A new parameter to define interplanetary coronal mass ejections

The interplanetary manifestations of coronal mass ejections, ICMEs, have many signatures in the solar wind but none of these signatures in the velocity, density, temperature, magnetic field, plasma composition or energetic particles uniquely and unambiguously identifies the occurrence of an ICME. Different investigators identify different events when confronted with the same data. Herein, we present a single physical parameter that combines information from multiple plasma components and that holds the promise of defining a beginning and an end of the region of influence ICME and an indication of the location of the encounter with the ICME relative to its central meridian. This parameter is the total plasma pressure perpendicular to the magnetic field, consisting of the sum of the magnetic pressure and plasma kinetic or thermal pressure. It provides a vehicle for classifying the nature of the ICME encounter and, in many cases, provides an unambiguous start and stop time of the event. However, it does not provide a start and stop time for any embedded flux rope. This identification depends on examination of the magnetic field.     

Force-free magnetic field in a cylindrical flux rope without a constant alpha

It is generally assumed that magnetic fields inside interplanetary magnetic clouds and flux ropes in the solar photosphere are force-free. In order to model such fields, the solution of rot B = B is commonly used where  = const. But comparisons of this solutions with observations show significant difference. To treat this problem,we examine the solutions with .     

The Magnetostatic Cleanliness Program for the Cassini Spacecraft

The Cassini spacecraft, launched in October 1997 and expected to reach Saturn in 2004, carries two magnetometer experiments on a 10-m boom, one at the mid-section of the boom and the other situated at the end of the boom. In order to gather valid scientific magnetic field data and avoid electromagnetic interference, the spacecraft had to comply with stringent magnetostatic cleanliness requirements. This paper describes the results of the Cassini magnetics cleanliness program that achieved the goal of minimizing the magnetic field interference with Cassini’s DC magnetic field science instruments.This revised version was published online in July 2005 with a corrected cover date.     

高灵敏度与高稳定性的飞机客舱内物品监测系统

介绍了一种新型的高稳定度、高灵敏度的飞机客舱内物品监测系统的工作原理和基本电路。该系统具有检测灵敏度高,抗干扰能力强,工作稳定可靠的特点。     

无陀螺磁控小卫星的大角度姿态捕获研究

为了解决无陀螺磁控小卫星的姿态稳定和捕获问题,本文针对偏置稳定的主动磁控小卫星姿态控制平台,基于磁控力矩的时间累积作用效果等效卫星角动量增量的规律,设计了一种仅利用角度反馈的卫星大角度磁捕获控制律。通过仿真和卫星在轨实测的验证,证明该方法具有良好的收敛效果和鲁棒性,工程实现简单,可靠性高,适用于中低轨道的通信小卫星。     

裂缝宽度对磁记忆信号的影响的研究

以经爆破试验的四件小钢管件裂纹为研究对象,找出裂纹宽度与磁记忆信号的关系,得出漏磁场变化梯度的最大值随裂缝宽度增加而增加。     

对单列向心球轴承摩擦系数的研究

本文在运用摩擦学滚动及弹性力学原理对单列向心球轴承滚珠及内圈受力情况进行系统分析及研究的基础上,提出一组可直接计算球轴承摩擦系数的理论公式,由本文导出的计算公式所示解析关系可清晰地看出,球轴承摩擦系数不仅与轴承内外径,滚珠对内圈（或外圈）的滑动摩擦系数,滚珠半径及数量有关,而且还与轴承的当量动载荷密切相关。     

近室温磁制冷工质选择的热力学准则

对近年来在制冷界研究相当活跃的磁制冷的工质，尤其是近室温磁制冷的工质－铁磁材料，在外加磁场中的热力学特性进行了分析、讨论，并在此基础上总结了选取近室温磁制冷工质的理论依据和原则，使实际中的选择工作有了针对性，减少了盲目性。     

一种双管正激磁集成变换器

双管正激磁集成变换器的高频变压器磁芯双向磁化，提高了磁芯利用率。本文研究了导通占空比、开关管导通管压降以及变压器两原边的磁化电感等参数不一致时，导致变压器磁芯偏磁问题。磁芯的磁化状态虽受上述参数的不一致影响而出现单向磁化现象，但不会出现单向磁饱和，双管正激磁集成变换器仍能稳定工作，为能否采用平均电流控制模式或电压控制模式提供了理论依据。文中分析了变压器原边环流产生机理，提出了一种减小环流的方法。使环流减小一半。     

稀土磁弹簧吸振器特性的研究

首先简要介绍稀土金属制成的磁弹簧吸振器的构造和工作机理，然后着重介绍三种规格磁弹簧吸振器特性的测试、计算和分析，并对磁弹簧刚度的可调节性及其刚度与磁弹簧的有关参数间的关系进行了分析，最后得出了一些有实际应用价值的结论。