空间在轨氢氧内燃机技术研究

用于空间在轨运行的氢氧内燃机是低温末级火箭流体集成系统（IVF）中的关键组件。分析了国内外空间在轨氢氧内燃机的发展现状,通过Chemkin燃烧软件仿真分析获得了氢氧内燃机设计关键参数。开展了氢氧内燃机地面点火验证试验。结果表明：氢氧内燃机具有较好的点火启动性能,通过降低混合比和压缩比能够将氢氧内燃机缸内的温度和压力控制在合理范围内。氢氧内燃机在稳定的转速下工作,所消耗的氢气、氧气质量流量小于低温贮箱的平均蒸发量。     

Analysis of total visual and CCD V-broadband observations of Comet C/1995 O1 (Hale-Bopp): 1995–2001

We developed a general method for determination of water production rates from groundbased visual observations and applied it to Comet Hale–Bopp. Our main objective is to extend the method to include total visual magnitude observations obtained with CCD detector and V filter in the analysis of total visual magnitudes. We compare the CCD V-broadband careful observations of Liller [Liller, W. Pre-perihelion CCD photometry of Comet 1995 O1 (Hale-Bopp). Planet. Space Sci. 45, 1505–1513, 1997; Liller, W. CCD photometry of Comet C/1995 O1 (Hale-Bopp): 1995–2000. Int. Comet Quart. 23(3), 93–97, 2001] with the total visual magnitude observations from experienced international observers found in the International Comet Quarterly (ICQ) archive. A data set of ∼400 CCD observations covering about the same 6 years time span of the ∼12,000 ICQ selected total visual magnitude observations were used in the analysis. A least-square method applied to the water production rates, yields power laws as a function of the heliocentric distances for the pre- and post-perihelion phases. The average dimension of the nucleus as well as its effective active area is determined and compared with values published in the literature.     

考虑喷注流强分布的纵向稳定性建模与分析

喷注器流强分布是除声学阻尼装置以外使液体火箭发动机稳定工作的重要措施,通过控制喷注流强分布使推进剂的燃烧尽量远离主要振型的波腹区,减少热声耦合振荡的能量源,从而达到抑制高频振荡的效果。因此,建立喷注流强分布与稳定性之间的综合分析模型,研究流强分布的不稳定性抑制特性具有重要实际意义。针对采用自击式喷嘴器、液滴蒸发作为燃烧速率控制过程的某自燃推进剂缩尺燃烧室高频纵向燃烧不稳定问题,近似采用蒸发速率峰值区代替集中燃烧释热区,引入燃烧室三维声学控制方程以考虑多喷嘴条件下燃烧响应空间分布,建立了针对喷注器流强分布条件下的高频纵向燃烧稳定性分析模型,并对喷注流强的稳定性抑制特性进行了分析,给出了不同分布流强下燃烧室一阶纵向信号的增长率变化规律。研究表明,喷注流强分布有利于燃烧室稳定,"驼峰区"喷注孔径的增大对改善高频纵向不稳定性更为显著,"驼峰区"流强增加30%,相应的增长率降低15%。     

Energy utilization rates during shuttle extravehicular activities

The work rates or energy utilization rates during EVA are major factors in sizing of life support systems. These rates also provide a measure of ease of EVA and its cost in crew fatigue. From the first Shuttle EVA on the STS-6 mission in 1983, we have conducted 59 man-EVA and 341 man-hours of EVA. Energy utilization rates have been measured on each of these EVA. Metabolic rate was measured during each EVA using oxygen utilization corrected for suit leakage. From 1981–1987, these data were available for average data over the EVA or over large segments of the EVA. Since 1987, EVA oxygen utilization data were available at 2-minute intervals. The average metabolic rate on Shuttle EVA (194 kcal/hr.) has been significantly lower than metabolic rates during Apollo and Skylab missions. Peak rates have been below design levels, infrequent, and of short duration. The data suggest that the energy cost of tasks may be inversely related to the degree of training for the task. The data provide insight on the safety margins provided by life support designs and on the energy cost of Station construction EVA.     

确定微型固体火箭发动机燃烧时间的CAA与CAD技术

应用计算机辅助分析(CAA)与计算机辅助绘图(CAD)方法,确定微型固体火箭发动机燃烧时间t_b。该方法自动化程度高、精度好,有可靠的理论依据。用它替代传统的没有任何理论根据的手工画角分线法,以提高小型固体火箭发动机内弹道数据处理的精度和速度是十分必要的。实践证明这是一种科学的可行的方法,值得推广。     

铝粉的辐射热反馈及对固体推进剂压强指数的影响

研究了含铝，含细ＡＰ固体推进剂中铝粉对推进剂表面的辐射热反馈，得出这种反馈是使该推进剂燃速压强指数上升的主要原因之一，在配方中添加超细铝粉可能氏压强指数的上升。     

Comparative study of productivity of the Rosetta target Comet 67P/Churyumov-Gerasimenko

In an attempt to evaluate correlations between several properties of comets we report the results of a cometary research involving a criterious analysis of gas and dust mass production rates in Comets 67P/Churyumov-Gerasimenko (main target of Rosetta Mission), 1P/Halley, Hyakutake (C/1996 B2), and 46P/Wirtanen and make a comparison between them.     

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.     

基于VXI总线的多通道多采样率数据采集系统实现

介绍一个多通道多采样率的数据采集系统。该系统输入64个模拟量均要转换成数字信号，数据采集卡为基于VXI总线的E1413，多通道之间的变采样率通过特殊的采样列表实现。文中给出了硬件组成、软件设计和测试结果。该系统已用于对飞机燃油试验台的测控。     

EFFECT OF SOLIDIFICATION RATE ON MICRO－STRUCTURES OF DIRECTIONALLYSOLIDIFIED SUPERALLOY DZ22

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