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。     

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.     

铝-铝超高速碰撞闪光现象的初步实验测量

 为了研究不同碰撞参数条件下超高速碰撞闪光的特点及闪光温度的变化规律,构建了高温计及附属实验测量系统平台,利用该平台进行了超高速碰撞闪光的初步测量。根据Planck辐射的基本理论,对每次实验的碰撞闪光强度进行了4种波长的采集并对温度进行了拟合计算,得到了碰撞闪光温度历史。实验结果表明：对于弹丸、靶板材料均为LY12铝而言,碰撞角度（与靶板平面夹角）相同、碰撞速度在5.35~5.97 km/s范围内时,碰撞速度对碰撞闪光温度影响不明显;然而,碰撞速度相近,碰撞角度越大,碰撞闪光温度越高。     

黑体辐射源的发展

黑体辐射源作为辐射测温仪器的校准装置,近几十年来随着红外测温技术的发展而取得了飞速进步。本文从黑体辐射源的发展历史、研究内容、发展方向和目前存在的问题几方面作了介绍。     

Solar particle dynamics during magnetic storms of July 23–27, 2004

It is a case study of a chain of three magnetic storms with a special attention to the particle dynamics based on CORONAS-F and SERVIS-1 low altitude satellite measurements. Solar proton penetration inside the polar cap and inner magnetosphere and dynamics at different phases of the magnetic storms was studied. We found, that solar protons were captured to the inner radiation belt at the recovery phase of the first and the second magnetic storms and additionally accelerated during the last one. No evidence of sudden commencement (SC) particle injection was found. Enhanced solar proton belt intensity with small pitch angles decreased slowly during satellite orbits for 30 days until the next magnetic storm. Then in 20–30 h we registered strong precipitation of these protons followed by the trapped proton flux dropout. Intensity decrease was more pronounced at lower altitudes and higher particle energies.     

Global dynamics of high area-to-mass ratios GEO space debris by means of the MEGNO indicator

In this paper we provide an extensive analysis of the global dynamics of high-area-to-mass ratios geosynchronous (GEO) space debris, applying a recent technique developed by Cincotta and Simó [Cincotta, P.M., Simó, C.Simple tools to study global dynamics in non-axisymmetric galactic potentials–I. Astron. Astrophys. (147), 205–228, 2000.], Mean Exponential Growth factor of Nearby Orbits (MEGNO), which provides an efficient tool to investigate both regular and chaotic components of the phase space.