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1.
龙门山飞仙关断层传播褶皱磁组构特征及构造意义 总被引：3，自引：0，他引：3
沿龙门山南段冲断前锋带飞仙关断层传播褶铍剖面钻取了270个磁组构定向岩芯样品,对其进行了磁性矿物与磁组构分析。通过等温剩磁和三轴热退磁实验确定了样品中的主要载磁矿物为赤铁矿。磁组构测试结果显示27个采样点的磁组构为中间组构与构造组构两种类型。通过对各点磁组构特征及各项磁组构参数进行详细分析,再结合断层传播褶皱运动学模型,得出断层传播褶皱形成过程中岩石应变及磁组构演化：断层扩展前的平行层缩短作用把原始的沉积组构改造成为中问组构;在断层扩展过程中,两翼地层的旋转抬升产生的简单剪切作用对地层磁化率各向异性产生影响,使得校正的磁化率各向异性度Pj值局部升高,以及在剪切变形强烈的区域形成构造磁组构。 相似文献
2.
胭脂坝岩体是秦岭造山带内具典型代表性意义的晚三叠世花岗岩,已有的年代学和地球化学研究对该岩体的侵位机制有不同认识。对岩体的岩石磁学进行分析,结合其岩相学特征,探讨了用磁组构约束岩体内部组构这一方法的可靠性。研究表明,胭脂坝岩体样品的平均磁化率Km值和校正磁化率各向异性度PJ值总体较低,与顺磁性花岗岩类一致。磁滞回线分析表明,绝大部分样品的磁化率来自顺磁性矿物的贡献,少部分高磁化率样品含有铁磁性矿物的贡献,但其浓度极低。高磁化率值样品的等温剩磁曲线获得和反向退磁曲线及χ-T曲线分析表明,铁磁性矿物为磁铁矿,且为多畴颗粒。结合岩相学特征,认为胭脂坝岩体低场磁组构反映了顺磁性的云母类矿物的组构特征,磁组构特征真实地记录了样品的内部组构特征。 相似文献
3.
在胶东地区招远-平度断裂带上的大磨曲家金矿区选取了典型的构造区域进行岩石磁组构研究。沿着断裂带在不同构造部位的36个采样点钻取了112个定向岩心样品,所有样品均沿勘探线布置。磁组构研究显示,研究区以弱磁性岩石为主,总体上,胶东群变质岩的磁化率值较高,而玲珑黑云母花岗岩的磁化率值较低,尤以碎裂程度高的强蚀变岩的磁化率值最低;磁化率各向异性方位主要为NE向挤压,磁组构所指示的构造应力场与大磨曲家矿区的区域挤压应力方向是相同的;对具不同程度矿化的81线的Au含量与80线磁组构各向异性度(P值)进行对比研究发现,P值与金品位呈负相关关系;弱矿化糜棱岩中的金矿化在磁面理发育的岩石中较为发育,成矿晚期,Au元素含量随着岩石磁性的减弱而增加,特别是在强应变后弛豫阶段矿液充填于相对张性的石英脉中Au含量最高。 相似文献
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本文对藏东昌都地区侏罗纪汪布组、东大桥组和小索卡组红层共71个采点开展了磁组构(AMS)研究。磁组构测试结果表明,早侏罗世汪布组岩石磁线理较磁面理发育,磁化率各向异性度较高,磁化率椭球最小轴K3散布于层面缩短方向,代表了与构造成因相关的磁组构;中侏罗世东大桥组和晚侏罗世小索卡组岩石则磁面理较磁线理发育,磁化率各向异性度较低,磁化率椭球最小轴K3与层面近垂直,指示了原生沉积磁组构。早侏罗世汪布组地层的磁组构揭示了其构造应力场方向为NE-SW向。中侏罗世东大桥组的磁组构指示了其沉积时的古水流方向为SE向(138.3°),而晚侏罗世小索卡组磁组构指示了其沉积时的古水流方向为NNW向(328.3°)。古水流方向的明显变化揭示了昌都地区从中侏罗世到晚侏罗世沉积物物源发生了相应的转变,表明昌都地区南早北晚的隆升过程。 相似文献
