共查询到19条相似文献，搜索用时 140 毫秒
1.
岩石磁组构在构造混杂岩带和韧性剪切带研究中的应用——以西天山地区为例 总被引：5，自引：2，他引：3
本文以西天山地区为例,讨论了岩石磁组构在构造混杂岩带和韧性剪切带中的作用和功能．指出岩石磁组构的某些参数能反映混杂岩带的变形类型,磁化率椭球体三个轴的方位在混杂岩基质中分布有规律,而在岩块中没有规律．在韧性剪切带中,磁组构的各向异性度Ｐ值绝大部分大于１．１,并有变化．磁面理的产化变化可用来求出韧性剪切带的位移量和变形路径．磁组构的Ｌ—Ｆ参数图可确定韧性剪切带的类型,最小主磁化率的方位可用来确定韧性剪切带的剪切指向． 相似文献
2.
岩石磁组构在构造混杂岩带和韧性剪切带研究中的应用：以西天山？… 总被引：4，自引：0，他引：4
本文以西天山地区为例,讨论了岩石磁组构造混杂岩带和韧性剪切中的作用和功能。指出岩石磁组构的某些参数能反映混杂岩带的变形类型,磁化率椭球体三个轴的方位在混杂岩基质中分布有规律,而在岩块中没有规律。在韧性剪切带中,磁组构的各向异性度Ｐ值绝大部分大于１．１,并有变化。磁面理的产化变化可用来求出韧性剪切带的位移量和变形路径。磁组构的Ｌ－Ｆ参数图可确定韧性剪切带的类型,最小主磁化率的方位可用来确定韧性剪切带 相似文献
3.
磁组构（上） 总被引：4，自引：0，他引：4
许同春 《地震地磁观测与研究》1989,10(3):70-77
地球科学领域岩石磁组构的研宄,对许多人来讲,还是一个陌生的课题。磁组构测量的是用磁化率量值椭球描述的岩石磁化率各向异性。由于它保留了成岩环境、动力变质的信息,可用于环境科学和应变分析。这期我们刊登科普文章《磁组构》,叙述这项技术的理论依据、测量及数据统计分析方法;介绍几项新成果,包括中国黄土、金伯利岩管及阜平县双重褶皱磁组构的研究,旨在向大家展示这一新的课题在地震地质、地球科学领域研究的可观前景。 相似文献
4.
石鼓尖岩体位于大别山核部天堂寨地区,为片麻理化石英二长岩.岩体磁组构分析显示,磁面理主体倾向SE,倾角较大,85%采样点的倾角介于40°~90°之间,与岩体的片麻理产状一致.岩体磁线理在东南部走向为NWW-SEE向,在岩体中部和北部,磁线理走向皆为NE-SW向.在岩体中部,磁线理向SW倾伏,北部磁线理向NE倾伏,磁线理倾角中等.磁化率各向异性度P值介于1.065~1.532之间;形态参数T介于0.005~0.694之间;弗林图解(F-L图解)显示K值均小于1,磁组构分析表明岩体是在SE-NW向挤压应力环境下侵位.石英C轴组构分析表明,岩体受到SE-NW向挤压应力,变形温度在400~500℃之间.显微构造显示岩石具有接近固态的变形组构特征,属同构造岩体变形组构.结合岩体磁组构、显微构造和石英C轴组构,指示石鼓尖岩体侵位冷凝成岩与区域NE向构造为同期,属同构造侵入岩体.石鼓尖岩体U-Pb定年结果表明,岩体锆石U-Pb年龄为(141±2.3)Ma,代表岩体侵位结晶年龄.综合分析认为,石鼓尖岩体侵位冷凝成岩时大别造山带仍然处于挤压环境,造山带由挤压向伸展转换的时间应该在141 Ma之后,岩体侵位时大别造山带的构造演化已受控于滨太平洋构造域.而邻近的天堂寨等巨大岩基则是伸展环境的产物. 相似文献
5.
四川盆地西南部西侧为龙门山冲断带,南面紧挨川西南褶皱带,其新生代构造变形特征对于认识青藏高原东南缘的变形机制具有一定的指示意义.磁组构是一种灵敏的应变指示计,在变形微弱的沉积岩地区尤为适用.本文在雅安-乐山剖面选取12个采样点进行磁组构分析,结合已有的天全-雅安飞仙关剖面的27个采样点数据,综合讨论川西南地区的构造变形特征.所有采样点的磁组构测试结果显示出3种弱变形的磁组构类型:沉积磁组构、初始变形磁组构和铅笔状磁组构.雅安-乐山剖面采样点的磁线理绝大部分为北东-南西走向,和龙门山南段的整体延伸方向一致,表明四川盆地西南缘新生代构造变形主要受控于龙门山的构造作用.飞仙关剖面的磁组构测试结果显示44%的采样点表现出磁线理和地层走向斜交的特征,由初始变形磁组构演变而来,并且所有异常磁组构仅局限在断层上盘,本文认为这是雅安地区新生代期间局部逆时针旋转引起变形叠加的结果. 相似文献
6.
