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利用美国国家环境预测中心NCEP全球再分析资料的温度图像结合天体引潮力附加构造应力,对2003年5月以来的国内MS≥6.0、国外MS≥7.0的地震作了统计分析。以2004年7月12日—2004年8月25日间西藏地区3次地震为例得出如下认识:NCEP温度异常图像可以较好地反映短临地震构造活动时空演变过程;天体引潮力附加构造应力对地应力处于临界状态的活动断层具有明显的诱发作用;利用NCEP温度异常图像与天体引潮力附加构造应力结合进行地震短临预测是具有良好应用前景的新思路;西藏的3次地震均发生在天体引潮力附加构造应力周期相同的相位上,即天体引潮力附加构造应力变化达到相对稳定的峰值的末端,而不是发生在天体引潮力附加构造应力最大时刻,同时2003—2004年在西藏发生的其它震例中,地震发生在上述周期相同的相位,因此认为应当对其它区域更长时间更多的震例作这方面的进一步研究 相似文献
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通过利用发震区域的天体引潮力附加构造应力变化模型, 研究了2005年11月26日江西九江MS5.7地震发震构造与天体潮汐引力的关系, 并利用该模型结合美国国家环境预报中心多源综合温度数据资料, 分析了九江地震前后发震区域热异常在时空上的动态变化特征. 结果显示, 一方面, 在时间序列变化上, 孕震区热异常表现出的起始—消亡演变过程与岩石在应力加载下的形变—破裂过程相吻合. 无论近地表大气还是上附多层大气, 热异常主要集中在活动断裂带及其附近区域, 与构造断裂带分布相一致; 同时, 热异常从近地表到高空消失的垂向分布, 符合地面对大气加热导致大气升温→抬升→扩散→消亡的大气动力学基本特性, 表明构造运动是本次温度异常变化的主控原因. 另一方面, 热异常变化遵循引潮力(低值—高值—低值)的变化过程, 显示出天体引力对发震断层温度异常识别具有一定的指示意义以及引潮力可能对构造应力处于临界状态的发震断层具有诱震作用, 预示利用引潮力附加构造应力与热异常变化相结合研究短临地震预测具有一定价值. 相似文献
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对2011年12月1日莎车Ms5．2地震的天体引潮力周期变化过程进行计算,并根据该周期分析了NCEP温度数据资料,提取地震前的异常增温变化图像。结果表明：天体引潮力对处于临界状态的活动断层具有诱发作用;震前温度变化发生明显异常,经历起始增温一异常加强一高峰一衰减一平静的演化过程;出现温度异常位置与震中位置有较好的空间对应关系;NCEP温度异常研究在地震前兆研究中有较好的实用价值。 相似文献
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本文讨论了在构造应力水平达到岩石破裂临界值时引潮力、潮汐附加应力的动态变化与地震序列之间的关系，选用了中国大陆1970年以来7级以上地震序列资料，分析了引潮力水平分量动态变化与强震发震时间之间的关系，结果显示在一定时空范围内前震、主震及余震序列发震时刻的引潮力存在优势方向，多数地震发震时刻与选取时段引潮力水平分量的方位角相位比平均值仅为35%；对于构造复杂地区，结果显示引潮力水平分量的方位角不仅存在一个优势方向，还明显存在其他优势方向，可能与发震构造有关.根据1966～1976年中国九大地震震源机制解计算潮汐正应力和滑动方向的剪应力及其变化率，结果显示多数地震发震时刻潮汐剪应力接近最大值. 相似文献
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2013年4月20日在我国四川省芦山（30.284o N, 102.955o E）发生MS7.0地震,计算该地区潮汐变化,地震时刻引潮力处于最低相位点,显示引潮力的诱震作用属于典型逆冲断层作用类型。以此潮汐周期为时间指示（4月12日~4月23日）,利用NOAA卫星地面长波辐射（OLR）数据资料分析全国范围地震前后热辐射值连续变化,结果显示：伴随潮汐演化,在全国范围（17°N-55°N ~ 73°E-155°E）内,震前OLR仅震中及其相关联断裂附近发生了显著而连续异常变化过程：在时间上经历了起始增温→异常加强→高峰→衰减→发震→平静的演化过程;在空间上异常位置与震中基本吻合,发展过程表现出沿断裂带由分散→汇聚→分散的破裂过程,与岩石应力加载破裂演化经历：初始微动破裂→扩张破裂→应力闭锁→地震爆发→平静阶段的力学过程完全吻合,显示天体引潮力对处于临界状态的活动断层具有诱发作用,而长波辐射异常是地震构造应力应变过程辐射表征。将引潮力与OLR异常结合在地震前兆研究中有一定的实用价值。 相似文献
