Comptonization of low-frequency radiation in accretion disks: Angular distribution and polarization of hard X-ray radiation

We present the results of computation for angular distribution and polarization of radiation for the set of the disk Thomson optical depth values.     

Whole-process modeling of titanium disc forming for gradient distributions of temperature and deformation

Gradient distributions of temperature and deformation (GDTD) are crucial for achieving dual-performance discs of titanium alloys which is required by the service environment of aeroengine. However, heating, cooling and deforming sequence in the whole process of the titanium disc forming, which leads to difficulties for achieving GDTD due to a lot of parameters. To solve this problem, a whole-process model of the titanium disc forming for GDTD has been established. In the model, heating and cooling via heat radiation, conduction and convection, and deforming by local loading with mold chilling are all considered. Experiments on heating and cooling as well as deforming were carried out by using a furnace and the Gleeble-3500 machine. The experimental data are used to determine thermal parameters and constitutive relations of the IMI834 titanium alloy, and then to verify the reliability of the model. Then the model was used to simulate the evolution rules of temperature and deformation of the titanium disc. The results show that the heating surface, furnace temperature, billet profile and loading rate play the core role for the control of GDTD, and thus a set of parameters were determined. Therefore, this work provides a base for developing a new forming technology of the dual-performance titanium discs with the approach of local heating and local loading.     

A Novel Magnetic Configuration for Space Radiation Active Shielding

Space radiation has been identified as the main health hazard to crews involved in manned Mars missions. Active shielding is more effective than passive shielding to the very energetic particles from cosmic rays. Particle motion in a magnetic field is studied based on the single-particle theory and Monte Carlo method. By comparing the shielding efficiency of different magnetic field configurations, a novel active magnetic shielding configuration with lower mass cost and power consumption is proposed for manned Mars missions. The new magnetic configuration can shield 92.8% of protons and 84.4% of alpha particles with E < 4 GeV·n-1, when considering the passive shielding contribution of 10.0 g·cm-2 Al Shielding, the required magnetic stiffness can be reduced from 27 Tm to 16 Tm. The detailed analysis of mass cost and power consumption shows that active shielding will be a promising means to protect crews from space radiation exposure in manned Mars missions.      

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。      

太阳微波射电快速精细结构亚类型的观测分析

通过分析"云南天文台4波段太阳射电快速同步观测系统"1990-01-1994－01取得的103个射电爆发,发现其中29个存在不同类型的快速精细结构（FFS）.尤其是发现了几个少见的亚类FFS现象.本文仅介绍两个亚类型:窄带变周期脉动和宽带慢漂移长周期脉动.这些现象表明太阳射电FFS的多样性,它们发生在射电爆发的不同阶段（耀斑不同相）,从而说明在耀斑演化中日冕非热电子的加速或注入可能贯穿于整个耀斑发展过程.由于耀斑后相FFS的发生,可验证耀斑后相存在磁重联和似环结构（耀斑后环）的重新形成.由于不同的亚类FFS反映日冕中存奇特别的环境条件,从而推测日冕中可能存在更复杂的多重类型的磁结构.      

辐射换热系统温度场的渐近特性研究

本文讨论辐射换热系统温度场的渐近特性,该问题与具有周期热源的人造卫星热模拟试验紧密相关。本文工作使文献[1,2]阐述的行之有效的方法得到进一步完善。     

γ射线辐射对空间光学玻璃透射率的影响

利用60Co γ-射线对钡冕玻璃（BaK3）、镧冕玻璃（LaK3）、火石玻璃（F10）、镧火石玻璃（LaF3）、轻火石玻璃（QF3）和重火石玻璃（ZF4）进行辐照,研究不同辐照剂量对光学透射率的影响及这些玻璃在空间光学系统中的适应性。光学透射率测试范围为400~1 100 nm。结果表明所有玻璃在辐照后可见光透射率都下降了,而在近红外波段下降不明显（除了QF3和LaF3）。尽管F10和QF3光学透射率在辐照前相似,但是辐照后F10衰减是所有玻璃中最小的,而QF3衰减最为严重。研究发现,当达到一定辐照剂量后,玻璃材料的透射率不再继续衰减,而是趋于稳定。这些结果为空间光学系统针对辐射进行冗余设计提供了依据。     

环氧基纳米复合材料抗真空紫外辐照性能研究

文章模拟真空紫外辐照条件,研究波长5~200 nm的真空紫外线(VUV)对环氧树脂648以及环氧基纳米复合材料的辐照损伤效应.质量损失、扫描电子显微镜、质谱仪和X射线光电子谱仪分析结果表明:纳米TiO2起到明显抗真空紫外辐照的作用.辐照后,与环氧树脂相比,环氧基纳米复合材料的质量损失大幅度降低,弯曲强度变化较小,出气量和出气成分减少,表面没有新的C峰出现,表面O 1s峰的主要成分没有发生变化.     

弹头包络球在红外突防中的应用研究

介绍了一种弹道导弹中段红外突防弹头包络球法,简要介绍了弹头包络球的构造,定量分析了弹头包络球和空包络球在中段飞行时各表面温度的变化,得到由于包络球采用了镀金属的绝热材料,很好地实现了弹头的辐射遮蔽,真假包络球表面温度基本相同.     

航空有机玻璃紫外光老化研究

对YB—DM-11航空有机玻璃试样在254nm和313nm两种波长的紫外光照射下,进行了2个月的加速老化试验,跟踪测试了有机玻璃的抗拉强度和重量变化规律。通过红外光谱（FTIR）、热分析（TG／DTA）、扫描电镜（SEM）和凝胶渗透色谱（GPC）等方法,分析了老化前后试样的结构和性能,结合老化前后有机玻璃的性能变化规律,揭示了有机玻璃在紫外光照射下的老化机理。