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1.
为划分临汾盆地第四纪地层,在临汾市东布设1个控制性钻孔,描述其所揭示的地层岩性特征。通过对钻孔剖面中269件孢粉样品的孢粉组合进行分带讨论,结合9个光释光样品和12个电子自旋共振样品的年龄测试结果,认为该控制性钻孔记录了379ka B.P.以来的沉积地层,其中埋深0~0.4m属于全新统,0.4~80.8 m属于上更新统(孢粉记录揭示出相对干燥寒冷的古气候特征,终末期气候转暖,降水增多),埋深80.8m以下属于中更新统(代表了温暖潮湿的古气候特征)。晚更新世以来平均沉降速率为0.64mm/a,远高于临汾盆地第四纪平均断陷速率,表明晚更新世以来临汾盆地的新构造运动呈现增强趋势。 相似文献
2.
华北平原东部地区晚更新世以来的孢粉序列与气候分期 总被引：14，自引：0，他引：14
本文应用图象识别方法,对华北平原东部地区(宝坻—濮阳)的五口井和一个剖面的孢粉资料进行了研究,将本区晚更新世晚期一全新世地层划分为五个孢粉组合带,七个孢粉组合亚带,共建九个孢粉植物群演化阶段。在此基础上根据植物生态特征,探讨了两万年以来的气候演变,确立了九个气候期,并发现全新世以来气候变化具有八次明显的降温及七次升温过程,存在着二千五百年及千年左右的波动周期 相似文献
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文中以14个钻孔地层编录为基础,结合前人研究资料,初步总结了福州盆地埋藏第四纪地层的沉积特征。福州盆地沉积始于晚更新世中期(约56.5ka BP),由砾石、砂、黏土、淤泥组成,总体表现为从下至上粒度变细的沉积序列,地层岩性横向变化较大;盆地内发育3层淤泥,第1,2层淤泥发育于全新世中晚期,时代为1.44～7.86ka BP,为“长乐海侵”的产物,第3层淤泥发育于晚更新世晚期,时代约为44～20ka BP,为“福州海侵”的产物;盆地埋藏晚第四纪地层可划分为上更新统和全新统,分为4个组,从老至新分别为龙海组(Q3pl)、东山组(Qhd)、长乐组(Qhc)与江田组(Qhj)。龙海组归属上更新统,划分为3段,其余3个组归属全新统 相似文献
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根据对南海ODP1144站下段孢粉分析, 将其自下而上分为两个孢粉组合带和11个组合亚带. 根据松粉、蕨类孢子及草本植物花粉含量的相互消长关系, 将PB带进一步划分为11个孢粉组合亚带(PB21~11), 分别与深海氧同位素分期相一致(对应MISs 21~11期). 间冰期孢粉组合以松粉和蕨类孢子含量增加、草本植物花粉含量降低为特征; 冰期则相反. 间冰期孢粉组合面貌反映其气候与现代相似. 各冰期出露的大陆架上生长了以禾本科、莎草科及蒿属为主的草本植物. 组合亚带PB12(对应MIS12期)中Artemisia花粉含量的增加及高的松粉沉积率值表明此次冰期气候相对干冷, 冬季风较强. 相似文献
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灵宝盆地位于华北板块南缘与秦岭造山带之间,是豫西北一系列北东-南西向断陷盆地之一.盆地内沉积地层主体为一套厚约2000m陆相碎屑岩夹泥灰岩、薄煤层沉积.本文根据盆地内的恐龙蛋、介形虫、腹足类、哺乳动物化石及少量孢粉等,将地层自下而上划分为下白垩统枣窳组、上白垩统南朝组、古近系古新统-下始新统项城群、中始新统川口组、上始新统庄里坡组及新近系上-中新世（组名暂未定）等6个地层单元.研究表明：下、上白垩统之间及其与项城群之间为不整合或超覆,上中新统与川口组或庄里坡组为不整合接触,整个地层是一套河流相沉积、局部洪泛洼地或小浅湖相沉积. 相似文献
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托斯台逆断裂-褶皱带晚第四纪活动特征 总被引：1，自引：0，他引：1
托斯台逆断裂-褶皱带位于乌鲁木齐山前坳陷的西部,为近东西向展布的新生代逆断裂．背斜带。它主要由北单斜带、中部背斜带和南单斜带3个构造带组成,在各构造带均发育逆活动断裂。地震勘探资料显示,南单斜带与中部背斜带为滑脱体,逆断裂在深部沿滑脱面与清水河子深断裂相汇。研究表明,北单斜带与中部背斜带逆断裂断错了晚更新世堆积物,在晚更新世有显著的活动;南单斜带逆断裂断错了全新世堆积物,在全新世时期有最新活动。中部背斜带逆断裂晚更新世以来水平缩短速率为0．6～1．3mm／a;南单斜逆断裂全新世水平缩短速率为0．2～0．6mm／a。 相似文献
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库松木楔克山山前断层是位于北天山西段再生造山带北缘一条重要的边界断层,是本次新发现和确定的一条活动断层。断层分为东、中、西三段:东段主要由4条断层斜列组合而成,单条断层长度为9~13 km,在晚更新世~全新世仍在强烈活动,晚更新世以来的垂直错动量为3~4 m,垂直活动速率为0.23~0.33 mm/a,全新世以来的垂直错动量为0.5~0.8 m;中段断层活动错断了中更新世至全新世地貌,形成多级断层陡坎和长约8~10 km的地震形变带,晚更新世以来垂直活动速率为0.5 mm/a;西段自晚更新以来无活动显示。 相似文献
10.
通过浅层高分辨率地震探测 ,结合钻孔资料 ,获得了测线处汾河断裂的准确位置 ,几何结构 ,活动性质、时代和速率等参数 ,并对其动力学属性进行了初步的讨论。地震探测揭露出汾河断裂的西支断层 ,为高角度东倾的斜滑断层 ,切割了第四系下部 ,上断点位于地下约 70m处。据钻孔剖面推断有 2条高角度相向而倾的斜滑断层 ,东支位于汾河东岸 ,断至全新统—上更新统 ,其底界面垂直错距约 8m。断裂北段另一个钻孔剖面表明 ,西支断层切割了全新统—上更新统 ,底界面垂直错距约6m。汾河断裂晚更新世以来的平均垂直滑动速率为 0 0 6～ 0 0 8mm/a ,大震平均重复间隔为 5 0～6 7ka 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
12.
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
13.
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
14.
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
17.
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
18.
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