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1.
酆晓  丁丽青 《华南地震》1998,18(4):23-30
应用时空域层次分析新思路及我国地震科技攻关成果对珠江三角洲地区的地震前兆资料进行了数据处理和综合分析,对该区的地震前兆场特征作了较全面系统的研究,并对目前存在的区域前兆异常场进行特征分析。研究认为,区内现有的前兆监测方法在中强地震发生前呈现出与正常动态变化相异的中期或中短期前兆异常反映,并具有相对丛集的总体特征。前兆异常场由东莞虎门重力、广州水化学等构成。最后对珠江三角洲地区近期的地震危险性进行了  相似文献   

2.
用地震异常前兆信息量综合数学表达式的方法,选择四川地区映震较好的前兆观测资料,进行地震短期异常前兆信息量的提取,分析四川地区地震短期异常前兆信息量综合时序值变化与四川及邻区6级以上强地震的关系,给出了四川及邻区6级以上地震短期综合预测的指标和方法,该方法能通过R值评分检验。用同样的方法提取不同学科前兆信息量地震短期综合预测的指标和方法,并进行地震预测效能检验,结果表明,不同学科前兆信息量短期综合地震预测效能存在一定的差异。  相似文献   

3.
滇西地区强震与地形变异常的前兆特征   总被引:2,自引:0,他引:2  
以形变(倾斜、应变)观测资料,采用经过实效检验分析后有效率较高的形变前兆参量及异常判别方法,以近年来发生在滇西地区的6级以上地震:武定地震、丽江地震、宁蒗地震以及姚安地震的震例,用滇西及川滇交界地区形变观测网的资料进行综合分析,重点对该地区强震前兆异常的时空演化及特征进行分析研究,对其在强震前中短阶段的前兆异常变化的基本特征进行了探讨。  相似文献   

4.
在地震综合信息量的基础上,改进了地震前兆异常的出现概率的计算方法,得到地震前兆综合加权信息量。利用“地震预报专家系统”的思想对每一异常事件进行综合评价,考虑到异常的可靠性、有效性、显著性及相互关联性。给予没的权重,以每一异常事件的最可能发震时间来估算异常出现的概率,计算了澜沧-耿马地震的地震前兆综合加权信息量,并对这种信息量变化的特点进行了分析。  相似文献   

5.
研究地震前兆数据的异常变化是地震短临预测的基础,本文提出一种地震前兆数据的异常智能检测新方法,利用长短期记忆单元的递归神经网络(LSTMRNN)构建数据趋势变化预测模型,通过模型预测的误差来提取数据的异常变化。该方法不需要对原始数据进行预处理,也不需要对异常数据判断的经验积累,适用于各类不同长度的地震前兆数据异常检测。通过使用三类真实的前兆观测数据的进行方法检验,将机器检测结果与人工识别结果进行对比分析,试验结果表明,基于LSTM-RNN的异常检测方法能够准确识别各类异常,可以代替人工用于地震前兆数据的异常检测。  相似文献   

6.
本文对青岛市地震前兆各台站监测现状和前兆监控能力进行了分析总结,得出青岛市地震前兆监控能力参考图,从而对今后的前兆异常分析和前兆规划建设有所帮助。  相似文献   

7.
许秋龙  李艳萍 《内陆地震》2004,18(3):228-234
在对地下流体单项前兆进行异常识别和效能评价的基础上,应用综合异常指数方法对新疆38项地下流体前兆观测资料进行分析,结果表明该方法不仅能较好地识别和提取地震短临前兆,还能对成组地震事件有所显示。  相似文献   

8.
高立新  索亚峰 《地震》2005,25(1):103-110
2003年8月16日内蒙古巴林左旗—阿鲁科尔沁旗间发生5.9级地震。 根据年度危险区的确定、 前兆异常跟踪及其主要依据, 分析了这次5.9级地震前大甸子井、 库伦井地下水位、 开鲁井水氡等前兆异常, 在此基础上, 对内蒙古附近区域的前兆异常也进行了分析和探讨, 表明该次地震前在内蒙古及附近区域出现了一组中期、 短期前兆异常及宏观异常, 文中还研究了该区域前兆异常的演化过程。  相似文献   

9.
在建立灰色与周期残差叠加模型的基础上,对用此方法识别地震前兆异常进行了研究;并用此方法对永年等前兆资料进行了处理分析,结果表明,这些手段在地震前分别有明显的异常显示。另外,本文还对其它有关问题进行了讨论。  相似文献   

