基于ULF标准的移动学习内容管理系统设计

设计了一套基于ULF标准的智能移动学习系统,为了较全面地分析学习过程．系统还加入了在线分析功能。系统方便教师编辑遵循ULF标准格式的学习材料,这不仅使数字教材的创建变得简单,而且让数字教材变为通用教材．节省了大量的人力物力。在学生的学习过程中．系统的移动教学功能使得学习变得无处不在,大大提高了学习效率。     

超低频天线设计中的运动感应噪声研究

为进一步改善超低频天线收信性能,建立了磁场天线的理想振动模型,分析了天线灵敏度设计对运动感应噪声的影响,详细推导了均匀灵敏度天线的运动感应噪声功率谱,并在相同条件下与抛物线型灵敏度天线作对比,对比结果表明,2种天线在不同频率和天线长度下诱发的噪声强度不同,但均匀灵敏度型天线诱发的噪声始终要多于抛物线型灵敏度天线。通过优化配置线圈的电磁结构,给出了实际天线灵敏度的设计方法。针对运动感应噪声功率谱影响较大的横向力分布谱密度,通过多项式拟合和指数拟合的方式设计了新的表达式,利用该表达式进行仿真实验,并在不同天线长度和潜艇航速下,与目前主流的横向力分布谱密度函数进行对比分析。仿真结果表明,数据拟合得到的运动感应噪声谱密度随着天线长度的增加而降低,随着潜艇航速的加快而增大;指数拟合方式诱发的运动感应噪声强度与主流表达式诱发的强度基本一致,多项式拟合方式诱发的运动感应噪声相对较低。     

超低频地磁信号谱分析系统研究与实现

针对超低频地磁信号谱的特点,利用MATLAB的数据显示与分析功能,完成了超低频地磁信号谱分析系统,系统共分为数据文件格式化、原始数据显示、数据谱分析三大模块,能够对采集到的数据按指定条件进行批量格式化并显示为二维分布图,同时可以对数据进行傅里叶变换或小波分析,也可以观察其维格纳分布图,实现了与国外同类软件相同的功能;采用本软件,对安阳信号采集站1980年5月12日的数据进行了处理,达到了预期效果.本系统具有自有知识产权,可有效提高地磁研究工作者的研究效率.     

Fast acceleration of “killer” electrons and energetic ions by interplanetary shock stimulated ULF waves in the inner magnetosphere

Energetic electrons and ions in the Van Allen radiation belt are the number one space weather threat. Understanding how these energetic particles are accelerated within the Van Allen radiation belt is one of the major challenges in space physics. This paper reviews the recent progress on the fast acceleration of "killer" electrons and energetic ions by ultralow frequency (ULF) waves stimulated by the interplanetary shock in the inner magnetosphere. Very low frequency (VLF) wave-particle interaction is considered to be one of the primary electron acceleration mechanisms because electron cyclotron resonances can easily occur in the VLF frequency range. Recently, using four Cluster spacecraft observations, we have found that, after interplanetary shocks impact the Earth’s magnetosphere, energetic electrons in the radiation belt are accelerated almost immediately and continue to accelerate for a few hours. The time scale (a few days) for traditional acceleration mechanisms, based on VLF wave-particle interactions to accelerate electrons to relativistic energies, is too long to explain our observations. Furthermore, we have found that interplanetary shocks or solar wind pressure pulses, with even small dynamic pressure changes, can play a non-negligible role in radiation belt dynamics. Interplanetary shocks interaction with the Earth’s magnetosphere manifests many fundamental space physics phenomena including energetic particle acceleration. The mechanism of fast acceleration of energetic electrons in the radiation belt responding to interplanetary shock impacts consists of three contributing parts: (1) the initial adiabatic acceleration due to strong shock-related magnetic field compression; (2) followed by the drift-resonant acceleration with poloidal ULF waves excited at different L-shells; and (3) particle acceleration due to the quickly damping electric fields associated with ULF waves. Particles end up with a net acceleration because they gain more energy in the first half of this cycle than they lose in the second. The results reported in this paper cast a new light on understanding the acceleration of energetic particles in the Earth’s Van Allen radiation belt. The results of this study can likewise be applied to interplanetary shock interaction with other planets such as Mercury, Jupiter, Saturn, Uranus and Neptune, and other astrophysical objects with magnetic fields.