异种金属材料磁脉冲焊接技术

通过对磁脉冲焊接技术结合机理的阐述,采用5A03Al-5A06Al、1050Al-AZ31Mg异种金属材料进行焊接试验.对所得的焊接接头进行气密性试验和剥离试验,检测其结合质量;结合光学显微镜,对比分析Al-Al、Al-Mg焊接接头的微观形貌特点;并采用SEM/EDS分析界面附近的元素分布;最后通过硬度试验,检测接头界...     

高精度光纤IMU的磁屏蔽方法及实验研究

惯性测量单元(IMU)是位置姿态系统(POS)的核心部分,IMU的精度很大程度上决定着POS精度.由于高精度光纤陀螺(FOG)的光纤线圈对磁场敏感,基于高精度FOG的IMU精度会受磁场影响而降低.本文研究了FOG磁敏感性机理,通过实验得出高精度光纤IMU对磁场敏感的结论.采用电磁场有限元分析软件Ansoft Maxwe...     

复合材料波纹板剪切载荷作用下的屈曲试验与分析

复合材料波纹板稳定性是飞机机翼结构设计需要考虑的重要方面,是目前飞机结构设计中的一大难点.为了建立波纹板屈曲的数值分析方法,对复合材料波纹板在剪切载荷作用下的屈曲进行试验、工程算法和有限元方法研究.通过试验,探索了3种不同波长的复合材料波纹板的屈曲载荷和破坏载荷;采用工程算法和有限元方法计算了8种不同波长的复合材料波纹...     

非牛顿流体在正弦波壁管内的减阻特性

通过添加高分子表面活性剂来有效降低流动阻力在水处理和石油开采等行业中具有重要的现实意义。实验研究了聚丙烯酰胺聚合物（PAM）溶液在正弦波壁管内的减阻特性。研究发现,PAM溶液在层流区域具有明显的减阻作用,在湍流区域却不是很明显;同时在波壁管内存在一个PAM的最佳减阻浓度。另外,通过f-Re曲线发现PAM溶液的过渡域转捩点比牛顿流体明显提前,流动可视化结果验证了上述结论;应用Fluent进行数值模拟得到的数值结果与实验基本吻合。     

轴流压气机子午流面计算中三维剪切作用的湍流模型

本文发展了一个轴流压气机子午流面二维计算中模拟三维剪切结构对子午流场作用的湍流模型。试验与这一模型进行了初步的比较。模型表明,在多级轴流压气机子午流场计算中,必须计入实际流场三维剪切结构对子午流场的湍流扩散作用。     

超声速自由剪切层流动的数值模拟和理论分析

本文从二维完全Ｎ－Ｓ方程出发，采用ＮＮＤ２Ｍ差分格式，计算了超声速自由剪切层流场，并且研究了上游扰动在剪切层内的传播规律。在数值模拟的基础上对流动涡结构进行了分析。     

复合材料面内剪切Iosipescue方法分析及试验研究

讨论了采用双Ｖ形开槽试样的Ｉｏｓｉｐｅｓｃｕ剪切试验方法的应用，分析了影响试验的因素，对Ｔ３００／５２２２复合材料单向板及π／４多向铺层层合板进行了试验研究。试验结果表明，此方法可以很好地用于复合材料剪切试验。     

一种精化的层合梁脱层模型

建立了一种精化的复合材料层合梁脱层模型。脱层梁被分为3个区,各区位移场为厚度坐标的三次函数,能满足层间位移和剪应力的连续条件、脱层界面的脱层条件和脱层边界点的位移连续条件。构造了其有限元模型。算例表明该模型较之基于经典理论和一阶剪切变形理论的脱层模型精度显著提高。     

Relationship Between Substorm Auroras and Processes in the Near-Earth Magnetotail

Although the auroral substorm has been long regarded as a manifestation of the magnetospheric substorm, a direct relation of active auroras to certain magnetospheric processes is still debatable. To investigate the relationship, we combine the data of the UV imager onboard the Polar satellite with plasma and magnetic field measurements by the Geotail spacecraft. The poleward edge of the auroral bulge, as determined from the images obtained at the LHBL passband, is found to be conjugated with the region where the oppositely directed fast plasma flows observed in the near-Earth plasma sheet during substorms are generated. We conclude that the auroras forming the bulge are due to the near-Earth reconnection process. This implies that the magnetic flux through the auroral bulge is equal to the flux dissipated in the magnetotail during the substorm. Comparison of the magnetic flux through the auroral bulge with the magnetic flux accumulated in the tail lobe during the growth phase shows that these parameters have the comparable values. This is a clear evidence of the loading–unloading scheme of substorm development. It is shown that the area of the auroral bulge developing during substorm is proportional to the total (magnetic plus plasma) pressure decrease in the magnetotail. These findings stress the importance of auroral bulge observations for monitoring of substorm intensity in terms of the magnetic flux and energy dissipation.     

Geoeffectivity of Coronal Mass Ejections

Coronal mass ejections and post-shock streams driven by them are the most efficient drivers of strong magnetospheric activity, magnetic storms. For this reason there is considerable interest in trying to make reliable forecasts for the effects of CMEs as much in advance as possible. To succeed this requires understanding of all aspects related to CMEs, starting from their emergence on the Sun to their propagation to the vicinity of the Earth and to effects within the magnetosphere. In this article we discuss some recent results on the geoeffectivity of different types of CME/shock structures. A particularly intriguing observation is that smoothly rotating magnetic fields within CMEs are most efficient in driving storm activity seen in the inner magnetosphere due to enhanced ring current, whereas the sheath regions between the shock and the ejecta tend to favour high-latitude activity.