New Paleomagnetic Study on Early Triassic Liujiagou Formation of North China Block *     

Tian Wuhong Faculty of Earth Sciences  China University of Geosciences  Wuhan Niu Xiukai Hebei Bureau of Geology  Mineral Resources  Shijiazhuang 《中国地质大学学报(英文版)》1998,(3)

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阿拉善地块前中生代构造归属的新认识   总被引：4，自引：0，他引：4  

杨振宇  袁伟  仝亚博  刘静  王艳 《地球学报》2014,35(6):673-681

阿拉善地块的构造归属长期以来存在争议。我们对阿拉善地块东南部牛首山地区中—晚泥盆世砂岩的物源开展碎屑锆石U-Pb年代学与Hf同位素研究。碎屑锆石U-Pb年龄谱主要分布在5个区间:0.4—0.7 Ga,1.0—1.3 Ga,1.5—1.8 Ga,2.4—2.8 Ga和3.0 Ga,并获得一颗年龄为(4022±17)Ma的冥古宙锆石。2.4—2.7 Ga、3.0 Ga碎屑锆石和它们对应的εHf(t)值明显不同于华北板块同时代碎屑锆石,暗示着阿拉善地块与华北板块中—晚泥盆世并未相连。同时,我们还对地块东部的早石炭世、晚二叠世和早中三叠世地层开展了详细的古地磁研究,获得了相应的视极移曲线。我们结合碎屑锆石年代学和古地磁学研究,提出阿拉善地块前中生代与柴达木—塔里木地块具有亲缘性,而很可能与华北地块分离。印支运动使阿拉善地块相对于华北发生了32度的逆时针旋转,正是这一旋转运动使河西走廊—阿拉善地块最终与华北地块拼合形成了统一地块。  相似文献   

长江三角洲DY03孔磁性地层研究及其意义   总被引：5，自引：0，他引：5  

黄湘通  郑洪波  杨守业  Mark Dekker  谢昕  章振铨  方国庆 《海洋地质与第四纪地质》2008,28(6)

长江三角洲地区晚新生代以来接受了大量沉积，长时间序列沉积地层研究对于三角洲沉积环境演化和长江变迁历史都具有重要研究意义。通过对长江三角洲DY03孔古地磁、磁化率以及岩性分析，初步建立了研究钻孔较为可靠的年代地层框架。研究发现，长江三角洲地区沉积序列中有多个具有全球对比意义的短时期磁性漂移事件，对磁性地层定年的进一步应用具有重要意义。分析表明，研究区晚新生代地层中普遍发育的硬黏土层不仅是晚第四纪地层对比的重要标志层，而且对整个晚新生代以来的沉积地层对比都会发挥重要作用。长江三角洲沉积演化基本呈现出早期受构造活动控制，后期受海平面升降和气候变化的制约。  相似文献   

南极鲍威尔海盆D4-9柱样古地磁及磁组构特征          下载免费PDF全文

陈亮  张玉芬  张志强  刘强  杨文丰 《极地研究》2014,26(1):111-119

为了探讨中更新世以来南极半岛东北部鲍威尔海盆沉积环境气候演变及古流向特征,对采自南极半岛东北部鲍威尔海盆内一根3m长柱样进行了古地磁和磁组构参数测试和特征分析。结果表明：1）该柱样在2.73m处为布容正极性与松山反极性期的界线,由此推算出在距今780ka到现代该区域沉积速率较低,约为0.35cm/ka。2）中更新世以来该区域共出现过5次暖沉积事件,并且在暖期事件中存在3次明显的冷期气候波动事件。3）该区域在暖期古流向方向不明显,水流方向变化频繁,而在暖期之间的过渡时期,古流向以近似南北向为主。  相似文献   

Geochronology,paleomagnetism and magnetic fabric of metamorphic rocks in the northeast Fraser Belt,Western Australia     

B. De Waele  S. A. Pisarevsky 《Australian Journal of Earth Sciences》2013,60(5):605-621

The first zircon U–Pb SHRIMP dating on high-grade meta-igneous units in the northernmost parts of the Fraser Belt along the southern margin of the Western Australian Yilgarn Craton, reveal crystallisation ages between 1299 ± 10 and 1250 ± 23 Ma. A small number of older xenocrystic zircons, incorporated in some samples, indicate the presence of Late Paleoproterozoic crust in the region. Zircon that crystallised within a melt accumulated in the neck of a boudinaged mafic unit was dated at 1296 ± 4 Ma, indicating that the emplacement of the igneous protoliths took place syntectonically. The anisotropy of magnetic susceptibility of the granulites indicates minimum axes with a mean inclination of 4° towards 130°, corresponding to a nearly vertical southwest–northeast (50–230°) magnetic foliation. This is very close to the structural trend of the Fraser Belt suggesting that the magnetic fabric was acquired syntectonically, during the collision between the Yilgarn and Gawler Cratons. The paleomagnetic data on the granulites overlap with published poles for various 1.2 Ga units in the Albany Belt and the 1.2 Ga Fraser dykes, possibly suggesting that the remanence was acquired during the second stage of the Fraser tectonism. A younger magnetisation component resembles a pole of uncertain age published for Bremer Bay in the Albany Belt.  相似文献   

