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第四纪时期地壳块体相对运动的古地磁记录的初步研究—以陇西和鄂… 总被引：3，自引：0，他引：3
为了探讨用古地磁方法确定第四纪时期地壳块体相对运动状况，选择了分别处于陇西块体和鄂尔多斯块体内的兰州九州台和陕西洛川两个黄土剖面作为实验对象，在这两个黄土剖面的４个相同年代的层位采集定向大样，作黄土沉积剩余磁化矢量测量，并用虚磁极法拟合，初步结果表明，约１１０万ａ来陇西块体相对于鄂尔多斯块体作顺时针旋转，其转动量达９．０±４．７°。 相似文献
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扬子地块显生宙古地磁视极移曲线及地块运动特征 总被引：16，自引：1，他引：15
在重新审视已有古地磁研究结果基础上,利用近年来最新研究成果,尤其是早古生代的古地磁数据,建立了扬子地块显生宙古地磁视极移曲线,为研究扬子地块乃至整个中国的大地构造演化提供了新的古地磁依据. 相似文献
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塔里木地块库车坳陷早日垩世古地磁结果及磁倾角偏低的成因探讨 总被引：1，自引：0，他引：1
运用主成分分离及线性区段等方法，使早白垩世样品明显分离出二线磁组分。叠加剩磁为喜山期重磁化，特征乘磁明显偏离现代地磁场方向，经倾斜校正后，有很好的一致性并通过了倒转换检验，给出塔里木地块库车坳陷早白垩世巴西盖组古地磁亲数据。综合已有的古地磁结果，获得了塔里木地块早白垩世平均剩磁方向及平均古地磁极，阐明了塔里木地块早白垩世磁倾角偏低这一现象，分析导致磁倾角偏低的诸多因素，认为压实作用可能是导致磁倾角偏低的重要因素之一。 相似文献
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古地磁多磁成分的分离技术 总被引：1，自引：4，他引：1
在古地磁的研究中，如何从复杂多样的退磁数据中获取能够代表岩石形成时期的古地磁场方向的原生剩磁组分，是关系到古地磁数据是否可靠、古地磁结果是否令人信服的根本环节之一，因此，如何充分利用实验室退磁数据所提供的各种信息去获取同源磁化的一组样品的原生剩磁方向是一个很有研究价值的问题。在总结前人的各种定性或定量的多磁成分分离技术的基础上，详细讨论了重磁化大圆的极和线性坳陷区内退磁平面的极的最佳拟合大圆的最小二乘拟合法，提出了综合使用主成分分析法、线性谱分析法、重磁化圆法以及退磁平面及重磁化大圆的二次拟合法，对来自同源磁化的一组样品进行系统分析，以获取一组样品的特征剩磁方向的方法，并应用于实际研究工作中。 相似文献
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印度与亚洲大陆碰撞形成了喜马拉雅造山带.该造山带是当今固体地球科学研究的重点和热点,是建立新的大陆动力学理论的最佳天然实验室.印度与亚洲大陆碰撞时限是正确认识和理解该造山带形成与演化、高原隆升的动力学过程等的起点.近南北向陆陆碰撞的最直接证据是碰撞带两侧块体在古纬度上的相互重叠.本文拟通过对相关古地磁资料的分析,结合近年来在拉萨地块南缘林子宗群火山岩和沉积岩夹层上获得的最新古地磁结果,探索当今古地磁数据所限定的印度和亚洲大陆发生初始碰撞的时间和古地理位置.结果表明,拉萨地块林子宗群形成时期(约64~44 Ma)古亚洲大陆最南缘的古地理位置(~10°N)限定了印度与亚洲大陆的初始碰撞最可能发生在65~50 Ma之间;如果以由印度洋海底地形所限定的东冈瓦纳大陆裂解前的印度板块形状为大印度模型,则印度与亚洲大陆的初始碰撞很可能发生在60~55 Ma之间. 相似文献
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塔里木地块新生代古地磁结果及显生宙视极移曲线 总被引：12，自引：3，他引：9
发表了塔里木盆地新生代古地磁新结果,并综合前人工作成果编制了塔里木地块显生宙古地磁视极移曲线,探讨了塔里木地块各个地质时期运动规律. 相似文献
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泥盆纪时期各板块的古地理重建缺乏可靠古地磁数据,以至于古特提斯洋在泥盆纪的演化过程存在争议,而高质量的古地磁数据定量限定板块的古纬度位置是解决上述问题的关键.本文对北羌塘地块早泥盆世平沙沟组灰岩进行了古地磁学研究,提供了一个较为可靠的古地磁数据.镜下观察及岩石磁学实验结果表明平沙沟组灰岩样品中的主要载磁矿物为磁铁矿和赤铁矿,并且没有重磁化的特征.系统热退磁与混合退磁实验结果表明,样品的天然剩磁强度较低,从54块样品中获得了较为集中的特征剩磁分量,在样品水平下的平均方向为Dg=358.5°,Ig=22.8°,kg=17.7,α95=4.6°,Ds=8.8°,Is=-0.9°,ks=18.1,α95=4.5°,通过了C级倒转检验,对应的古地磁极为λp=54.8°N,φp=251.2°E,(dp/dm=2.3°/4.5°),这一极位置与石炭纪以来可靠的古地磁极位置存在差异,很... 相似文献
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华北地块显生宙古地磁视极移曲线与地块运动 总被引：27，自引：4，他引：23
在较详细地补充报道了华北地块早古生代研究成果基础上,根据国内外一些公认的古地磁数据可靠性标准,以及岩石地层是否受后期的构造改造(如旋转作用)和热作用(如重磁化)等标准,对这些新老数据作了较为严格筛选,选出一批可靠性较高、易于被国内外同行普遍接受的数据.编制了一条华北地块显生宙古地磁视极移曲线,并讨论了华北地块显生宙的运动特征. 相似文献
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利用几个典型全球板块相对运动模型的欧拉矢量,计算沿这些模型板块边界段的两两板块之间的相对运动速度,据此进一步计算一定时间尺度内这些板块边界段的面积变化. 并依据已有对相应各边界段性质-包括张性、压性及走滑性质的研究,设定组成各边界段的两个板块如何分别承担其面积变化的情况,得到各模型中每个板块的面积变化和全球表面积变化总量. 结果显示,在近100万年时间尺度内,地球南半球表面积增大、北半球表面积减小,地球总表面积变化为2.9万～3.6万km~2. 如果假设地球表面积的增量完全由体积膨胀引起,这将对应地球半径160～250 m的增加. 以NUVEL-1模型为例,全球14个板块中,非洲、 南美与南极三个板块的面积持续增大,其余11个板块的面积在逐步减小;不过,非洲、南美与南极这三个板块面积增大部分之和,能够完全抵消掉其余11板块面积之减小,而且使全球总体表面积增加. 本文进一步讨论了一些其他因素,例如俯冲带前进与后退等影响地球表面积变化的情况. 相似文献
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The authors give a computer fit of Corsica and Sardinia. The rotation angles are 40° and 59°. A comparison with paleomagnetic results is made. 相似文献
