基于Event的侧向碰撞风险改进模型

Event模型是一种基于长方体碰撞模板的碰撞风险评估模型,用该模型评估所得的碰撞风险概率过于保守。将碰撞模板改为圆柱体,建立了基于碰撞圆柱体的Event模型。在相同条件下运用Event模型和改进的Event模型对平行航路的侧向碰撞风险进行了评估计算,后者的碰撞风险是原Event模型碰撞风险的86.9％,仿真结果表明改进模型碰撞风险评估更精确,能够为中国平行航路的开辟进行安全评估计算提供理论依据。     

飞机钣金零件展开计算方法的研究和应用现状

分析了飞机钣金零件展开的复杂性,按照飞机钣金零件的结构和成形分类,对钣金零件展开计算方法进行了综述和归类,在此基础上提出了典型飞机钣金零件数字化展开计算方法的解决思路。     

引导场对无碰撞电流片低频电磁不稳定性的影响

通过数值求解无碰撞电流片中可压缩磁流体力学模型下得到的一般形式的色散关系,讨论了无碰撞电流片中引导场对低频电磁波不稳定性的影响.结果表明,平衡态磁场中的引导场,对于三维扰动传播的波不稳定性有很强的影响.(1)在电流片中间平面上(z=0),无引导场时,没有不稳定性发生,但若存在引导场,不稳定性便发生,并随着引导场的增强,不稳定性明显增强,不稳定的波模可能是低混杂模.(2)在中间平面附近(z=0.2),电流片是不稳定的.随着引导场的增强,不稳定性增长率明显地增强,不稳定的波模从平行和反平行两个方向传播变为反平行方向一个方向传播,并且是斜传播的,具有低频哨声模或低混杂模的特征.(3)在电流片边缘附近(z=0.8),引导场对不稳定的波模和增长率没有明显影响,不稳定的波模都是准平行的哨声波.      

管子与管板的联接方式述评

文章对换热器中管子和管板的几种常用联接方式从制造、使用及维修的角度进行了分析、比较。指出液袋胀接是一种很有发展前途的胀接技术,粘胀联接和螺纹联接各有独到的优越性。     

铝合金薄板K_c测试新方法的探讨

通过用圆(或椭圆)孔试件测量金属薄板平面应力断裂韧性Kc的方法,与通过用中心穿透裂纹试件Kc的标准方法相比较之后,将Whitney和Nuismer用于复合层压板中的点应力破坏准则,推广到铝合金薄板Kc的测量。 在理论和实验分析的基础上,拟合出与实验结果相一致的经验公式。     

子午面内Alfvén波的传播特征

本文使用由ＷＫＢ近似得到的Ａｌｆｖｅｎ波传播的张量表达式,具体计算和讨论了一种太阳子午面内含盔形－电流片磁位形的流场中Ａｌｆｖｅｎ波的传播特征,主要结果是：（１）Ａｌｆｖｅｎ波磁场起伏随日心距离的增加而衰减,其中极开区的衰减远快于赤道区,但随着距离的增大,这种纬度关系将迅速变弱,以致在较远空间,磁起伏相差很小,衰减很慢;（２）Ａｌｆｖｅｎ波的相对磁场起伏ｂ／Ｂ随着距离的增加而迅速增大,在几个太阳半径之后变化不再明显,达到所谓的＂饱和＂;在大日心距离的盔形电流片附近,Ａｌｆｖｅｎ波将成为重要的磁场组成部分;（３）Ａｌｆｖｅｎ波速度起伏纬度关系较为明显,相对速度起伏。ｕ／Ｕ随着距离增大而衰减,电流片区衰减得较快,但这种纬度差别将变弱．与黄道面内Ａｌｆｖｅｎ波传播特征的具体比较表明,磁场涨落的变化特征与背景场位形存在着十分密切的关系,但速度涨落与背景场没有这种明显关系．     

方板对角拉伸诱导压应力的分析

利用有限元法分析方板在单向和双向对角拉伸条件下诱导压应力的变化规律。计算和实验表明,施加横向拉力,实现双轴向拉伸,能明显减小横向诱导压应力及其分布范围,从而抑制皱曲的发生和发展。     

Kink-like mode of a double gradient instability in a compressible plasma current sheet

A linear MHD instability of the electric current sheet, characterized by a small normal magnetic field component, varying along the sheet, is investigated. The tangential magnetic field component is modeled by a hyperbolic function, describing Harris-like variations of the field across the sheet. For this problem, which is formulated in a 3D domain, the conventional compressible ideal MHD equations are applied. By assuming Fourier harmonics along the electric current, the linearized 3D equations are reduced to 2D ones. A finite difference numerical scheme is applied to examine the time evolution of small initial perturbations of the plasma parameters. This work is an extended numerical study of the so called “double gradient instability”, – a possible candidate for the explanation of flapping oscillations in the magnetotail current sheet, which has been analyzed previously in the framework of a simplified analytical approach for an incompressible plasma. The dispersion curve is obtained for the kink-like mode of the instability. It is shown that this curve demonstrates a quantitative agreement with the previous analytical result. The development of the instability is investigated also for various enhanced values of the normal magnetic field component. It is found that the characteristic values of the growth rate of the instability shows a linear dependence on the square root of the parameter, which scales uniformly the normal component of the magnetic field in the current sheet.     

Plasma sheet oscillations and their relation to substorm development: Cluster and double star TC1 case study

We examined two consecutive plasma sheet oscillation and dipolarization events observed by Cluster in the magnetotail, which are associated with a pseudo-breakup and a small substorm monitored by the IMAGE spacecraft. Energy input from the solar wind and an associated enhancement of the cross-tail current lead to current sheet thinning and plasma sheet oscillations of 3–5 min periods, while the pseudo-breakups occur during the loading phase within a spatially limited area, accompanied by a localized dipolarization observed by DSP TC1 or GOES 12. That is, the so-called “growth phase” is a preferable condition for both pseudo-breakup and plasma sheet oscillations in the near-Earth magnetotail. One of the plasma sheet oscillation events occurs before the pseudo-breakup, whereas the other takes place after pseudo-breakup. Thus there is no causal relationship between the plasma sheet oscillation events and pseudo-breakup. As for the contribution to the subsequent small substorm, the onset of the small substorm took place where the preceding plasma sheet oscillations can reach the region.     

模拟有限长涡片旋转的一种新数值模型

本文把涡格法中的超收敛性推广到自由涡片的演化问题，涡片的演化由ＢｉｒＫ－ｈｏｆｆ－Ｒｏｔｔ方程所控制，该方程具有强烈的非线性，难以用解析法求解。在数值模拟中通常离散涡方法。本研究表明对自由涡片的旋转问题在精确解和离散涡方法结果之间的误差主要来自点涡近似。使用基于超收格式的新数值模型可以显著地提高数值解的精度。