共查询到19条相似文献，搜索用时 109 毫秒
1.
《地震地磁观测与研究》2016,(6)
通过将廊坊、富克地磁台站数据与国内地磁台站十三陵、三亚台以及国际标准地磁台站MMB台的观测数据对比分析,发现各地磁台站数据变化幅度相近、相关性高,对地磁暴有明显响应,且磁暴期间各时段扰动幅度相近。同时,以高质量地磁数据为基础,采用快速傅里叶变换,对廊坊与富克地磁台站的地磁观测数据开展地磁脉动提取,研究发现,两个台站在地磁暴期间均能观测到明显的Pi1、Pi2、Pc5地磁脉动,且Pc5的持续时间、平均强度、变化幅度和Pi1的持续时间、变化幅度及Pi2的变化幅度均有明显增加,为今后开展地磁脉动与高能电子增强事件相关性研究奠定了基础。 相似文献
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本文利用低纬地磁台站的Pi1、Pi2地磁脉动（Pi1-2）资料和地球同步轨道的Pc5地磁脉动资料,对2004年1月到2006年12月38个磁暴事件的地磁脉动参数进行了统计分析.在此基础上,考虑相对论电子的局部加速机制,并加入损失机制,建立了一个初步的磁暴期间地球同步轨道相对论电子通量对数值的预报模型.利用该模型,我们对上述38个磁暴事件进行预报试验,最优化结果是：相对论电子通量对数值的预测值和观测值之间的线性相关系数为0.82,预报效率为0.67.这说明该模式具有较好的预报效果,也表明利用地磁脉动参数进行相对论电子通量预报是可行的. 相似文献
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1996年9月我们在河南信阳——汤阴布设了由６个测点组成的测线,对Pi2地磁脉动进行了同时观测,并对该南北测线上Pi2地磁脉动出现的同时性进行了探讨．分析结果指出,Pi2地磁脉动首先出现在测线最南端的信阳测点,越往北同一变化出现的时间越晚．该区域地表的南北向似传播速度约为140ｋｍ/s．基于Pi2地磁脉动随时间变化的不稳定性,以及基子波的可延伸性与局部化特性,我们选择合适的基子波形式,利用子波变换分析了Pi2脉动所含主要的周期变化成分的周期和振幅随时间的变化,指出其周期和振幅都随时间有复杂的变化形式． 相似文献
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对北京十三陵地磁台站2005年全年的地磁数据进行了统计分析,总结了该地区Pc6脉动的周期分布和发生率等特征.对Pc6脉动与TID的关系也做了一些尝试性探讨.我们选择北京大学多普勒雷达观测到TID事件同十三陵台站观测到Pc6脉动进行比较研究,在2004年12月23日至2006年3月11日这段时间内,共有42个事件满足要求.经过分析发现TID事件与Pc 6脉动在波动频率和波形上有比较好的相关性,讨论了Pc6脉动与TID可能的诱发源. 相似文献
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本文试图建立一个产生低纬Pi2 脉动的亚暴三维电流体系模型.用这个模型可以模拟地球表面不同纬度和经度上记录的Pi2脉动的波形和偏振图,与低纬Pi2脉动的多台观测结果基本相符.从而定量地解释了Pi2脉动和亚暴电流体系的关系. 相似文献
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采用IMAGE链22个台站的地磁脉动10 s数据，分析了2000年6月15～16日磁暴期间Pc5地磁脉动的频率、振幅、位相和极化特征：（1）磁暴初相和主相期间Pc5脉动的主频率随纬度的升高而降低，但是恢复相期间主频率随纬度的升高而升高，主相期间Pc5的主频率比初相和恢复相期间的低；（2）Pc5脉动初相期间的振幅有一个主峰在64°N附近，主相期间在66°N附近，恢复相期间在71°N附近；位相在主峰两侧随着纬度变化了大约180°， 从初相到恢复相主峰位置向高纬地区大约移动了7°；（3）Pc5地磁脉动的偏振极化椭圆初相期间在PEL站（6346°N）接近线偏振，主相期间在MAS站（6607°N）接近线偏振，恢复相期间在BJN站（7133°N）接近线偏振，并分别在这几个台站两侧的偏振椭圆的旋转方向反向. 相似文献
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本文根据OMNI、TC-2卫星、LANL系列卫星、Cluster星簇卫星(C1-C4)以及加拿大的8个中高纬地磁台站的观测数据,研究了2005年8月24日强磁暴(SYM-Hmin~ -179 nT)主相期间的强亚暴(ALmin~ -4046 nT)事件特征.该强磁暴在大振幅(IMF Bz min~ -55.57 nT)、短持续时间(~90 min)的行星际磁场条件下产生,有明显的磁暴急始(SSC),强度较大且持续时间较短.发生在磁暴主相期间的亚暴发展的主要特征如下:亚暴增长相期间,C1-C4卫星先后穿越中心等离子体片;亚暴膨胀相触发后,在近地磁尾(X~-6RE)可观测到磁场偶极化现象;等离子体无色散注入区在亚暴onset开始后迅速沿经向扩展,但被限制在有限的经度范围;磁纬60°附近,Pi2地磁脉动振幅超过了100 nT.膨胀相开始后,在中、高磁纬地磁台站可观测到负湾扰,近地磁尾可观测到Pi2空间脉动,中磁尾区域可观测到尾向流、磁重联以及O+/H+数密度比值在亚暴onset之后增大等现象.分析表明该强磁暴主相期间的强亚暴现象发生时序是自内向外:X~-6RE处TC-2观测到磁场偶极化(~09:42:30 UT),同步轨道卫星LANL1994-084观测到等离子体无色散注入(~09:44:30 UT),X~-17.8RE处C1观测到磁场重联(~09:45:30 UT),由此推断该亚暴事件很可能是近地磁尾不稳定性触发产生,其发生区域距离地球很近. 相似文献