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Pacific plate equatorial sediment facies provide estimates of the northward motion of the Pacific plate that are independent of paleomagnetic data and hotspot tracks. Analyses of equatorial sediment facies consistently indicate less northward motion than analyses of the dated volcanic edifices of the Hawaiian-Emperor chain. The discrepancy is largest 60–70 Ma B.P.; the 60- to 70-Ma equatorial sediment facies data agree with recent paleomagnetic results from deep-sea drilling on Suiko seamount [1] and from a northern Pacific piston core [2]. Equatorial sediment facies data and paleomagnetic data, combined with K-Ar age dates along the Emperor chain [3], indicate a position of the spin axis at 65 Ma B.P. of 82°N, 205°E in the reference frame in which the Pacific Ocean hotspots are fixed. This pole agrees well with the position of the spin axis in the reference frame in which the Atlantic Ocean hotspots and the Indian Ocean hotspots are fixed [4,5], supporting the joint hypotheses that (1) the Pacific Ocean hotspots are fixed with respect to the hotspots in other oceans, (2) the hotspots have shifted coherently with respect to the spin axis, and (3) the time average of the earth's magnetic field 65 Ma B.P. was an axial geocentric dipole. Global Neogene paleomagnetic data suggest that a shift of the mantle relative to the spin axis has been occurring during the Neogene in the same direction as the shift between 65 Ma B.P. and the present. All data are consistent with a model in which the hotspots (and by inference the mantle) have shifted with respect to the spin axis about a fixed Euler pole at a constant rate of rotation for the last 65 Ma. 相似文献
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V. A. Bol’shakov 《Izvestiya Physics of the Solid Earth》2008,44(7):593-602
A new correlation scheme is proposed for the Belovo and Volodarka loess-soil sections on the basis of the author’s paleomagnetic studies. It is shown that the paleomagnetic stratigraphy and correlation of sections of the Loess Plateau, China, are not self-consistent. The paper gives recommendations for correct use of the paleomagnetic method in the study of loess sections. 相似文献
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A. V. Khokhlov 《Izvestiya Physics of the Solid Earth》2014,50(4):562-567
Understanding the character of variations in the magnetic field of the Earth in the geological past requires a mathematically substantiated method for testing the statistical hypotheses against the real paleomagnetic data. As known, the paleomagnetic data from lava flows are sort of momentary snapshots of the state of the ancient magnetic field. Being quite fragmentary in time and space, these data compose what is referred to as a sample in statistics: on the close discrimination of the lava flows, the internal correlations in the data are absent. It is well known that the distributions of the paleomagnetic directions from the sedimentary data differ from the distributions in lavas, which is mainly due to the effect of averaging of the magnetization over the time interval corresponding to the accumulation of sedimentary layers represented in the rock specimen. Assuming the rate of sedimentation to be known for each specimen, one can suggest the method for the quantitative testing the statistical consistency of the paleomagnetic data in the sediments with the model variations of the magnetic field of the Earth in terms of the Giant Gaussian Process (GGP). It turned out that the averaging effect can well be allowed for by the coefficients of GGP, and the scheme of the further testing is in this case identical to the scheme of testing the paleomagnetic data obtained from lavas. 相似文献
