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1.
《地球物理学进展》2016,(5)
黄土高原风尘沉积序列厚度大、地层连续,是高分辨率古地磁研究和古气候研究的理想材料.然而,缺少精确年龄控制点制约了黄土古气候信息的区域对比和海陆对比研究.地磁极性漂移是地球磁场长期变化过程中的基本行为之一,全球同步性使其成为古气候研究可靠的年龄控制点.布容正极性时记录了多次极性漂移事件,为高分辨率黄土古气候学提供的新的途径.通过回顾近年来的研究成果可知,黄土沉积物广泛记录了Laschamp和Blake地磁极性漂移事件,且部分剖面中存在Mono Lake事件的报道.此外尚未明确限定的倾角变负波动不断提出,极大地拓展了黄土沉积物极性漂移事件研究的深度和广度.然而,部分高沉积速率黄土剖面存在极性事件缺失现象对黄土沉积物可以稳定记录地磁极性漂移事件提出了质疑.目前对这一现象的解释有剩磁获得机制、Lock-in效应、沉积间断和气候响应等.然而,热退磁可有效去除化学剩磁(CRM)的影响,与CRM密切相关的剩磁获得机制无法解释相近区域内极性事件记录的差异.黄土沉积物较浅的Lock-in效应否定了其会普遍引起极性事件记录的缺失.黄土高原内部低沉积速率(小于10 cm/Ka)地区千年尺度极性事件和地磁场长期变化的记录否定了黄土沉积存在千年尺度的沉积间断.本文通过分析已有研究成果,认为极性漂移期间地磁场稳定性较差,导致磁性颗粒记录的磁场信息存在差异,可能是极性事件记录缺失的主要原因. 相似文献
2.
在岩石地层分析和测年实验分析的基础上,综合运用地球物理测井、浅层反射地震和古地磁测年等多种地球物理方法划分河北平原厚覆盖区第四纪地层.通过对QHJ01孔的岩芯观察,按照沉积物岩性、颜色、沉积组合和沉积环境分析将揭露的松散沉积物分为8大岩性段.根据QHJ01孔古地磁样品磁倾角变化划分古地磁极性带,0～82.8 m为布容正极性时,82.8～235.8 m为松山反极性时,235.8 m以下为高斯正极性时.综合运用古地磁、浅层地震、地球物理测井方法和岩石地层分析判断第四系和中更新统底界分别为235.8 m和82.8 m,运用地球物理测井结合C14、光释光测年实验和岩石地层分析判断上更新统和全新统底界分别为53.3 m和24.9 m. 相似文献
3.
对黄土高原定边、西峰、渭南三个剖面中古土壤层S1的定向连续古地磁样品作了详细的岩石磁学和古地磁学研究，均未发现Blake极性事件．在对其成因进行了分析研究后，提出如下看法：（1）六盘山以东黄土高原北部边缘的风成沉积可能存在局部的不连续性，因而没有记录Blake极性事件；（2）黄土沉积物的主要载磁矿物力磁铁矿，次生磁性矿物对剩磁的贡献可能大于原生磁铁矿，故在六盘山以东黄土高原北部边缘没有发现Blake极性事件；（3）六盘山以东黄土高原中部和南部地区，强烈的成土作用掩盖了持续时间较短的Blake极性事件；（4）六盘山以西的黄土高原具高速稳定沉积的特点，且成土作用弱，可记录Blake极性事件． 相似文献
4.
地磁极性倒转是地球磁场的重要特征之一.研究极性转换过程中地球磁场的时空分布规律是认识地磁倒转机制的重要途径.国际上利用湖相和海相沉积物以及火山岩体对转换场形态学作了大量的研究工作,但由于湖相沉积物的剩余磁性受生物扰动和化学变化影响大,所得结果可靠性较低;深海沉积物则 相似文献
5.