一般认为磁组构能有效地反映岩石所经历的应变特征.为了研究不同类型的磁组构和不同期次应变之间的关系,对来自华南地块两个地区的早三叠世灰岩样品进行了岩石磁学、磁组构以及应变特征的对比分析.来自湖北通山县的样品经历了三期构造变形,这为解析磁组构和多期次应变提供了理想的机会.岩石磁学结果显示携磁矿物主要为磁铁矿.磁化率各向异性（AMS）和非磁滞剩磁各向异性（AAR）结果显示其最小轴与层面垂直,最大轴和中间轴分布于层面内,反映了沉积和压实作用产生的应变,而后期构造应变在磁组构中没有体现.来自广东连县的样品发育有渗透性压溶缝面理和方解石脉,说明经历了构造应变.AMS结果没有显示占优势的组构方向.AAR结果显示三轴组构,其最大轴分布于最大应力方位,与构造应变特征吻合,最初的压实组构被构造应变组构所代替.上述结果表明：（1）AAR可以很好地反映渗透性应变的特征,而AMS有时会失效;（2）应变的尺度要小于样品的尺度,磁组构才能有效地反映应变. 相似文献
7.
8.
近年来,针对秦岭造山带晚三叠世花岗岩体侵位机制的巨大争议,一些研究采用磁组构方法分析了岩体的内部组构特征及其与区域构造的关系,提出了具有重要意义的新认识.然而,目前这些研究均缺乏对岩体磁组构本质意义的分析,利用该方法约束岩体内部组构的可靠性并不十分清晰.针对这一问题,本文以秦岭造山带内具典型代表性意义的晚三叠世糜署岭花岗岩体为例,开展了该岩体的磁组构、岩石磁学、矿物形态组构和显微构造的综合研究.结果表明,糜署岭岩体的磁化率总体较低,属钛铁矿系列花岗岩.绝大部分样品的磁化率受控于顺磁性的黑云母等铁镁硅酸盐矿物,部分高磁化率样品包含了少量多畴磁铁矿等铁磁性组分的贡献,且随磁化率增大,铁磁性组分的贡献更为明显.样品的磁组构也主要是黑云母组构或由黑云母与磁铁矿的亚组构复合而成.由于样品中磁铁矿含量较低且与黑云母密切共生,磁组构与黑云母形态组构基本一致,因此,黑云母与磁铁矿的亚组构基本共轴.糜署岭岩体的磁组构本质上等同于黑云母组构,反映了黑云母等页硅酸盐矿物在岩体中的分布,可以有效的指示岩体的内部构造特征.宏观和显微构造观察还显示,糜署岭岩体的内部组构形成于岩浆侵位的晚期阶段,叠加了同岩浆期区域构造的关键信息,是从岩体构造角度开展区域构造演化的良好载体. 相似文献
9.
《地球物理学进展》2015,(6)
含铁建造型金矿和构造蚀变岩型金矿是坦桑尼亚国主要的金矿类型,含铁建造型金矿与条带状含铁建造(BIF)密切相关,而构造蚀变岩型金矿则与热液构造活动有一定的联系,条带状含铁建造(磁铁石英岩)和辉绿岩二者具有强磁性,不仅都能够在地表引起很强的ΔT负磁异常,而且其异常形态有很大的相似性,均呈线性串珠状展布;为分辨识别隐伏异常源,圈定与各自有关联的找矿靶区、间接发现这两种类型的金矿床,归纳总结了从五个方面对隐伏的条带状含铁建造和辉绿岩所引起的磁异常特征进行识别:(1)岩石半出露特征,(2)区域地层(或构造)分布特征,(3)磁异常强度的高低,(4)2.5维反演计算,(5)磁异常的排列关系;对磁异常特征进行解译判别,有效地指导了在隐伏绿岩带内圈定找矿靶区、进而间接发现与各自有关联的含铁建造型金矿和构造蚀变岩型金矿的作用. 相似文献
10.
盆地内细粒沉积物的磁组构特征可以记录盆地发育演化的关键构造信息.然而,反转盆地内细粒沉积物的磁组构有何特征,其与盆地发育和反转变形有何关系,目前仍需要深入探索.针对这一问题,本文以东、西秦岭分界处的白垩纪徽成盆地为例,在野外构造观察的基础上,对该盆地内的细粒沉积岩,特别是同沉积断层附近的细粒沉积岩(包括生长地层),开展了系统的岩石磁学、常温和低温磁组构研究.野外观察表明,徽成盆地白垩纪地层内发育了大量NNE走向的正断层,邻近断层的局部区域可见露头尺度的生长地层.盆地内细粒沉积物的磁化率值总体较低,岩石磁学实验表明,磁化率主要由顺磁性矿物控制,但也含有少量磁铁矿和赤铁矿等铁磁性矿物的贡献.常温和低温磁组构特征都表明,徽成盆地白垩纪地层内透入性的发育了NWW-SEE向的磁线理,与主要的(同沉积)正断层垂直或高角度相交,并显示出初始变形组构的特征,记录了盆地发育时以NWW-SEE向拉张为主的古应力信息.这一伸展应力场与控制徽成盆地发育的文县—太白断裂带呈锐夹角,表明断裂带在盆地发育时以左行走滑伸展为主.此外,与常温磁组构相比,低温磁组构显著提高了顺磁性组构的信号强度,突显了磁组构的优势方位,可以更为有效的反映岩石组构和应变信息.尽管徽成盆地白垩纪地层经历多期次构造变形,但其初始变形组构并未明显改造,为解析盆地构造属性提供了重要信息. 相似文献
11.
