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高超声速飞行器进气道等关键部件引起的激波与边界层相互作用将导致流动分离,从而改变当地压力分布与局部受热情况,影响飞行稳定性与飞行安全,因此需要对高超声速流动的分离现象进行细致研究。采用高精度5阶特征型WENO格式与3阶TVD型Runge-Kutta方法,求解三维Navier-Stokes方程,对立楔诱导的高超声速激波与边界层相互作用引起的分离流动流场结构进行了细致的数值模拟与分析。结果表明,5阶特征型WENO格式分辨率远高于类TVD格式;Ma=6时得到清晰的激波结构、分离涡结构及其演化过程和壁面极限流线的拓扑结构,证明了WENO格式应用于高超声速分离流动的可行性与高分辨率;对不同来流Mach数的对比证明Mach数的增大抑制流动分离,导致分离涡减小。 相似文献
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The Magnetic Field of Mercury 总被引:1,自引:0,他引:1
Brian J. Anderson Mario H. Acuña Haje Korth James A. Slavin Hideharu Uno Catherine L. Johnson Michael E. Purucker Sean C. Solomon Jim M. Raines Thomas H. Zurbuchen George Gloeckler Ralph L. McNutt Jr. 《Space Science Reviews》2010,152(1-4):307-339
The magnetic field strength of Mercury at the planet’s surface is approximately 1% that of Earth’s surface field. This comparatively low field strength presents a number of challenges, both theoretically to understand how it is generated and observationally to distinguish the internal field from that due to the solar wind interaction. Conversely, the small field also means that Mercury offers an important opportunity to advance our understanding both of planetary magnetic field generation and magnetosphere-solar wind interactions. The observations from the Mariner 10 magnetometer in 1974 and 1975, and the MESSENGER Magnetometer and plasma instruments during the probe’s first two flybys of Mercury on 14 January and 6 October 2008, provide the basis for our current knowledge of the internal field. The external field arising from the interaction of the magnetosphere with the solar wind is more prominent near Mercury than for any other magnetized planet in the Solar System, and particular attention is therefore paid to indications in the observations of deficiencies in our understanding of the external field. The second MESSENGER flyby occurred over the opposite hemisphere from the other flybys, and these newest data constrain the tilt of the planetary moment from the planet’s spin axis to be less than 5°. Considered as a dipole field, the moment is in the range 240 to 270 nT-R M 3 , where R M is Mercury’s radius. Multipole solutions for the planetary field yield a smaller dipole term, 180 to 220 nT-R M 3 , and higher-order terms that together yield an equatorial surface field from 250 to 290 nT. From the spatial distribution of the fit residuals, the equatorial data are seen to reflect a weaker northward field and a strongly radial field, neither of which can be explained by a centered-dipole matched to the field measured near the pole by Mariner 10. This disparity is a major factor controlling the higher-order terms in the multipole solutions. The residuals are not largest close to the planet, and when considered in magnetospheric coordinates the residuals indicate the presence of a cross-tail current extending to within 0.5R M altitude on the nightside. A near-tail current with a density of 0.1 μA/m2 could account for the low field intensities recorded near the equator. In addition, the MESSENGER flybys include the first plasma observations from Mercury and demonstrate that solar wind plasma is present at low altitudes, below 500 km. Although we can be confident in the dipole-only moment estimates, the data in hand remain subject to ambiguities for distinguishing internal from external contributions. The anticipated observations from orbit at Mercury, first from MESSENGER beginning in March 2011 and later from the dual-spacecraft BepiColombo mission, will be essential to elucidate the higher-order structure in the magnetic field of Mercury that will reveal the telltale signatures of the physics responsible for its generation. 相似文献
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CHEN Guodinga SUN Hengchaoa WANG Junb aSchool of Mechanical Engineering Northwestern Polytechnical University Xi’an China bAVIC Commercial Aircraft Engine Co. Ltd Shanghai China 《中国航空学报》2011,(3):355-362
The lubrication design and heat transfer determination of bearing chambers in aeroengine require a sufficient understanding of the oil droplet-film interaction and physical characteristic in an oil/air two-phase flow state.The analyses of oil droplet movement,mass and momentum transfer during the impingement of droplet/wall,as well as wall oil film thickness and flow velocity are very important for the bearing chamber lubrication and heat transfer calculation.An integrated model in combination with droplet movement,droplet/wall impact and film flow analysis is put forward initially based on the consideration of droplet size distribution.The model makes a contribution to provide more practical and feasible technical approach,which is not only for the study of droplet-film interaction and physical behavior in bearing chambers with oil/air two-phase flow phenomena,but also useful for an insight into the essence of physical course through droplet movement and deposition,film formation and flow.The influences of chamber geometries and operating conditions on droplet deposition mass and momentum transfer,and wall film thickness and velocity distribution are discussed.The feasibility of the method by theoretical analysis is also verified by the existing experimental data.The current work is conducive to expose the physical behavior of wall oil film configuration and flow in bearing chamber,and also significant for bearing chamber lubrication and heat transfer study under oil/air two-phase flow conditions. 相似文献
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以某型涡扇发动机为研究对象, 构建了基于神经网络的航空发动机智能性能诊断方法, 讨论了测量噪声及测量偏差对诊断结果的影响及其处理方法.建立一簇并行的神经网络组和发动机模型, 通过比较各模型输出与发动机测量参数之间的误差, 判断传感器是否存在测量偏差.仿真结果表明, 该方法能有效消除测量噪声, 准确判断并隔离有测量偏差的传感器, 得出正确的发动机性能诊断结果. 相似文献
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典型二元高超声速进气道设计方法研究 总被引:1,自引:2,他引:1
综合了一系列典型二元高超声速进气道的设计和性能估算方法, 给出了可行的设计原则.在满足流量、增压以及工作范围(起动性能和反压承受能力)的条件下, 给出了进气道进口、外压波系、内压缩通道、唇罩及隔离段的设计方法.采用此方法, 以H=22800 m、Ma0=6为设计点, 完成了一高超声速进气道的初步设计, 并估算得到了进气道性能参数、进气道的起动马赫数和反压承受能力, 对比CFD计算结果, 误差不大.通过该方法得到的进气道具有结构简单、流量系数大、压缩损失小的特点, 不通过优化即可得到性能较为良好的模型. 相似文献
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高强Al-Cu-Li-X铝锂合金2A97三级时效工艺及性能研究 总被引:2,自引:0,他引:2
以新型高强Al-Gu-Li-X铝锂合金2A97为研究对象,通过拉伸试验研究两种三级时效工艺及其改型工艺对合金性能的影响.结果表明,含有δ′相二次析出过程的三级时效和含有δ′相回溶过程的三级时效处理合金的强度和塑性达到T6峰值时效水平,三级时效改型工艺由于增加变形使前者合金的强度升高,塑性降低,使后者的强度显著提高.三级时效和单级时效合金的主要显微组织有δ′相、θ″/θ′相和T1相.三级时效改型工艺由于增加变形促进δ′相析出和δ′相回溶,同时变形促进T1相析出,从而改变了主要强化相δ′相和T1相的数量. 相似文献
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