Flutter analysis of an airfoil with bounded random parameters in incompressible flow via Gegenbauer polynomial approximation

The effects of parameter uncertainty on the flutter characteristics of a two-dimensional airfoil in an incompressible flow were investigated through Gegenbauer polynomial approximation. The uncertain parameters, such as the linear and cubic pitch stiffness coefficients are modeled as bounded random variables with λ-PDFs (probability density functions). With the aid of Gegenbauer polynomial approximation, the two-dimensional stochastic airfoil system is transformed at first into its equivalent deterministic one. Then the Hopf-bifurcation point is determined through the equivalent deterministic system, and the onset of the flutter, together with the flutter frequency against the probability density distribution parameter and the intensity of the random variable is explored. In addition, the ranges of the peak pitch and plunge responses against the flight speed and the PDFs of the peak pitch response are obtained. Numerical results show how the probability density distribution parameters and the intensities of random parameters affect the flutter onset speed, flutter angular frequency, the upper and lower boundaries of peak responses, and the PDFs of peak responses.     

顺序函数法求解二维非稳态热传导逆问题

基于有限控制体积法对二维非稳态热传导问题的数值模拟，导出了处理二维非稳态热传导逆问题的顺序函数法，并用该方法来对一典型的圆环域边界条件反演问题进行了反演计算，结果表明，顺序函数法是求解二维非稳态热传导逆问题的有效方法，当测量噪声比较小时，顺序函数法能得出较高精度的反演结果；当测量噪声增大时，反演结果仍能较好地再现出精确解在空间和时间方向上的变化趋势，具有一定精度。     

EXPERIMENTAL RESEARCH ON STRESS INTENSITY FACTOR K_Ⅲ FOR 3-D CRACK BY CAUSTICS

ＥＸＰＥＲＩＭＥＮＴＡＬＲＥＳＥＡＲＣＨＯＮＳＴＲＥＳＳＩＮＴＥＮＳＩＴＹＦＡＣＴＯＲＫⅢＦＯＲ３┐ＤＣＲＡＣＫＢＹＣＡＵＳＴＩＣＳＷｕＤａｆａｎｇ，ＧａｏＺｈｅｎｔｏｎｇ（ＩｎｓｔｉｔｕｔｅｏｆＳｏｌｉｄＭｅｃｈａｎｉｃｓ，ＢｅｉｊｉｎｇＵｎｉｖｅ...     

月面巡视器太阳能帆板功率衰减特性研究

太阳能帆板的功率衰减特性分析,对地外天体表面探测器的功率平衡、电源系统健康管理以及长寿命在轨管理有重要意义。通过对月面巡视器在轨运行第2到11月昼的电流遥测进行研究,提出了一种基于有限遥测的太阳能帆板功率衰减特性分析方法。首先利用一种滞环的方法对大量的电流遥测进行数据处理;然后进行日月距离和太阳入射角的归一化,通过数据拟合计算,得出落月第一年太阳能帆板功率衰减约为2.5%,并利用巡视器历次月昼唤醒时刻的太阳入射角变化情况验证了该方法的有效性,对地外天体的太阳能帆板功率衰减特性计算提供一定参考。     

试论高等数学教学与 CAI

阐述了ＣＡＩ在数学教学中的重要作用，以实例说明了在ＣＡＩ实验课教学中应注意的几个方面，并对目前数学ＣＡＩ教学所面临的问题进行了探讨     

超声速条件下多体干扰与分离试验研究

采用根据国外公开文献设计的类CAV模型,在0．6m×0．6m 跨/超声速风洞中开展了多体干扰与分离网格测力试验研究,初步获得了典型多体飞行器分离过程中的气动特性变化规律。试验结果表明,载荷模型气动特性受分离位置变化影响非常明显。载荷模型沿轴向分离时,气动力（矩）逐步接近自由流中气动力（矩）值,载荷模型法向位置改变会引发其气动力（矩）值发生更为剧烈的变化。引发这种现象的原因有两个：一是尾迹和头激波的发展改变了不同轴向位置处载荷模型的表面流态,从而影响了其气动特性;二是母机模型底部流动具有明显的非对称膨胀特征,不同法向位置处流速大小和方向差异明显,导致载荷模型气动特性随法向位置变化更为剧烈。     

高速加工HSK工具系统的力学模型

根据HSK工具系统的结构和工作机理建立了HSK工具系统的力学模型,分析了影响工具系统刚度的主要因素和载荷与加工质量之间的关系,揭示出HSK工具系统刚度变化的基本规律,理论分析结果与实验结果吻合.在此基础上,提出评估工具系统的性能不仅要考虑工具系统的静刚度,而且要进一步考虑工具系统的动刚度.最后,给出了HSK工具系统型号的选择原则,并建立了相应的优化操作条件.     

Response of Hainan GPS ionospheric scintillations to the different strong magnetic storm conditions

Using the GPS ionospheric scintillation data at Hainan station (19.5°N, 109.1°E) in the eastern Asia equatorial regions and relevant ionospheric and geomagnetic data from July 2003 to June 2005, we investigate the response of L-band ionospheric scintillation activity over this region to different strong magnetic storm conditions (Dst < −100 nT) during the descending phase of the solar cycle. These strong storms and corresponding scintillations mainly took place in winter and summer seasons. When the main phase developed rapidly and reached the maximum near 20–21 LT (LT = UT + 8) after sunset, scintillations might occur in the following recovery phase. When the main phase maximum occurred shortly after midnight near 01–02 LT, following the strong scintillations in the pre-midnight main phase, scintillations might also occur in the post-midnight recovery phase. When the main phase maximum took place after 03 LT to the early morning hours no any scintillation could be observed in the latter of the night. Moreover, when the main phase maximum occurred during the daytime hours, scintillations could also hardly be observed in the following nighttime recovery phase, which might last until the end of recovery phase. Occasionally, scintillations also took place in the initial phase of the storm. During those scintillations associated with the nighttime magnetic storms, the height of F layer base (h’F) was evidently increased. However, the increase of F layer base height does not always cause the occurrence of scintillations, which indicates the complex interaction of various disturbance processes in ionosphere and thermosphere systems during the storms.     

一种非均匀面阵单快拍自适应处理方法

提出一种基于虚拟阵列内插技术的非均匀面阵单快拍自适应处理方法。首先,通过虚拟阵列内插技术将非均匀面阵转化为均匀面阵,继而采用均匀面阵的单快拍方法对其进行自适应处理,从而突破了非均匀面阵单快拍处理瓶颈,实现了期望信号恢复和干扰置零。最后,通过仿真实验对方法进行性能验证。     

带通FSS结构的插入相位延迟特性

基于互导纳法研究实心半波壁频率选择表面(Frequency selective surface,FSS)的插入相位延迟(Insertion phase delay,IPD)特性,考察FSS结构的IPD与加载介质的IPD之间的关系,分析了介质厚度、极化状态等因素的影响,重点关注交叉极化状态,考察极化角及入射角变化时的去极化效应.结果表明,解决带通FSS结构交叉极化问题的方法是保证TE和TM两种主极化状态下谐振频率的一致性,从而减小两种极化状态的IPD之差.