10.
杨芬  金明培  赵家本 《中国地震》2007,23(2):175-183
本文使用前兆群体异常信息提取的方法,即应用前兆群体非均匀度ID和前兆综合信息量S数学分析,以及相关计算软件,对滇西地震预报实验场及邻区(N24~28°,E98~102°)的断层形变和地下流体各种监测手段的多台项观测资料进行了系统计算分析。研究结果表明:多台多测项前兆群体异常的映震效果优于多台单测项前兆群体异常的应震效果;前兆群体异常与中强地震的对应关系较好,且一组前兆群体异常一般会对应2次以上中强地震,显示了前兆群体异常与地震成组对应关系,而不是以往单次前兆与单个地震一一对应关系。  相似文献   

11.
The data on geomagnetic reversals are compared with the changes in the organic world and with the lower-mantle plumes. The times of the formation of plumes and the times of their appearance on the Earth’s surface relate to the intervals characterized by the different frequencies of geomagnetic reversals, i.e., there is no interrelation between the formation of plumes and the frequency of the changes in the geomagnetic field polarity. At the same time, a certain synchronism is observed between the frequency of the geomagnetic reversals and the boundaries of the biostratigraphic ages, i.e., the changes in the organic world in the long-period range. A hypothesis is proposed, which explains the change in the sign of the geomagnetic field by the combined effect of the irregular rotation of the internal core relative to the mantle and the changes in the slope angle of the axis of the Earth’s rotation, which, in turn, results in synchronous events on the Earth’s surface: the rates of changes in the organic world.  相似文献   

12.
Summary The maintenance of the axisymmetric component of the flow in the atmosphere is investigated by means of a steady-state, quasi-geostrophic formulation of the meteorological equations. It is shown that the meridional variations in the time-averaged axisymmetric variables can be expressed as the sum of three contributions, one being due to the eddy heat transport, another to the eddy momentum transport, and a third to the convective-radiative equilibrium temperature which enters the problem through the specification of a Newtonian form of diabatic heating. The contributions by the large scale eddies are evaluated through the use of observed values for the eddy heat and momentum transports.The contributions from each of the three forcing mechanisms to the temperature and zonal wind fields are invstigated individually and found to be of about equal importance. The sum of the three contributions are also presented for the temperature, the zonal wind, the stream function associated with the mean meridional circulation and the corresponding vertical motion. Although the results fail to reproduce the main observed features of the lower stratosphere, they are found to be in good agreement with observations in the middle latitude troposphere. At any pressure level, for example, the computed mean zonal wind has a jet-like profile and the axis of the jet is found to slope to the south with height, as observed in the atmosphere.Based in part on a thesis submitted by the first author as partial fulfillment of the requirements for the Ph.D. degree at the University of Michigan. — Publication No. 194 from the Department of Meteorology and Oceanography, The University of Michigan.  相似文献   

13.
Summary The author mentions the aims of the World-wide gravity project he established in the Ohio State University in Columbus, in 1950. He outlines the practical procedure of the gravimetric computations of the undulationsN and the vertical deflection components and and emphasizes that only by the global international cooperation and additional gravity observations at sea carried out during the last decade it has been possible to gather to Columbus the needed gravity material. Since there exist still large gravimetrically unsurveyed areas it is of vital significance to study what gravity anomalies are best to be used for these regions. The given figures concerning the accuracy of theN, and , estimated theoretically and obtained in practice, indicate that in the gravimetrically well surveyed parts of the world like in Europe and the United States we can get gravimetrically on basis of existing gravity material theN-values with accuracy of about 5–10 meters, and and with the accuracy of about 1. The geoid undulationsN are already computed in Columbus for more than 6000 points of the northern hemisphere. The sample maps show the interesting geoid of Europe and vicinity between the latitudes 60° and 30° and longitude 5° W and 30° E, drafted on basis of more than 1000N-values computed at the corners of 1°×1° squares. It is interesting to realize that the geoid undulations in all this area are positive, the extreme values being between 40 and 50 meters. The geophysical significance of the geoid maps of this kind is pointed out.  相似文献   