极性转换期间地球磁场形态学研究 总被引：3，自引：1，他引：2
本文对采自中国黄土高原西峰（35.7°N,107.6°E）和段家坡（34.2°N,109.2°E）两个剖面中黄土层L8和古土壤层S8的1281块定向古地磁样品做了详细的岩石磁学和古地磁学研究.证实了Matuyama-Brunhes（M-B）极性转换带位于L8的中下部.提出了下列观点:1.M-B极性转换过程与地球磁场方向变化相联系的持续时间为3600-4500a,而与地球磁场强度变化相联系的持续时间则为8000-9000a,即强度变化存在“超前和滞后” 效应;2.M-B转换场的形态是由三次快速倒转和一次不成功的倒转构成,或者说,转换场具有快速变换极性的振荡特征;3.M-B转换过程中地球磁场并不是以轴对称的非偶极子场为主,而是偶极子场至少与非偶极子场相当;4.中国黄土-古土壤沉积物所含磁性矿物的主要成分是磁铁矿,它是研究极性转换期间地球磁场详细结构的良好物质. 相似文献
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7.
根据无限稀释溶液中物质的分子扩散系数,估算沉积物中污染物的扩散系数时,需确定地层因数与孔隙度的关系.本研究将Miller Soil Box应用于测定青岛近岸不同粒径砂质沉积物与孔隙水的电阻率,以确定沉积物的地层因数,并结合沉积物的孔隙度,通过曲线拟合建立地层因数与孔隙度的关系式.研究结果表明,运用Ullman和Aller给出的经验m值(当φ≤0.7时,m取2)计算近岸砂质沉积物中污染物的分子扩散系数,将会引起40%~50%的误差;近岸砂质沉积物地层因数与孔隙度的关系可以采用Archie公式表示,即F=φ-m,m=1.52;经验证分析,可取m=1.52代入Ds=D0.φm-1公式,计算浅水砂质沉积物中污染物的分子扩散系数. 相似文献
8.
沉积物金属元素变化的粒度效应--以太湖沉积岩芯为例 总被引：12，自引：3，他引：9
水体沉积物中金属元素含量变化除了与人为污染有关之外,在很大程度上受沉积物粒度、矿物组成等沉积物性质的影响．在进行沉积物金属元素研究中,要充分考虑沉积物金属元素含量变化的粒度效应．本文通过对太湖MS岩芯中17种金属元素、沉积物粒度、矿物组成等指标的分析,研究了金属元素变化特征以及与沉积物粒度组成的关系．MS岩芯金属元素变化可分为两类,第一类主要为Al、Fe、K等,该类元素在沉积岩芯中下部含量较高,岩芯上部含量较低;第二类为Na元素,在沉积岩芯中下部含量较低,岩芯上部含量升高．MS岩芯中金属元素与粘土含量之间具有显著相关关系,经沉积物粒度(粘土含量)校正后,沉积岩芯中金属元素含量趋于稳定．因此,沉积物粒度组成(粘土含量)是影响金属元素含量的主要因素,在研究太湖沉积物金属元素变化规律及进行金属污染评价时,应对金属元素含量进行粒度校正． 相似文献
9.
湖泊底泥疏浚环境效应:Ⅳ.对沉积物微生物活性与群落功能多样性的影响及其意义 总被引：5，自引：1，他引：4
通过为期一年的疏浚模拟试验,在试验室培养疏浚与对照柱样研究了底泥疏浚对沉积物微生物活性和群落功能多样性的影响。研究结果表明,太湖梅梁湾研究区模拟疏浚表层30cm对沉积物物理、化学和微生物性质影响较大。疏浚沉积物微生物活性显著低于未疏浚沉积物的微生物活性,疏浚对沉积物微生物活性影响较大且在一年的试验周期内难以恢复。底泥疏浚对沉积物微生物功能多样性产生影响,疏浚后初期新生表层沉积物的微生物群落多样性指数显著低于未疏浚沉积物,底泥疏浚改变了沉积物中微生物群落组成,并会导致微生物群落功能多样性降低。底泥疏浚对微生物活性与微生物群落功能多样性产生影响,从而对沉积物中生源要素的循环产生影响。 相似文献
10.
