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1.
从地震构造和地震活动角度,对郯庐断裂带下辽河-莱州湾段和潍坊-嘉山段进行了对比,认为这两段的地震构造环境具有明显不同,地震活动明显属于不同模式。其中下辽河-莱州湾段属群集型地震活动类型;潍坊-嘉山段属特征型地震活动类型。对于下辽河-莱州湾段,未来应注意在新的活跃期或活跃幕到来时群集型强震、中强震的连续发生;对于潍坊-嘉山段,则应注意断层分段本身所控制的地震复发重现规律。  相似文献   

2.
高国英  韩月鹏 《内陆地震》1995,9(4):357-362
对1880 ̄1993年新疆及邻区7级以上强震活动特征进行了分析讨论,认为研究时段内7级以上强震活动有明显的活跃与平静交替现象。研究时段内的强震活动经历了5个轮回,每个轮回包括一个平静幕和一个活动幕,每个活动幕都有相对的主体活动区,主体活动区和7级以上单个强震都具有沿西昆仑-南天山-北天山-阿尔泰地震带往返迁移的特征。各地震带6级以上地震活动也具有明显的由西南向北东整体迁移的特征,并且这种时、空、强  相似文献   

3.
通过对中国大陆及邻区4个Ⅰ级活动地块中1972—2003年全部地震资料的系统分析,认为强震中期阶段典型的地震活动演化图像是中等地震聚集活动,震前震中区附近的地震密度和有效速率增高。文中用中等地震增长率来刻划强震孕育过程中中等地震活动的加速增长,结果表明:中等地震聚集活动密度的增长率能够较好地反映强震前中期异常变化特征,对各活动地块的分析表明华北地块中等地震增长率达到180%以上时,未来1~3a中等地震异常聚集区及其附近会发生强震;而西域、青藏和滇缅地块中等地震增长率达到250%以上时,应注意中等地震异常聚集区及其附近强震的发生。因此,中等地震增长率可以作为中期预报的定量化指标  相似文献   

4.
郯庐断裂带中段全新世活断层的特征滑动行为与特征地震   总被引:16,自引:0,他引:16  
晁洪太  李家灵 《内陆地震》1994,8(4):297-304
郯庐断裂带中段全新世活断层由3个独立的破裂段组成。从各破裂段的运动性质、位移分布看,断层的运动属特征地震型滑动。地震活动以强震活动为主,强震具有周期性原地重复发生的特点,且其强度基本相同;中强地震缺失或很少发生;b值在高震级范围内具低b值的非线性关系。这些特点正是特征地震的典型表现.根据郯庐断裂带中段活断层全新世以来的活动特点看,未来该区仍然以特征地震方式活动.按郯庐带的强震复发间隔和各段的最新一次活动时代推算,未来一段时期内新沂-宿迁段复发大震的可能性较大,安丘段次之,莒县-郯城段复发大震的可能性则很小。  相似文献   

5.
通过对中国大陆及邻区4个Ⅰ级活动地块中1972-2003年全部地震资料的系统分析,认为强震中期阶段典型的地震活动演化图像是中等地震聚集活动,震前震中区附近的地震密度和有效速率增高.文中用中等地震增长率来刻划强震孕育过程中中等地震活动的加速增长,结果表明:中等地震聚集活动密度的增长率能够较好地反映强震前中期异常变化特征,对各活动地块的分析表明华北地块中等地震增长率达到180%以上时,未来1~3a中等地震异常聚集区及其附近会发生强震;而西域、青藏和滇缅地块中等地震增长率达到250%以上时,应注意中等地震异常聚集区及其附近强震的发生.因此,中等地震增长率可以作为中期预报的定量化指标.  相似文献   

6.
地震活动与黄河下游大堤潜在危险性的探讨   总被引:2,自引:0,他引:2  
黄河下游为一条地下悬河,存在着严重的地震危险性,未来强震会引起大堤失稳开裂,造成特大水灾,本文研究了黄河下游菏泽和滨州地区断裂及地震活动特征,对比历史上地震发生以黄河大堤的影响,认为黄河东明-梁山段和滨州段将是黄河下游具潜在危险的地段,并提出了防御措施,这对减轻避免黄河下游地区因地震活动而引起的水灾具有重要意义。  相似文献   

7.
冯德益 《华南地震》1996,16(4):1-10
利用反映震级-频度关系的参量C值,η值,b值和b值谱以及反映地震空间分布的森下指等研究了近海地震活动的一些主要特征,发现近海强震前地震活动性指标及图象的变化特征与陆地上强震前的特征存在一定差异;给出了新研究的可用于近海及滨海地区强震预报的短期和临震  相似文献   

8.
研究了四川雅江,盐源至云南永胜复杂地震构造区的分段地震活动性以及震源力学作用形式和震型特征;以现今强震活动空段,最新地壳形观测图像,突出的震群活动给出该地震构区未来强震危险性的认识。  相似文献   

9.
临汾盆地地震危险性浅析   总被引:1,自引:0,他引:1  
本文通过强震地震穴的地震序列分析,华北地震迁移、汾渭地震带地震丛式分布,和地震丛的强度分析以及汾渭地震带分段及强弱段相间分布特征,与本活动期地震丛活动空间分布等论述了临汾地震的危险性。  相似文献   

10.
澜沧—耿马地震短期和临震阶段的地震活动特征   总被引:1,自引:0,他引:1  
郑月君  陆远忠 《地震》1994,(5):78-83
本文主要分析了澜沧-耿马地震震前短临阶段的地震活动特征,包括b值、震群、临震的小震活动等,文中也简要回顾了大同地震前的地震活动特征。同时探讨了地震系列的算法复杂性在实际震例中应用的可能,表现为在时间分布上强震前大小地震的有序性增加,随机性降低的过程。目的是寻找强震前一定时空范围内,中期向短期阶段过渡及短临阶段普遍存在的地震活动图象的演化信息。  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.
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   

17.
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   

18.
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   

19.
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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