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131.
132.
非定常压力测量中信号失真的管传递函数修正方法 总被引:1,自引:1,他引:0
使用外置压力传感器测量非定常压力会造成非定常测量信号失真. 这是由连接外置传感器和测点之间的管道传压系统引成的. 阐述了一种修正这种非定常信号失真的方法.从而使得运用外置传感器测量非定常压力成为可能.这种技术使用已知的管传递函数在频域中修正非定常测量信号的失真. 同时修正失真信号振幅的变化和相位角的偏移.给出了这种修正技术的运用实例:在叶轮机颤振试验中测量叶片表面非定常压力和在非定常旋涡脱落试验中测量尾迹. 相似文献
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Lars Stenseng Ole Baltazar Andersen 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2012
A number of geophysical phenomenons in the open ocean are still unresolved by conventional altimetry, but could be resolved through the potential improvements offered by Synthetic Aperture Radar (SAR), also called Delay-Doppler, altimetry. The SAR altimeter offers the following benefits with respect to conventional satellite altimetry: factor of 20 improvements in the along-track resolution, the along-track footprint length which does not vary with wave height (sea state), and improved precision in sea surface height measurements or sea surface slope measurements. 相似文献
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Vortex-acoustic coupling is one of the most important potential sources of combustion instability in solid rocket motors (SRMs). Based on the Von Karman Institute for Fluid Dynamics (VKI) experimental motor, the influence of the thermal inhibitor position and temperature on vortex-shedding-driven pressure oscillations is numerically studied via the large eddy simulation (LES) method. The simulation results demonstrate that vortex shedding is a periodic process and its accurate frequency can be numerically obtained. Acoustic modes could be easily excited by vortex shedding. The vortex shedding frequency and second acoustic frequency dominate the pressure oscillation characteristics in the chamber. Thermal inhibitor position and gas temperature have little effect on vortex shedding frequency, but have great impact on pressure oscillation amplitude. Pressure amplitude is much higher when the thermal inhibitor locates at the acoustic velocity anti-nodes. The farther the thermal inhibitor is to the nozzle head, the more vortex energy would be dissipated by the turbulence. Therefore, the vortex shedding amplitude at the second acoustic velocity antinode near 3/4L (L is chamber length) is larger than those of others. Besides, the natural acoustic frequencies increase with the gas temperature. As the vortex shedding frequency departs from the natural acoustic frequency, the vortex-acoustic feedback loop is decoupled. Consequently, both the vortex shedding and acoustic amplitudes decrease rapidly. 相似文献
137.
An improved delayed detached eddy simulation (IDDES) method based on the k-x-SST (shear stress transport) turbulence model was applied to predict the unsteady vortex breakdown past an 80o/65o double-delta wing (DDW), where the angles of attack (AOAs) range from 30° to 40°. Firstly, the IDDES model and the relative numerical methods were validated by simulating the massively separated flow around an NACA0021 straight wing at the AOA of 60°. The fluctuation properties of the lift and pressure coefficients were analyzed and compared with the available measurements. For the DDW case, the computations were compared with such mea-surements as the mean lift, drag, pitching moment, pressure coefficients and breakdown locations. Furthermore, the unsteady properties were investigated in detail, such as the frequencies of force and moments, pressure fluctuation on the upper surface, typical vortex breakdown patterns at three moments, and the distributions of kinetic turbulence energy at a stream wise section. Two dominated modes are observed, in which their Strouhal numbers are 1.0 at the AOAs of 30°, 32° and 34° and 0.7 at the AOAs of 36o, 38° and 40°. The breakdown vortex always moves upstream and downstream and its types change alternatively. Furthermore, the vortex can be identified as breakdown or not through the mean pressure, root mean square of pressure, or even through correlation analysis. 相似文献
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提出了一种三维霜冰结冰的数值模拟方法。基于欧拉-拉格朗日法计算空气-水滴两相流流场,获得了表面水滴撞击特性以及撞击量,求解质量守恒和能量守恒方程获得网格单元内的结冰量,三维霜冰的结冰计算程序采用用户自定义(UDF)编写,FLUENT提供的动网格功能实现了结冰后的网格重构。计算了4°攻角,液态水含量为1 g/m3,水滴直径20μm,结冰时间6 min,温度分别为-19.4°和-28.3°时NACA0012翼型的结冰,并与相关文献结果进行了对比,计算结果与文献实验结果吻合较好,验证了方法的合理性和可靠性。分析了不同的粒径、液态水含量、来流速度等对撞击特性以及结冰的影响,随着粒径、来流速度的增加,水滴收集系数、撞击区和结冰厚度增大,随着液态水含量的增加,水滴收集系数和撞击区是不变的,但是结冰厚度增加。 相似文献
140.
All four giant planets in the solar system possess irregular satellites, characterized by large, highly eccentric and/or highly
inclined orbits. These bodies were likely captured from heliocentric orbit, probably in association with planet formation
itself. Enabled by the use of large-format digital imagers on ground-based telescopes, new observational work has dramatically
increased the known populations of irregular satellites, with 74 discoveries in the last few years. A new perspective on the
irregular satellite systems is beginning to emerge.We find that the number of irregular satellites measured to a given diameter
is approximately constant from planet to planet. This is surprising, given the radically different formation scenarios envisioned
for the gas giants Jupiter and Saturn compared to the (much less massive and compositionally distinct) ice giants Uranus and
Neptune. We discuss the new results on the irregular satellites and show how these objects might be used to discriminate amongst
models of giant planet formation. 相似文献