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1.
青藏高原的隆升与扩展不仅导致欧亚大陆内部发生强烈的构造变形,亦对高原周缘的地貌格局及气候变化产生了重大影响.青藏高原东北缘新生代以来的隆升时代与响应过程一直备受争议,而界定青藏高原东北缘构造带隆升时序是解决争议的关键之一.本研究围绕青藏高原东北缘,在陇中盆地、六盘山褶皱逆冲带和鄂尔多斯地块西南缘地区进行了磷灰石和锆石裂变径迹测试分析和热史模拟.测试分析结果表明研究区样品的磷灰石裂变径迹年龄范围分布于136～16 Ma,裂变径迹的长度范围介于11.9～13.3μm;锆石裂变径迹年龄结果为258～79 Ma,但多数样品的年龄介于160～99 Ma;热史模拟结果揭示了研究区新生代以来至少经历了两期隆升和冷却降温事件,即始新世期间(55～30 Ma)和中中新世(17～12 Ma)以来.始新世期间(55～30 Ma)发生的隆升事件可能是印度大陆与欧亚大陆陆陆碰撞远程效应的直接响应,表明印度与欧亚大陆碰撞之初或不久,其应力即已传导至东北缘边界;中中新世(17～12 Ma)以来的隆升剥露冷却事件奠定了青藏高原东北缘现今构造格局. 相似文献
2.
日喀则弧前盆地的埋藏和剥蚀历史——来自低温热年代学的约束 总被引：1，自引：0，他引：1
日喀则弧前盆地紧邻印度板块与欧亚大陆碰撞带,研究其剥蚀历史对理解印度板块与欧亚大陆碰撞对造山带剥蚀的影响具有重要意义。文中利用磷灰石裂变径迹(AFT)及锆石和磷灰石的(U-Th)/He(ZHe和AHe)年龄数据,结合已发表的低温热年代数据探讨日喀则弧前盆地的热演化和剥露历史。日喀则弧前盆地磷灰石裂变径迹年龄存在明显的南北差异,南部磷灰石裂变径迹年龄为74～44Ma,对应的剥蚀速率为0. 03～0. 1km/Ma,剥蚀量≤2km;北部磷灰石裂变径迹年龄为27～15Ma,剥蚀速率为0. 09～0. 29km/Ma,但缺失早新生代的热演化历史。而磷灰石的(U-Th)/He年龄表明15Ma BP之后日喀则弧前盆地整体呈现一致的剥露历史。低温热年代数据表明日喀则弧前盆地南部自新生代以来尽管受到印度板块与欧亚大陆碰撞及后期断层活动的影响,海拔由海平面抬升至4. 2km,但一直保持缓慢的剥蚀,表明高原隆升并未直接促使该地区的岩石剥蚀速率加快,这与快速剥蚀即代表造山带开始隆升的假设不相符。此外,日喀则弧前盆地北部的低温热年代学研究表明晚渐新世—早中新世Kailas盆地仅发育于日喀则弧前盆地与冈底斯造山带之间的狭长地带,并在短期内经历了快速的埋藏和剥露。 相似文献
3.
本文通过背斜褶皱变形与低温热年代学年龄(磷灰石和锆石(U-Th)/He、磷灰石裂变径迹)端元模型研究,约束低起伏度、低斜率地貌特征的四川盆地南部地区新生代隆升剥露过程.四川盆地南部沐川和桑木场背斜地区新生代渐新世-中新世发生了相似的快速隆升剥露过程(速率为~0.1 mm/a、现今地表剥蚀厚度1.0~2.0 km),反映出盆地克拉通基底对区域均一性快速抬升冷却过程的控制作用.川南沐川地区磷灰石(U-Th)/He年龄值为~10-28.6 Ma, 样品年龄与古深度具有明显的线性关系,揭示新生代~10-30 Ma以速率为0.12±0.02 mm/a的稳态隆升剥露过程.桑木场背斜地区磷灰石裂变径迹年龄为~36-52 Ma,古深度空间上样品AFT年龄变化不明显(~50 Ma)、且具有相似的径迹长度(~12.0 μm).磷灰石裂变径迹热演化史模拟表明桑木场地区经历三个阶段热演化过程:埋深增温阶段(~80 Ma以前)、缓慢抬升冷却阶段(80-20 Ma)和快速隆升剥露阶段(~20 Ma-现今),新生代隆升剥露速率大致分别为~0.025 mm/a和~0.1 mm/a.新生代青藏高原大规模地壳物质东向运动与四川盆地克拉通基底挤压,受板缘边界主断裂带差异性构造特征控制造就了青藏高原东缘不同的边界地貌特征. 相似文献
4.
