磁云膨胀速度对无力场磁通量管模型拟合结果的影响

为了考察磁云膨胀速度对磁通量管模型拟合结果的影响,选取了1998-2003年中15次引起了较大地磁暴(Dstmin＜-50 nT)的典型磁云事件进行了拟合.与未考虑膨胀速度模型的拟合结果比较,膨胀速度的引入能较好地改善拟合结果,与观测数据的偏差最大能减小30%,并且拟合所得的膨胀速度基本符合统计规律.这个结果说明膨胀的磁通量管模型能更好地反映实际观测的磁云.同时,初步分析了考虑膨胀速度前后磁云各拟合参数的变化.      

固胶对保偏光纤环的影响

阐述了固胶对光纤环及光纤陀螺两个重要性能参数——温度性能和振动性能的作用和影响,针对某项目对光纤陀螺实际要求的条件进行了陀螺的全方面试验,并分析试验结果.试验和分析结果表明,固胶对光纤环和光纤陀螺的影响是由涂胶工艺不当带来的,涂胶量及涂胶的均匀度是产生影响的两个主要因素,胶的温度性能及自身固化后状态对光纤环性能也会产生影响.得出结论:固胶工艺或固胶方式、方法对光纤环的性能有极大的影响,特别是对光纤环在温度变化时的影响表现更为明显,另外,固胶对光纤环的影响,还表现在胶固化后的状态.      

磁等离子发动机超导附加线圈的电磁特性分析

在工程应用上提供附加场的传统水冷铜线圈存在体积大、质量大、电耗高等显著缺点,因此体积小、质量小的高温超导磁线圈在附加场的磁等离子发动机（Applied FieldMagnetoPlasmaDynamicThruster,AF MPDT）中的应用受到了广泛关注。文章为满足02T的大孔径中心磁场需求,对内径160mm、高度30mm、材料为Bi 2333/Ag的三层双饼高温超导线圈进行了电磁特性试验研究。基于电输运法原理建立了高温超导线圈的临界电流测试系统,测量了不同层级和有无铁板情况下的线圈临界电流IC。试验发现,不同层级的临界电流IC最大有12%的差别,以中间层的IC值最大;聚磁铁板对线圈电磁特性具有正面影响,最高能将IC值提升42%。文章也开展了超导磁线圈电磁场仿真分析,研究了铁板尺寸和位置对线圈电磁特性的影响,得出了优化的聚磁铁板设计方案。     

磁场敏感度（EMS）自动测试系统

介绍一种磁场敏感度自动测试系统,该系统可检验电子仪器对磁场的敏感程度。可按国家标准GB6833.2～87和国家军用标准GJB151-86、GJB152-86进行测试,还可根据用户的需要产生更强的磁场。着重介绍该系统主要技术性能指标、工作原理、结构设计、软件设计和误差分析,并且与国外的测试系统进行了比较。     

CXG—2型磁悬规转子横向稳定的研究

本文针对CXG-1型磁悬规的转子横向振动现象进行了分析探讨,提出CXG-2型磁悬规的转子横向阻尼方案,并给出实施后的实验结果。     

Numerical Modeling of the Ring Current and Plasmasphere

Over the last 25 years, considerable scientific effort has been expended in the development of quantitative models of the dynamics of Earth's inner magnetosphere, particularly on studies of the injection of the storm-time ring current and of dynamic variations in the shape and size of the plasmasphere. Nearly all modeling studies of ring-current injection agree that time-varying magnetospheric convection can produce approximately the ion fluxes that are observed in the storm-time ring current, but the truth of that assumption has never been demonstrated conclusively. It is not clear that the actual variations of convection electric fields are strong enough to explain the observed flux increases in ~100 keV ions at the peak of the storm-time ring current. Observational comparisons are generally far from tight, primarily due to the paucity of ring-current measurements and to basic limitations of single-point observations. Also, most of the theoretical models combine state-of-the-art treatment of some aspects of the problem with highly simplified treatment of other aspects. Even the most sophisticated treatments of the sub-problems include substantial uncertainties, including the following: (i) There is still considerable theoretical and observational uncertainty about the dynamics of the large-scale electric fields in the inner magnetosphere; (ii) No one has ever calculated a force-balanced, time-dependent magnetic-field model consistent with injection of the storm-time ring current; (iii) The most obvious check on the overall realism of a ring-current injection model would be to compare its predicted Dst index against observations; however, theoretical calculations of that index usually employ the Dessler-Parker-Sckopke relation, which was derived from the assumption of a dipole magnetic field and cannot be applied reliably to conditions where the plasma pressure significantly distorts the field; (iv) Although loss rates by charge exchange and Coulomb scattering can be calculated with reasonable accuracy, it remains unclear whether wave-induced ion precipitation plays an important role in the decay of the ring current. However, considerable progress could be made in the next few years. Spacecraft that can provide images of large regions of the inner magnetosphere should eliminate much of the present ambiguity associated with single-point measurements. On the theoretical side, it will soon be possible to construct models that, for the first time, will solve a complete set of large-scale equations for the entire inner magnetosphere. The biggest uncertainty in the calculation of the size and shape of the plasmasphere lies in the dynamics and structure of the electric field. It is still not clear how important a role interchange instability plays in determining the shape of the plasmapause or in creating density fine structure.     