长江中下游湖泊沉积物中磷的形态及藻类可利用量 总被引：13，自引：1，他引：13
调研了长江中下游地区25个浅水湖泊的35个样点表层沉积物中磷的地球化学形态特征,以及太湖沉积物中藻类可利用磷(AAP)的空间分布,垂向分布特征及其蓄积量,探讨了浅水湖泊表层沉积物中磷的赋存量,地球化学形态及其与水草,湖水磷浓度,叶绿素(Chl-a)浓度之间的关系.结果表明,长江中下游地区浅水湖泊的表层沉积物中可交换态磷(Ex-P)含量与水体总磷(TP),溶解性总磷(DTP)及溶解性反应活性磷(SRP)浓度关系密切,有水草湖区的沉积物中生物易利用磷(Bio-P)含量显著低于无水草湖区及藻型湖区.太湖梅梁湾沉积物泥芯中,表层3 cm沉积物中Ex-P含量显著增高,而夏季还原条件下容易转变为溶解态磷的铁磷(Fe-P)含量峰值则出现在4～10cm深度.太湖表层沉积物的Bio-P含量与夏季叶绿素浓度密切相关,说明表层沉积物的Bio-P及AAP可以作为沉积物内源释放风险的指示参数.太湖表层1 cm底泥中所含有的AAP量估计多达268.6吨,风浪扰动能将大量的AAP带入水体,对太湖蓝藻水华暴发起着不可忽视的作用. 相似文献
11.
TianShui Yang Masayuki Hyodo ZhenYu Yang ShiHong Zhang Toshiaki Mishima HuaiChun Wu HaiYan Li Yi Li XingAn Shi Kan Wang YiMing Ma 《中国科学:地球科学(英文版)》2014,57(8):1929-1943
Paleomagnetic records of the Gauss-Matuyama reversal were obtained from two loess sections at Baoji on the Chinese Loess Plateau. Stepwise thermal demagnetization shows two obvious magnetization components. A low-temperature component isolated between 100 and 200–250°C is close to the present geomagnetic field direction, and a high-temperature component isolated above 200–250°C reveals clearly normal, reversed, and transitional polarities. Magnetostratigraphic results of both sections indicated that the Gauss-Matuyama reversal consists of a high-frequency polarity fluctuation zone, but the characteristic remanent magnetization directions during the reversal are clearly inconsistent. Rock magnetic experiments demonstrated that for all the specimens with normal, reversed, and transitional polarities magnetite and hematite are the main magnetic carriers. Anisotropy of magnetic susceptibility indicates that the studied loess sediments have a primary sedimentary fabric. Based on virtual geomagnetic pole latitudes, the Gauss-Matuyama reversal records in the two sections are accompanied by 14 short-lived geomagnetic episodes (15 rapid polarity swings) and 12 short-lived geomagnetic episodes (13 rapid polarity swings), respectively. Our new records, together with previous ones from lacustrine, marine, and aeolian deposits, suggest that high-frequency polarity swings coexist with the Gauss-Matuyama reversal, and that the Gauss-Matuyama reversal may have taken more than 11 kyr to complete. However, we need more detailed analyses of sections across polarity swings during reversals as well as more high-resolution reversal records to understand geomagnetic behavior and inconsistent characteristic remanent magnetization directions during polarity reversals. 相似文献
12.
Models of geomagnetic reversals as a stochastic or gamma renewal process have generally been tested for the Heirtzler et al. [1] magnetic polarity time scale which has subsequently been superseded. Examination of newer time scales shows that the mean reversal frequency is dominated in the Cenozoic and Late Cretaceous by a linearly increasing trend on which a rhythmic fluctuation is superposed. Subdivision into two periods of stationary behavior is no longer warranted. The distribution of polarity intervals is visibly not Poissonian but lacks short intervals. The LaBrecque et al. [2] polarity time scale shows the positions of 57 small-wavelength marine magnetic anomalies which may represent short polarity chrons. After adding these short events the distribution of all polarity intervals in the age range 0–40 Myr is stationary and does not differ significantly from a Poisson distribution. A strong asymmetry develops in which normal polarity chrons are Poisson distributed but reversed polarity chrons are gamma distributed with indexk = 2. This asymmetry is of opposite sense to previous suggestions and results from the unequal distribution of the short polarity chrons which are predominantly of positive polarity and concentrated in the Late Cenozoic. If short-wavelength anomalies arise from polarity chrons, the geomagnetic field may be more stable in one polarity than the other. Alternative explanations of the origin of short-wavelength marine magnetic anomalies cast doubt on the inclusion of them as polarity chrons, however. The observed behavior of reversal frequency suggests that core processes governing geomagnetic reversals possess a long-term memory. 相似文献
13.
