排序方式: 共有266条查询结果,搜索用时 31 毫秒
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基于刚度下降的疲劳累积损伤模型的研究 总被引:5,自引:0,他引:5
复合材料在静态和动态载荷作用下的损伤是十分复杂的,对损伤的精确建模是关系到复合材料力学行为描述的关键问题.从应变等效性假设出发,通过分析和描述疲劳过程中刚度和应变的演化规律,提出能够描述材料疲劳损伤演化过程的、以应变定义的和在疲劳过程中真实地反映材料动态本构关系的损伤因子,建立考虑残余应变的刚度下降复合材料疲劳损伤模型.T300/KH-304是我国新近研制的高性能航空复合材料,应用此模型开展对其疲劳损伤行为的分析与研究.在岛津液压伺服试验机上,加载频率控制在4.1 Hz,对这种材料的层合板进行4个常幅应力水平的疲劳实验,建立了T300/KH-304复合材料的疲劳模型的数学表达,经验证模型优于经典的疲劳模型的S-N曲线拟合精度,最大的误差仅为2.4%,且能反应疲劳损伤的发展规律. 相似文献
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基于DTW的涡扇发动机气路故障定量诊断方法 总被引:7,自引:0,他引:7
提出了一种利用动态过程信息对气路故障进行定量诊断的新方法.采用动态时间规整(DTW, Dynamic Time Warping)技术,对动态测试样本同已知的故障模式进行相似性度量,充分利用发动机的过渡态特征信息,实现了发动机气路部件故障的定量诊断.结果表明:这种方法的漏报率和误报率低,具有很高的诊断准确性,对测量噪声和其它不确定性具有很好的鲁棒性. 相似文献
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Geochemistry of Carbonates on Mars: Implications for Climate History and Nature of Aqueous Environments 总被引:1,自引:0,他引:1
Paul B. Niles David C. Catling Gilles Berger Eric Chassefière Bethany L. Ehlmann Joseph R. Michalski Richard Morris Steven W. Ruff Brad Sutter 《Space Science Reviews》2013,174(1-4):301-328
Ongoing research on martian meteorites and a new set of observations of carbonate minerals provided by an unprecedented series of robotic missions to Mars in the past 15 years help define new constraints on the history of martian climate with important crosscutting themes including: the CO2 budget of Mars, the role of Mg-, Fe-rich fluids on Mars, and the interplay between carbonate formation and acidity. Carbonate minerals have now been identified in a wide range of localities on Mars as well as in several martian meteorites. The martian meteorites contain carbonates in low abundances (<1 vol.%) and with a wide range of chemistries. Carbonates have also been identified by remote sensing instruments on orbiting spacecraft in several surface locations as well as in low concentrations (2–5 wt.%) in the martian dust. The Spirit rover also identified an outcrop with 16 to 34 wt.% carbonate material in the Columbia Hills of Gusev Crater that strongly resembled the composition of carbonate found in martian meteorite ALH 84001. Finally, the Phoenix lander identified concentrations of 3–6 wt.% carbonate in the soils of the northern plains. The carbonates discovered to date do not clearly indicate the past presence of a dense Noachian atmosphere, but instead suggest localized hydrothermal aqueous environments with limited water availability that existed primarily in the early to mid-Noachian followed by low levels of carbonate formation from thin films of transient water from the late Noachian to the present. The prevalence of carbonate along with evidence for active carbonate precipitation suggests that a global acidic chemistry is unlikely and a more complex relationship between acidity and carbonate formation is present. 相似文献
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《Acta Astronautica》2007,60(10-11):930-938
The Dawn project is progressing toward its 2007 launch on a mission to orbit main belt asteroids (1) Ceres and (4) Vesta. Designed to provide insights into important questions about the evolution of the solar system, Dawn will spend more than 0.5 years in orbit about each of these bodies. This challenging mission is enabled by an ion propulsion system. In contrast to missions that use conventional chemical propulsion, the use of this system creates a strong coupling of allowable flight system mass and available power, thereby requiring different methods of managing these and other technical resources. Now that the project is nearing launch, the refinement of resource estimates allows the identification of excess margin, which is being applied in novel ways to benefit the project both in development and in operations. 相似文献