基于嫦娥一号高能粒子数据的地球磁层屏蔽效应研究

月球绕地球运行轨道约有1/4位于地球磁层内,因此,地球磁层是否会为月球轨道附近高能粒子提供足够的磁场屏蔽对于探索月球活动具有重要影响.嫦娥一号是中国首颗绕月人造卫星,其绕月飞行的工作轨道距离月球表面200 km.通过对嫦娥一号高能粒子探测器(HPD)的探测数据进行分析,比较了当月球位于地球磁层内外6个不同能道(能量范围4～400 MeV)时质子通量的变化,发现当月球位于地球磁层内时,这些能道的质子通量并没有发生显著减少,结果表明地球磁层不能为月球轨道附近高能粒子提供显著的磁屏蔽.     

Short term topological changes of coronal holes associated with prominence eruptions and subsequent CMEs

We study the short-term topological changes of equatorial and polar coronal hole (CH) boundaries, such as a variation of their area and disintegration, associated to reconnection with nearby (within 15° distance) quiescent prominence magnetic fields leading to eruptions and subsequent Coronal Mass Ejections (CMEs). The examples presented here correspond to the recent solar minimum years 2008 and 2009. We consider a temporal window of one day between the CH topological changes and the start and end times of prominence eruptions and onset of CMEs. To establish this association we took into account observational conditions related to the instability of prominence/filaments, the occurrence of a CME, as well as the subsequent evolution after the CME. We found an association between short-term local topological changes in CH boundaries and the formation/disappearance of bright points near them, as well as, between short-term topological changes within the whole CH and eruptions of nearby quiescent prominences followed by the appearance of one or more CMEs.     

地磁定位方法综述

地磁导航具有可用区域广泛、无累积误差、无源和隐蔽性强等优势,是未来定位导航与授时(PNT)体系中潜在的重要导航定位手段之一。地磁导航技术包括磁场信息的测量、地磁基准图的建立和地磁定位方法的设计3个重要内容。本文主要围绕地磁定位方法,调研总结了当前主流的地磁滤波、地磁匹配和磁场同时定位与构图(SLAM)三类方法的原理及技术发展路线,重点分析了不同方法的优缺点、适用场景、时效性、对磁图和传感器的需求,并对地磁定位方法的发展方向进行了展望。     

AlNiCo合金中α1相取向程度对磁稳定性的影响

AlNiCo合金具有优异的温度稳定性和磁稳定性，在惯性仪表中广泛应用，其磁稳定性对于仪表的精度和寿命具有重要影响。AlNiCo合金中主要包括强磁性的α1相和弱磁性的α2相，通常情况下取向一致的α1相为磁体提供矫顽力和磁化强度。通过磁场热处理的方法控制α1相的取向，研究其对磁稳定性的影响规律，探索提高AlNiCo合金磁稳定性的新思路。研究发现，随机取向的AlNiCo-0样品虽然矫顽力和剩磁较低，但是具备更低的磁粘滞系数，稳定性优于各向异性的AlNiCo-0.25样品，这主要是由于其能垒分布更加平缓。微磁模拟的结果进一步表明，取向垂直于易轴的α1相更有助于形成稳定的磁畴结构。