Estimation of Galactic Cosmic Ray exposure inside and outside the Earth’s magnetosphere during the recent solar minimum between solar cycles 23 and 24

The evidently low solar activity observed between solar cycles 23 and 24 during the years 2008–2010 led to a substantial increase in the Galactic Cosmic Ray (GCR) intensity in comparison with preceding solar minima. As the GCRs consist of highly-ionizing charged particles having the potential to cause biological damage, they are a subject of concern for manned missions to space. With the enhanced particle fluxes observed between 2008 and 2010, it is reasonable to assume that the radiation exposure from GCR must have also increased to unusually high levels. In this paper, the GCR exposure outside and inside the Earth’s magnetosphere is numerically calculated for time periods starting from 1970 to the end of 2011 in order to investigate the increase in dose levels during the years 2008–2010 in comparison with the last three solar minima. The dose rates were calculated in a water sphere, used as a surrogate for the human body, either unshielded or surrounded by aluminium shielding of 0.3, 10 or 40 g/cm².     

A space radiation shielding model of the Martian radiation environment experiment (MARIE)

The 2001 Mars Odyssey spacecraft was launched towards Mars on April 7, 2001. Onboard the spacecraft is the Martian radiation environment experiment (MARIE), which is designed to measure the background radiation environment due to galactic cosmic rays (GCR) and solar protons in the 20–500 MeV/n energy range. We present an approach for developing a space radiation-shielding model of the spacecraft that includes the MARIE instrument in the current mapping phase orientation. A discussion is presented describing the development and methodology used to construct the shielding model. For a given GCR model environment, using the current MARIE shielding model and the high-energy particle transport codes, dose rate values are compared with MARIE measurements during the early mapping phase in Mars orbit. The results show good agreement between the model calculations and the MARIE measurements as presented for the March 2002 dataset.     

旋转形导体上任意取向线天线辐射场的探讨

对任意旋转平滑形导体上任意取向的线天线所辐射的扬进行探讨。采用了矩量法和傅里叶分析法,给出了导体感应电流谐量表示式,由此可求辐射场。进而以球体上任意取向赫芝振子为例求出辐射场,并与经典法公式计算结果比较,两者一致。     

环绕式微带共形天线辐射特性的研究

基于腔模理论和等效原理推导出环绕式微带共形天线远区场的表达式。根据该表达式算得的TM_(01)模天线方向图在相对介电常数较小时与文献〔3〕的结果相吻合。同时还研完了圆柱半径对天线方向图的影响。     

基于Space radiation 5.0软件平台分析典型GEO空间辐射环境

文章介绍了兰州空间技术物理研究所真空低温技术与物理国家重点实验室从美国引进的空间辐射环境及效应分析软件Space Radiation 5.0的结构功能模块,采用该软件计算分析了典型的GEO（地球同步轨道）空间辐射环境。计算表明:GEO的总剂量效应比较严重,主要是由捕获电子和太阳耀斑质子辐射引起的;GEO的带电粒子主要由质子、α粒子、碳离子、氮离子、氧离子等重核离子组成,此轨道上的单粒子效应主要由太阳宇宙射线中的高能质子和重离子以及银河宇宙射线的重离子引发。     

等离子体环境下圆柱开槽天线特性的研究

本文用磁流体力学的方法研究了等离子体环境下圆柱体开槽天线的辐射问题,推导了槽天线的方向图和阻抗的计算公式,计算了不同等离子体参量的横槽的方向图,并且把计算的结果与用不考虑纵波影响的复介电常数方法得到的结果进行了比较。     

等离子体天线的原理及特性

根据等离子体柱天线的系统构成,分析了等离子体柱天线的基本工作原理,讨论了表面波在等离子体柱天线中的传播特性、等离子体柱内的电子分布,以及天线的长度、噪声与辐射特性。分析表明：表面波能激发和维持等离子体柱,等离子体柱可构成等离子体天线,且具易隐身、可控性等优点。     

宇航抗辐射加固集成电路技术发展与思考

宇航抗辐射加固集成电路是航天工程的核心基础技术。长期以来,美欧等国家对抗辐射加固集成电路持续支持并严格禁运,宇航集成电路的发展和自主可控是我国向航天强国迈进的关键核心基础之一,受到国家的高度重视。本文总结了宇航抗辐射加固集成电路发展特点和我国发展现状,分析了未来宇航抗辐射加固集成电路的发展需求,探讨了未来需要重点关注的3个技术方向,即软加固的天算芯片、高压功率器件加固和单粒子效应仿真。     

辐射器展开角度对航天器热控能力影响的研究

为了在有限的结构尺寸下提高航天器热控系统的散热能力,提出与流体回路耦合的可展开式辐射器热控方案,建立可展开式辐射器空间散热模型,分析辐射器不同展开角度下系统的热控特性。结果表明,随着辐射器展开角度的变化,辐射器吸收的空间热流也随之发生变化,并最终决定热控回路的流量分配。在工程应用中,基于热控流体回路,通过调节可展开式辐射器的展开角度,可以有效提高航天器热控系统的能力范围。     

火焰筒内燃气辐射的蒙特卡罗法计算

用概率统计方法计算了航空发动机燃烧室火焰筒内燃气对壁面的辐射热流, 计算中考虑了燃气的辐射及吸收特性。该计算程序适用于二维轴对称的环型燃烧室和单管燃烧室辐射热流的计算, 并对计算结果进行误差分析。介绍了算例计算结果, 为了检验该计算程序的可靠性, 对角系数进行了校核计算, 其结果是令人满意的。此外, 文中还介绍了对某环型燃烧室和一假想单管燃烧室的计算及误差分析结果。