1999年8月16日EUV增亮事件数值研究的初步结果

我们基于TRACE卫星上EUV观测,采用三阶迎风紧致格式模拟了1999年8月16日EUV增亮事件。数值模拟结果可以给出这次EUV增亮事件的形成和演化过程的一种可能的解释。重联X点处最初的重联流可能与EUV增亮相对应。合并磁岛产生的高度叠加的抛射流,可能与最初表现为吸收特征随后表现为EUV发射结构的提升物质相对应。双向重联喷流可能与继续沿着似乎开放磁力线向上喷发,或流向太阳表面的提升物质相对应。     

Electron dynamics in collisionless magnetic reconnection

Magnetic reconnection provides a physical mechanism for fast energy conversion from magnetic energy to plasma kinetic energy. It is closely associated with many explosive phenomena in space plasma, usually collisionless in character. For this reason, researchers have become more interested in collisionless magnetic reconnection. In this paper, the various roles of electron dynamics in collisionless magnetic reconnection are reviewed. First, at the ion inertial length scale, ions and electrons are decoupled. The resulting Hall effect determines the reconnection electric field. Moreover, electron motions determine the current system inside the reconnection plane and the electron density cavity along the separatrices. The current system in this plane produces an out-of-plane magnetic field. Second, at the electron inertial length scale, the anisotropy of electron pressure determines the magnitude of the reconnection electric field in this region. The production of energetic electrons, which is an important characteristic during magnetic reconnection, is accelerated by the reconnection electric field. In addition, the different topologies, temporal evolution and spatial distribution of the magnetic field affect the accelerating process of electrons and determine the final energy of the accelerated electrons. Third, we discuss results from simulations and spacecraft observations on the secondary magnetic islands produced due to secondary instabilities around the X point, and the associated energetic electrons. Furthermore, progress in laboratory plasma studies is also discussed in regard to electron dynamics during magnetic reconnection. Finally, some unresolved problems are presented.     

Double Star TC-1 observation of the earthward flowing plasmoids in the near magnetotail

We analyze Double Star TC-1 magnetic field data from July to September in 2004 and find that plas-moids exist in the very near-Earth magnetotail. It is the first time that TC-1 observes the plasmoids inthe magnetotail at X > ?13 RE. According to the difference of the magnetic field structure in plasmoids,we choose two typical cases for our study: the magnetic flux rope on August 6 with the open magneticfield and the magnetic loop on September 14 with the closed magnetic field. Both of the cases are as-sociated with the high speed earthward flow and the magnetic loop is related to a strong substorm. Theions can escape from the magnetic flux rope along its open field line, but the case of the closed mag-netic loop can trap the ions. The earthward flowing plasmoids observed by TC-1 indicate that the mul-tiple X-line magnetic reconnection occurs beyond the distance of X=?10 RE from the earth.     

用直线段电流磁场公式计算水冷磁体磁场

水冷磁体设计,须计算水冷磁体产生的磁场以获得磁体磁场的空间分布,使设计出的磁体满足实验要求.水冷磁体磁场计算在工程上常用的计算方法是椭圆积分法.此方法计算的水冷磁体的磁场均匀度比实际做成的磁体产生的磁场均匀度偏高.原因之一是磁体上的电流路径并不是工程上假设的闭合圆环路径,而是与之等半径的螺旋线状的路径.这是工程理论计算...     

The evidence for the evolution of interplanetary small flux ropes: Boundary layers

We have examined the Wind data in 1996 and identified 21 small interplanetary magnetic flux ropes(SIMFRs),and all the 21 SIMFRs have boundary layer structures.The durations of the boundary layers varied from several minutes to 30 minutes.These boundary layers also have properties of high proton temperature,density,and plasma beta.These boundary layers are formed by magnetic reconnections.In addition,in three events magnetic reconnections were occurring inside the boundary layers.It indicates that the flux rope structures have propagated for some period of time,and their boundaries were still evolving through interaction with the background solar wind.Namely it is very possible that the SIMFRs came from the solar corona.     

避开矢量分析推导磁场能量密度公式

本文避开矢量分析，引入通量管概念，应用场元方法，推导磁场能量密度的普遍表达式．方法简单，意义显明．     

电磁场变换式的直接推导

利用等效替代方法和麦克斯韦方程组,可以不通过狭义相对论而直接导出非相对论情形下的电磁场变换式,从而给出一种求电场和磁场间关系的简捷途径.     

似稳磁场激发的涡旋电场

根据Ｍａｘｗｅｌｌ电磁场理论建立似稳磁场激发电场满足的方程,给出该方程在无界空间的解,并论证似稳磁场的涡旋电场等于多极电砀的叠加。     

纵向涡发生器强化换热的场协同分析

通过在流道内安装三角形涡发生器可以产生纵向涡旋。本文以场协同理论为指导讨论了在较低壁温（小于120℃）条件下、Re在800－7000范围内,空气介质在强迫对流的情况下,水平加热片上安装三角形涡发生器的强化换热机制。     

Energetic electrons associated with magnetic reconnection in the sheath of interplanetary coronal mass ejection

Magnetic reconnection is an important universal plasma dissipation process that converts magnetic energy into plasma thermal and kinetic energy,and simultaneously changes the magnetic field topology.In this paper,we report the first observation of energetic electrons associated with asymmetric reconnection in the sheath of an interplanetary coronal mass ejection.The magnetic field shear angle was about 151°,implying guide-field reconnection.The width of the exhaust was about 8×104 km.The reconnection rate was estimated as 0.044-0.08,which is consistent with fast reconnection theory and previous observations.We observed flux enhancements of energetic electrons with energy up to 400 keV in this reconnection exhaust.The region where ener- getic electron fluxes were enhanced is located at one pair of separatrices in the higher density hemisphere.We discuss these observation results,and compare with previous observations and recent kinetic simulations.     

Recent progresses in theoretical studies and satellite observations for collisionless magnetic reconnection

As an essential mechanism in large scale fast magnetic energy releases and field reconfigurations processes in space,astrophysical, and laboratory plasmas,magnetic reconnection,particularly collisionless magnetic reconnection,has been studied for more than 65 years.Many progresses have been achieved in recent years and basic features of the process have been well understood,largely due to more and more satellite observation data available in the last decade.However,a few outstanding issues are still remained unresolved.We in the paper review the development of collisionless magnetic reconnection studies and major achievements in recent years,and also briefly discuss the open questions remained to be answered in studies of collisionless magnetic reconnection.     

用类比迁移法证明互感系数相等

利用电偶极子与磁偶极子（小载流线圈）在主、被动方面的相似性,通过电偶极子在周围空间的电场分布类比出磁偶极子在相同方位上的磁场分布。从而可进一步计算出两线圈的磁通量,给出一种互感系数相等的证法。     

再谈稳恒磁场的高斯定理的证明

由毕奥－ 萨伐尔定理证明了稳恒磁场的高斯定理     

论电机理论中的波形系数概念

分析了电机设计理论和同步电机双反应理论中的波形系数概念,并且指出：电机设计理论中由电势求磁通时引入波形系数是不合理的;双反应理论中波形系数的定义是合理的．