It has been indicated that the Rao-Cramer inequality can be used to estimate the resolvability of intervals with opposite geomagnetic field polarity based on marine anomalies and for measurement planning. Specifically, it has been elucidated that the width of a detected interval of one polarity is determined more exactly than its center. 相似文献
14.
In order to assist in global correlation of the Pliocene/Pleistocene boundary, a paleomagnetic survey has been made of the world type section for the boundary, in Calabria, Italy. A total of 116 specimens from 36 sites were collected from the section, which as sampled is about 30 m thick. All sites possess stable remanent magnetism and northern hemisphere virtual geomagnetic poles, consistent with deposition during a period of normal polarity. If this period was during the Gilsa event, a minimum sedimentation rate of 17 cm per 1000 years would be required. Since a normal polarity chemical overprint, acquired during the last 0.69 m.y. could also explain the data, thermomagnetic analyses were made of selected samples. The results show the presence of highly unstable superparamagnetic material, which is most likely a product of post-depositional chemical precipitation. This observation enhances the possibility that any longer-duration precipitation could have created coarse and thus magnetically more stable components, the effects of which could not be readily distinguished from the original remanent magnetism.The difficulties of distinguishing between original depositional remanent magnetism and post-depositional chemical remanent magnetism, in outcropping marine sediments, as well as the large range of possible natural causes of the latter, is summarized in the form of a discussion of feasible Eh and pH changes occurring between original deposition at upper bathyal dephts and final sampling above sea level. It is considered that, in the absence of experimental means to distinguish the roles of original and chemically overprinted paleomagnetic signals, similarity of magnetic polarity stratigraphy between sections of sediments representing different paleoenvironments and sedimentation rates is a necessary if insufficient requirement for diagnosis of real geomagnetic behavior during deposition, as opposed to posidepositional effects. 相似文献
15.
Reversals and excursions of Earth's geomagnetic field create marker horizons that are readily detected in sedimentary and volcanic rocks worldwide. An accurate and precise chronology of these geomagnetic field instabilities is fundamental to understanding several aspects of Quaternary climate, dynamo processes, and surface processes. For example, stratigraphic correlation between marine sediment and polar ice records of climate change across the cryospheres benefits from a highly resolved record of reversals and excursions. The temporal patterns of dynamo behavior may reflect physical interactions between the molten outer core and the solid inner core or lowermost mantle. These interactions may control reversal frequency and shape the weak magnetic fields that arise during successive dynamo instabilities. Moreover, weakening of the axial dipole during reversals and excursions enhances the production of cosmogenic isotopes that are used in sediment and ice core stratigraphy and surface exposure dating. The Geomagnetic Instability Time Scale (GITS) is based on the direct dating of transitional polarity states in lava flows using the 40Ar/39Ar method, in parallel with astrochronologic age models of marine sediments in which oxygen isotope and magnetic records have been obtained. A review of data from Quaternary lava flows and sediments gives rise to a GITS that comprises 10 polarity reversals and 27 excursions that occurred during the past 2.6 million years. Nine of the ten reversals bounding chrons and subchrons are associated with 40Ar/39Ar ages of transitionally-magnetized lava flows. The tenth, the Gauss-Matuyama chron boundary, is tightly bracketed by 40Ar/39Ar dated ash deposits. Of the 27 well-documented geomagnetic field instabilities manifest as short-lived excursions, 14 occurred during the Matuyama chron and 13 during the Brunhes chron. Nineteen excursions have been dated directly using the 40Ar/39Ar method on transitionally-magnetized volcanic rocks and these form the backbone of the GITS. Excursions are clearly not the rare phenomena once thought. Rather, during the Quaternary period, they occur nearly three times as often as full polarity reversals. 相似文献
16.
The application of the magnetostratigraphy for dating of clastic and chemogenic cave sediments has been limited by the complex conditions underground and the lack of age constraints on these deposits for correlation with geomagnetic polarity timescale (GPTS). Without age constraints any correlation of obtained results cannot be explicit. Additionally, the dynamic character of cave infilling, exhumation and fossilisation expressed by unconformities within preserved sedimentary profiles can hide a substantial part of the geological time. The detailed internal division of deposits (breaks in deposition and related processes) and scarcity of fossils make the correlation of obtained magnetostratigraphic log with geomagnetic polarity timescales sometimes problematic. The analytical results confirmed that the complete step/field procedure offered by demagnetisation methods must be applied. The application of complete analysis only to pilot samples and shortened, selected field/step approach, to other samples did not offer sufficient data set for reliable interpretation. 相似文献
17.