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福建省地处我国东南沿海,每年5—10月都会受到台风的侵袭,目前建有厦门、漳州、福州三个连续重力观测台站。以2014年第10号强台风"麦德姆"为例,利用重力观测资料研究:(1)台风引起的地脉动信号的强度和卓越频率的变化规律;(2)台风卓越周期与台风强度和移动速度的关系;(3)连续重力资料非潮汐信息提取。结果表明:(1)台风靠近台站时地脉动信号增强,登陆后迅速减弱,福州台记录的信号卓越频率要比其他台站高;(2)台风卓越周期与台风强度和台风移动速度的关系比较复杂;(3)用现代滤波器能有效滤除长期存在的干扰信号。 相似文献
11.
《Journal of Atmospheric and Solar》2007,69(15):1775-1796
We have examined the spatial and temporal correlation of high-latitude Pi1B and Pi2 pulsations, mid-latitude Pi2 pulsations, and auroral substorm onsets identified in the IMAGE far ultraviolet imager (FUV) data. Numerous search coil and fluxgate magnetometers at high latitudes (65–80° in Antarctica and Greenland) and mid-latitude fluxgate magnetometers are used. We find that Pi1B onset times agree well with onset times of intense isolated auroral substorms identified by the IMAGE FUV instrument: Pi1B onsets occurred within the 2 min cadence of the imager. For any given event, we find that Pi1B are localized to approximately 4 h of local time and 7° of magnetic latitude relative to the initial auroral brightening location as observed by IMAGE FUV. Not surprisingly, we also find that Pi1B pulsations occur typically between 2100 and 0200 MLT. Comparison to Pi2 records from these and other lower-latitude stations shows that in almost all cases Pi1B activity coincides within ±2 min with Pi2 activity. Power law fits showed that Pi1B amplitude fell off with distance−2.9 for two strong events (i.e., similar to the r−3 falloff of the signal from a dipolar source), and only slightly more rapidly than the falloff of Pi2 activity (d−2.8). Given the global nature of Pi2 pulsations versus the localized nature of Pi1B events in this study, we conclude that the mechanism that drives Pi1B pulsations is likely different from that responsible for Pi2 pulsations. 相似文献
12.
Pi2地磁脉动的理论进展 总被引：1，自引：1，他引：1
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。 相似文献
13.