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Bethany L. Ehlmann Gilles Berger Nicolas Mangold Joseph R. Michalski David C. Catling Steven W. Ruff Eric Chassefière Paul B. Niles Vincent Chevrier Francois Poulet 《Space Science Reviews》2013,174(1-4):329-364
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydrothermal alteration (volcanic- or impact-induced), diagenesis, metamorphism, and magmatic precipitation. Diverse clay minerals have been detected from orbital investigation of terrains on Mars and are globally distributed, indicating geographically widespread aqueous alteration. Clay assemblages within deep stratigraphic units in the Martian crust include Fe/Mg smectites, chlorites and higher temperature hydrated silicates. Sedimentary clay mineral assemblages include Fe/Mg smectites, kaolinite, and sulfate, carbonate, and chloride salts. Stratigraphic sequences with multiple clay-bearing units have an upper unit with Al-clays and a lower unit with Fe/Mg-clays. The typical restriction of clay minerals to the oldest, Noachian terrains indicates a distinctive set of processes involving water-rock interaction that was prevalent early in Mars history and may have profoundly influenced the evolution of Martian geochemical systems. Current analyses of orbital data have led to the proposition of multiple clay-formation mechanisms, varying in space and time in their relative importance. These include near-surface weathering, formation in ice-dominated near-surface groundwaters, and formation by subsurface hydrothermal fluids. Near-surface, open system formation of clays would lead to fractionation of Mars’ crustal reservoir into an altered crustal reservoir and a sedimentary reservoir, potentially involving changes in the composition of Mars’ atmosphere. In contrast, formation of clays in the subsurface by either aqueous alteration or magmatic cooling would result in comparatively little geochemical fractionation or interaction of Mars’ atmospheric, crustal, and magmatic reservoirs, with the exception of long-term sequestration of water. Formation of clays within ice would have geochemical consequences intermediate between these endmembers. We outline the future analyses of orbital data, in situ measurements acquired within clay-bearing terrains, and analyses of Mars samples that are needed to more fully elucidate the mechanisms of martian clay formation and to determine the consequences for the geochemical evolution of the planet. 相似文献
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研究了3种针对镍基单晶合金各向异性低循环疲劳寿命建模的方法,分别为基于单晶合金弹性模量与晶体取向相关性的方法,与各向异性屈服函数相关的方法和传统滑移系的方法。对基于屈服函数的方法进行了修正以将其应用于单晶合金。利用公开文献中DD3单晶合金的低循环疲劳数据对修正的模型进行了验证,并对采用这3种方法得到的数据进行了比较。结果表明:修正的疲劳寿命模型和基于取向函数的寿命模型的预测结果与试验数据相比基本落在3倍分散带内,而采用基于滑移系的方法所得结果在4倍分散带内。基于屈服函数的修正模型和另外2种模型均可以较好地与3维有限元应力分析直接衔接,便于涡轮叶片结构级的寿命预测。 相似文献
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航空发动机燃烧室贫油熄火极限的预测方法研究对于全面掌握燃烧室性能和有效工作范围,进而对提高燃烧室设计水平,完善中国航空发动机设计体系,有着重要的理论和工程意义。在总结国内外相关研究的基础上,对适合于工程应用的预测方法进行了归纳总结,其中包括半经验模型、火焰体积法、基于数值计算的Lefebvre经验公式、等效反应器网络图法、火焰前锋法和RANS燃烧流场特征法。针对每种方法,详细阐述了其特点,并对存在的问题进行了分析。最后,提出了完善贫油熄火预测方法的一些建议。 相似文献
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