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在应用传统的磁组构方法进行岩石构造变形分析时,发现这些方法中有许多不完善之处,如变形岩石磁化率量值椭球和应变椭球是否可以对应及对应条件,初始磁组构是否会影响变形碉石磁化率量值椭球与应变椭球的对应关系,岩石脆性破裂前的塑性变形是否影响磁组构,韧性变形如何影响磁组构,能否用磁组构来推断主应力方向,Ｒａｔｏｒｅ（１９８０）最小磁化率指向对韧性剪切带运动方向和方式的分析在多期变形区是否适用等,并据此提出解 相似文献
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通过藏南乌郁盆地渐新世地层磁组构和岩石磁学的系统研究,结合研究区地质构造环境,揭示了该套地层不同层位普遍具有反磁组构特征.代表性样品的岩石磁学数据表明,其主要携磁矿物为单畴磁铁矿和/或磁赤铁矿(反磁组构),并含有不可忽略的顺磁性以及超顺磁性颗粒.AMS-磁组构三角关系数据图解显示出部分样品的磁组构为正磁组构与反磁组构混... 相似文献
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航磁异常的构造解释和华北-塔南-扬子超陆块演化 总被引：11，自引：0，他引：11
在现代地球磁场中,总体感磁效应与岩石的磁化率无关。典型地区大比例尺构造组构填图结果与岩石磁组构的对照分析,证明磁线理和构造线理具有一致的矢量特征。强烈韧性剪切导致岩石中区域一致的矿物定向和磁化率各向异性,是干扰现代地球磁场、产生特定航磁异常分布格局的主要因素。对五种基本的区域尺度构造 航磁异常样式的成因进行了分析,证明华北地区的航磁异常的分布样式与结晶基底的基本构造格架基本一致。并据此对塔里木、扬子地体基底岩石的构造性质进行了解释,提出存在前寒武纪华北－ 塔南－ 扬子超陆块。结合显生宙构造演化的地质证据,划分出新太古代克拉通化、古元古代左行韧性剪切改造和活动带发育、中－ 新元古代裂解和活动大陆边缘、古生代原地改造和中生代再裂解五个演化历史阶段 相似文献
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通过与粉尘堆积,以及玄武岩和片麻杂岩风化剖面磁组构的对比,探讨了以贵州平坝白云岩之上红色粘土剖面磁组构特征及其成因指示意义。红色粘土的各向异性较弱,并且不具有明显的沉积磁组构;母岩的组构特征对红色粘土磁化率各向异性没有明显的控制“痕迹” ;红色粘土与粉尘堆积物之间磁组构特征的明显差异,表明它们在物源和形成机制方面是不同的;红色粘土磁化率及磁组构特征反映出红色粘土中磁性矿物的物质来源和成因具有一定的特殊性。 相似文献
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岩石组构记录了地壳形成与演化的关键信息,提取这些信息对分析和恢复地球动力学过程具有重要意义。磁化率各向异性(AMS)是一种重要的岩石组构方法,可以有效地揭示岩石的应变特征,分析其地球动力学过程,是研究构造变形性质以及应力作用方式的有效手段。本文在梳理AMS的研究历史、主要成果和最新进展的基础上,系统阐述了AMS的基本原理以及在剪切带的应用:①岩石组构具有复杂性,AMS作为一种间接组构手段受控于矿物的物理特性、含量以及变形变质等多方面因素;②AMS可以提供剪切带的运动学以及不同部位应变状态的信息;③对于剪切带,AMS主要受控于磁性矿物(矿物成分和粒度的变化导致全岩磁化率各向异性的变化)、构造变形强度(决定磁线理发展的重要因素)以及流体的作用(流体导致磁性矿物的类型与定向性的变化)。 相似文献
11.
