Prediction of forming limit curve （FLC） for AI-Li alloy 2198-T3 sheet using different yield functions

The Forming Limit Curve （FLC） of the third generation aluminum-lithium （Al-Li） alloy 2198-T3 is measured by conducting a hemispherical dome test with specimens of different widths. The theoretical prediction of the FLC of 2198-T3 is based on the M-K theory utilizing respectively the von Mises, Hill＇48, Hosford and Barlat 89 yield functions, and the different predicted curves due to different yield functions are compared with the experimentally measured FLC of 2198-T3. The results show that though there are differences among the four predicted curves, yet they all agree well with the experimentally measured curve. In the area near the planar strain state, the predicted curves and experimentally measured curve are very close. The predicted curve based on the Hosford yield function is more accurate under the tension-compression strain states described in the left part of the FLC, while the accuracy is better for the predicted curve based on Hill＇48 yield function under the tension-tension strain states shown in the right part.     

Prediction of forming limit curve (FLC) for Al-Li alloy 2198-T3 sheet using different yield functions

The Forming Limit Curve (FLC) of the third generation aluminum-lithium (Al-Li) alloy 2198-T3 is measured by conducting a hemispherical dome test with specimens of different widths. The theoretical pred...     

NMOHEMS探头模型的制作及实验方法研究

NMOHEMS探头设计的有效性及其运动的CFD仿真计算方法都需要实验进行检验,利用计算机辅助设计结合三维快速成型技术制作了探头模型,在实验室水箱和水库两种环境下设计并完成了模型实验。其中,水箱实验利用有限实验水深,精确调整探头质量,利用高速摄像和图像处理技术,对多个较小质量探头的下沉运动进行了精密测量,详细的误差分析和修正后,获得不同质量探头运动的下落曲线和极限速度,以调整CFD仿真计算方法;水库实验利用自主研制的实验装置,对较大质量探头的下沉运动进行测量,误差修正后的极限速度为1．923m／s,验证了探头设计的有效性。     

数控机床轻量化技术研究进展

随着工业技术的快速发展,对数控机床和生产系统的要求越来越多地聚焦在节能与绿色发展等问题上,这给数控机床开发人员带来了新的挑战。轻量化技术不仅能够节省大量材料,而且还能优化机床结构的性能,为高性能数控机床的研制创造了有利条件。阐述了轻量化技术在数控机床中的应用,讨论了轻量化设计方法对机床绿色循环制造及其可持续发展的影响;着重分析了实现数控机床轻量化设计目标的有效方法及技术手段,并且对轻量化技术在数控机床设计中的发展前景进行了展望,提出一些建议。     

Detached-eddy simulation of supersonic flow past a spike-tipped blunt nose

Space vehicle in atmosphere travels mostly at supersonic speed and generates a very strong bow shockwave around its blunt nose. Oblique shock and conical separated flow zone generated by a forward disk-tip spike significantly reduce the drag by reducing the high pressure area on the blunt nose. This study employs improved delayed detached eddy simulation to investigate the characteristic flow structures around a spike-tipped blunt nose at Mach number of 3 and Reynolds number(based on the blunt-body diameter) of 2.72x10~8. The calculated time-averaged quantities agree well with experimental data. Characteristic frequencies in different flow regions are extracted using fast Fourier transform. It is found that two distinct instability modes exist: oscillation mode and pulsation mode. The former is related to the foreshock/turbulence interaction with nondimensional frequency at around 0.004. The latter corresponds to the interaction between turbulence and shock structures around the blunt nose, with a typical coherent structure shedding frequency at 0.092.     

木星探测器轨道计算中的动力学

针对木星探测任务中轨道计算所面临的轨道动力学问题进行研究。首先，对木星探测轨道计算中涉及的时空参考系进行概述，比较了木星动力学时(TDJ)与质心动力学时(TDB)的差异；其次，对木星的定向参数模型及转换关系进行描述，给出了木星天球参考系与固联参考系的转换关系；再次，对木星探测器定轨计算中所需考虑的动力学模型进行讨论，提供了各类摄动加速度计算所需的公式；最后，对木星探测器JUNO的星历数据进行动力学拟合，检验了动力学模型的正确性。     

A star identification algorithm based on radial and dynamic cyclic features of star pattern

A full-sky star identification algorithm based on radial and dynamic cyclic patterns is presented with the aim of solving the “lost-in-space” problem. The dynamic cyclic pattern match is applied with a maximum cumulate comparison method to identify sensor-catalog pairings in initial match, which substantially eliminates the effects of the star position noise, magnitude noise, and false stars. After initial match pairings of stars are obtained, a chain part extension technique is employed to quickly search for the longest match chain as the final result. Experimental results indicate that the proposed algorithm is highly robust to star position noise, magnitude noise and false stars. In a series of simulations, the identification rate of the algorithm is 97.50% with 2.0 pixels star position noise, 96.90% with 0.4 Mv star magnitude noise and 95.30% with four false stars respectively. Moreover, the algorithm achieves an identification rate of 58.08% when only six stars are in the field of view.     

准静态电磁热弹性体第二类H-R型广义变分原理

应用变积方法建立了准静态电磁热弹性体的势能原理和第二类H-R型广义变分原理,并检验了变分原理的正确性,为电磁热弹多场问题的近似计算提供理论基础。     

大椭圆星载轨道预报系统设计

分析了大椭圆星载轨道预报对模型精度的要求,对大椭圆轨道动力学模型进行了合理的简化,比较了多个单步数值迭代算法的优劣,选择了适合大椭圆星载轨道预报要求的单步迭代算法,建立了大椭圆星载轨道预报系统.仿真结果验证了该预报系统的可用性与高效性.