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郯庐带中强地震前后多参数综合异常时空特征研究 总被引：1，自引：0，他引：1
本文应用基于地震对应概率谱的多参数滑动极值相关度方法对郯庐断裂带进行时间和空间扫描计算。 时间计算结果显示绝大多数目标地震发生之前均有高值异常现象出现; 空间扫描计算结果显示中强地震前1年左右, 震区及其附近区域多参数滑动极值相关度出现高值异常现象, 且异常区域逐渐扩大增强, 地震多发生在异常区域内或者附近。 中强地震发生后, 高值异常区逐渐缩小, 震后1年左右异常区域基本消失; 中强地震平静时段的多参数滑动极值相关度均无高值异常区域出现。 相似文献
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基于地震对应概率谱的多参数综合异常空间特征研究 总被引：2，自引：0，他引：2
本文应用基于地震对应概率谱的多参数滑动极值概率方法对新疆南天山西段多种地震学参数资料进行定量化的异常识别提取, 通过对该区中强地震前多参数滑动极值概率的空间演化过程进行全时空扫描, 定量识别了该区中强地震的前兆综合异常时空异常特征。 研究结果表明, 南天山西段1980年以来发生的10次(组)中强地震前1～2年, 震区附近区域多参数滑动极值概率均出现了高值异常变化过程, 震后1年左右高值异常区逐步分散、 缩小乃至消失, 而中强地震平静时段滑动极值概率普遍无高值异常区域出现。 相似文献
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文章采用多种地震学参数的地震对应相关谱(ECRS)方法,分析研究阿拉善左旗及邻区ML≥5.0地震多种地震学参数的地震对应相关谱时空演化特征。结果表明,目标地震前多参数滑动极值平均概率时序曲线会出现高值异常;震前约1年左右,空间图像出现高值异常,接近临震异常区域会扩大增强,震后1~2年异常区域逐渐弱化消失。研究结果可为此地区中强地震危险性的判定提供科学依据。 相似文献
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通过对1992~2008年间各期观测资料进行全时空扫描,分析华北地区网区重力场的演化特征,总结震前异常的形态、持续时间和变化幅度,指出重力场空间变化易于发生地震的部位,并对一些问题进行讨论。结果显示:华北地区重力场总体变化不具明确规律性;大量测点存在明显的背景性趋势性异常变化;重力场变化与网区及周边地区中强地震的活动联系密切,较明显的重力场异常反应多发生在震前2年左右时间,且常伴有大面积高值异常区出现。重力变化"0"线、高梯度带、异常中心(含极值)附近是重力场空间变化易于发震的部位。 相似文献
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对1971年以来中国台湾地区11次MS≥7.0主震进行震前地震活动性参数的时空扫描分析。选取参数b、E、N、Mav、S进行震前时间扫描特征分析,结果表明:所选参数在震前异常表现为低值,地震多数发生在低值持续时或者低值异常恢复后1年内。选取Ab和S进行震前空间扫描特征分析,结果表明:地震多数发生在异常区出现明显收缩或扩大之后,震中主要分布在异常区最大面积边缘或外围附近。 相似文献
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《地震研究》2015,(4)
结合地震前兆信息量综合数学表达式和小波变换、EMD分解技术,遴选郯庐断裂带中南段及其附近地区67个台点91个测项的连续性、可靠性较高前兆观测资料,多频域剖析前兆观测资料的变化特征、多层次挖掘地震前兆观测异常、最大程度地展示前兆群体映震效能。结果显示,地震综合前兆信息量时序曲线,在ML≥5.0地震前会出现不同程度的高值异常(S时序≥0.1),一般高值异常出现1~6个月内,研究区有发生ML≥5.0地震的可能;地震前兆信息量综合空间扫描的结果显示,未来的震中区多位于最早出现S窗≥0.2异常区的边缘区域,但异常区域的迁移规律性特征不明显,这可能与资料分析时段研究区内发生地震的震级较小及前兆台点的空间分布不匀有一定的关系。 相似文献
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运用刻画强震前中,小地震在时空分布上不均匀性的参量ＧＬ值的方法,系统研究了华北地区２８次Ｍｓ≥５．０中强震前ＧＬ≥１．０的高值异常在空间上的分布特征和时间上的变化特征,系统开展了该地区不同地震活动水平的计算震级下限,时间窗,空间窗的合理性研究。对计算中所选取的参数进行优化和修改;采用全时空扫描的方法研究,追踪华北地区历次中强震前ＧＬ值的异常变化。结果表明：华北地区８２％的中强震前约１～３．５年内,在未来震中的附近出现明显的高值异常区,地震多发生在异常区的边缘或附近。ＧＬ值异常区的时间曲线表明,异常持续时间为３～２５个月不等,异常持续时间优势分布为３～１４个月,约占总异常的７８％;异常结束后,地震发生的优势分布为０～１４个月,约占总异常数的８３％,由此认为,ＧＬ值方法可能成为华北地区中强震预测的一个较为有效的方法 相似文献
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根据加卸载响应比理论，通过对1991-1996年江苏省部分井孔观测资料固体潮加卸载响应比的计算发现，在中强地震前一年左右的时间震中区附近的井孔出现了响应比高值异常。通过空间图像扫描可能看出；在苍山地震前一年左右。徐州，宿迁地区出现了加卸载响应比的高值集中区；在南黄海地震前一年左右。在镇江，苏州地区出现了高值集中区，之后高值集中区有自西向东迁移即有向震中区迁移的迹象。 相似文献
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D. M. Pechersky A. A. Lyubushin Z. V. Sharonova 《Izvestiya Physics of the Solid Earth》2010,46(7):613-623
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
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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
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Prof. Dr. W. A. Heiskanen 《Pure and Applied Geophysics》1958,41(1):1-18
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
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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
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V. E. Pavlov T. Yu. Tolmacheva R. V. Veselovskiy A. V. Latyshev A. M. Fetisova I. V. Bigun 《Izvestiya Physics of the Solid Earth》2017,53(5):702-713
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
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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
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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
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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