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苏家屯台电磁辐射异常与地震关系研究 总被引：2，自引：0，他引：2
苏家屯观测台是位于辽宁沈阳的一个地方性专业地震观测台站，用EMAOS-L数字化电磁辐射观测仪进行电磁观测。本文将该台站4年多的电磁辐射观测资料和这期间观测到的Ms4．0以上的震例进行了收集和整理，从观测仪器的性能指标、地质构造特征、电磁信息的来源等方面进行了震例的电磁前兆异常特征分析。研究认为，该台站前兆异常突出，电、磁异常同步性好，异常信息与发生在上地壳的震源深度小于20km的地震具有良好的对应性，同时，对震级较大的地震，其前兆异常有日变周期特性。 相似文献
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本文叙述了海城、唐山、松潘大地震前地下水前兆异常的典型图象和规律性。参照已经建立的地下水前兆异常的机制和孕震模型,本文用地下水动力学原理剖析了异常机制与实际观测资料之间统一的合理性,并建立了数学模型。按照这一模型进行的地下水理论前兆场正演的结果,与大地震前实际观测的地下水异常的典型图象,基本上是一致的。 相似文献
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采用山西省的洞体形变（倾斜）观测资料，使用实效检验较有效的连续形变前兆参量及异常判别方法，结合具体的震例进行综合分析，得出适合山西洞体形变有震异常提取的两种方法即：多台异常信息提取法和相关距平去年周期法，对这两种方法进行预报效能统计检验，得出了它们的R值评分分别为0．40和0．24，其中多台异常信息提取方法R值最高。 相似文献
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对黑龙江省地电阻率台网近些年的观测资料进行了整理分析,对台网的两个地电阻率台观测资料进行了评估,发现林甸台地电阻率数据受各种干扰非常严重,无法提取震兆信息,而绥化台的观测数据质量较高,映震效能较好。绥化地震台地电阻率观测曲线具有规则年周期变化特征,以此为依据进行各向异性的前兆异常特征的研究,发现利用原始曲线法和归一化月速率方法,在中强地震前震区一定区域内的电阻率各向异性值（S）会出现上升型或下降型异常变化。分析认为速率法对于提取短临异常,判断发震时间较为理想。 相似文献
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大地电场观测地震前兆异常提取技术研究 总被引：15，自引：1，他引：14
首都圈地区布设的11个地电场观测台于2001年9月已正式投入观测,现已积累了近7年的资料．使用大地电场观测系统中同一测向的长、短极距测值的比值方法,对其中的10个台和邻区2个台的资料进行了处理,发现该方法能够较好地排除来自大地电场及自然电场远场的变化信息,突出了可识别的地震前兆异常信息．研究结果表明,2006年7月4日河北文安MS5.1震前,多数台站的地电场观测资料出现比值异常变化,从而证明了这次地震前地电场观测存在着短临异常前兆变化信息,只是由于这些信息混杂于正常大地电场变化的背景中,使用常规的分析方法无法识别和提取．研究结果还表明,地电场观测的台址条件和台址到震中区的距离与震前地电场比值异常出现的时间和幅度有关． 相似文献
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《地震工程学报》2018,(Z1)
介绍近年来甘肃深井地电阻率(ρs)实验观测的资料和震例,证明SA(甘肃单孔深井垂直观测方案)是一种前兆效能更好的方案。文中从水平层状介质的角度解释更好的机制和原理,定量估算几种装置的前兆效能,结果表明:(1)在平凉深井台站,SA装置的前兆效能是深井水平向装置的3.3倍;(2)在兰州观象台,新建的SA装置完整地记录到一个震例(异常时间段50d,其中短临时间段10d,异常变幅2.4%),而原有地面观测装置不能分辨该震例。从地面观测到深井水平向观测,解决了最棘手的电磁干扰问题,使ρs曲线成形连续;从深井水平向观测到SA方案,解决装置的前兆效能问题和最突出的季节性年变问题,使震例的特征清晰可见。文中针对需求介绍SA装置构建的方案。观测资料表明:SA方案是解决当今电磁干扰问题的最佳途径,是提高装置前兆效能的方向。 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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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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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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The depth to the top of magnetic dykes can be estimated from total field aeromagnetic data using the relation between the depth to magnetic sources and the autocorrelation function of magnetic data. By using synthetic anomalies we show that in the ideal case, depth can be determined to an accuracy of 10% or better, when the anomaly sources are two-dimensional dykes. However, the estimated depths depend on the width of the dykes. The estimated depth is about 0.6 times the actual depth to the top of thin dykes, and around the true depth for thick dykes having width-to-depth ratio around 3. The depth is considerably overestimated for very thick dykes (e.g., contacts, which is a special case of the thick dyke). Thus, the autocorrelation method requires that the width-to-depth ratio of the dyke is estimated independently to correctly estimate the depths. Alternatively, it must be assumed that the width-to-depth ratio for the two-dimensional source body is between 1.5 and 4. 相似文献
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As is known, the secular deceleration of the Earth's diurnal rotation is explained mainly by the tidal friction in the ocean. Below we consider this mechanism in some detail, taking into account also elastic deformations of the mantle under the action of ocean loading and the interaction between the tide-generating body, ocean tidal wave, liquid outer core, and solid inner core. It is shown that elastic displacements of the core-mantle boundary under the action of ocean loading are of about the same amplitude and phase as the elastic loading displacements of the Earth's outer surface. As a result, side by side with the mechanism of secular deceleration of diurnal rotation of the mantle, there are also (1) the opposite mechanism of secular acceleration of diurnal rotation of the outer liquid core and of the solid inner core and (2) the mechanism of excitation of differential rotation in the liquid core. Taking these effects into account, we compare theoretical and modern observed data on the eastward drift of the solid inner core. It is shown that the best agreement may be obtained if the turbulent viscosity of the liquid core is about 2 × 10
3
Poise 相似文献
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On data of bottom sampling, carried out by means of grab, trawl and underwater photography in August–September of 1993 in the area of the Pechora Sea, quantitative regularities of macrobenthos distribution are described for the ecological monitoring purposes. Maps of -biodiversity and biomass indices, bottom communities and trophic zones, singled out by dominant method, are presented. Assessment of structure changes of the investigated area bottom communities during the last 60–70 years is fulfilled. It is shown that the described communities on the whole are of natural undisturbed character and that the revealed changes are within the natural fluctuations in the abundance of benthic populations or may be interpreted in terms of methodical differences in the data analysis and generalization by different authors. 相似文献
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地震激励下处于深水中的桥墩和周围水体的相互作用将对桥梁结构的动力响应产生较大影响。首先对地震作用下水-桥墩的相互作用理论做了概括,给出了动水压力对桥墩的作用效应及各自的适用范围;对主要的三种考虑流固耦合效应的分析方法做了对比,探讨了地震作用下影响水-结构相互作用的主要因素,并对今后的研究提出了建议。 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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在数据完整率达到95%的基础上,为进一步确保中国大陆构造环境监测网络GNSS基准站观测数据质量,选取2010—2020年全国基准站观测数据,采用TEQC软件进行质量检验,分类整理其中多路径效应计算结果呈典型特征的台站,结合观测环境状态,对多路径效应存在的区域性特征进行分析,发现除接收机天线周围发生遮挡外,硬件更换、台站周围地势差等因素,均对多路径效应产生不同程度的影响,可为建站选址和观测环境监测工作提供参考。 相似文献