天山是中亚造山带重要组成部分,其中-新生代构造热演化及隆升剥露史研究是认识中亚造山带构造变形过程与机制的关键.本文应用磷灰石(U-Th)/He技术重建中天山南缘科克苏河地区中-新生代构造热演化及隆升剥蚀过程.磷灰石(U-Th)/He数据综合解释及热演化史模拟表明该地区至少存在晚白垩世、早中新世、晚中新世3期快速隆升剥蚀事件,起始时间分别为~90Ma、~13Ma及~5Ma,且这3期隆升剥蚀事件在整个天山地区具有广泛的可对比性.相对于磷灰石裂变径迹,磷灰石(U-Th)/He年龄记录了中天山南缘地质演化史中更新和更近的热信息,即中天山在晚中新世(~5 Ma)快速隆升剥蚀,其剥蚀速率为~0.47mm·a~(-1),剥蚀厚度为~2300m.总体上,中天山科克苏地区隆升剥蚀起始时间从天山造山带向昭苏盆地(由南向北)逐渐变老,表明了中天山南缘隆升剥蚀存在不均一性,并发生了多期揭顶剥蚀事件. 相似文献
5.
天山中新世早期快速剥露：磷灰石裂变径迹与（U-Th）／He低温热年代学证据 总被引：1，自引：0，他引：1
天山造山带新生代剥露过程与构造演化历史一直是国内外地学界关注的热点．本文联合运用磷灰石裂变径迹（AFT）和（u—Th）／He（AHe）低温热年代学技术,重建了新疆天山巴仑台剖面基岩山体的热演化历史,分析了剥露速率的变化特征,结合前人研究成果进一步探讨了新生代天山地区剥露作用过程的基本特点．结果表明,巴仑台剖面磷灰石样品的裂变径迹年龄集中在40～60Ma,（U—Th）／He年龄为10～40Ma;裂变径迹时间一温度史模拟结果表明巴仑台地区中新世早期以来剥露作用明显增速,剥露速率由之前的〈30mMa-1增大为〉1001TIMa-1;基于AFT与AHe年龄,利用年龄～封闭温度法以及矿物对法计算得到的剥露速率也表明该地区新生代剥露作用自中新世早期开始加速,并且在晚中新世剥露作用进一步增强．本文所揭示的快速剥露过程也存在于天山造山带其他地区．从整个天山造山带来看,开始于中新世早期的快速剥露是新生代天山地区一次重要的剥露作用过程． 相似文献
6.
运用裂变径迹分析方法,探讨分析了合肥盆地中新生代的构造热演化特征. 上白垩统和古近系下段样品的磷灰石裂变径迹（AFT）数据主体表现为靠近部分退火带顶部温度(±65℃)有轻度退火,由此估算晚白垩世至古近纪早期合肥盆地断陷阶段的古地温梯度接近38℃/km,高于盆地现今地温梯度(275℃/km).下白垩统、侏罗系及二叠系样品的AFT年龄(975～25Ma)和锆石裂变径迹(ZFT)年龄(118～104Ma)均明显小于其相应的地层年龄,AFT年龄－深度分布呈现冷却型曲线形态,且由古部分退火带、冷却带或前完全退火带及其深部的今部分退火带组成,指示早白垩世的一次构造热事件和其随后的抬升冷却过程. 基于AFT曲线的温度分带模式和流体包裹体测温数据的综合约束,推算合肥盆地早白垩世走滑压陷阶段的古地温梯度接近67℃/km. 径迹年龄分布、AFT曲线拐点年龄和区域抬升剥蚀时间的对比分析结果表明,合肥盆地在早白垩世构造热事件之后的104Ma以来总体处于抬升冷却过程,后期快速抬升冷却事件主要发生在±55Ma. 相似文献
7.
