排序方式: 共有61条查询结果,搜索用时 63 毫秒
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采用放大试验规模(处理量1 m3/h)的H2O2(过氧化氢)/UV(紫外线)/O3(臭氧)氧化技术处理肼类推进剂污水,在30.0±1.6 ℃,pH=9.0±0.2的条件下,研究肼类的过氧化氢增强光解臭氧化降解。对比不同氧化技术的协同效应以及对污水降解的影响,重点考察过氧化氢、紫外线、臭氧和初始浓度等工艺参数对降解效果的影响,对氧化技术的应用进行了优化。研究结果表明:该技术可使COD去除率提高27.66%,肼类的降解速率随着过氧化氢投加量、紫外线辐射强度、O3投加速率和水质地提高而升高,随着初始质量浓度的提高而下降。在最佳工艺下,处理5 000 mg/L质量浓度的废水,处理60 min时,COD去除率分别为98.62%(偏二甲肼)、99.17%(甲基肼)、99.94%(肼)和93.25%(单推-3)。 相似文献
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在建立数学物理模型的基础上,对低地球轨道环境和地面试验环境下有无保护涂层的聚酰亚胺所受原子氧冲蚀及紫外线的综合作用进行了数值模拟,获得了具有工程应用价值的计算结果,并讨论了数学物理模型中各参数对基蚀曲线形状的影响.从数值模拟结果与美国太空试验结果的比较可以看出,得出的数值模拟的结果是正确的,对航天器设计具有重要的指导意义. 相似文献
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Paul O’Brien 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The ASTROSAT satellite is an Indian National Space Observatory under development in India. Due for launch in 2010, ASTROSAT will carry a complement of five scientific instruments enabling simultaneous observations from the optical through to the hard X-ray energy band. This capability will enable broad-band spectroscopy and high time-resolution monitoring of both galactic and extra-galactic targets, such as X-ray binaries and AGN. One of the instruments is being built in collaboration with the Canadian Space Agency and another in collaboration with the University of Leicester. ASTROSAT also carries a scanning sky monitor to observe the variable X-ray sky. After an initial period of science verification and guaranteed time, a certain fraction of ASTROSAT observing time will also be made available to the community via a call for proposals. Here I summarise the instrument complement and principle scientific objectives of the mission. 相似文献
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The remote sensing of comets in the ultraviolet bandpass has been a valuable tool for studying the structure, composition,
variability, and physical processes at work in cometary comae. By extension, these studies of comae have revealed key insights
into the composition of cometary nuclei. Here we briefly review the ultraviolet studies of comets, and then take a look toward
the future of such work as anticipated by the advent of several key new instruments.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
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K. Werner J. Barnstedt W. Gringel N. Kappelmann H. Becker-Roß S. Florek R. Graue D. Kampf A. Reutlinger C. Neumann B. Shustov A. Moisheev E. Skripunov 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008,41(12):1992-1997
The World Space Observatory Ultraviolet (WSO/UV) is a multi-national project grown out of the needs of the astronomical community to have future access to the UV range. WSO/UV consists of a single UV telescope with a primary mirror of 1.7 m diameter feeding the UV spectrometer and UV imagers. The spectrometer comprises three different spectrographs, two high-resolution echelle spectrographs (the High-Resolution Double-Echelle Spectrograph, HIRDES) and a low-dispersion long-slit instrument. Within HIRDES the 102–310 nm spectral band is split to feed two echelle spectrographs covering the UV range 174–310 nm and the vacuum-UV range 102–176 nm with high spectral resolution (R > 50,000). The technical concept is based on the heritage of two previous ORFEUS SPAS missions. The phase-B1 development activities are described in this paper considering performance aspects, design drivers, related trade-offs (mechanical concepts, material selection etc.) and a critical functional and environmental test verification approach. The current state of other WSO/UV scientific instruments (imagers) is also described. 相似文献
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热控涂层紫外辐照试验方法的研究 总被引:1,自引:1,他引:1
几种有机热控涂层在真空下进行模拟太阳紫外辐照的试验。在真空条件和大气条件下测试涂层性能的变化,以比较热控涂层在进行紫外辐照时,原位测试和非原位测试的差异。 相似文献
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红外/紫外双色制导系统数学模型及数字仿真 总被引:1,自引:0,他引:1
介绍了便携式防空导弹双色导引头中所采用的数字式控制系统代替传统的模拟式控制系统的方法。对导引头和自动驾驶仪部分的数学模型作了简化,并作了全弹道数字仿真。仿真结果表明,该双色制导体系设计方便,抗干扰能力强等。 相似文献
10.
S. A. Stern D. C. Slater J. Scherrer J. Stone M. Versteeg M. F. A’hearn J. L. Bertaux P. D. Feldman M. C. Festou Joel Wm. Parker O. H. W. Siegmund 《Space Science Reviews》2007,128(1-4):507-527
We describe the design, performance and scientific objectives of the NASA-funded ALICE instrument aboard the ESA Rosetta asteroid flyby/comet rendezvous mission. ALICE is a lightweight, low-power, and low-cost imaging spectrograph optimized for cometary far-ultraviolet (FUV) spectroscopy. It will be the first UV spectrograph to study a comet at close range. It is designed to obtain spatially-resolved spectra of Rosetta mission targets in the 700–2050 Å spectral band with a spectral resolution between 8 Å and 12 Å for extended sources that fill its ~0.05^ × 6.0^ field-of-view. ALICE employs an off-axis telescope feeding a 0.15-m normal incidence Rowland circle spectrograph with a toroidal concave holographic reflection grating. The microchannel plate detector utilizes dual solar-blind opaque photocathodes (KBr and CsI) and employs a two-dimensional delay-line readout array. The instrument is controlled by an internal microprocessor. During the prime Rosetta mission, ALICE will characterize comet 67P/Churyumov-Gerasimenko's coma, its nucleus, and nucleus/coma coupling; during cruise to the comet, ALICE will make observations of the mission's two asteroid flyby targets and of Mars, its moons, and of Earth's moon. ALICE has already successfully completed the in-flight commissioning phase and is operating well in flight. It has been characterized in flight with stellar flux calibrations, observations of the Moon during the first Earth fly-by, and observations of comet C/2002 T7 (LINEAR) in 2004 and comet 9P/Tempel 1 during the 2005 Deep Impact comet-collision observing campaign. 相似文献