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  

解用明 《华北地震科学》1998,16(3):62-66,74

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   

新四面体理论与磁极倒转     

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   

The challenge of predicting the occurrence of intense storms     

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 (D_ST < -300 nT) are associated with high speed CMEs, their DST indices show large variation. The most intense storm of November 20, 2003 (D_St∼ - 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 < D_St < -100 nT) and only 50% of the super-intense (DST < -200 nT) storms could be correctly predicted.  相似文献   

海底观测网技术进展与发展趋势     

李风华郭永刚吴立新李整林 《海洋技术学报》2015,34(3):33-35

海底观测网络由于其特有的能源供给与信息传输优势,受到了广泛关注与重视。文中简要回顾了国内外海底观测网技术的发展现状,并就海底观测网技术发展趋势进行了探讨。  相似文献   

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朱春春  李征航  屈小川  申小平 《大地测量与地球动力学》2015,35(1):81-86

??RINEX HO???????GPS?????λ?????е???(?????????)????????????????????GPS???????е??????????(ΔI_H)^p,q_i,g??????????(ΔI_H)^p,q_i,g????γ?????????????????????????????????????????????????????￡???Bernese 5.0???????????????????????????????δ???и????????????????????л????????????????????????????????Δb_H???????????Δb_H???????С????????????????????Δ??b??H??????????????????????????????????????????ε??С??Δb_H?????????  相似文献   

近58a南岳高山站气候变化特征分析     

潘筱龙  叶成志  张剑明  陈德桥 《南京气象学院学报》2015,7(1):68-78

采用1953—2010年南岳高山站逐日气象资料,运用线性回归、突变分析和小波分析方法,对该站平均风速、气温和降水的气候变化特征进行了分析,并对与平均风速变化密切相关的气温和降水进行了年际变化特征比较.结果表明:1)年和四季平均风速均呈明显减小趋势,在20世纪90年代前后风速有由大到小的突变,年平均风速存在显著的准2 a和准4 a周期;2)年平均气温、最低气温、最高气温均呈明显升高趋势,气温存在显著的准2 a和准4 a周期,且于20世纪90年代中期前后气温有由偏低向偏高的突变;3)年降水量呈下降趋势,存在显著的准2 a和准3 a周期;4)风速与平均气温、最高气温和最低气温呈负相关关系,均通过0.01显著性检验,风速与降水的相关性没有通过显著性检验,但风速与降水的变化趋势在20世纪60年代中后期、70年代中期到21世纪初有较好的反相位变化.  相似文献   

青海西部祁漫塔格成矿带找矿新进展及其意义   总被引：16，自引：2，他引：14  

张爱奎  莫宣学  李云平  吕军  曹永亮  舒晓峰  李华 《地质通报》2010,29(7):1062-1074

青海省祁漫塔格成矿带位于东昆仑造山带北西段,带内以往开展了以铁为主的找矿工作,发现一批矽卡岩型中型矿床。近年来带内找矿取得了重大突破:①发现一种新类型矿床——"虎头崖"式层控型大型多金属矿床;②低缓磁异常区多金属和铁矿找矿效果显著,发现四角羊-牛苦头大型多金属矿床,野马泉矿区多金属矿规模达到中型,尕林格矿区发现深部厚大的铁矿体。在系统地综合总结这些成果的基础上,探讨了找矿新进展的意义,划分了3处成矿远景区,并初步讨论了各成矿远景区内进一步找矿的方向。  相似文献   

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����  ����  ��־��  ���³�  ��� 《大地测量与地球动力学》2014,34(5):114-119

??GNSS??????????У??轫GNSS?????????????????????????????????????????GNSS???????????????????????????????????????????????????????????????????????????????????????????????????????????????е???????????????????????е????λ???ó????????????????????????????????????????????????????????????????о???GNSS????????????????????????????????????????????????????????????????????????????????????????????????????????????  相似文献   

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陈鹏  陈家君 《大地测量与地球动力学》2014,34(2):105-110

??2012??1???????????????????г??????????????????????????????????????????????????????????????????????????????????????????????????????????????????????к?????????????????????????????????--??????????????????????????????  相似文献   

Variation of the 0+ ion density during low and high solar activity as measured by the SR0SS-C2 satellite     

《Atmósfera》2014,27(3):227-237

The O⁺ ion density measured by the SROSS-C2 satellite during solar minima (year 1995, F_10.7 = 77) and maxima (year 2000, F_10.7 = 181) has been analyzed for studying diurnal, seasonal, latitudinal and geomagnetic variations. The study region covers an area encompassed between 5-3 5° N latitude and 65-95° E longitude over India at a ~500 km altitude (F2 region). The year 2000 shows significant enhancement in the annual average of O⁺ ion density and attainment of post sunset secondary enhancement compared to 1995. Attributed to photoionization, daytime shows a maximum ionization compared to nighttime. However, attainment of post sunset secondary maxima is attributed to the strong pre-reversal enhancement in the vertical E x B drift. The effect of geomagnetic activity Kp through the E x B drift dynamic movement on O⁺ ion density distribution studies indicates periodicities of seven and nine days in 1995 and 2000, respectively, and polynomial dependency of the O⁺ ion density on geomagnetic activity Kp. Further on, stratification of the O⁺ ion density according to latitude (5-35° N) indicates high density in mid-latitudes (12-24° N) compared to high and low latitudes, except in the winter of 1995, which shows a distinct trend (i.e., density decreases with increasing latitude).  相似文献