大型构件蠕变时效成形技术研究

蠕变时效成形技术是为实现大型整体壁板构件高性能与精确成形协同制造而发展起来的一种新型钣金成形方法.分析了大型整体壁板构件的特点和蠕变时效成形技术的原理,从蠕变时效材料本构建模、模具型面回弹补偿和模具设计3个关键方面重点阐述了蠕变时效成形技术的研究进展,并且从材料本构向构件本构发展、蠕变成形向塑变与蠕变复合成形发展和简单热力能场向多级复合能场时效成形发展3个研究热点阐述了该技术进一步发展面临的挑战.     

Winter cross polar cap current estimation

Digital ionosonde and magnetometer observations from a polar cap station are used to estimate the fraction of Region 1 current that flows across the polar cap. For a winter case study using data for 2001 Feb 18 the cross-cap current was 3.9 × 10⁴ A Pedersen current and 6 × 10⁴ A Hall current. This total current is only a small percentage, ∼5%, of the Region 1 current.     

零磁通直流电流传感器及其在电流标准源中的应用

介绍零磁通电流检测原理,探讨100A直流电流测量用传感器的设计方法,对该传感器在高精度直流电流标准源中的应用进行论述。     

火星磁场产生的原因及其分布

构建了一个可以得到火星赤道面上磁场分布的模型. 模型根据卫星观测数据, 提出了火星电离层、磁层顶和磁尾电流片上都各自通有电流的假设. 由电流的连续性条件可知, 这三种背景条件下的电流之间满足一定关系, 即火星磁层顶上的总电流是电离层上的总电流与磁尾电流片上的总电流之和. 这些电流产生的磁场与太阳风磁场共同构成了火星赤道面上磁场分布. 通过计算发现, 采用这种磁场模型得到的结果与目前卫星所观测的结果以及与采用其他方法得到的结果符合得较好.      

民用飞机配电网络过流保护分析方法研究

飞机配电网络过流保护分析是验证飞机电网设计合理性、可靠性和安全性的重要内容之一.因此,主要对飞机配电网络过流保护分析方法进行了研究,并提出了一种特性曲线法.该特性曲线法基于导线载流特性曲线和电网保护装置过流保护动作特性曲线,分析方法简单、实用,可用于支持合格审定阶段飞机配电网络设计验证.     

航天器海上测控技术现状分析与发展思考

为了满足后续航天测控任务的需要,紧跟未来航天测控技术发展步伐,实现航天器海上测控的可持续发展和航天测量船综合效益的全面提升,简要回顾航天器海上测控技术的发展历程,分析海上航天测控系统的现状及其发展需求,指出海上航天测控技术需要重点发展的几个方向。     

Locating Current Sheets in the Solar Corona

Current sheets are essential for energy dissipation in the solar corona, in particular by enabling magnetic reconnection. Unfortunately, sufficiently thin current sheets cannot be resolved observationally and the theory of their formation is an unresolved issue as well. We consider two predictors of coronal current concentrations, both based on geometrical or even topological properties of a force-free coronal magnetic field. First, there are separatrices related to magnetic nulls. Through separatrices the magnetic connectivity changes discontinuously. Coronal magnetic nulls are, however, very rare. Second, inspired by the concept of generalized magnetic reconnection without nulls, quasi-separatrix layers (QSL) were suggested. Through QSL the magnetic connectivity changes continuously, though strongly. The strength of the connectivity change can be quantified by measuring the squashing of the flux tubes which connect the magnetically conjugated photospheres. We verify the QSL and separatrix concepts by comparing the sites of magnetic nulls and enhanced squashing with the location of current concentrations in the corona. Due to the known difficulties of their direct observation, we simulated coronal current sheets by numerically calculating the response of the corona to energy input from the photosphere, heating a simultaneously observed Extreme Ultraviolet Bright Point. We did not find coronal current sheets at separatrices but at several QSL locations. The reason is that, although the geometrical properties of force-free extrapolated magnetic fields can indeed hint at possible current concentrations, a necessary condition for current sheet formation is the local energy input into the corona.     

关于大电流测试问题的研究

采用电流比较仪,AD交直流标准电阻,高准确度数字多用表组成校验系统,解决大电流测试问题.     

同步三轴卫星初期能源过剩预案处理策略

同步三轴卫星中的能源分系统是卫星各系统中重要的组成部分,能源系统中任何异常将严重影响卫星功能的发挥。预想能源系统中分流器异常,通过对南分流器异常的分析,提出两种应对策略,并在仿真计算的基础上进行可行性分析,得出一种切实可行的应对策略,为同步三轴卫星长期管理中异常处理提供了分流器异常的可行性预案。     

火星空间大尺度电流体系分布特征

在MHD模型基础上, 对火星空间环境的电流分布进行了模拟. 结果表明, 火星空间存在着弓激波电流、磁堆积区电流、电离层电流和磁尾电流. 弓激波电流在激波曲面上均由北向南自成体系, 电流密度在弓激波顶区域较大. 在向阳面磁堆积区边界电流与电离层电流彼此耦合形成完整的回路, 在背阳面磁堆积区边界电流与磁尾中心电流片耦合形成完整的回路.