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381.
轴向密流比对叶栅性能有较大的影响,本文对该问题进行理论及实验研究,导出了叶栅主要性能参数与轴向密流比的关联方程,通过压气机叶栅吹风实验,得到了不同轴向密流比条件下的叶栅性能。理论计算与实验结果吻合的程度令人满意,表明文中所得出的理论关联式可以有效地估算轴向密流比对叶栅流动的影响,具有一定的实用价值。 相似文献
382.
为在弹塑性状态下计算孔边局部应力,本文基于能量法则,推导出计算孔边局部应力的方法。本文的方法简单实用,准确度较修正诺伯法计算结果要高,文中附有涡轮盘偏心孔的计算实例,并对计算结果进行了分析。 相似文献
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介绍的民机数据总线信号测试仪综合了当前民机上主要采用的ARINC429、ARINC419、CSDB和RS232等数字式航空数据总线规范的接口,具有和这些总线接口设备通讯的能力,可以灵活方便地应用于机载设备检测,装机交联实验当中。 相似文献
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研究了通道进口雷诺数和总出流比对带肋和双排出流孔通道流量系数和压力分布的影响。实验研究的通道入口雷诺数为3×104~1.5×105,通道总出流比为0.09~0.22。结果表明:通道总出流比较小时,流量系数沿流向减小。通道进口雷诺数增加,流量系数先增加,之后基本不变;通道总出流比较大时,流量系数基本不变;各工况下总压系数沿流向依次经历迅速减小、基本不变、继续减小的过程;沿流向各位置上的总压系数在通道进口雷诺数为6×104~9×104时最小;出流比增大,沿流向各位置上的总压系数随之增大。 相似文献
388.
Anastassopoulos V. Lampropoulos G. 《IEEE transactions on aerospace and electronic systems》1992,28(2):420-427
A constant false alarm rate (CFAR) detection method which is based on a combination of median and morphological filters (MEMO) is proposed. The MEMO algorithm has robust performance with small CFAR loss, very good behavior at clutter edges and high detection performance in the case of closely spaced narrowband signals (targets). The proposed MEMO method is favourably compared with cell averaging (CA) and ordered statistics (OS) CFAR detectors. The Monte Carlo method is employed to analyze the MEMO-CFAR detector 相似文献
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This work is concerned with binary systems that we call ‘moderately close’. These are systems in which the primary (by which we mean the initially more massive star) fills its Roche lobe when it is on the giant branch with a deep convective envelope but before helium ignition (late case B). We find that if the mass ratio q(= M 1/M 2) < q crit = 0.7 when the primary fills its Roche lobe positive feedback will lead to a rapid hydrodynamic phase of mass transfer which will probably lead to common envelope evolution and thence to either coalescence or possibly to a close binary in a planetary nebula. Although most Algols have probably filled their Roche lobes before evolving off the main-sequence we find that some could not have and are therefore ‘moderately close’. Since rapid overflow is unlikely to lead to an Algol-like system there must be some way of avoiding it. The most likely possibility is that the primary can lose sufficient mass to reduce q below q crit before overflow begins. Ordinary mass loss rates are insufficient but evidence that enhanced mass loss does take place is provided by RS CVn systems that have inverted mass ratios but have not yet begun mass transfer. We postulate that the cause of enhanced mass loss lies in the heating of the corona by by magnetic fields maintained by an α — ω dynamo which is enhanced by tidal effects associated with corotation. In order to model the the effects of enhanced mass loss we ignore the details and adopt an empirical approach calibrating a simple formula with the RS CVn system Z Her. Using further empirical relations (deduced from detailed stellar models) that describe the evolution of red giants we have investigated the effect on a large number of systems of various initial mass ratios and periods. These are notable in that some systems can now enter a much gentler Algol-like overflow phase and others are prevented from transferring mass altogether. We have also investigated the effects of enhanced angular momentum loss induced by corotation of the wind in the strong magnetic fields and consider this in relation to observed period changes. We find that a typical ‘moderately close’ Algol-like system evolves through an RS CVn like system and then possibly a symbiotic state before becoming an Algol and then goes on through a red giant-white dwarf state which may become symbiotic before ending up as a double white dwarf system in either a close or wide orbit depending on how much mass is lost before the secondary fills its Roche lobe. 相似文献