P. R. Sutcliffe 《Annales Geophysicae》1997,15(10):1257-1264
The pattern recognition capabilities of artificial neural networks (ANNs) have for the first time been used to identify Pi2 pulsations in magnetometer data, which in turn serve as indicators of substorm onsets and intensifications. The pulsation spectrum was used as input to the ANN and the network was trained to give an output of +1 for Pi2 signatures and –1 for non-Pi2 signatures. In order to evaluate the degree of success of the neural-network procedure for identifying Pi2 pulsations, the ANN was used to scan a number of data sets and the results compared with visual identification of Pi2 signatures. The ANN performed extremely well with a success rate of approximately 90% for Pi2 identification and a timing accuracy generally within 1 min compared to visual identification. A number of potential applications of the neural-network Pi2 scanning procedure are discussed. 相似文献
14.
IntroductionThere are many kinds of fluctuations in magnetosphere plasma, frequencies concerned are ofa broad range (10--3~106 Hi). Except for electro-magnetic waves (whistled, hydromagnetic wave Alven wave), there is static electric wave mode (plasma wave -- election acoustic wave, ionacoustic wave). Among them, a main fluctuation of hydromagnetic wave phenomena is geomagnetic pulsation. Dungey (1954) believed at first in 1954 that this kind of pulsations can be attributed to hydromagnetic w… 相似文献
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The results of studying the distribution character of the amplitudes and time intervals between wave packets of Pi2 geomagnetic
pulsations, observed during the nighttime development of magnetospheric substorms and in the absence of these phenomena, have
been presented. The analog records from the midlatitude Borok Geophysical Observatory (geographic coordinates φ = 58.03°;
λ = 38.97°) for 1995 and 1997 have been used to analyze Pi2 pulsations. Three groups of pulsations have been analyzed: Pi2
observed during sub-storms related to the external impact on the magnetosphere, Pi2 spontaneously originating during substorms,
and Pi2 observed in the absence of substorms on the nightside of the magnetosphere. Interplanetary magnetic field B
y and B
z components and the solar wind dynamic pressure (ρV
2) have been considered as possible triggers of magnetospheric substorms. It has been indicated that the distributions of the
amplitude and the duration of time intervals between Pi2 bursts are approximated by the power and exponential functions, respectively,
which is typical of intermittent processes. The hypothesis that the processes of magnetospheric plasma turbulization can be
among the Pi2 pulsation burst sources has been put forward. It is assumed that the obtained characteristic values can be used
to qualitatively estimate the degree of plasma turbulence on the nightside of the magnetosphere when a sequence of Pi2 wave
packets is excited. 相似文献
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18.
V. I. Degtyarev I. P. Kharchenko A. S. Potapov B. Tsegmed S. E. Chudnenko 《Geomagnetism and Aeronomy》2010,50(7):885-893
The dynamics of the Pc5 and Pi1 pulsation characteristics and relativistic electron fluxes at geostationary orbit were comparatively
analyzed for three nine-day intervals, including quiet periods and periods of geomagnetic storms. It was shown that relativistic
electron fluxes increase considerably when the power of global Pc5 pulsations and the index of midlatitude irregular Pi1 pulsations
increase simultaneously. The correlation between the characteristics of Pi1 and Pc5 geomagnetic pulsations and the level of
the relativistic electron flux at geostationary orbit during the magnetic storm recovery phase were studied. It was shown
that the correlation coefficient of the relativistic electron maximal fluxes during the magnetic storm recovery phase with
the parameter of midlatitude Pi1 pulsations is slightly higher than such a correlation coefficient with the solar wind velocity. 相似文献
19.
中低纬地区地磁脉动的研究 总被引：1，自引：0，他引：1
杨少峰 《地震地磁观测与研究》1992,13(1):50-57
近年来我们对中低纬地区地磁脉动进行了大量的观测和研究。本文不仅介绍了观测仪器的设计、台网设置及数据处理方法。而且还简要地介绍了一些主要科研成果,如低纬Pc3脉动特点,低纬Pi2脉动偏振特性。南极地区的地磁脉动观测结果,以及在磁暴和太阳耀斑期间在低纬地区观测的地磁脉动。这对于进一步认识中低纬地区地磁脉动是十分有益的。 相似文献