Paleomagnetic dating of ironstone nodules (‘nuts’) from the Yowah opal field,central southern Queensland     

P. W. Schmidt  B. L. Dickson 《Australian Journal of Earth Sciences》2017,64(6):743-752

To constrain the age of Australian opal formation, we have undertaken a paleomagnetic study of oxidised ironstone ‘nuts’ from Yowah, Queensland. Following standard methods, we have calculated a mean direction of declination D = 191.4°, inclination I = 61.7° (α₉₅ = 4.0°), indicating a paleomagnetic pole position at latitude λ_p = 71.3°S, longitude ?_p = 119.4°E (A₉₅ = 5.3°). The direction comprises both normal and reverse polarities that fail a reversal test most probably owing to contamination by small recent/present-day components. The mean direction should not be significantly affected. A chi-square comparison with paleomagnetic poles for dated Cenozoic rocks in eastern Australia, poles derived from the Global Moving Hotspot Reference Frame and the Cenozoic pole path for North America, appropriately transferred to Australian coordinates, yields a mean age estimate of 35 ± 7 Ma, i.e. late Eocene to early Oligocene. This is interpreted as the age of the ironstone formation, which places a maximum age for the formation of precious Yowah opal. This result confirms and tightens the age for the nearby Canaway weathered profile.  相似文献   

末次间冰期以来洛川黄土天然剩磁记录的可靠性     

韩朋  翟云峰  栗粲圪  张运  杨会会  靳春胜 《吉林大学学报(地球科学版)》2017,47(3)

地磁倒转和漂移不仅是研究地球动力学的重要手段之一,也能使地磁年代框架更加准确。通过对洛川黄土剖面L1、S1进行详细的岩石磁学、古地磁研究,结果表明:L1、S1中主要的载磁矿物是磁铁矿,但赤铁矿也可能携带稳定的特征剩磁;洛川黄土剖面能够记录Blake漂移,并发生于(123±2)ka。通过S1中1 092~1 240cm处6套平行样品的古地磁结果,表明洛川黄土难以记录Blake漂移的形态学特征;L1未记录到Mono Lake和Laschamp漂移,但是在175cm处识别出1次明显的地磁异常事件,年代约17.9ka。我们认为该地磁异常事件应为Hilina Pali/Tianchi漂移。此外,导致同一极性事件在不同地区记录产生差异的可能原因有中国黄土存在千年尺度的沉积间断、较低的沉积速率及黄土剖面所处地理位置的不同。同一剖面平行样品间地磁漂移形态学存在差异,可能是由于极性漂移期间较低的古地磁场强度抑制了黄土剩磁记录能力所致。  相似文献   

印支地块思茅地区始新统磁倾角偏低现象及其构造意义     

安纯志  杨振宇  仝亚博  李晨皓  王恒  高亮  韩志锐  徐颖超 《吉林大学学报(地球科学版)》2017,47(2)

对印支地块思茅地区始新世陆相红层进行古地磁研究,获得勐伴剖面特征剩磁方向为Ds=118.2°,Is=22.1°,k=31.6,α95=10.9°;勐腊剖面特征剩磁方向为Ds=47.6°,Is=22.8°,k=20.2,α95=5.9°。其特征剩磁方向与前人研究结果基本一致。利用Hodych等的磁倾角校正方法得到校正磁倾角为28.4°±4.3°,对前人的数据重新进行E/I统计得到的校正磁倾角值为30.7°,置信区间为[25.4°,35.9°],两种不同方法得到了较一致的结果,思茅地区的古近纪磁倾角显示了一定程度的偏低。E/I磁倾角偏低检验方法在应用时存在一定的局限性,变形微弱地层的古地磁学数据适合进行E/I磁倾角偏低校正,以避免倾伏褶皱或差异性旋转变形作用对E/I磁倾角偏低校正的影响。Hodych等提出的磁倾角校正方法是现今比较可靠的磁倾角校正方法。结合前人印支地块的古地磁研究成果,本次研究结果表明印支地块思茅地区自始新世以来相对于华南板块向南滑移量约500km。  相似文献   

