急始磁暴期间的地磁脉动

本文重点分析了在1989年3月13日发生的强急始型磁暴期间观测到的丰富的地磁脉动现象.文中列出各种地磁脉动发生的时间和波形曲线范例,并对各种地磁脉动做了傅里叶谱分析.这不仅可以帮助我们了解这些地磁脉动和磁暴的关系,而且能使我们进一步认识磁暴过程的能量传输实质.     

Pi2地磁脉动的理论进展

目前，国内外在Ｐｉ２脉动的理论研究上取得了很大进展，现在问题的焦点是如何完整地解释Ｐｉ２脉动的全球特征和激发机制。解释Ｐｉ２脉动的理论主要有三种，即瞬态响应机制，亚暴电流楔理论和磁层空腔振荡理论。本文介绍了这三种理论的由来和发展，分析了每种理论在Ｐｉ２脉动研究中的贡献，并对Ｐｉ２脉动理论研究的进一步发展提出一些看法。     

Polarization characteristics of Pc3 pulsations at Zhongshan Station of Antarctica

In this paper the data of geomagnetic pulsations at Zhongshan Station from February 3 to Novernber 30 in 1996 are analyzed in ordcr to study polarization characteristics of Zhongshan Station Pc3 pulsations which comprises the cusp Pc3 pulsation and the nightside Pc3 pulsation. For the cusp Pc3 pulsation. the right-handed polarization is always dominant. But their orientation of major axes of polarizations changes with season, NW-SE is dominant in summer and NE-SW in winter. For the nightside Pc3 pulsation,the right-handed with NE-SW is always dominant before midnight. But the left-handed with the mixing orientation of major axes is dominant in summer and the NE-SW with the mixing polarization sense is dominant in winter after midnight. It means that the two types of Zongshan Station Pc3 pulsations have different sources.     

1997年3月9日漠河日全食期间地磁脉动的主要特征

１９９７年３月９日漠河日全食期间分别在漠河地磁台,北京怀柔地磁脉动站和三亚地磁台开展了地磁脉动的观测。本文重点分析了３月９日０７：００ＬＴ至１１：００ＬＴ日全食前后漠河地区地磁脉动的观测资料,研究了日全食期间地磁脉动的主要特征,并对日全食期间地磁脉动的激发机制做了较深入的人。     

Propagation characteristics of the Pc3 frequency range pulsations in the cusp latitudes

Two induction magnetometers have been installed at Zhongshan Station and Davis Station, Antarctica respectively. We adopt with cross-spectral analysis technique to analyze the data of the two induction magnetometers, in June, September,December 1996 and March 1997. to investigate the Pc3 frequency range pulsation occurrence and propagation characteristics in the cusp latitudes. The results are summarized as following:At Zhongshan-Davis Stations, the Pc3 frequency range pulsations occur mainly around the local noon/ local magnetic noon and local magnetic midnight respectively. In daytime, the pulsations have a seasonal variation in amplitude, occurrence and temporal range, all of them are sma1lest in winter. But in nighttime, the pulsations have no such a variation. The pu1sation amplitude in nighttime is much larger than the one in daytime all oveI the year. The pulsation propagating direction is mainly western in daytime and irregularly in nighttime. It can be thought that the different sources of the pulsation and the ionospheric electric conductivity are mainly responsible for these characteristics.     

新疆喀什地区地震前地磁脉动异常分析

1996年11月17日至29日在新疆喀什地区发生8次地震,震前均观测到地磁脉动异常．文中对未发生地震期间地磁脉动观测的背景环境以及喀什台常见的地磁脉动进行分析,然后对地震前地磁脉动异常现象进行研究,并初步探讨这种震前地磁脉动异常的产生机制．这种震前发生的地磁脉动异常在地震的短期预报上可能有广泛的应用前景．     

2000年4月6日磁暴期间磁扰变化在低续子午链的纬度效应

利用低纬地磁午链上H和D分量的分均值数据，分析了2000年4月6日磁暴期间磁扰变化的纬度效应。主要特点是：（1）急始期间H分量急始跃变 幅随磁纬降低而减小，且急始变幅的下降率磁纬降低而逐渐增大；（2）初相期间H分量第2峰值的变幅和初相持续时间随磁纬降低而减小；（3）主相期间H分量迅速减小，并随纬度降低最大变幅明显增加；（4）恢复相H分量呈两阶段上升趋势，前一阶段迅速上升，后一了阶段上升速度明显减小。最后对这些磁扰变化的纬度效应与空间电流体系的密切关系作了讨论。     

极隙区纬度Pc 5脉动的传播和起源

南极中山站和戴维斯站均位于极隙区纬度附近,均安装了完全相同的感应式磁力计.选择两站的数据,1997年3月和1996年6、9、12月,运用信号互谱技术进行统计分析,结果得到:在中山站-戴维斯站,Pc5脉动出现时间范围较广,但以地方时中午/磁中午及磁午夜附近出现频次多,其振幅、传播及发生率季节变化不大.振幅白天变化小,中午有小峰,夜间有时有大值.传播方向白天以磁中午为界,晨侧向西传播,直至磁凌晨;昏侧向东传播,约在5:00MLT处转向.夜间约以20:00 MLT为界,之前向西传播,之后向东传播,磁黄昏附近,Pc5脉动传播方向变化较多,显得不规则.这些特征,反映了Pc5脉动在不同地方时段有不同的起源.     

地磁脉动记录仪的计时系统

本文简单介绍我们研制的地磁脉动记录仪计时系统,讲述了工作原理和电路特点,并附有计时系统的电路图.本计时系统结构简单,易于改装制作,可供地磁测量人员参考使用.     

The characteristics of Pi2 pulsations at Great Wall Station,Antarctica

ＴｈｅｃｈａｒａｃｔｅｒｉｓｔｉｃｓｏｆＰｉ２ｐｕｌｓａｔｉｏｎｓａｔＧｒｅａｔＷａｌｌＳｔａｔｉｏｎ，ＡｎｔａｒｃｔｉｃａＹａｎｇＳｈａｏｆｅｎｇ（杨少峰）ａｎｄＸｉａｏＦｕｈｕｉ（肖福辉）（ＩｎｓｔｉｔｕｔｅｏｆＧｅｏｐｈｙｓｉｃｓ，Ａｃａｄｅｍ...