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1.
高速列车进入带缓冲结构隧道的压力变化研究(I) 总被引:1,自引:0,他引:1
给出了列车穿越带有缓冲结构的隧道压力变化的三维粘性流场数值模拟过程,控制方程为三维粘性、可压缩、非定常流的N.S方程,空间离散采用了中心有限体积法格式,时间采用预处理二阶精度多步后差分格式进行离散,对列车与隧道之间的相对运动采用移动网格技术处理。对不同的缓冲结构缓解隧道内瞬变压力及压力梯度的作用进行了研究。研究结果表明,缓冲结构的设置能够有效地降低隧道内的压力和压力梯度的最大值,其原因在于缓冲结构延长了压缩波压力上升的时间,降低列车突入隧道时所形成的最大压力梯度;另一方面由于压缩波在缓冲结构和列车、隧道之间多次的反射,也降低了压力峰值。 相似文献
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主要介绍了客车行李舱门的工作原理.对比了传统的与新式的行李舱门的结构,并提出了新式客车行李舱门的设计方案。根据运动要求确定出机构的主要尺寸参数,对AD杆进行受力情况分析,通过强度计算证实这种机构工作的可靠性. 相似文献
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切削加工的发展趋势 总被引:4,自引:0,他引:4
刘会英 《航空精密制造技术》2002,38(3):20-22
从加工技术和机床技术两个方面介绍了切削加工领域的先进技术和发展趋势。描述了高速切削技术的现状,直线电机的应用,高效环保切削加工,机床的并联机构及相关的测量控制系统。 相似文献
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《中国航空学报》2020,33(12):3176-3188
Numerical simulation and theoretical analysis were conducted to study the hysteresis inside scramjet isolator during the reciprocating process of back pressure variation. It is revealed that only a regular reflection is theoretically possible for two leading shocks when the inflow Mach number is greater than 2.0, and no hysteresis can occur in the transition between shock reflection types. Nevertheless, wall suction, gas injection, and background waves cause non-uniformity of the incoming flow and would make hysteresis possible. Besides the classical hysteresis in the transition between shock reflection, new kinds of hysteresis were found in both the deflection angle of separated boundary layer and the location of the shock train. Moreover, the occurrence of hysteresis in the deflection angle of the separated boundary layer is accompanied with the shock reflection hysteresis. In the case with background waves or gas injection, hysteresis in the starting position of leading shock was observed too. As back pressure decreases, the leading shock does not follow the same path as that as the back pressure increases, and it is anchored at the location where the background shock or the injection interacts with the leading shock. It is inferred that, if two strong adverse pressure gradient regions move towards and interact with each other, hysteresis will take place when they start to separate. 相似文献
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Nonlinear dynamic modeling of a helicopter planetary gear train for carrier plate crack fault diagnosis 总被引:3,自引:3,他引:0
《中国航空学报》2016,(3):675-687
Planetary gear train plays a significant role in a helicopter operation and its health is of great importance for the flight safety of the helicopter. This paper investigates the effects of a planet carrier plate crack on the dynamic characteristics of a planetary gear train, and thus finds an effec-tive method to diagnose crack fault. A dynamic model is developed to analyze the torsional vibra-tion of a planetary gear train with a cracked planet carrier plate. The model takes into consideration nonlinear factors such as the time-varying meshing stiffness, gear backlash and viscous damping. Investigation of the deformation of the cracked carrier plate under static stress is performed in order to simulate the dynamic effects of the planet carrier crack on the angular displacement of car-rier posts. Validation shows good accuracy of the developed dynamic model in predicting dynamic characteristics of a planetary gear train. Fault features extracted from predictions of the model reveal the correspondence between vibration characteristic and the conditions (length and position) of a planet carrier crack clearly. 相似文献
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中国正在大力发展城际高速铁路运输,而在线路中有隧道时,列车进出隧道所产生的微压波问题已经成为限制高速铁路安全、环保、健康发展的障碍。大量研究表明:隧道出口的微压波强度与压缩波的压力梯度成正比,可以通过分析压缩波的压力梯度变化来评价降低微压波的效果。采用模型试验方法,对缓冲设施、减压竖井降低压缩波峰值和压力梯度峰值的效果进行了测试分析。实验结果表明:减压竖井降低首波压力峰值、压力梯度峰值效果明显;洞口缓冲设施降低首波压力峰值的效果不明显,降低压力梯度峰值效果明显,并且降低压力梯度的效果与速度相关。 相似文献
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As Ulysses moved inward and southward from mid-1992 to early 1994 we noticed the occasional occurrence of inter-events, lasting about 10 days and falling between the recurrent events, observed at proton energies of 0.48–97 MeV, associated with Corotating Interaction Regions (CIR). These inter-events were present for several sequences of two or more solar rotations at intensity levels around 1% of those of the neighbouring main events. When we compared the Ulysses events with those measured on IMP-8 at 1 AU we saw that the inter-events appeared at Ulysses after the extended emission (>10 days) of large fluxes of solar protons of the same energy that lasted at least one solar rotation at 1 AU. The inter-events fell completely within the rarefaction regions (dv/dt<0) of the recurrent solar wind streams. The interplanetary magnetic field (IMF) lines in the rarefactions map back to the narrow range of longitudes at the Sun which mark the eastern edge of the source region of the high speed stream. Thus the inter-events are propagating at mid-latitudes to Ulysses along field lines free from stream-stream interactions. They are seen in the 0.39–1.28 MeV/nucleon He, which exhibit a faster decay, but almost never in the 38–53 keV electrons. We show that the inter-events are unlikely to be accelerated by reverse shocks associated with the CIRs and that they are more likely to be accelerated by sequences of solar events and transported along the IMF in the rarefactions of the solar wind streams. 相似文献