《International Geology Review》2012,54(5):441-456
Granulite from 66 sites along the Além-Paraiba dextral shear zone were collected for magnetic analyses. The rocks were affected by the Braziliano orogeny, which was responsible for the present structural pattern. Magnetic fabrics were determined applying anisotropy of low—field magnetic susceptibility (AMS, all sites) and anisotropy of remanence magnetization (ARM, in 21 sites). The ferromagnetic minerals are magnetite, titanohematite, and in some samples, minor pyrrhotite. Hysteresis curves show that both para— and ferromagnetic minerals are the carriers of AMS. Thus AMS is due to the preferred crystallographic orientation of paramagnetic matrix minerals and titanohematite, to the shape anisotropy of magnetite grains, or to a combination of all three. ARM was performed imposing both anhysteretic remanence (AAR) and isothermal remanence (AIRM). The AMS, AAR, and AIRM fabrics are coaxial and are tectonic in origin. Their parallelism indicates that both ferromagnetic and paramagnetic minerals recorded the same metamorphic event. A passive—marker model is suggested for ferromagnetic minerals at the outcrop scale. The magnetic foliation is very close to the strike of the Além Paraíba shear zone, suggesting that this generated the local rock fabrics during the Braziliano orogeny. 相似文献
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Microstructural and magnetic investigations (anisotropy of magnetic susceptibility, AMS) on sections across basement–cover interfaces (BCI) revealed a complex evolution in the crystalline basement rocks beneath and in the basal units of the Caledonian fold-and-thrust belt: (1) Pre-Caledonian mylonitic fabrics in basement granite relate to steep shear zones. (2) Palaeoweathering formed smectite and illite at the expense of feldspar and mica. Secondary Fe-bearing clay minerals and the intensity of the chemical weathering control the bulk susceptibility. Changing susceptibility and AMS relate to a (time) sequence from primary magnetite to secondary paramagnetic clay to pyrite and ferrimagnetic pyrrhotite. (3) Burial compaction with BCI-parallel fabrics. (4) Caledonian cleavage, overprinted by décollement zones with S–C–C′ fabrics. Décollement cataclasis overprinted pre-existing magnetic fabrics and produced horizontal magnetic lineations and subhorizontal foliations defined by the S–C–C′ fabrics. Clay mineral enrichment, together with subsequent, BCI-parallel compaction fabrics, decreased the shear strength in the basement rocks beneath the BCI. Detachments initiated at such low-strength zones and produced allochthonous units with their footwall within crystalline basement rocks, an observation of general importance for orogenic fold-and-thrust belts. 相似文献
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Franti?ek Hrouda 《Journal of the Geological Society of India》2010,75(1):254-266
Measurement of Anisotropy of Magnetic Susceptibility (AMS) has become an important tool for Structural Geological analysis
in the past few decades. In the past, AMS data have been used for petrofabric analysis of deformed rocks as well as for gauging
strain. However, the AMS of some rocks can be carried by both ferromagnetic and paramagnetic minerals. Separating effects
of these mineral groups on the rock’s AMS is difficult because of expensive and commercially less available instrumentation.
On the other hand, instrumentation is available in most rock magnetic and palaeomagnetic laboratories for resolving bulk susceptibility
into ferromagnetic and paramagnetic components. Mathematical modelling was made of the relationship between bulk susceptibility
and AMS. If the contribution of the ferromagnetic or the paramagnetic fraction to the rock susceptibility is dominant (let
us say higher than 80%), the resultant AMS is relatively near to the AMS of the dominating fraction in all aspects, the degree
of AMS, shape parameter and orientation of principal susceptibilities. In the interpretation of the AMS of rocks with dominating
one fraction, the resolution of the AMS into paramagnetic and ferromagnetic components is not necessary, the resolution of
bulk susceptibility into components is sufficient that can be made using the instrumentation available in most rock magnetic
and palaeomagnetic laboratories. 相似文献
14.
