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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. 相似文献
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I. Büsching M.S. Potgieter 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
The discovery of direct evidences for the acceleration of high energetic particles at the shell supernova remnant RXJ1713.7-3946 underlined the need to calculate the cosmic ray (CR) distribution in the Galaxy on a spatial grid fine enough to resolve the changes in the CR density due to these kind of objects. It was shown before by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005] that the discrete nature (both in space and time) of super novae (SN) as sources of Galactic CR leads to CR spectra changing in space and time, resulting in a range of possible CR spectra at a given location in the Galaxy. As the most frequent SN types Ib and II are found within spiral arms, one can expect a significant difference of the range of possible spectra in and outside spiral arms. We investigate the variability of the local interstellar CR proton spectrum during the motion of the Sun in and out of spiral arms in its journey around the Galactic center. Using the code described by Büsching et al. [Büsching, I., Kopp, A., Pohl, M., Schlickeiser, R., Perrot, C., Grenier, I. Cosmic-ray propagation properties for an origin in supernova remnants. ApJ 619, 314–326, 2005], the proton CR density in the Galaxy is calculated with high spatial and temporal resolution (75 pc in galactocentric radius r and azimuth φ at the position of the Sun and 20 pc in z (perpendicular to the galactic plane), with a time step of 1 kyr), assuming stochastically distributed point sources with a probability distribution that resembles the spiral structure of our Galaxy. We find the averaged CR flux outside the spiral arm to be about 50% of that inside a spiral arm. We further find spatial and temporal variations of the CR flux inside spiral arms. 相似文献
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李书玉!新疆库尔勒信箱库尔勒 《遥测遥控》2001,(3)
介绍一种新研制的超小型信标机 ,该机采用锁相环技术 ,输出信号质量高。信标机安装在氢气球悬挂的金属铝球内 ,可综合检验同一场区内的引导雷达、脉冲雷达、遥测跟踪站等设备的动态跟踪性能 ,实现测控系统的动态联调和合练。 相似文献
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方旭东%杨鸿昌%安章荣 《宇航材料工艺》2002,32(2):35-37
对碳纤维/钛超混杂复合材料CTIL-1在高温高湿的条件下进行加速老化试验,为了便于分析比较,同时列出了T300/648在相同老化条件下的拉伸、弯曲和层剪性能。在加速老化180d后,CTIL-1的拉伸、弯曲性能的保留率均在80%以上,层剪强度保留率也在60%以上,表明该材料有较好的老化性能。 相似文献
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固体火箭发动机绝热层脱粘的红外热像检测规律 总被引:1,自引:1,他引:0
闪光灯激励的红外热像检测法是一种非接触式的光学无损检测技术,有望应用于固体火箭发动机绝热层脱粘的在线检测。为了推进该技术在固体火箭发动机绝热层脱粘检测中的应用,用数值模拟和实验方法研究了固体火箭发动机绝热层脱粘脉冲热像检测的规律,得到了决策参数与结构参数之间的定量关系;提出了检测极限的确定准则,并计算了脱粘大小和深度(绝热层厚度)的检测极限;提出了脱粘尺寸的测量方法及误差修正公式。所得的方程、数据和结论为固体火箭发动机绝热层脱粘的红外无损检测提供了科学依据和操作准则。 相似文献