Revisiting the space-time gradient method: A time-clocking perspective,high order difference time discretization and comparison with the harmonic balance method

This paper revisits the Space-Time Gradient(STG) method which was developed for efficient analysis of unsteady flows due to rotor–stator interaction and presents the method from an alternative time-clocking perspective. The STG method requires reordering of blade passages according to their relative clocking positions with respect to blades of an adjacent blade row. As the space-clocking is linked to an equivalent time-clocking, the passage reordering can be performed according to the alternativ...     

单向电永磁作动器结构优化与动态特性分析

针对电磁作动器的使用要求,设计出一种具有能耗低、吸力大及响应快等特点的新型单向电永磁作动器。结合有限元仿真软件,利用有限元法研究作动器的结构参数如铁芯齿形结构、平面结构、无永磁结构、铁芯的倾斜角度及衔铁位移（气隙厚度）等因素对作动器电磁吸力和响应速度的影响。结果表明,电磁吸力随着作动衔铁位移的增加而大幅度减小;倾角结构的铁芯设计能使作动器性能达到最佳,且铁芯的倾斜角度为50°时,电磁吸力有最大值3071N。     

基于PIV速度场测量的压强梯度计算

介绍了基于PIV速度场测量结果计算压强梯度的基本原理和3种不同的计算方法,并通过对流高斯涡模型系统研究了离散格式选取、PIV参数设置和流场特征等对压强梯度计算的影响.结果表明:PIV速度测量的精度是压强梯度计算的关键性影响因素,1%噪声对结果的影响比其他过程高约2个数量级;时间分辨率和空间分辨率的设置并非越高越好,而是有个合适的中间值;拉格朗日方法在大多数情况下优于欧拉方法,但当流动结构较复杂时性能较差,应根据流动类型和流场特征合理选取压强梯度计算方法.      

缺口件疲劳寿命预测新方法

采用有限元方法针对缺口件多轴疲劳实验结果进行模拟。结果表明,相同路径条件下,随着缺口半径减小缺口根部附近的应力梯度显著增加。基于缺口根部应变值,采用等效应变法进行疲劳寿命预测,预测结果随缺口半径的减小而偏于保守。采用应力梯度法确定有效距离,相同路径下,随着缺口半径的减小有效距离减小;依据该有效距离处的等效应变进行疲劳寿命预测,总体预测结果较为分散且偏于不安全。基于实验及有限元模拟结果,提出了基于应变梯度的有效距离确定的新方法,大部分疲劳寿命预测结果位于2倍分散带内。     

Mesh-dependence of Material with Softening Behavior

The issue of mesh-dependence emerges when the conventional continuum damage model is applied to handling the softening behavior. In order to circumvent the mesh-dependence, the non-local theory is introduced into the conventional damage model and the finite element formulas are derived for two-dimensional gradient-enhanced damage model. A new element is proposed in which the basic unknown quantities are displacement, non-local equivalent strain and the gradient of non-local equivalent strain. The element and constitutive equation proposed in this article are added to the finite element software ABAQUS through user subroutine UEL. Numerical results show that the gradient-enhanced damage model can eliminate the mesh-dependence and is effective for dealing with the issue of softening behavior.     

The effects of the solar magnetic polarity and the solar wind velocity on Bz-component of the interplanetary magnetic field

We have studied the effect of both solar magnetic polarity and the solar wind velocity on the Bz-component of the interplanetary magnetic field, IMFBz, for the minimum activity of the solar cycles 21, 22, 23 and 24. We made a statistical study of IMFBz in the first section which is considered as an extension of Lyatsky et al. (2003). They made a statistical study of IMFBz for two periods of minimum solar activity 22 and 23 related to 1985–1987 and 1995–1997 when the solar magnetic field had opposite polarity. Our results seem to be consistent with the results obtained by Lyatsky et al. (2003). We found that there is a dependence of IMFBz on the IMFBx and the solar magnetic polarity for the minimum periods of the selected four solar cycles. In addition, we found that there is a dependence of IMFBz on the solar wind velocity.     

终端区点融合进近程序设计方法研究

流量的增长导致终端区拥挤和航班延误,增大了管制压力和公司成本.以长沙黄花国际机场36号跑道为例,空城受限,4条航线汇聚一点,梯度曲折多变,航班排序难,指挥复杂度高.结合我国飞行程序设计和管制间隔要求,根据点融合的基本概念,设计跑道点融合进近程序,确定相关参数.对程序进行容量和下降梯度评估表明,静态容量可达到63架次/h,是当前运行最大流量的3.7倍;下降梯度得到明显改善,为连续下降实施奠定了基础.     

Solar flare forecasting model supported with artificial neural network techniques

Nowadays operational models for solar activity forecasting are still based on the statistical relationship between solar activity and solar magnetic field evolution. In order to set up this relationship, many parameters have been proposed to be the measures. Conventional measures are based on the sunspot group classification which provides limited information from sunspots. For this reason, new measures based on solar magnetic field observations are proposed and a solar flare forecasting model supported with an artificial neural network is introduced. This model is equivalent to a person with a long period of solar flare forecasting experience.     

磁转速表指针摆动的故障分析

就磁转速表活动系统的动态特性以及在附加交变力矩的作用下，指针摆动随转速变化的规律，从理论上进行了分析，并结合实际探讨了指针摆动的故障原因。     

The evolution of mirror type magnetic fluctuations in the magnetosheath based on multipoint observations

Two orbits were selected in January–February 2006 when the separation between the Cluster spacecraft was large and mirror type magnetic field fluctuations were observed by all spacecraft in different regions of the terrestrial magnetosheath. Minimum variance analysis was applied to find the mirror type fluctuations, and the amplitude of the fluctuations was determined individually. Mirror mode structures are moving along the streamlines frozen in the plasma. A model was developed for the calculation of plasma flowtime from the bow shock to the observation point. The growth rate of the field strength perturbations was estimated by comparing the amplitudes of fluctuations observed simultaneously at distant locations (∼10,000 km) based on the assumption that δB ∼ exp(γt). The obtained growth rate values were about an order of magnitude smaller than those provided by linear models and they decreased in the inner regions of the magnetosheath, indicating some saturation in the growth of the waves when proceeding towards the magnetopause. The results of these two case studies suggest that mirror type fluctuations originate from the compression region downstream of the quasi-perpendicular bow shock, and the growth of the fluctuations cannot be described by linear approximations.