluxes reached the highest level for the time of observations from mid 1957 and were by 17% higher than the previous extremum value of May 1965. In the mean time the ground-based neutron monitors showed the remarkably less count rate enhancement. These results argue for the significant change in the energy spectrum of incoming particles in 2008–2009 in the energy range of ∼100–1500 MeV/n.     

波音737NG飞机冲压空气系统控制原理及常见故障分析

简要介绍了冲压空气系统的组成和原理，着重分析了系统是如何通过电路设计实现不同的工作模式，以及不同模式下系统各部件的工作状态，最后就系统常见故障和MEL放行进行了简单说明。     

Ka频段低轨遥感卫星可变编码调制应用效能研究

分辨率的不断提高对低轨遥感卫星的星地数据传输能力提升提出了迫切需求,导致X频段星地数传通道压力急剧增加,而Ka频段可用带宽是X频段的4倍,理论上可大幅提升传输能力。当前低轨遥感卫星的星地数据传输通常采用固定编码调制（CCM）和可变编码调制（VCM）,均未利用地面站仰角增大时大气衰减减小所带来的信道条件改善,对链路资源造成浪费。针对此问题,对指定地面站和链路可用度,综合考虑自由空间损耗和大气衰减随接收仰角增加而同时减小的特性,提出基于DVB S2标准的Ka频段星上VCM系统实现方案,给出传输效能评估标准,并对降雨特性不同的喀什站、北京站、三亚站CCM,VCM的Ka频段传输效能进行了对比仿真分析,以寻找出适合不同站点的星地数传方案。仿真结果表明：干旱少雨的喀什站更适合采用CCM,且链路可用度高达99.82%;雨量中等的北京站可根据用户使用需求灵活选择CCM或VCM;而降雨丰富的三亚站更适合采用VCM,不仅可将传输效能提升8.37%,还可将链路可用度提升11.23%。     

基于宽带调制信号的无源互调测试研究

随着收发共用和数字调制技术（如BPSK、QPSK）在卫星通信中大量使用，原有的连续波（continous wave,CW）无源互调（passive intermodulation，PIM）测试系统存在验证不充分的问题。设计了宽带调制信号PIM测试方法改进了原有的测试系统，通过采用通道功率测试PIM，测试研究结果表明BPSK、QPSK数字调制无源互调量值均高于连续载波信号2~9dB，考虑到卫星运行可靠性，采用数字调制宽带工作模式改进原有测试系统后更接近实际工作方式，提高了地面验证可靠性。     

新型机电一体化微磁力矩器设计与实现

现代微小卫星的发展需要磁力矩器具备轻量化、低功耗、小型化、集成化等特点。提出了一种新的微型磁力矩器设计方式,采用机电一体化设计思想,使控制电路内嵌于支架的端面上,实现了磁力矩器结构和驱动电路的集成化和整体结构的小型化,明显优于传统的分离设计方式。采用单绕组线圈+脉冲宽度调制(PWM)换向驱动控制的形式,相比常规的双绕组线圈电流幅度控制形式,线圈的重量和体积都减少了一半,功耗更低,控制更加简便。驱动电路具有电流采样功能,可以实现闭环控制,相对于传统的开环控制策略控制精度更高。此外还对磁力矩器的线圈参数和磁芯参数进行了最优设计。所设计的磁力矩器在某微小卫星上已成功应用,表明了该设计方案的有效性和优越性。     

带LCD复位的正—反激组合式变换器的理论分析与实验验证

正－反激组合式变换器中，两个变压器轮流向负载传递功率，ＬＣＤ缓冲网络实现了功率器件的零电压关断，并且将多余的能量回馈电网，减小了关断损耗，提高了效率，文中详细分析了该变换器的工作原理，列出了各种工作状态下的等值电路和微分方程，给出了各工作状态转换的条件，并绘制了５０Ｗ１００ｋＨｚ实验电路的实验波形，验证了理论分析的正确性。     

Cosmic ray anisotropies in the outer heliosphere

The observation of the directional distribution of energetic and cosmic ray particles has been done with the Voyager spacecraft over a long period. Since 2002, when the first flux enhancements of charged particles associated with the approach of Voyager 1 to the solar wind termination shock were observed, these anisotropy measurements have become of special interest. They play an important role to understand the magnetic field and shock structure and the basics of the modulation of cosmic ray and anomalous particles at and beyond the termination shock. They also serve as motivation to study the spatial behavior of galactic and anomalous cosmic ray anisotropies with numerical modulation models in order to illustrate how the radial anisotropy, at different energies, change from upstream to downstream of the termination shock. Observations made by Voyager 1 indicate that the termination shock is a complicated region than previously thought, hence the effects of the latitude dependence of the termination shock’s compression ratio and injection efficiency on the radial anisotropies of galactic and anomalous protons will be illustrated. We find that the magnitude and direction of the radial anisotropy strongly depends on the position in the heliosphere and the energy of particles. The effect of the TS on the radial anisotropy is to abruptly increase its value in the heliosheath especially in the A > 0 cycle for galactic protons and in both polarity cycles for anomalous protons. Furthermore, the global effect of the latitude dependence of the shock’s compression ratio is to increase the radial anisotropy for galactic protons throughout the heliosphere, while when combined with the latitude dependence of the injection efficiency this increase depends on modulation factors for anomalous protons and can even alter the direction of the radial anisotropy.