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黄土高原秦安中新世黄土-古土壤序列的蜗牛化石初步研究 总被引：5，自引：2，他引：5
通过对秦安中新世黄土-古土壤序列蜗牛化石的初步调查研究表明, 在距今22~6.2 Ma期间长达近16 Ma的黄土-古土壤沉积发育过程中, 无论黄土还是古土壤地层中都保存有较丰富的蜗牛化石种类, 目前发现的15种蜗牛化石全部是陆生种类, 化石个体保存完整, 为原地埋藏的种群, 未发现水生的种类, 多数为第四纪黄土-古土壤序列中的常见种类, 可划分为冷干和温湿两个生态类群, 冷干类主要见于黄土地层中, 温湿类主要分布于古土壤地层中. 自中新世至第四纪期间, 蜗牛化石Metodontia(间齿螺)类和Cathaica(华蜗牛)类的属种具有明显的演化趋势, 新的种类的出现和演化与这一时期大的气候环境的改变在时代上有较好的一致性, 反映了蜗牛生态种类对全球/区域性环境格局变化的响应. 初步研究结果表明, 中新世黄土-古土壤序列与第四纪黄土-古土壤序列有着相似的沉积背景. 研究结果为秦安中新世黄土-古土壤序列沉积环境、气候演化等提供了生物化石证据. 相似文献
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深井盆地南缘断裂特征与活动性研究 总被引：1，自引：0，他引：1
深井盆地是山西断陷盆地带北段内部一个规模很小的次级盆地,为中更新世以来发育的三角型山间小型盆地。盆地附近断裂发育,构造复杂,深井盆地南缘断裂为主控边界断裂,控制着盆地的发展演化。本文通过对地形地貌、断裂剖面、地层测年及地震活动等方面的分析和研究,获得了断裂活动时代和活动速率等参数,综合阐述了断裂的空间展布及活动特征。研究表明:深井盆地南缘断裂晚第四纪期间仍在活动,最新活动时代为晚更新世晚期;断裂具有分段性,西段长约6km,多处可见断裂错断晚更新世地层剖面,属正断倾滑性质;东段表现为盆地与黄土斜坡直接接触,由西向东断裂地貌表现逐渐减弱,未见明显的断裂剖面,止于NW向构造,附近发生的4次4 3/4级地震与该段断裂关系密切。 相似文献
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秦王川盆地西缘断裂发育于陇中盆地地震构造区内部,本文对其进行了综合研究。浅层人工地震探测表明,该断裂在最小埋深130m处有显示,联合钻探结果表明该深度处为新近纪湖相沉积地层,泥岩层顶面向盆地方向呈斜坡状,槽探未揭露出断层。综合研究表明该断裂发育在新近纪地层内部,并未上穿第四纪沉积物,属于前第四纪隐伏断层。秦王川盆地在古近纪—新近纪山间泛湖盆的基础上,由于区域构造应力不均匀挤压抬升,形成山间负向地形,成为第四纪多变环境下河流堆积的拗陷盆地。秦王川盆地西缘断裂不具有控制中强地震空间分布的作用和形成地表破裂的能力,对盆地的构造稳定性不构成影响,亦不影响兰州新区的规划发展。 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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临汾盆地第四纪断层活动的几种表现 总被引：2，自引：0，他引：2
临汾盆地第四纪断层非常发育，按其走向可分为ＮＮＥ、ＮＥ、ＮＷ和ＥＷ向几组。本文指出第四纪期间，这些断层活动的表现形式为河流现代过程的变异，谷沟形态异常，或使晚新生代沉积相带迁移和晚更新世以来的地层错断等。 相似文献
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广东深圳断裂带活动性的第四纪地质和地貌研究 总被引：4，自引：0，他引：4
深圳断裂带分布着一系列第四纪盆地,发育了以晚更新世河流相为主的沉积物,其厚度一般小于10—15米。它们的出现与断裂破碎带、岩溶地层分布及断裂早期活动有关。但是,未见错动了第四纪沉积物的断层。从约180万年以来,断裂带内发育了四级夷平面和三级河流阶地。不同时期地壳相对升降平均速率估计为约0.04毫米/年至0.2毫米/年。 在第四纪地质时期,深圳断裂带总体处于区域性的间歇性抬升过程,断裂活动不明显 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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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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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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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 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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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 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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A special high-resolution routine of the EISCAT radar has been used to investigate the structure and development of the poleward wall of a deep trough in electron density. The feature was tracked by the radar during a 7-hour period under very quiet geomagnetic conditions. The field-aligned nature of the structure enabled an estimate to be made of the inclination of the geomagnetic field above EISCAT that was in good agreement with the current model. Observations of narrow field-aligned enhancements in electron temperature demonstrated that the wall of this trough is a dynamic feature, reforming regularly as the electron density responds on a time scale of tens of minutes to energy input from soft-particle precipitation. 相似文献