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991.
为将富油燃烧/快速淬熄/贫油燃烧(RQL)用于高温升燃烧室设计,以实现温升与排放的良好统一,对不同主燃孔位置下
的单头部矩形燃烧室流动、淬熄区气流混合、燃烧和排放特性进行数值模拟。结果表明:燃烧室中心回流区的长度和高度随着主
燃孔轴向距离的增大而增大。随着主燃孔轴向距离的增大,主燃孔射流深度增加,射流角度逐渐向下游偏转,导致淬熄区内气流
的混合效果减弱;随着主燃孔位置的后移,富油区内的当量比显著增大,导致CO和碳烟的生成量迅速增加,淬熄区内的沿程高温
区域面积逐渐缩小,燃烧效率逐渐降低。当X/H=0.7时,燃烧室沿程NO生成量始终处在较大值;而当X/H=0.9时,燃烧室沿程NO
生成量始终处于较小值,但CO的生成量增大。 相似文献
992.
993.
球载高能天文望远镜的超视距自动跟踪 总被引:1,自引:0,他引:1
本文在HAPI-4原有系统的基础上,利用80C196超16位单片机,首次实现了球载姿态指向控制系统的数字化;借助于全球卫星定位系统GPS,实现了气球位置的高精度定位和时间的绝对定标;采用小型高密度磁带机作为球载数据流存储器,利用海事卫星实现超视距测控,形成了新一代的球载高能望远镜控制系统. 相似文献
994.
Yinjie Yang Shin-ichi YokoboriAkihiko Yamagishi 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Earthly microorganisms might have contaminated Mars for millions of years by intellectual activities or natural transfer. Knowledge on the preservation of microorganisms may help our searching for life on outer planets, particularly Mars-contaminated earthly microorganisms at ancient time. Extreme dryness is one of the current Mars characteristics. However, a humid or watery Mars at earlier time was suggested by evidence accumulated in recent decades. It raises the question that whether water helps preservation of the microorganisms or not, particularly those with high possibility of interplanetary transfer like spores and Deinococci. In this study, we examined the effects of desiccation and high humidity on survival and DNA double strand breaks (DSB) of Escherichia coli, Deinococcus radiodurans and spores of Bacillus pumilus at 25, 4 and −70 °C. They exhibited different survival rates and DSB patterns under desiccation and high humidity. Higher survival and less DSB occurred at lower temperature. We suggest that some Mars-contaminated bacteria might have been viably preserved on cold Mars regions for long periods, regardless of water availability. It is more likely to find ancient spores than ancient Deinococci on Mars. In our search for preserved extraterrestrial life, priority should be given to the Mars Polar Regions. 相似文献
995.
利用Ansys对镀锌锅上方空间的温度场进行模拟。在模拟过程中,利用Ansys软件中的FlotranCFD模块建立模型,计算锌锅上方空间的流场和温度场分布情况,分析温度的主要影响因素,为热镀锌生产线的工程设计提供了理论依据。此方法也为温度分析提供了一种新的思路。 相似文献
996.
997.
Igor S. Veselovsky Serge Koutchmy 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Several important issues are open in the field of solar variability and they wait their solution which up to now was attempted using critical ground-based instrumentations. However, accurate photometric data are attainable only from space. New observational material should be collected with high enough spatial and spectral resolution, covering the whole visible range of the electromagnetic spectrum as well infrared and ultraviolet to reconstruct the total solar irradiance: (1) the absolute contributions of different small-scale structural entities of the solar atmosphere from the white light flares and from micro-flares are still poorly known; (2) we do not know the absolute contributions of different structural elements of the solar atmosphere to the long-term and to the cyclic variations of the solar irradiance, including features of the polar regions of the Sun; (3) the variations of the chromospheric magnetic network are still poorly evaluated; (4) only scarce information is available about the spectral variations of different small-scale features in the high photosphere. Variability of the Sun in white light can be studied with higher spectral, spatial and time resolution using space-born telescopes, which are more appropriate for this purpose than ground based observatories because of better seeing conditions, no interference of the terrestrial atmosphere and a more precise calibration procedure. Scientific requirements for such observations and the possible experimental tools proposed for their solution. Suggested solar studies have broader astrophysical importance. 相似文献
998.
A. Zanini M. Storini O. Saavedra 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
The worldwide distribution of High Mountain Observatories provides a unique opportunity for performing contemporary measurements under different geomagnetic/altitude conditions and for collecting long-term data series. In this context, the history and some activities performed at two historical Research Stations are summarized: Chacaltaya Laboratory (Bolivia) and the Testa Grigia Research Station (Italy). 相似文献
999.
Three-dimensional computational fluid dynamics analyses have been employed to study the compressible and turbulent flow of the shock train in a convergent–divergent nozzle. The primary goal is to determine the behavior, location, and number of shocks. In this context, full multi-grid initialization, Reynolds stress turbulence model (RSM), and the grid adaption techniques in the Fluent software are utilized under the 3D investigation. The results showed that RSM solution matches with the experimental data suitably. The effects of applying heat generation sources and changing inlet flow total temperature have been investigated. Our simulations showed that changes in the heat generation rate and total temperature of the intake flow influence on the starting point of shock, shock strength, minimum pressure, as well as the maximum flow Mach number. 相似文献
1000.