南京下蜀土的岩石磁学特征 总被引：5，自引：0，他引：5
对南京附近的下蜀土进行了岩石磁学测定，通过磁化率各向异性测量研究了它的沉积磁性组构特征，下蜀土的各异向性很不明显，各向异性废Ｐ小于水成岩的Ｐ值（＞１．０２），且与困面理度Ｆ高度相关，与磁线理度Ｌ相关不明显，这种特征与中国中部风成黄土极相似。对新生圩剖面进行的磁化率测量发现用化率曲线上有７个旋回的波峰、波谷变化，这与剖面中的古土壤－黄土系列相一致，说明下蜀土的剖面磁化率同样可以作为地层划分与对比，反映古气候冷暧变化的物理参数。对典型下蜀土样品进行的低温磁化率测量揭示出古土壤和黄土的成颗粒的构成不同，古土壤以超顺磁质为主，黄土以顺磁质为主。细小磁颗粒在古土壤中的积聚可能与古土壤的发育及古气候的暧湿程度有关。 相似文献
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岩石压磁效应是构造应力作用的产物,根据压磁与应力二者转换计量公式和压磁矢量特性,探求压磁效应与成矿元素预富集-富集的对应关系:①压磁系数和磁化率的变化强度与断裂规模和矿床大小相对应,磁化强度大的岩石有利于金元素的富集,抗磁性矿种和铁磁性矿种分别集中与磁斥力和磁引力有内在联系;②粘滞剩磁和剩磁矫顽力是压磁不可逆性的两个重要参数,对成矿阶段所出现的抗磁性与顺磁性矿物交替规律、岩体转动使磁铁矿和黄铜矿二者对顶分布、基性程度高比重大的矽卡岩矿物呈反向分带序列的存在等都具有一定的相关关系;③含金量高的黄铁矿和方铅矿等硫化物矿石条带常平行于石英脉分布,是受压磁的大小、方向和应力三者作用的共同控制;④压磁效应和岩石粒化有利于成矿元素的富集;⑤压磁引起的电磁波效应有利于对围岩矿质的萃取和深部铁磁性元素的富集。基于压磁三重特性(与应力转换性、大小和方向性)和元素磁性四大类(铁磁性、反铁磁性、顺磁性和抗磁性)的划分,可建立构造应力-磁化强度(感磁 剩磁,压磁属剩磁的一种)-矿质聚集三者间量化关系。 相似文献
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We resolve the anisotropy of magnetic susceptibility (AMS) axes along fault planes, cores and damage zones in rocks that crop out next to the Dead Sea Transform (DST) plate boundary. We measured 261 samples of mainly diamagnetic dolostones that were collected from 15 stations. To test the possible effect of the iron content on the AMS we analyzed the Fe concentrations of the samples in different rock phases. Dolostones with mean magnetic susceptibility value lower than −4 × 10−6 SI and iron content less than ∼1000 ppm are suitable for diamagnetic AMS-based strain analysis. The dolostones along fault planes display AMS fabrics that significantly deviate from the primary “sedimentary fabric”. The characteristics of these fabrics include well-grouped, sub-horizontal, minimum principal AMS axes (k3) and sub-vertical magnetic foliations commonly defined by maximum and intermediate principal AMS axes (k1 and k2 axes, respectively). These fabrics are distinctive along fault planes located tens of kilometers apart, with strikes ranging between NNW-SSE and NNE-SSW and different senses of motion. The obtained magnetic foliations (k1–k2) are sub-parallel (within ∼20°) to the fault planes. Based on rock magnetic and geochemical analyses, we interpret the AMS fabrics as the product of both shape and crystallographic anisotropy of the dolostones. Preferred shape alignment evolves due to mechanical rotation of subordinate particles and rock fragments at the fault core. Preferred crystallographic orientation results from elevated frictional heating (>300 °C) during faulting, which enhances c-axes alignment in the cement-supported dolomite breccia due to crystal-plastic processes. The penetrative deformation within fault zones resulted from the local, fault-related strain field and does not reflect the regional strain field. The analyzed AMS fabrics together with fault-plane kinematics provide valuable information on faulting characteristics in the uppermost crust. 相似文献
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Foreland basin growth strata are ideal recorders of deformation rates and kinematics in tectonically active regions. This study develops a high-resolution chronostratigraphic age model to determine folding rates in the Eocene-Oligocene terrestrial growth strata of the Berga Conglomerate Group, NE Spain. The Berga Conglomerate Group was sampled for rock magnetic, magnetostratigraphic, and magnetic susceptibility (χ) cyclostratigraphy analyses. Analysis of rock magnetic measurements indicate a mixed mineral assemblage with both paramagnetic and ferromagnetic minerals. A new magnetic reversal stratigraphy constrains the time frame of folding and is in agreement with previous interpretations. Time series analysis of χ variations show statistically significant power at expected orbital frequencies and provides precession-scale (20 kyr) temporal resolution. Strain measurements including anisotropy of magnetic susceptibility (AMS) fabrics and bedding plane strain worm burrow distortion are consistent with fixed hinge, flexural folding kinematics. Fault-related folding was modeled using χ cyclostratigraphy timing and strain measurement kinematic constraints. The onset of folding was at 33.85 Ma and the end of deformation is less constrained but is younger than 31.06 Ma. Deformation and sediment accumulation rates are unsteady at 20 kyr time scales but appear artificially steady at polarity chron time scales. 相似文献