Dynamic processes in the outer heliosphere: voyager observations and models

We review recent Voyager 2 observations in the vicinity of 70 AU. The character of the solar wind plasma data between 2002 and 2003 changed to a regime in which the speed, density and magnetic field magnitude are positively correlated. The average speed of the solar wind at Voyager 2 increased between early 2003 and mid-2004, which we attribute to a return of fast coronal hole flow. We use solar wind data at Earth as input to numerical models which include the effect of pickup ions to model the radial evolution of the solar wind. The model reproduces the basic features of the observations. As a specific example, we investigate the propagation of the Halloween (Oct.–Nov.), 2003 storms in the outer heliosphere. The model predictions are in reasonable agreement with Voyager 2 observations.     

RESEARCH ON DYNAMICAL BEHAVIOR AND DESIGN OF CONTROL PARAMETER FOR NONLINEAR MAGNETIC-CONTROL SYSTEM

Ｍａｇｎｅｔｉｃｌｅｖｉｔａｔｉｏｎｔｅｃｈｎｏｌｏｇｙｉｓａｎａｃｔｉｖｅｓｅｇｒｅｇａｔｅｔｅｃｈｎｏｌｏｇｙ．Ｉｔｉｓｆｉｔｆｏｒｈｉｇｈｓｐｅｅｄｍｏ－ｔｉｏｎ，ｂｅｃａｕｓｅｉｔｉｓｆｒｅｅｏｆｔｈｅｌｉｍｉｔｏｆｄａｍｐｉｎｇｆｏｒｃｅ．...     

多层太阳大气模式中Alfven波的传播

将实际的太阳大气划分为多个等温层次，导出了均匀倾斜磁场下线性Alfven波通过任意多等温层的能量透射率，结果表明，两等温层模式与三等温层模式的结果存在本质的区别。在两等温层中，温度的跃变式增高对Alfven波起着高通滤波的作用，而三等温层中在高频端Alfven波的透射率显示为振荡形态，对实际大气温度模式的计算结果表明，太阳低层大气更适合于周期为数秒的Alfven波的能量传输。     

太阳帆技术综述

文章简要阐述了太阳帆的概念、主要结构和技术，参考美国L’Garde公司的太阳帆展开设计，对涉及的充气及刚化予以概述，为研究分析太阳帆的展开技术提供借鉴。     

磁液悬浮式离心血泵实验研究

磁液悬浮式离心血泵是第三代人工辅助心脏系统的核心部件,血泵的好坏直接影响到整个系统的工作性能。本文针对一种新型磁液悬浮式离心血泵开展血泵性能测试的实验研究,通过设计实验系统测试获得血泵各项性能参数,并对此种新型血泵的综合性能进行评价,为新型磁液悬浮式离心血泵的研制工作提供实验依据。     

Estimation of the bias of the Minimum Variance technique in the determination of magnetic clouds global quantities and orientation

Magnetic clouds (MCs) are highly magnetized plasma structures that have a low proton temperature and a magnetic field vector that rotates when seen by a heliospheric observer. More than 25 years of observations of magnetic and plasma properties of MCs at 1 AU have provided significant knowledge of their magnetic structure. However, because in situ observations only give information along the trajectory of the spacecraft, their real 3D magnetic configuration remains still partially unknown. We generate a set of synthetic clouds, exploring the space of parameters that represents the possible orientations and minimum distances of the satellite trajectory to the cloud axis, p. The synthetic clouds have a local cylindrical symmetry and a linear force-free magnetic configuration. From the analysis of synthetic clouds, we quantify the errors introduced in the determination of the orientation/size (and, consequently, of the global magnetohydrodynamic quantities) by the Minimum Variance method when p is not zero.     

Rayleigh问题的Monte Carlo直接模拟

利用流场直接模拟的Ｍｏｎｔｅ Ｃａｒｌｏ方法数值模拟了Ｒａｙｌｅｉｇｈ问题的流场，获得了相应的结果，结果与解析解及经验解吻合较好，ＤＳＭＣ方法避免了求解复杂的控制方程，在流动比较复杂的情形下，有很大的优越性，是研究稀薄气体流动的一种好方法。     

太阳活动、黑潮海温年季变化与长江中游旱涝灾害

本文采用太阳１０．７ｃｍ辐射流量（Ｆ１０．７）作为太阳活动指标，根据最近３０多年的太阳活动、西太平洋黑潮区海温和长江中游干支流地区雨量观测数据，分析了三者之间的关系，研究发现长江中游地区旱涝明显地受太阳活动和黑潮海温年季变化的共同控制．可根据某些特征，利用两年之前的太阳１０．７ｃｍ辐射流量和当年春季之前黑潮海温的观测数据，分析判断长江中游当年夏季是否发生旱涝灾害的趋势．     

电子回旋共振中和器内静磁场及微波电磁场的数值计算

为了研究电子回旋共振中和器内静磁场和微波电磁场的分布规律,设计合理的磁路结构以形成电子回旋共振区,并使微波强电场区与电子回旋共振区重合,采用有限元分析软件对中和器内的静磁场和微波电磁场进行了数值计算。计算结果表明:永磁体及磁轭的尺寸均影响电子回旋共振区的分布;天线伸入长度越长,微波电场越强。微波频率为4.2GHz时,六块相同的长12mm,宽8mm,高5mm的条形永磁铁与磁轭组成的磁路结构,可以产生合理的电子回旋共振区。L型天线伸入长度为5mm时微波强电场区可与电子回旋共振区重合。     

光纤陀螺磁屏蔽效能仿真及实验研究

光纤陀螺处于磁场环境中会产生漂移,降低了光纤陀螺精度。光纤陀螺的磁场敏感性制约了其在高精度导航领域的应用。本文建立了光纤陀螺三维磁屏蔽仿真模型,给出了光纤陀螺磁屏蔽效能与磁屏蔽结构参数之间的关系并得到实验验证,为光纤陀螺磁屏蔽设计提供了依据。