各向异性板料成形极限面的研究

成形极限曲线(FLD)是表示板料成形性能的重要指标。由于板料各向异性的存在,导致了使用1条FLD来表示板料整个面内的成形极限存在很大误差。通过试验分析了板料面内的各向异性对板料应力和应变成形极限曲线的影响,研究了利用三维空间的成形极限曲面代替二维坐标下的FLD来表示材料整个面内的成形极限的方法,经过分析认为板料成形极限面可以为板料成形有限元仿真提供更准确的成形极限判据。     

气液针栓喷注单元雾化角模型

为了准确预测气液针栓喷注单元的雾化角,基于动量守恒建立了液束撞击气膜的雾化角理论模型,通过试验结果获得变形因子,并分析了结构参数和工况参数对雾化角的影响规律.结果表明:局部动量比对雾化角影响最大,其他结构参数和工况参数都是通过影响局部动量比而进一步决定雾化角;随着局部动量比增大,液束变形程度减小,液束变形导致有效撞击动...     

钣金件快速精确加工中的激光切割工艺分析

针对δ0．5mm～δ6mm钣金件的结构特点,通过比较常用加工工艺和激光切割过程工艺．选出适合实际的优化方案。验证了不同切割参数对切割质量的影响。在工艺参数为：脉冲功率2．4kW、脉冲宽度约10ms、功率密度10^7W/cm^2的情况下,激光切割δ0．5mm～δ6mm钣金件获得了良好的切割质量,尺寸精度控制在误差（±100μm）范围内。工艺方案合理,生产率高。     

轧波胀形成形工艺应用研究

介绍了轧波成形+胀形的工艺过程、设备原理及技术改进.首先用轧波成形制出工件的大概形状,然后再用胀形工艺校圆.该成形方法不仅要求工装简单,而且成形精度较高,适用于旋转环形钣金零件.     

固定管板式换热器的危险工况分析和管、壳应力在设计中的作用

本文在前文的基础上,阐明危险工况(或称可能出现的危险工况)和真正危险工况之间的区别和联系,仅由操作条件只能列出危险工况而无法得出真正的危险工况,真正的危险工况不仅和操作条件有关,而且和换热器的结构条件和各部件相对尺寸有关。 根据换热器的具体结构条件、各元件相对尺寸和危险工况,管板、管子或壳体应力的最大值都有可能首先超过各自的强(刚)度校核条件。所以,在设计时不论管板、管子或壳体都应由各个危险工况求出其可能出现的最大应力值并校核满足,不能以并非最大的应力值进行校核,更不能因管子或壳体应力(特别是带有膨胀节时)绝对值较低而认为其强度不会成为问题,甚至不予计算。     

我国利润表编制中存在的问题与改进

文章论述了利润表设计的理论依据,通过我国利润表同国外利润表比较,发现我国利润表的编制基础对会计信息的陈报存在不利影响,并结合实际情况,提出了未来利润表改进办法.     

The plasma sheet and boundary layers under northward IMF: A multi-point and multi-instrument perspective

During conditions of northward interplanetary magnetic field (IMF), the near-tail plasma sheet is known to become denser and cooler, and is described as the cold-dense plasma sheet (CDPS). While its source is likely the solar wind, the prominent penetration mechanisms are less clear. The two main candidates are solar wind direct capture via double high-latitude reconnection on the dayside and Kelvin–Helmholtz/diffusive processes at the flank magnetopause. This paper presents a case study on the formation of the CDPS utilizing a wide variety of space- and ground-based observations, but primarily from the Double Star and Polar spacecraft on December 5th, 2004. The pertinent observations can be summarized as follows: TC-1 observes quasi-periodic (∼2 min period) cold-dense boundary layer (compared to a hot-tenuous plasma sheet) signatures interspersed with magnetosheath plasma at the dusk flank magnetopause near the dawn-dusk terminator. Analysis of this region suggests the boundary to be Kelvin–Helmholtz unstable and that plasma transport is ongoing across the boundary. At the same time, IMAGE spacecraft and ground based SuperDARN measurements provide evidence of high-latitude reconnection in both hemispheres. The Polar spacecraft, located in the southern hemisphere afternoon sector, sunward of TC-1, observes a persistent boundary layer with no obvious signature of boundary waves. The plasma is of a similar appearance to that observed by TC-1 inside the boundary layer further down the dusk flank, and by TC-2 in the near-Earth magnetotail. We present comparisons of electron phase space distributions between the spacecraft. Although the dayside boundary layer at Polar is most likely formed via double high-altitude reconnection, and is somewhat comparable to the flank boundary layer at Double Star, some differences argue in favour of additional transport that augment solar wind plasma entry into the tail regions.     

Ring Current Dynamics

This chapter reviews the current understanding of ring current dynamics. The terrestrial ring current is an electric current flowing toroidally around the Earth, centered at the equatorial plane and at altitudes of ∼10,000 to 60,000 km. Enhancements in this current are responsible for global decreases in the Earth’s surface magnetic field, which have been used to define geomagnetic storms. Intense geospace magnetic storms have severe effects on technological systems, such as disturbances or even permanent damage of telecommunication and navigation satellites, telecommunication cables, and power grids. The main carriers of the ring current are positive ions, with energies from ∼1 keV to a few hundred keV, which are trapped by the geomagnetic field and undergo an azimuthal drift. The ring current is formed by the injection of ions originating in the solar wind and the terrestrial ionosphere into the inner magnetosphere. The injection process involves electric fields, associated with enhanced magnetospheric convection and/or magnetospheric substorms. The quiescent ring current is carried mainly by protons of predominantly solar wind origin, while active processes in geospace tend to increase the abundance (both absolute and relative) of O⁺ ions, which are of ionospheric origin. During intense geospace magnetic storms, the O⁺ abundance increases dramatically. This increase has been observed to occur concurrently with the rapid intensification of the ring current in the storm main phase and to result in O⁺ dominance around storm maximum. This compositional change can affect several dynamic processes, such as species-and energy-dependent charge-exchange and wave-particle scattering loss.     

细长锥体有攻角绕流的非对称分岔及其涡结构的数值模拟

本文用ＮＮＤ格式计算了具有复杂涡结构的细长锥体有攻角绕流问题，着重研究了非对称分离的分岔现象以及分岔前后涡结构的演变，数值计算结果表明，大约在ａ／（２β）＝１．０时，Ｎ－Ｓ方程出现分岔解，同时还给出了分岔前后涡结构及物理最分布的特征。     

周期性多电流片系统中涡旋诱发重联过程的相互作用

运用二维可压缩磁流体动力学(MHD)模拟方法考察了周期性多电流片系统中涡旋诱发重联(VIR)过程的发展演化.结果表明,相邻电流片中的VIR过程发生相互作用,相距越近,作用越强烈.反对称和对称波模VIR过程的线性增长率随电流片间距的减小而分别增大和降低.当电流片间距小于某临界值时,反对称波模VIR完全被抑制.相对于对称波模VIR,反对称波模VIR过程对空间多电流片系统的发展会发挥更大作用.