飞行体的海空背景反射与辐射计算

研究了对近海飞行体的红外特性有重要影响的海空背景辐射的反射特性.讨论了波浪面起伏随机规律,随机起伏对海面自身辐射及对阳光反射的影响,推演了此种随机起伏波浪面的自身辐射及反射的阳光在观测点形成的辐照度的计算方法.给出的算例结果表明,海空背景对飞行体的红外特性尤其对其前半球的红外特性有重要的意义.     

地磁场的长期变化对辐射带质子通量计算的影响

用不同年代的国际地磁参考场(IGR)模式及最新的辐射带粒子通量模式,计算了低高度上空间某点的辐射带质子通量随时间的变化,讨论了地磁场的长期变化对L-B坐标及辐射带带电粒子通量计算的影响,对正确使用地磁场模式计算磁壳参量L及辐射带粒子通量模式给予了说明和建议.      

电子束固化技术及在复合材料制造领域的应用

对辐射固化与光固化进行了比较,阐述了电子束辐射固化的基本过程,并对电子束固化复合材料的技术特点进行了概述.此外,还详细总结了电子束固化复合材料技术的发展状况,包括可电子束固化的树脂体系,辐敏剂以及活性稀释剂的选择和应用,固化机理的研究等.最后,还对复合材料的低能电子束固化技术以及新型树脂体系的探索进行了总结.     

中段弹道目标的温度场与红外辐射特性计算

红外辐射特性是预警系统探测识别弹道中段目标的重要特征之一。通过计算飞行时目标与太阳、地球的相对位置,确定目标的受外辐射照射状态。利用有限容积法计算锥形目标的三维温度场,采用双向反射分布函数（BRDF）计算目标表面对太阳、地球辐射的反射特性,并结合自身红外辐射,得到了不同类型中段目标红外辐射特性变化情况和空间分布情况。最后,分析了外部辐射环境和目标材料特性对目标红外辐射特性的影响,为中段预警探测提供了参考。     

一种空间用抗原子氧复合膜β布的原子氧、温度、紫外辐射效应的试验研究

在原子氧剥蚀效应地面模拟设备中对一种抗原子氧复合材料β布进行了原子氧剥蚀效应试验、试样湿度升高对原子氧效应的影响试验以原子氧与紫外辐射复合效应试验研究，对试验前后β布试样的质量及表面形貌进行了比较，得出了在材料在设备中的反应特点以及温度变化、紫外辐射对材料的原子氧效应的影响规律。另外对这种材料与原子氧的反应机理进行了分析，得出了一些有意义的结论。     

复杂边界条件下的多层多孔壁温度场的计算模型

经过推导给出了具有孔内和内外表面对流换热及外表面热辐射复杂边界条件下的多层多孔壁温度场的计算模型,并以具有陶瓷隔热涂层的全气膜覆盖气冷叶片为例进行了温度场计算。计算结果表明：陶瓷涂层具有明显的隔热效果,并可明显地减小冷却空气用量;燃气温度对壁温影响较大;考虑热辐射将更加符合实际物理过程;对于涡轮叶片若不考虑热辐射将低估壁温 1. ５％ ～3. ５％ 。该模型可用于多层多孔壁冷却结构形式的发动机高温部件的优化设计。     

高稳晶振在空间辐照条件下的频率特性变化

在空间恶劣环境下要求星载高稳晶振正常有效地工作,需要对其在空间辐照环境下的频率特性变化进行研究,利用地面辐照设备模拟空间辐照环境,通过不断增加辐照剂量,研究晶振相位噪声、短期频率稳定度、谐杂波以及输出功率等特性。     

Simulations of MATROSHKA experiment outside the ISS using PHITS

The radiation environment at the altitude of the International Space Station (ISS) is substantially different than anything typically encountered on Earth in both the character of the radiation field and the significantly higher dose rates. Concerns about the biological effects on humans of this highly complex natural radiation field are increasing due to higher amount of astronauts performing long-duration missions onboard the ISS and especially if looking into planned future manned missions to Mars. In order to begin the process of predicting the dose levels seen by the organs of an astronaut, being the prerequisite for radiation risk calculations, it is necessary to understand the character of the radiation environment both in- and outside of the ISS as well as the relevant contributions from the radiation field to the organ doses.     

Analysis of the space radiation doses obtained simultaneously at two different locations outside the ISS

Space weather and related ionizing radiation has been recognized as one of the main health concerns for the International Space Station (ISS) crew. The estimation of the radiation effect on humans outside the ISS requires at first order accurate knowledge of their accumulated absorbed dose rates, which depend on the global space radiation distribution, solar cycle and local variations generated by the 3D mass distribution surrounding the ISS. The R3DE (Radiation Risks Radiometer-Dosimeter for the EXPOSE-E platform) on the European Technological Exposure Facility (EuTEF) worked successfully outside of the European Columbus module between February 2008 and September 2009. A very similar instrument named R3DR for the EXPOSE-R platform worked outside the Russian Zvezda module of the ISS between March 2009 and August 2010. Both are Liulin-type detectors, Bulgarian-built miniature spectrometer-dosimeters. The acquired approximately 5 million deposited energy spectra from which the flux and absorbed dose rate were calculated with 10 s resolution behind less than 0.41 g cm⁻² shielding. This paper analyses the spectra collected in 2009 by the R3DE/R instruments and the long-term variations in the different radiation environments of Galactic Cosmic Rays (GCR), inner radiation belt trapped protons in the region of the South Atlantic Anomaly (SAA) and relativistic electrons from the Outer Radiation Belt (ORB). The R3DE instrument, heavily shielded by the surrounding structures, measured smaller primary fluxes and dose rates from energetic protons from the SAA and relativistic electrons from the ORB but higher values from GCRs because of the contribution from secondary particles. The main conclusion from this investigation is that the dose rates from different radiation sources around the International Space Station (ISS) have a large special and temporal dynamic range. The collected data can be interpreted as possible doses obtained by the cosmonauts and astronauts during Extra Vehicular Activities (EVA) because the R3DE/R instruments shielding is very similar to the Russian and American space suits average shielding (,  and ). Fast, active measurements are required to assess accurately the dose accumulated by astronauts during EVA.     

导航卫星高精度太阳光压摄动分析建模及验证

为提高导航卫星精密定轨与轨道预报精度,提出了一种导航卫星太阳光压摄动的分析建模方法.相较于其他摄动因素模型完善且精度较高,光压摄动由于太阳活动导致太阳能量误差、卫星姿态控制误差和表面材料老化等问题,是最难以精确建模的摄动源,也是动力学模型最大的误差源.基于此,提出了一种基于卫星的姿态控制规律,通过分析法建立卫星太阳光压摄动模型,给出了光压摄动加速度在星体坐标系中的模型,并以GPSBlock IIR为例进行了验证.计算结果表明,该仿真分析法所建立的摄动模型与T30模型、ECOM模型精度接近,达到了光压建模研究的初步计算要求.