贺兰山隆升时限及其演化 总被引：3，自引：0，他引：3
贺兰山横亘于鄂尔多斯盆地西北缘,其隆升时限与盆地的构造属性和发展演化密切相关.对其隆起的时间前人有晚三叠世、晚侏罗世等多种认识.对贺兰山现存地层的分布和岩浆及热液活动等资料分析,认为晚三叠世-中侏罗世贺兰山并未隆升,其隆起时间应在中侏罗世之后.通过对与贺兰山相邻的银川地堑沉积地层及沉降速率的研究,指出贺兰山大规模隆升时间为始新世,在上新世以来发生了快速隆升.根据对不同时代样品磷灰石和锆石裂变径迹测试结果的分析,精细刻画了贺兰山的隆升-冷却过程,指出其隆升至少经历了晚侏罗世—早白垩世初、早白垩世中晚期、晚白垩世和始新世以来4个阶段.其中,晚白垩世和始新世以来的隆升最为明显.早白垩世中晚期为区域冷却过程.综合分析和总结各方面研究结果,认为贺兰山隆升的最早时间在晚侏罗世,此时隆升规模较为局限;晚白垩世的隆升与鄂尔多斯盆地整体的抬升相对应;始新世开始发生大规模的隆升,上新世隆升速率进一步加快. 相似文献
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9.
西藏甲马多金属矿区热历史的裂变径迹证据 总被引：7，自引：0，他引：7
用裂变径迹法测试了甲马矿区矽卡岩矿石和外围砂岩总计5个磷灰石和锆石样品, 其中磷灰石裂变径迹年龄为(16.1±0.9)和(18.8±1.1) Ma, 代表成矿热液后期活动的时代; 砂岩磷灰石裂变径迹年龄为(22.0±4.3) Ma, 锆石裂变径迹年龄为(20.9±2.0) Ma, 代表早期成矿时代; 另一个砂岩锆石年龄为(341.6±79.1) Ma, 与成矿作用关系不大, 是矿物源区特征的反映. 热历史分析表明, 成矿作用开始时间应早于25～22 Ma. 矿区平均冷却速率为5～6℃/Ma, 其中在90～80℃期间降温缓慢; 矿区剥蚀程度约为2.7 km, 剥蚀速率大于抬升速率. 相似文献
10.
本文通过峨眉山基底卷入构造带低温热年代学(磷灰石和锆石裂变径迹、锆石(U-Th)/He)研究,结合典型构造-热结构特征诠释峨眉山晚中-新生代冲断扩展变形与热年代学耦合性.峨眉山磷灰石裂变径迹(AFT)和锆石(U-Th)/He(ZHe)年龄值分别为4~30Ma和16~118Ma.ZHe年龄与海拔高程关系揭示出ZHe系统抬升剥蚀残存的部分滞留带(PRZ).低温热年代学年龄与峨眉山构造分带性具有明显相关性特征:万年寺逆断层上盘基底卷入构造带AFT年龄普遍小于10Ma,万年寺逆断层下盘扩展变形带AFT年龄普遍大于10 Ma;且空间上AFT年龄与断裂带具有明显相关性,它揭示出峨眉山扩展变形带中新世晚期以来断层冲断缩短构造活动.低温热年代学热史模拟揭示峨眉山构造带晚白垩世以来的多阶段性加速抬升剥蚀过程,基底卷入构造带岩石隆升幅度大约达到7~8km,渐新世以来抬升剥蚀速率达0.2~0.4mm·a-1,其新生代多阶段性构造隆升动力学与青藏高原多板块间碰撞过程及其始新世大规模物质东向扩展过程密切相关. 相似文献
11.
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.
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
13.
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
16.
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 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.
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
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