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.     

飞行过载对燃烧室化学反应流场影响

为了研究飞行过载对固体火箭发动机燃烧室化学反应流场影响,以Liang模型模化铝滴燃烧,以有限化学反应速率模型模化湍流燃烧,对过载条件下发动机内流场进行了数值分析,数值结果与试验结果取得了趋势上的一致。研究表明,文中采用的数值计算方法可有效重现发动机热结构故障点;飞行过载改变了流场温度、粒子浓度、化学反应速率等参数分布;过载条件下燃烧室绝热结构表面铝滴积聚及剧烈的化学放热反应是导致其异常烧蚀的原因之一,铝滴局部积聚燃烧会导致温度场畸变;热结构设计必须与流动结构匹配。     

基于混合整数规划模型的物流中心选址方法

物流中心是物流企业效益链的重点环节,物流中心的选址直接关系着企业的发展。文章讨论了在多元网点布局情况下,混合整数规划模型在选址过程中的应用,并对模型的算法和求解进行了讨论。     

高温超导磁悬浮助推缩比试验系统动态测试分析

基于磁悬浮助推技术概念研究方案建立了一套悬浮加速缩比试验系统.从整体缩比模型振动试验出发,主要研究悬浮质量以及悬浮刚度对整体系统动态性能的影响,并在进行缩比单元动态试验结论的基础上,建立试验模型的加速试验动态采集系统,对整体模型进行运行性能试验.在试验基础上提出了提高磁悬浮推进系统运行稳定性的依据,并据此提出相应可行的解决方案设想.通过模型加速试验并采集试验数据定性分析磁浮系统的综合运动性能,以更好地评估系统稳定特性和品质,也为进一步研究磁悬浮助推发射的气动、分离系统稳定性和可靠性提供参考.     

更替某型飞机电压限定器的研究

文章在介绍某型电压限定器工作原理的基础上,阐述了利用集成电路技术和自动控制技术进行该型电压限定器国产化研制的方法,给出了电压限定器探测及延时电路、均衡控制电路、防止误动作保护电路的详细设计方案,解决了激磁控制、均衡控制、故障鉴别等国产化研制过程中遇到的问题,保证了新研制产品与原有进口产品的可互换使用,提高了设备的工作可靠性。     

EB-PVD制备箔材的厚度均匀性研究

从真空蒸镀中使用的小平面蒸发源理论出发,针对电子束物理气相沉积中为改善箔材厚度分布所须旋转大基板进行蒸镀的情况,建立了该过程的数学模型;并利用该模型对不同的坩埚位置所沉积的箔材厚度进行了定性分析,从而实现了对坩埚与基板相对位置的优化,使基板上沉积的箔材厚度分布可以达到最均匀的状态.最后通过K值的提出使理论和实际箔材厚度的结果趋于一致,即证明所建立的数学模型是合理的.     

CVI反应器内部气体流场的有限元模拟及优化设计

采用有限元计算方法,研究了CVI反应器内部的流场特征.对于形状简单的构件,构件的放置方式和阵列对气体的流动状态具有显著的影响.与横向阵列相比,纵向阵列能充分保证构件沿其长度方向流场均匀性,减小回流现象;在反应器中,随着纵向阵列试样数量的增加和分布均匀性的提高,气体流动速度增大,流场均匀性提高.减少反应器内部的自由空间,是提高流场品质和化学气相沉积效果的关键.基于减少反应器内部的自由空间的原则,针对杯形复杂构件,提出了通过加入与其几何形状相适应的导流板工装,有效避免了在构件内部和外部形成回流区,实现流场的优化设计.     

基于SFEM的SRM纤维缠绕结构的可靠性分析

采用纽曼级数展开的蒙特卡罗随机有限元方法(SFEM),分析了固体火箭发动机(SRM)复合材料缠绕的燃烧室在内压正态变化下的应力响应,然后利用应力强度干涉原理分析计算其可靠性.     

激光冲击残余应力场的有限元分析

建立模拟激光冲击残余应力场的非线性弹塑性有限元模型,预测AISI 304奥氏体不锈钢厚、薄靶材经激光冲击后表面以及内部的残余应力场分布.模拟过程中,考虑材料高应变率(106s-1)下的力学性能和激光诱导冲击波的精确加载,分析激光功率密度、激光光斑尺寸、激光脉宽、激光冲击次数、激光单面与双面冲击等激光冲击参数以及初始残余应力等因素对不锈钢靶材残余应力分布的影响.数值模拟结果与X射线衍射法测量值吻合较好.在有初始残余拉应力(250MPa)存在的情况下,激光冲击仍能使304奥氏体不锈钢靶材形成残余压应力层,说明激光冲击工艺可提高奥氏体不锈钢焊接构件的抗应力腐蚀开裂能力.