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73.
Marc A. Vallée Larry Newitt Ian R. Mann Mouhamed Moussaoui Régis Dumont Pierre Keating 《Pure and Applied Geophysics》2007,164(1):161-176
Geomagnetic activity affects aeromagnetic surveys. Geomagnetic variations are quite complex and can be quantified in different
ways. A measure of geomagnetic activity that is useful for planning aeromagnetic surveys is the Pc3 pulsation index developed
by the Australian Space Weather Agency. Purposeful to developing guidelines for planning aeromagnetic surveys in Canada, we
study the variations in Pc3 index amplitude over Canada in 2000. This study shows distinct patterns associated with the sub-auroral
zone, the auroral zone, and the polar cap. Average Pc3 index activity is higher during the months of February, July, September,
and November in the auroral and sub-auroral zones. The station in the polar cap exhibits maximum activity near midday during
the summer months. Detailed analysis of a magnetic storm shows that Pc3 index amplitude during the beginning of the solar
storm is least important at the polar cap. The mean Pc3 index also relates to solar wind parameters such as the solar wind
velocity and the vertical polarity of the interplanetary magnetic field. Analysis of the morning maximum of the Pc3 index
observed in the auroral zone can be used to develop guidelines for planning aeromagnetic surveys in Canada and other areas
of the world affected by auroral zones. 相似文献
74.
高玉芬 《地震地磁观测与研究》1998,19(1):58-63
分析表明,目前广泛应用的AE指数虽然在一定程度能反映极区地磁活动特征,但其物理意义不清,不能描述亚暴活动的物理过程,不宜用来作磁层相空间重构等非线性过程的研究。AU和AL虽是不可缺少的描述极光电集流活动的指数,但仍须消除规则日变化SR的影响、改进推导方法(和台站布局)。 相似文献
75.
J. Vassal M. Menvielle Y. Cohen M. Dukhan V. Doumouya K. Boka O. Fambitakoye 《Annales Geophysicae》1998,16(6):677-697
In the framework of the French-Ivorian participation to the IEEY, a network of 10 electromagnetic stations were installed at African longitudes. The aim of this experiment was twofold: firstly, to study the magnetic signature of the equatorial electrojet on the one hand, and secondly, to characterize the induced electric field variations on the other hand. The first results of the magnetic field investigations were presented by Doumouya and coworkers. Those of the electric field experiment will be discussed in this study. The electromagnetic experiment will be described. The analysis of the electromagnetic transient variations was conducted in accordance with the classical distinction between quiet and disturbed magnetic situations. A morphological analysis of the recordings is given, taking into consideration successively quiet and disturbed magnetic situations, with the results interpreted in terms of the characterization of external and internal sources. Particular attention was paid to the effects of the source characteristics on the induced field of internal origin, and to the bias they may consequently cause to the results of electromagnetic probing of the Earth; the source effect in electromagnetic induction studies. During quiet magnetic situations, our results demonstrated the existence of two different sources. One of these, the SRE source, was responsible for most of the magnetic diurnal variation and corresponded to the well-known magnetic signature of the equatorial electrojet. The other source (the SR*E source) was responsible for most of the electric diurnal variation, and was also likely to be an ionospheric source. Electric and magnetic diurnal variations are therefore related to different ionospheric sources, and interpreting the electric diurnal variation as induced by the magnetic field diurnal variation is not relevant. Furthermore, the magnetotelluric probing of the upper mantle at dip equator latitudes with the electromagnetic diurnal variation is consequently impossible to perform. In the case of irregular variations, the source effect related to the equatorial electrojet is also discussed. A Gaussian model of equatorial electrojet was considered, and apparent resistivities were computed for two models of stratified Earth corresponding to the average resistive structure of the two tectonic provinces crossed by the profile: a sedimentary basin and a cratonic shield. The apparent resistivity curves were found to depend significantly on both the model used and the distance to the center of the electrojet. These numerical results confirm the existence of a daytime source effect related to the equatorial electrojet. Furthermore, we show that the results account for the observed differences between daytime and night-time apparent resistivity curves. In particular, it was shown that electromagnetic probing of the Earth using the classical Cagniard-Tikhonov magnetotelluric method is impossible with daytime recordings made at dip latitude stations. 相似文献
76.
本介绍了1992年1月23日黄海Ma5.3级地震(121.2°E,35.2°N)肖沂沭带部分流动磁测点地磁异常变化及预报情况。 相似文献
77.
张北6.2级地震前后地磁Z分量的日变化 总被引:9,自引:3,他引:6
利用河北省及邻省、市共17个地磁台相对观测Z分量资料,总结分析了张北6.2级地震前后的日变化。认为,一次较强地震前可能有多次异常出现,日变反向可作为中短期异常,而后出现的日变低点位移,当分界线连续在某区出现,地震可能进入短临阶段。日变反向的极值区附近和低点位移连续汇集地区可能是未来震中。对于震前出现的多次异常进行追踪预报,可能效果较好。 相似文献
78.
王战 《地球科学与环境学报》1990,(2)
本文以最新修正了的新四面体理论模型来解释地球磁极倒转现象及其规律性。文章简要回顾了依附于收缩说的地球四面体理论的兴衰,接着简述了应归属于脉动说范畴的新四面体理论研究的最新进展——地球多级驻波(式)脉动演化模型。新模型可概括为:地球的形态在演化过程中呈“准球体→负准四面体→准球体→正准四面体→准球体→…”的驻波脉动;在呈每种形体的大阶段中,又包含着次级、更次级的驻波脉动。然后论述了地磁极性倒转的规律性(即多变→固定[正向]→多变→固定[反向] →多变→…)以及新模型对其所做的解释(即固定正向和固定反向阶段分别为负和正准四面体阶段,多变阶段为准球体阶段)。 相似文献
79.
Nandita Srivastava 《Journal of Astrophysics and Astronomy》2006,27(2-3):237-242
Geomagnetic super-storms of October and November 2003 are compared in order to identify solar and interplanetary variables
that influence the magnitude of geomagnetic storms. Although these superstorms (DST < -300 nT) are associated with high speed CMEs, their DST indices show large variation. The most intense storm of November
20, 2003 (DSt∼ - 472 nT) had its source in a comparatively small active region and was associated with a relatively weaker, M-class flare,
while the others had their origins in large active regions and were associated with strong X-class flares. An attempt has
been made to implement a logistic regression model for the prediction of the occurrence of intense/superintense geomagnetic
storms. The model parameters (regression coefficients) were estimated from a training data-set extracted from a data-set of
64 geo-effective CMEs observed during 1996–2002. The results indicate that logistic regression models can be effectively used
for predicting the occurrence of major geomagnetic storms from a set of solar and interplanetary factors. The model validation
shows that 100% of the intense storms (-200 nT < DSt < -100 nT) and only 50% of the super-intense (DST < -200 nT) storms could be correctly predicted. 相似文献
80.
??RINEX HO???????GPS?????λ?????е???(?????????)????????????????????GPS???????е??????????(ΔIH)p,qi,g??????????(ΔIH)p,qi,g????γ?????????????????????????????????????????????????????£???Bernese 5.0???????????????????????????????δ???и????????????????????л????????????????????????????????ΔbH???????????ΔbH???????С????????????????????Δ??b??H??????????????????????????????????????????ε??С??ΔbH????????? 相似文献