青藏高原东南缘新生代地壳运动的转换   总被引：1，自引：0，他引：1  

裴军令  仝亚博  蒲宗文  景先庆  蔡瑜杭  李建锋 《地球学报》2019,40(1):106-116

在青藏高原东南缘保山地体东部上新世营盘组玄武岩中开展的古地磁学研究,获得了可靠的高温剩磁分量。地层校正后的特征剩磁分方向为Ds=166.5o, Is=–19.3o, k=41.9, a95=5.1o, N=22(采点)。褶皱检验显示其为原生特征剩磁分量。上新世古地磁数据显示,保山地体东部区域自上新世以来相对于东亚构造稳定区古地磁参考极发生了14.5o±4.8o的逆时针旋转运动。虽然保山地体东部上新世的逆时针旋转运动与保山地体其它区域古近纪至中新世的顺时针旋转变形截然相反,但是其与畹町走滑断裂和南汀河走滑断裂上新世以来的左旋走滑运动相吻合。本次研究通过保山地体和腾冲地体内部新生代古地磁数据及地体边界构造带活动演化的综合分析,指出自古近纪早期印度板块与欧亚大陆初始碰撞以来,青藏高原东南缘腾冲地块和保山地体在渐新世末期至早中新世时期,以及上新世早期分别发生了地壳运动方式的转换。保山地体地壳的运动学方式直接控制了地体边界走滑断裂的构造演化过程。  相似文献   

Paleomagnetism and Cyclostratigraphy of the Middle Ordovician Krivolutsky Suite,Krivaya Luka Section,Southern Siberian Platform: Record of Non-Synchronous NRM-Components or a Non-Axial Geomagnetic Field?     

Rodionov  V.P.  Dekkers  M.J.  Khramov  A.N.  Gurevich  E.L.  Krijgsman  W.  Duermeijer  C.E.  Heslop  D. 《Studia Geophysica et Geodaetica》2003,47(2):255-274

The Middle Ordovician Volginsky and Kirensky fossil zones were sampled in the Krivaya Luka section (Krivolutsky suite) that outcrops along the Lena river in Siberia. The Volginsky and Kirensky zones are coeval to the Llandeilo in the global geologic time scale. The Krivaya Luka section consists of siltstones, clays, sandstones, and limestones, and displays a remarkably distinct sedimentary cyclicity, especially in its reddish middle part.Stepwise thermal demagnetization yields three NRM components. Component A, isolated in the 100—250°C interval can be either normal or reversed. The normal A-component has a direction close to recent local magnetic field. The reversed A-component directions are scattered around a direction close to that of the lower Triassic Siberian traps. Component B has unblocking temperatures that range from 400 to 500°C and is represented mainly by normal polarity directions. The B-component, isolated from rocks of the middle part of the section is of a normal polarity with D = 176.5°, I = 30.0° and a North pole position at 16.2°S, 111.3°E. The other parts of the section are characterized by intermediate B-directions, which resulted possibly by partially overlapping A- and C-components. The highest temperature dual-polarity component C was isolated in the 550—670°C interval, resulting in the detection of two complete polarity zones and three magnetic reversals. The C-component is characterized by the following mean directions: for the reversed component D = 335.7°, I = 6.9°, and for the normal component D = 188.6°, I = 28.0°, which is very close to the normal polarity directions of the B-component. The corresponding paleomagnetic North pole for reversed polarity rocks is 32.6°S, 137°E, which is typical of Middle Ordovician rocks from Siberia – the mean pole for Llanvirn-Llandeilo is 30°S, 136°E (cf. Smethurst et al., 1998) – whereas for normal polarity rocks the pole position 17.2°S, 99.1°E is markedly different. Nevertheless, we assume that the C-component records the ancient geomagnetic field of Ordovician times, even though it does not pass the reversals test. This could be explained by overlapping NRM unblocking temperature spectra for the B and C components. In this case, the paleomagnetic pole positions should be interpreted with some caution.In addition, the section was logged and sampled in detail for cyclostratigraphic purposes. Spectral analysis in the depth domain using the high-field susceptibility as input parameter showed that the observed cyclicity is most likely orbitally forced. Detected spectral peaks (significant at the 95% confidence level) were close to the expected positions of the periodicities of precession, obliquity and eccentricity for the Ordovician. Consequently, the average sediment accumulation rate is estimated at 3.5 cm/kyr. Extrapolating this sedimentation rate yields a total duration of at least 1 Myr for the Volginsky fossil zone and 1.2 Myr for the entire Krivaya Luka section.  相似文献