磁粉探伤机周向电流单片微机控制器的研制

本文介绍一种新型磁粉探伤机周向电流的单片计算机控制器，文中详细介绍控制器的控制原理，结构，控制程序。该控制器对周向电流采用闭环控制，直接设定磁化电流，可保证电流稳定，电流设定值和实际电流值相差小于１０％，控制器还具有了出错检测，自动退磁功能。     

板料应力成形极限判据的有限元分析程序

为了解决在板料成形有限元数值模拟中以依赖于加载路径的应变成形极限为判据所存在的问题,以板料塑性变形时所遵循的应力应变转换关系、H ill二次厚向异性准则为计算模型,基于有限元商用分析软件DYNAFORM,开发了用于板料塑性成形工艺的以应力成形极限为判据的有限元分析程序。利用该程序分析了两种拉深件的有限元数值模拟结果,实现了用应力成形极限图作为判据对板料成形极限的预测分析。所开发的以应力成形极限作为判据的有限元分析程序为分析多道次板成形的成形极限提供了新的手段。     

紧凑热交换器优化设计

对各种传热表面的板翅式紧凑热交换器进行了优化设计计算，建立了通用优化程序系统。此程序既适用于一般地面热交换器，也适用于飞机空调中的热交换器。与传统的设计计算相比较，优化设计的效果很好。热交换优化后，肋片的形状变得更加合理，芯体传热表面更加紧。通过各种肋片的计算得出，条状肋片为板翅式肋片中的最佳者。     

空间等离子体导致高电压太阳阵的电流收集

给出一种能方便计算空间等离子体引起高电压太阳阵（HVSA）电流收集的理论统计模式，通过对物理过程分析认为空间等离子体致HVSA的功率损耗对HVASA的设计是不应忽视的。     

气泡和液滴在上升或下降时大变形的数值模拟

本文在考虑界面张力的条件下用涡片方法导出了二维无粘气泡和液滴在另一种静止无粘流体中上升或下降时运动和变形的支配方程，提出了求解支配方程的数值方法，并在数值模拟的例子中研究了空气泡和煤油滴在水中上升时及水滴在煤油中下降时的变形规律，研究了数值模拟中界面张力对界面形状的影响，气泡上升的数值模拟结果与相应的试验结果基本一致。数值模拟结果表明本方法可正确模拟饣泡和液滴在上升或下降过程中的大变形，直到界面发     

硬铝合金预拉伸、热处理后成形性能的正交试验研究

在铝合金实际成形工艺的基础上通过正交试验研究了成形过程的各个因素:热处理前的变形、试件取样拉伸方向、时效时间及材料厚度对淬火后铝合金各成形性能指标的影响,得到了这些因素对材料各个性能指标的影响规律和新淬火状态下铝合金成形性能的特点,指出了热处理后材料的变形效应并没有消失,甚至依然显著地影响着某些成形性能,给出了2D12铝合金板料在新淬火状态下的本构关系,为成形工艺的制定及数值模拟分析提供了依据。     

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.     

流动显示的现状和发展

本文以第四届国际流动显示会议为主要内容,结合其它资料介绍流动显示的现状和发展。     

金属板料的激光冲击变形分析及其实验研究

介绍了激光冲击变形机理和冲击波产生原因,并建立了激光冲击下的板料变形模型,且推导了板料变形量计算公式。根据爆轰波和爆炸气体动力学理论,建立了激光冲击成形中激光-能量转换体-靶材系统爆轰波压力的估算式,并根据冲击波压力估算式估算所需激光脉冲能量,从而探讨了板料变形与激光能量、冲击波压力之间的关系,并进行实验研究。实验结果表明,板料厚度对变形量的影响与变形理论模型的分析基本相同,其变形量随厚度的增加而呈指数曲线减小,其轮廓形状也由小圆锥形逐渐向小球冠状变化。     

Fractal Structure of the Heliospheric Plasma Sheet at the Earth''''s Orbit

An analysis of the data from the Wind and IMP-8 spacecraft revealed that a slow solar wind, flowing in the heliospheric plasma sheet, represents a set of magnetic tubes with plasma of increased density (N > 10cm-3 at the Earth's orbit). They have a fine structure at several spatial scales (fractality), from 2°-3°(at the Earth's orbit, it is equivalent to 3.6-5.4h, or (5.4-8.0)×106km) to the minimum about 0.025°, i.e. the angular size of the nested tubes is changed nearly by two orders of magnitude. The magnetic tubes at each observed spatial scale are diamagnetic, i.e. their surface sustains a flow of diamagnetic (or drift) current that decreases the magnetic field within the tube itself and increases it outside the tube. Furthermore, the value of β= 8π[N(Te + Tp)]/B2 within the tube exceeds the value of βoutside the tube. In many cases total pressure P = N(Te + Tp) + B2/8πis almost constant within and outside the tubes at any one of the aforementioned scales.