14.
15.
陈伯舫 《华南地震》2004,24(4):8-10
综合APIA、HONOLULU、PAMATAI 3个地磁台三分量的11年周期变化的形态后,可定性地提出该变化源于内场。如内源为核幔边界的电涡流,则其中心点应位于3台之间。  相似文献   

16.
Until recently, the existing data prevented the geophysicists from accurately dating the Bysy-Yuryakh stratum, which outcrops in the middle reach of the Kotuy River, constraining the time of its formation to a wide interval from the end of the Late Cambrian to the beginning of the Silurian. The obtained paleomagnetic data unambiguously correlate the Bysy-Yuryakh stratum to the Nyaian regional stage and constrain its formation, at least a considerable part of it, by the Tremadocian. This result perfectly agrees with the data on the Bysy-Yuryakh conodonts studied in this work and yields a spectacular example of the successful application of paleomagnetic studies in solving important tasks of stratigraphy and, correspondingly, petroleum geology. Within the Bysy-Yuryakh stratum, we revealed a large normal-polarity interval corresponding to the long (>1 Ma) period when the geomagnetic reversals were absent. This result, in combination with the data for the Tremadocian and Middle–Upper Cambrian sequences of the other regions, indicates that (1) the rate of occurrence of the geomagnetic reversals on the eve of the Ordovician Moyero superchron of reversed polarity was at most one reversal per Ma; (2) the superchron does not switch on instantaneously but is preceded by a certain gradual change in the operation conditions of the dynamo mechanism which, inter alia, manifests itself by the reduction of the frequency of geomagnetic reversals with the approach of the superchron. This finding supports the views according to which a process preparing the establishment of the superchrons takes place at the core–mantle boundary.  相似文献   

17.
18.
The global database on the paleointensity, containing determinations of the virtual dipole moment (VDM) for a stable (normal) regime of the geomagnetic field in a time interval of up to 3.5 Ga, is supplemented by new VDM determinations and analyzed. The field generation process started no later than 3–3.5 Ga (earlier data are absent) at the stage of the Earth’s core formation. Since that time, the dipole value has differed from its present value by no more than an order of magnitude, and the deviations that have already been detected tend toward smaller values. The distribution of VDM values in the time interval 0–400 Ma is bimodal, which apparently reflects the presence of two different generation levels of the geomagnetic field distinguished by a relatively large value (close to the present field value) and a relatively small value (approximately half as large as the present value). The total duration of decreased VDM values appreciably exceeds that of increased VDM values (179.1 and 28.6 Myr, respectively). On the whole, data on the paleointensity do not contradict the hypothesis about the dipole nature of the field over the last 400 Myr; however, the number of determinations at high paleolatitudes is too small to draw decisive conclusions on the validity (or invalidity) of the dipole field approximation based solely on paleointensity data.  相似文献   

19.
The nutations of the planets Mars andEarth are investigated and compared. Alarge number of interior structureparameters are involved in the nutationcomputations. The comparison between the observations and the computationsprovides several constraints on these parmeters andtherefore allows a better understanding of the physics of the interior of theplanet. For the Earth, the high precision of the observations of the nutationshas led to a very good determination of interior properties of the planet. ForMars, observations of nutations are not yet available, and we review how theamplitude of the Martian nutations depends on the hypotheses consideredfor its interior. Although Mars is very similar to the Earth, its interior is not well known;for example, we don't knowif its core is liquid or solid. Only if the core is liquid,the Free Core Nutation (FCN) normal mode exists and can alter the nutationswhich are close to the resonance. From the observed geoids, it is known thatboth planets are not in hydrostatic equilibrium. The departure is larger forMars than for the Earth, and consequently, the implication of considering a convective mantle instead of a mantle in hydrostatic equilibrium described byClairaut's equation for the initial equilibrium state of the planet is largeron the Martian nutations than on the Earth nutations. The consequences of theuncertainty in the core dimensions are also examined and shown to be of a veryhigh influence for Mars if the core is liquid, due to the potential changes inthe FCN resonance. The influence of the presence of an inner core, which isknown to exist for the Earth, could be more important for Mars than for theEarth if the inner core is large. Due to the presence of Tharsis on Mars, thetriaxiality of this planet has, additionally, larger effects than on Earth.  相似文献   

20.
Geomagnetism and Aeronomy - The evolution of the magnetic configuration in the solar corona is studied. The curvature of the K-corona helmets obtained from an analytical approximation of the...  相似文献   

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