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利用天体引潮力周期变化模型和地面长波辐射(OLR)数据资料,分析2010~2011年云南、西藏地区的4次M5.0以上地震震前OLR异常,探讨了诱发地震的外部因素,即天体引潮力周期与红外异常发展的关联特征。结果显示:以临近发震时刻所在周期引潮力值最低点日期为OLR参照背景,获取的地震前后NOAA长波辐射OLR日增量分布图像显示:震中附近热异常明显,异常受构造控制,且其分布与断裂关系密切;异常演化经历起始-加强-高峰-衰减-再增强-发震-平静的过程,符合岩石因应力增加而破裂的规律。一方面表明地应力的临界状态演化过程可通过OLR辐射变化来反映。另一方面表明引潮力可以改变构造内部地应力的状态。 相似文献
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《地震地磁观测与研究》2016,(6)
2014年8月3日中国云南省鲁甸发生M_S6.5地震,震源机制显示为走滑断层,利用NOAA卫星地面长波辐射(OLR)数据资料,对地震前后热辐射值连续变化进行分析,结果显示:在中国大陆范围(20°—45°N,80°—120°E)内,仅震中及相关联断裂附近,地面长波辐射(OLR)在时间上经历了起始增温→异常加强→高峰→衰减→发震→平静的演化过程,在空间上异常沿断裂由北向南向震中迁移。对鲁甸地区引潮力进行计算,结果显示,天体引潮力对本次地震具有显著诱发作用,长波辐射异常可能是地震构造应力应变过程的辐射表征。 相似文献
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分析甘肃岷县M_S6.6地震前后潮汐变化发现,发震时刻引潮力处于最低相位点,显示引潮力的诱震属于典型逆冲断层作用类型。以潮汐周期为时间指示,利用NOAA卫星地面长波辐射(OLR)数据,分析震中及其邻近区域(30°~40°N,90°~110°E)地震前后(7月17~25日)地面长波辐射值的连续变化状况,结果显示,震前仅震中及其相关联断裂附近OLR发生了显著且连续的异常变化,在时间上经历了起始增温—异常加强—峰值—衰减—发震—平静的演化过程;在空间上异常区域覆盖震中,与汶川地震引发的应变积累正影响区之南北地震带北段基本吻合;在形态演化上,表现出沿断裂带分散—汇聚—分散的破裂过程,并与岩石应力加载破裂的初始微动破裂—扩张破裂—应力闭锁—地震爆发—恢复平静阶段的力学过程完全吻合。这可能预示该地震发震前后天体引潮力对处于临界状态的活动断层具有诱发作用以及长波辐射异常在一定程度上对地震构造应力应变过程辐射进行表征。 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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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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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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俯冲带作为地球最为庞大的循环系统的重要组成部分,已成为地球科学的研究热点之一.很多俯冲带,特别是环太平洋俯冲带内的中深源地震,在空间上呈明显的分层分布,并且各层地震具有不同的震源机制,即所谓的双地震带现象.本文简要介绍了环太平洋双地震带形态特征与震源机制的空间分布,并回顾了双地震带的几种成因模型.根据形态特征和震源机制的差异,中源深度的双地震带可以分为两类,其中,一类双地震带对应上、下二层分别为压缩和张性的地震分布;另一类双地震带的震源分布较浅,且其浅部地震以横向压缩为主.此外,日本本州东北俯冲带的地震分布可能是由三层地震带组成的,而且汤加、伊豆-小笠原地区还发现深源深度的双地震带.通过对双地震带的形态特征以及其热力学条件的研究,人们从抗弯作用、脱水脆化、相变断层等多方面,尝试建立解释双地震带成因的模型.目前,大多数研究利用数值计算结果,结合蛇纹石脱水脆化、相变断层模型,能够不同程度地分别解释中源和深源双地震带成因.不过,这些模型几乎相互独立,并不能同时解释中源和深源双地震带.有人试图尝试用统一模型解释中深源地震成因,例如,先前存在的断层模型,不过该模型还不很具有说服力.也可能是多种因素的联合作用,共同影响着俯冲板内的温度场、应力场分布. 相似文献