地球磁场多次发生南北(正负)磁极位置的变换和白垩纪超静磁带(CNS)的异常现象,这已为大家所公认.但造成这种异常现象的原因,则是迄今未能很好解答的一个难题. 应用非线性理论对地球磁极倒转和白垩纪超静磁带进行了分析, 认为超静磁带事件意味着地球核幔相互作用和外核流体运动可能处于能量最低的状态，地球磁场系统通过不断地与外界交换物质和能量，维持一种空间或时间的有序结构.在121～83Ma期间,无外星撞击地球引起地磁极性倒转,可能是白垩纪超静磁带出现的原因之一.地球磁场极性的随机倒转具有混沌运动的自逆转特性,混沌理论给地磁极性倒转提出了一个简明的动力机制解释. 相似文献
18.
Richard Weaver Andrew P. Roberts Andrew J. Barker 《Earth and Planetary Science Letters》2002,200(3-4):371-386
Paleomagnetic, rock magnetic, and sedimentary micro-textural data from an early Miocene mudstone sequence exposed in Okhta River, Sakhalin, Russia, indicate the presence of pyrrhotite and magnetite at different stratigraphic levels. Sites that contain only magnetite have a reversed polarity characteristic remanent magnetization (ChRM) with a low-coercivity overprint, which coincides with the present-day geomagnetic field direction. Pyrrhotite-bearing sites have stable normal polarity ChRMs that are significantly different from the present-day field direction. After correction for bedding tilt, the ChRM data fail a reversals test. However, the normal polarity pyrrhotite ChRM directions become antipodal to the tilt-corrected magnetite ChRM directions and are consistent with the expected geocentric axial dipole field direction at the site latitude after 40% partial unfolding. These data suggest that the pyrrhotite magnetization was acquired during folding and after lock-in of the magnetite remanences. Electron microscope observations of polished sections indicate that fluid-associated halos surround iron sulphide nodules. Pyrrhotite is present in randomly oriented laths in and around the nodules, and the nodules do not appear to have been deformed by sediment compaction. This observation is consistent with a late diagenetic origin of pyrrhotite. Documentation of a late diagenetic magnetization in pyrrhotite-bearing sediments here, and in recent studies of greigite-bearing sediments, suggests that care should be taken to preclude a late origin of magnetic iron sulphides before using such sediments for geomagnetic studies where it is usually crucial to establish a syn-depositional magnetization. 相似文献
19.
地球磁场相对强度研究现状与展望 总被引：2，自引：6，他引：2
对利用沉积物确定地球磁场相对强度的实验方法进行了综述评述，在些基础上本文总结了目前常用的恢复沉复沉积物记录古强度的方法，重点介绍了全新世、晚更新世和布容时地球磁场相对强度变化特征，评价了环境因素对沉积物记录地球磁场相对强度的影响。对未来有关地球磁场相对强度研究发展趋势提出了借鉴。 相似文献
20.
A paleomagnetic record of the geomagnetic field during its change of polarity from the reversed Matuyama epoch to the normal Brunhes epoch has been obtained from sediments of ancient Lake Tecopa in southeastern California. The polarity switch occurs in siltstone of uniform composition, and anhysteretic magnetization experiments indicate that the magnetic mineralogy does not change markedly across the transition. Within the transition interval, intensity of the magnetization drops to a minimum of 10% of the intensity after the transition. The interval of low field intensity preceded and lasted longer than the interval during which the field direction reversed, the latter being shorter than the interval of low intensity by a factor of at least 2.5. The VGP's make a smooth transit from reversed to normal polarity, with the path lying in the sector of longitude between 30°E and 60°W. Pole paths for the Brunhes-Matuyama transition recorded in California and Japan are completely different, indicating that the dipole field decayed. The transition field appears to be nondipolar, and there is no evidence for an equatorial component. Since there is little dispersion of the VGP's about a great circle path, it is possible that large-scale drift of the nondipole field ceased during this polarity transition. 相似文献