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A. M. Fetisova R. V. Veselovskiy Yu. P. Balabanov N. V. Sal’naya 《Izvestiya Physics of the Solid Earth》2017,53(5):635-644
One of the key challenges which are traditionally encountered in studying the paleomagnetism of terrigenous sedimentary strata is the necessity to allow for the effect of shallowing of paleomagnetic inclinations which takes place under the compaction of the sediment at the early stages of diagenesis and most clearly manifests itself in the case of midlatitude sedimentation. Traditionally, estimating the coefficient of inclination flattening (f) implies routine re-deposition experiments and studying their magnetic anisotropy (Kodama, 2012), which is not possible in every standard paleomagnetic laboratory. The Elongation–Inclination (E–I) statistical method for estimating the coefficient of inclination shallowing, which was recently suggested in (Tauxe and Kent, 2004), does not require the investigation of the rock material in a specially equipped laboratory but toughens the requirements on the paleomagnetic data and, primarily, regarding the volume of the data, which significantly restricts the possibilities of the post factum estimation and correction for inclination shallowing. In this work, we present the results of the paleomagnetic reinvestigation of the Puchezh and Zhukov ravine (ravine) reference sections of the Upper Permian and Lower Triassic rocks in the Middle Volga region. The obtained paleomagnetic data allowed us to estimate the coefficient of inclination shallowing f by the E–I method: for both sections, it is f = 0.9. This method was also used by us for the paleomagnetic data that were previously obtained for the Permian–Triassic rocks of the Monastyrskii ravine (Monastirskoje) section (Gialanella et al., 1997), where the inclination shallowing coefficient was estimated at f = 0.6. 相似文献
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运用主成分分离及线性区段等方法 ,使早白垩世样品明显分离出二组磁组分 .叠加剩磁为喜山期重磁化 ,特征剩磁明显偏离现代地磁场方向 ,经倾斜校正后 ,有很好的一致性并通过了倒转检验 ,给出塔里木地块库车坳陷早白垩世巴西盖组古地磁新数据 .综合已有的古地磁结果 ,获得了塔里木地块早白垩世平均剩磁方向及平均古地磁极 ,阐明了塔里木地块早白垩世磁倾角明显偏低这一现象 .分析导致磁倾角偏低的诸多因素 ,认为压实作用可能是导致磁倾角偏低的重要因素之一 . 相似文献
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基于岩石剩余磁化强度的矢量特性,使用古地磁学方法对钻孔岩心进行重新定向,对于解译地下构造、分析应力特征、判定成矿方向等问题具有重要意义.针对华南地区复杂构造下的倾斜钻孔岩心,本文构建了古地磁学岩心定向新方法理论,结合多次坐标转换和磁场一致性扫描,实现了基于黏滞剩磁的岩心重定向;设计了定向所需的成套古地磁学岩心定向、测量、取样装置,并将该方法和装置应用于华南铀矿钻孔的重定向,恢复后的岩心特征剩磁计算获得的早白垩世古地磁极位置与同期华南地块的极位置一致.该方法对地球物理深部探矿技术的改进有一定意义.此外,所设计的研究装置在古地磁学研究对象的拓展中也具有应用前景. 相似文献
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Detailed paleomagnetic data from the Wairoa Syncline, a middle Miocene to the present forearc basin on the East Coast of the North Island, New Zealand, show that the rate of clockwise rotation for the last 5 Ma has been 7–8°/Ma of which less than 1.5°/Ma can be explained by apparent polar wander due to motion of the Australian or Pacific plates. This rotation is similar to a present-day rate of 7°/Ma determined from geodetic data. Between 5 and 20 Ma ago the rate of tectonic rotation is poorly determined and may be between 0° and 2°/Ma.
The change in the rate of rotation of the Wairoa Syncline around 5 Ma is probably related to a markedly different tectonic style in the New Zealand region within the last 5 Ma, associated with a change in position of the Euler poles of rotation for the Pacific-Australian plates. 相似文献