Modeling and data analysis of a Forbush decrease

We study the Forbush decrease of the galactic cosmic ray intensity observed in 9–25 September 2005 using the experimental data and a newly developed time-dependent three dimensional modeling. We analyze neutron monitors and muon telescopes, and the interplanetary magnetic field data. We demonstrate a clear relationship between the rigidity (R) spectrum exponent (γ) of the Forbush decrease and the exponent (ν) of the power spectral density of the components of the interplanetary magnetic field in the frequency range of ∼ 10⁻⁶–10 ⁻⁵ Hz. We confirm that an inclusion of the time-dependent changes of the exponent ν makes the newly developed nonstationary three dimensional model of the Forbush decrease compatible with the experimental data. Also, we show that the changes of the rigidity spectrum exponent γ does not depend on the level of convection of the galactic cosmic rays stream by solar wind; depending on the changes of the exponent ν, i.e. on the state of the turbulence of the interplanetary magnetic field.     

一种近壁理论湍流模型初探

在传统的k-ε湍流模型基础上,在近壁区放弃求解ε方程而代之以根据共振三波理论模型在近壁区系统计算的ε值构成封闭,通过对NACA0012二维翼形流场的计算,初步验证并适当修正了新的理论模型,由于注意到了理论模型计算结果的无量纲性,从而改善了该流场的计算结果,得到了与实验更为相符的C_p分布。本文的分析还表明,逆压力梯度对ε的影响非常显著,验证了理论分析和计算得到的结论。      

前缘形状对涡轮叶栅损失影响的机理

通过改变前缘几何形状来分析其在设计攻角、非设计攻角下前缘附近的流动机理.研究结果表明:在宽工况范围内椭圆型前缘表现出了较优越的性能,不但在设计攻角下能很好抑制吸力峰的强度以避免前缘分离泡的产生,而且在较宽的攻角范围内都能保证前缘附近边界层状态基本不变.当正攻角很大时,不同前缘形状前缘附近都会出现分离泡,且会诱导边界层发生转捩,但椭圆型前缘边界层开始发生转捩的攻角会向大攻角方向移动.在20°攻角下,椭圆型前缘叶型的损失相比基准叶型下降了7%左右.进口湍流度的增加不会改变吸力峰的强度但可以减弱前缘分离泡的强度.     

大气边界层风洞流场特性的模拟

风洞中大气边界层模拟的准确度是保证风洞试验结果准确度的重要因素。本文采用了一种新型曲边梯形尖塔,并结合粗糙元等被动装置对风洞大气边界层模拟进行了研究,模拟出我国规范中的A、B、C和D类四种地貌并将结果和已有的研究结果进行比较。结果显示：所采用新型结构尖塔可以显著提高风洞大气边界层中部以上高度的湍流度,整个湍流度剖面基本覆盖了西方主要国家规范对此项指标的建议值。文中还调试出平均风速剖面不变而湍流度分布可变的流场,为开展相关的结构抗风研究奠定了基础。     

轴流压气机静子角区分离流动的DDES数值研究

为进一步加深对压气机静子角区分离流动非定常性和湍流特性的认识,以某台用于低速模拟的多级低速轴流压气机的第3级改型静子为研究对象,采用延迟脱落涡模拟(DDES)方法进行详细的数值研究.结果表明:压气机静子角区分离流动受到叶片几何参数和来流条件的综合影响;通道涡是引起静子角区分离的主要涡系结构,其发展过程伴随着大小尺度发簪...     

A three-equation transition model with mechanical considerations

A three-equation transition model based on the transition V-model is proposed for subsonic flows in this study. Considering the mechanical approximation of the generation process of the pre-transitional vorticities, the value of laminar Reynolds shear stress related to the mean shear deformation was calculated in the original transition V-model. Then a new transition model, named V-SA model, was proposed, which considered the phenomenological process of transition and presented great results for flows with and without pressure gradient. It is well-known that the baseline Shear Stress Transport (SST) turbulence model shows excellent performance of accuracy and robustness in plentiful flow cases, but it is important to predict boundary layer transition. The current model (V-SST) successfully couples the V-model to the SST turbulence model by introducing the effective turbulent viscosity and additional correction terms into the transport equations. A thorough evaluation of its ability to predict transition features is performed versus the well-documented flat plate of ERCOFTAC, including T3A and T3B without pressure gradient, T3L2 and T3L3 with semi-circular leading edge, the three-dimensional 6:1 prolate-spheroid under two angles of attack, and the NLR-7301 airfoil under different Mach numbers. Numerical results show that the current model has an attractive and superior performance in the simulation of boundary layer transition processes     

Ka频段双极化低剖面卫通相控阵天线

当前国内外低轨通信互联网星座发展迅猛，面向卫通天线跨星跨波束快速切换、低剖面应用需求，提出了一种Ka频段层叠式缝隙耦合双圆极化发射相控阵天线。基于多层PCB叠层瓦式架构，将天线层、电源与控制层、功分网络层和芯片层一体化集成。基于“双线极化天线+移相控制”设计实现左右旋圆极化及其极化切换，采用子阵相位旋转排布实现天线整阵二次圆极化。测试结果表明：天线工作频段为27.5~31GHz，29.2GHz处法向等效各向同性辐射功率值为16.5dBW，可实现±60°扫描，法向轴比＜2dB，左右旋圆极化可切换，天线子阵厚度3mm。相比传统砖式相控阵天线，大幅降低了剖面和重量，对卫通天线低剖面、波束快速切换等具有重要应用意义。     

Bayesian uncertainty analysis of SA turbulence model for supersonic jet interaction simulations

The Reynolds Averaged Navier-Stokes(RANS) models are still the workhorse in current engineering applications due to its high efficiency and robustness. However, the closure coefficients of RANS turbulence models are determined by model builders according to some simple fundamental flows, and the suggested values may not be applicable to complex flows, especially supersonic jet interaction flow. In this work, the Bayesian method is employed to recalibrate the closure coefficients of Spalart-Allma...