基于 MTF的潜航体尾迹 SAR成像仿真

基于水动力学理论和波流弱相互作用理论,运用波作用量谱平衡方程研究了潜航体的尾流场与表面波作用后的表面尾迹,探讨了采用传递变换函数实现表面尾迹SAR成像的可行性。研究表明,波作用量谱平衡方程能够较准确地计算出潜航体尾流场与表面波之间的非线性相互作用;传递变换函数能够快速有效实现海面后向散射系数到SAR图像的转换,且保证了较高的精度。     

空间站柔性太阳电池翼对日跟踪控制

空间站柔性太阳电池翼高稳定对日跟踪驱动控制,对于保障空间站长期在轨能源安全和平稳运行具有重要意义。在推导柔性太阳电池翼动力学模型、柔性体模态分析和截断、Alpha对日定向装置机电系统模型、非线性传动系统模型的基础上,对空间站柔性太阳电池翼对日跟踪控制系统进行设计。采用Heaviside五次样条变速规划、位置和速度两级闭环、速度环陷阱滤波器柔性振动抑制的组合方案,实现空间站柔性太阳电池翼高稳定驱动控制。通过对典型工况的仿真校核,验证所设计的控制方案可实现跟踪精度优于0.3°、速度偏差±0.005(°)/s、稳定度优于7%@0.065(°)/s的性能指标。同时,Alpha对日定向装置的启动和变速过程中驱动力矩不大于30 N·m,稳速运行期间驱动力矩不大于5 N·m。各项性能指标要好于国际空间站Alpha对日定向装置,满足使用要求。     

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。     

卫星测控直扩信号安全性能评价体系研究

为了定量评估直扩信号的安全性能,在给出卫星测控直扩信号安全防护定义的基础上,对卫星测控直扩信号安全性能评价指标进行了研究.在深入分析直扩信号典型威胁的基础上,提出了等效码长、调制指数、码速率截获因数、等效码长截获因数、码序列截获因数、干扰因数等衍生指标,分析、仿真了它们的影响因素,得到了它们与基本指标的关系,初步建立了直扩信号安全性能评价体系,为后续安全性能评估打下基础.     

On-orbit verification of fuel-free attitude control system for spinning solar sail utilizing solar radiation pressure

This paper introduces a new attitude control system for a solar sail, which leverages solar radiation pressure. This novel system achieves completely fuel-free and oscillation-free attitude control of a flexible spinning solar sail. This system consists of thin-film-type devices that electrically control their optical parameters such as reflectivity to generate an imbalance in the solar radiation pressure applied to the edge of the sail. By using these devices, minute and continuous control torque can be applied to the sail to realize very stable and fuel-free attitude control of the large and flexible membrane. The control system was implemented as an optional attitude control system for small solar power sail demonstrator named IKAROS (Interplanetary Kite-craft Accelerated by Radiation Of the Sun). In-orbit attitude control experiments were conducted, and the performance of the controller was successfully verified in comparison with the ground-based analytical performance estimation.     

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%。     

Towards Synthesis of Solar Wind and Geomagnetic Scaling Exponents: A Fractional Lévy Motion Model

Mandelbrot introduced the concept of fractals to describe the non-Euclidean shape of many aspects of the natural world. In the time series context, he proposed the use of fractional Brownian motion (fBm) to model non-negligible temporal persistence, the ‘Joseph Effect’; and Lévy flights to quantify large discontinuities, the ‘Noah Effect’. In space physics, both effects are manifested in the intermittency and long-range correlation which are by now well-established features of geomagnetic indices and their solar wind drivers. In order to capture and quantify the Noah and Joseph effects in one compact model, we propose the application of the ‘bridging’ fractional Lévy motion (fLm) to space physics. We perform an initial evaluation of some previous scaling results in this paradigm, and show how fLm can model the previously observed exponents. We suggest some new directions for the future.