Study of the radiation fields in LEO with the Space Application of Timepix Radiation Monitor (SATRAM)

We present the analysis of data taken by the Space Application of Timepix Radiation Monitor (SATRAM). It is centred on a Timepix detector (300?$\mathrm{\mu }$m thick silicon sensor, pixel pitch 55?$\mathrm{\mu }$m, 256?×?256 pixels). It was flown on Proba-V, an Earth observing satellite of the European Space Agency (ESA) from an altitude of 820?km on a sun-synchronous orbit, launched on May 7, 2013. A Monte Carlo simulation was conducted to determine the detector response to electrons (0.5–7?MeV) and protons (10–400?MeV) in an omnidirectional field taking into account the shielding of the detector housing and the satellite. With the help of the simulation, a strategy was developed to separate electrons, protons and ions in the data. The measured dose rate and stopping power distribution are presented as well as SATRAM’s capability to measure some of the stronger events in Earth’s magnetosphere. The stopping power, the cluster height and the shape of the particle tracks in the sensor were used to separate electrons, protons and ions. The results are presented as well. Finally, the pitch angles for a short period of time were extracted from the data and corrected with the angular response determined by the simulation.     

多约束条件下月球南极探测返回窗口设计

针对月球南极探测任务,综合考虑中国地基深空测控系统现状、月球南极地区光照及地球再入终端等约束条件,利用月球反垂点概念,提出一种从环月轨道出发的三级返回窗口搜索策略.其次,提出一种改进多圆锥截线法,将月球非球形摄动加入到区间的轨道外推中,基于二级返回窗口对返回轨道进行了初步设计.给出以月球南极地区Shackleton撞击坑边缘一点为假定落点,于2020年自月球南极地区返回的仿真算例.仿真结果表明：一方面,窗口搜索方法可以有效解决多约束条件下的月球南极返回窗口设计问题;另一方面,改进多圆锥截线法作为一种初始轨道设计方法,可以有效减少再入误差,同时为后续高精度轨道积分提供良好初值.     

Effects of dust polarity and nonextensive electrons on the dust-ion acoustic solitons and double layers in earth atmosphere

Propagation of dustion acoustic solitary waves (DIASWs) and double layers is discussed in earth atmosphere, using the Sagdeev potential method. The best model for distribution function of electrons in earth atmosphere is found by fitting available data on different distribution functions. The nonextensive function with parameter $q=0.58$ provides the best fit on observations. Thus we analyze the propagation of localized waves in an unmagnetized plasma containing nonextensive electrons, inertial ions, and negatively/positively charged stationary dust. It is found that both compressive and rarefactive solitons as well as double layers exist depending on the sign (and the value) of dust polarity. Characters of propagated waves are described using the presented model.     

空间粒子辐射对卫星中集成芯片的影响

本文分析了在“风云一号(B)”气象卫星环境中各种粒子辐射在集成芯片临界体积中产生的能量沉积, 即LET(线性能量传输);得到了银河宇宙线1≤Z≤28、银河宇宙线异常成分(C、N、O、Ne、Ar、Fe)、内辐射带质子等产生的LET, 计算了其分别产生的单粒于事件(SEU)翻转率。      

陆地卫星地面接收站微波系统扩充方案

讨论了为接收Landsat-6而扩充的陆地卫星地面接收站微波系统方案。该工作完成后,不仅能实现对Landsat-5、Landsat-6、SPOT 卫星的兼容,而且配上相应的解调器也能接收ERS-1、JERS-1及中国即将发射的资源卫星及其它工作在8025～8400MHz 的任何卫星的发射数据。     

航天器天线有关技术的论述

论述了航天器天线的特点及其与航天器总体的关系;天线的辐射场方向图及增益有关问题;天线的电磁兼容及天线的计算机辅助设计。     

旋转体源声辐射的近场分析

详细讨论了旋转运动声源的近声场频域解。所得近场解析式表现为远场解基础上的近场修正。范例计算显示出这种修正的特点, 并表明源的旋转半径和轴向偏移对声场影响的性质。风扇实验初步证明了文中分析。      

资源卫星CCD多光谱扫描仪系统的像质评价

综述了资源卫星ＣＣＤ多光谱扫描仪系统像质评价的重要性。内容和影响像质的主要因素;还综述了ＳＰＯＴ和ＴＭ使用的评价准则、评价方法以及卫星发射前的图像质量预估和在卫星发射后的像质评估结果。     

Flower卫星星座设计方法研究

介绍了一种具有共地面轨迹和良好相位特性的新颖的Flower卫星星座设计方法。与常见的星座设计方法不同,在地球中心固定坐标系中可以更好的体现Flower星座的特点。通过Flower星座模型参数与星座中卫星轨道参数之间的关系式,实现了Flower星座的研究设计软件SatSim。结合Satellite Tool Kit仿真软件,给出了利用Flower星座设计一个能为GEO卫星进行导航的卫星导航系统实例,探讨了将Flower星座广泛应用于更多卫星星座系统设计的可能。     

激光与空气作用过程中辐射能量损失的研究

激光与空气相互过程中,与辐射相关的各种过程起着特别重要的作用。研究了高温气体辐射对气体流体力学过程的影响。辐射能量密度和压力对气体状态和运动的影响完全可以忽略不计,而流场的辐射能量损失不能忽略。利用光线追踪法,运用辐射输运方程,根据光线在网格中的传播路径,计算空气吸收的激光能量;根据网格厚度,确定辐射能量损失。数值求解含能量源项的流体控制方程,对激光击穿空气的等离子流场演化过程进行了模拟,得到了辐射能量损失随入射激光能量的变化规律。