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导管长度对管式减涡器流阻与温降特性影响 总被引:1,自引:0,他引:1
采用数值模拟与模型试验研究相结合的方法对管式减涡器开展研究,分析了导管长度对管式减涡器各截面间压力损失系数、温降系数及其权重的影响。通过模型试验验证了数值模拟方法的可靠性。研究结果表明:增大导管长度可以显著降低管式减涡器压力损失的同时提高其温降。共转盘腔和导管是管式减涡器流阻与温降特性的主要影响因素,两者权重此消彼长。增大导管长度时,通过牺牲导管内压力损失和降低共转盘腔内压力损失以降低管式减涡器压力损失。快速增大的导管内温降是管式减涡器温降系数提高的主要原因。与光滑共转盘腔模型相比,当导管长度L/b=0.786时,管式减涡器压力损失系数降低了83.70%,温降系数提高了45.02%。 相似文献
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435.
航空发动机鼓筒零件内腔尺寸的测量与评价 总被引:2,自引:0,他引:2
主要介绍应用三坐标扫描功能对航空发动机某鼓筒零件内腔尺寸进行扫描测量并将数据导入到CAD软件中实现图形化处理,进行测量结果的评价方法。 相似文献
436.
《中国航空学报》2020,33(6):1788-1798
Different yield criterion has great difference in predicting the deformation of tube with different material. In order to improve the prediction accuracy of the cross-sectional deformation of the double-ridged rectangular tube (DRRT) during rotary draw bending (RDB) process, Mises isotropic yield criterion, Hill’48 and Barlat/Lian anisotropic yield criteria commonly used in practical engineering are introduced to simulate RDB of DRRT. The inverse method combining uniaxial tensile test of whole tube and response surface methodology was proposed to identify the parameters of Hill’48 and Barlat/Lian yield criteria of small-sized H96 brass extrusion DRRT as well. Then based on ABAQUS/Explicit platform, the FE models of RDB process of DRRT considering Mises, Hill’48 and Barlat/Lian yield criteria were built. The results show that: The variation trend of cross-sectional deformation ratio is same when using different yield criteria. The cross-sectional deformation ratio by using Mises yield criterion is close to that by using Hill’48 yield criterion. However, there is a quite difference between by using Barlat/Lian yield criterion and by using Mises or Hill’48 yield criteria. The prediction values of cross-sectional height deformation by using three yield criteria all underestimate the experiment ones, and the prediction values of cross-sectional width deformation overestimate the experiment ones. By comparing the simulation results of cross-sectional deformation of the DRRT with different yield criteria and experiment ones, Barlat/Lian yield criterion is found to be suitable for describing the RDB process of DRRT. 相似文献
437.
深入研究了CATIA/VPM并行协同设计环境下产品与工装之间的数据组织管理及相应的关联设计技术,提出了跨产品结构树的产品工装数据组织管理及关联设计方法。该技术既是对现有全三维关联设计技术的进一步探索,又为实现产品工装一体化设计提供了一条可行的解决途径,具有重要的应用价值和现实意义。 相似文献
438.
Inner flange and side wrinkling often occur in rotary-draw bending process of rectangular aluminum alloy wave-guide tubes, and the distribution and magnitude of wrinkling is related to geometrical parameters of the tubes. In order to study the effects of geometrical parameters on wrinkling of rectangular wave-guide tubes, a 3D-FE model for rotary-draw bending processes of thin-walled rectangular aluminum alloy wave-guide tubes was built based on the platform of ABA-QUS/Explicit, and its reliability was validated by experiments. Simulation and analysis of the influence laws of geometrical parameters on the wave heights of inner flange and side wrinkling were then carried out. The results show that inner flange wrinkling is the main wrinkling way to rectan- gular wave-guide tubes in rotary-draw bending processes, but side wrinkling cannot be neglected because side wrinkling is 2/3 of inner flange wrinkling when b and h are smaller. Inner flange and side wrinkling increase with increasing b and h; the influence of b on side wrinkling is larger than that of h, while both b and h affect inner flange wrinkling greatly. Inner flange and side wrinkling decrease with increasing R/h; the influence of h on inner flange and side wrinkling is larger than that of R. 相似文献
439.
摇摆对水平管内单相水阻力特性的影响分析 总被引:1,自引:0,他引:1
对摇摆状态下25mm和34.5mm管径水平管内单相水阻力特性进行了实验研究,通过实验发现,摇摆状态下单相水摩擦压降有明显的周期性,并与摇摆周期相同。雷诺数降低、摇摆振幅增加以及管径增加都会使摩擦压降增加。通过对摇摆周期、摇摆幅度、雷诺数和管径等影响因素的分析,给出了摇摆状态下单相水摩擦系数的计算公式。计算结果表明,得到的摩擦压降满足摇摆条件周期波动的特点,计算结果与实验结果符合较好。 相似文献
440.
S.A. Dyadechkin V.S. Semenov H.K. Biernat T. Penz 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2008
Cosmic strings are topological defects which were generated at a transition phase of the very early Universe and are probably responsible for large-scale structure forming. However, they may pull through all history and exist in the recent epoch. Thus, they can have influence for the recent Universe interacting with different objects. We consider the cosmic string behavior in the vicinity of a spinning black hole by means of a numerical simulation. Here we present preliminary results of this work via a comparison of cosmic string and magnetic flux tube behavior in the Kerr metric. Such an approach follows from the similarity of the equations which describe these objects. Therefore, many aspects of this behavior may be comparable. 相似文献