Flood basalts, such as the Deccan Traps of India, represent huge, typically fissure-fed volcanic provinces. We discuss the
structural attributes and emplacement mechanics of a large, linear, tholeiitic dyke swarm exposed in the Nandurbar–Dhule area
of the Deccan province. The swarm contains 210 dykes of dolerite and basalt >1 km in length, exposed over an area of 14,500 km2. The dykes intrude an exclusively basaltic lava pile, largely composed of highly weathered and zeolitized compound pahoehoe
flows. The dykes range in length from <1 km to 79 km, and in thickness from 3 to 62 m. Almost all dykes are vertical, with
the others nearly so. They show a strong preferred orientation, with a mean strike of N88°. Because they are not emplaced
along faults or fractures, they indicate the regional minimum horizontal compressive stress (σ
3) to have been aligned ~N–S during swarm emplacement. The dykes have a negative power law length distribution but an irregular
thickness distribution; the latter is uncommon among the other dyke swarms described worldwide. Dyke length is not correlated
with dyke width. Using the aspect ratios (length/thickness) of several dykes, we calculate magmatic overpressures required
for dyke emplacement, and depths to source magma chambers that are consistent with results of previous petrological and gravity
modelling. The anomalously high source depths calculated for a few dykes may be an artifact of underestimated aspect ratios
due to incomplete along-strike exposure. However, thermal erosion is a mechanism that can also explain this. Whereas several
of the Nandurbar–Dhule dykes may be vertically injected dykes from shallow magma chambers, others, particularly the long ones,
must have been formed by lateral injection from such chambers. The larger dykes could well have fed substantial (≥1,000 km3) and quickly emplaced (a few years) flood basalt lava flows. This work highlights some interesting and significant similarities,
and contrasts, between the Nandurbar–Dhule dyke swarm and regional tholeiitic dyke swarms in Iceland, Sudan, and elsewhere.
Editorial responsibility: J. White 相似文献
12.
《Earth and Planetary Science Letters》2006,241(3-4):978-992
The effects of dyke intrusion on the magnetic properties of host sedimentary rocks are still poorly understood. Therefore, we have evaluated bulk magnetic parameters of standard palaeomagnetic samples collected along several sections across the sediments hosting the Foum Zguid dyke in southern Morocco. The study has been completed with the evaluation of the magnetic fabric after laboratory application of sequential heating experiments.The present study shows that: (1) close to Foum Zguid dykes, the variations of the bulk magnetic parameters and of the magnetic fabric is strongly related with re-crystallization and Fe-metasomatism intensity. (2) The thermal experiments on AMS of samples collected farther from the dyke and, thus, less affected by heating during dyke emplacement, indicate that 300–400 °C is the minimum experimental temperature necessary to trigger appreciable transformations of the pre-existing magnetic fabrics. For temperatures higher than ca. 580 °C, the magnetic fabric transformations are fully realized, with complete transposition of the initial fabric to a fabric similar to that of samples collected close to the dyke. Therefore, measured variations of the magnetic fabric can be used to evaluate re-crystallization temperatures experienced by the host sedimentary rock during dyke emplacement. The distinct magnetic behaviour observed along the cross-sections strongly suggests that samples collected farther from the dyke margins did not experience thermal episodes with temperatures higher than 300 °C after dyke emplacement. (3) AMS data shows a gradual variation of the magnetic fabric with distance from the dyke margin, from sub-horizontal K3 away from the dyke to vertical K3 close to the dyke. Experimental heating shows that heat alone can be responsible for this strong variation. Therefore, such orientation changes should not be unequivocally interpreted as the result of a stress field (resulting from the emplacement of the dyke, for instance). (4) Magnetic studies prove to be a very sensitive tool to assess rock magnetic transformations, thermally and chemically induced by dyke intrusion in hosting sediments. 相似文献
13.
Magma flow revealed by magnetic fabric in the Okavango giant dyke swarm, Karoo igneous province, northern Botswana 总被引：1，自引：0，他引：1
C. Aubourg G. Tshoso B. Le Gall H. Bertrand J.-J. Tiercelin A.B. Kampunzu J. Dyment M. Modisi 《Journal of Volcanology and Geothermal Research》2008,170(3-4):247-261
To determine the magma flow direction of the giant, 179 Ma Okavango dyke swarm of northern Botswana, we measured the anisotropy of magnetic susceptibility (AMS) of 23 dykes. Dykes are located in two sections (Shashe and Thune Rivers), which are about 300 km and 400 km from the presumed magma source respectively; the Nuanetsi triple point. We collected samples from the margins of the dykes in order to use the imbrication of magnetic foliation to determine magma flow direction. About half of the magnetic fabric in the dykes is inverse, i.e. with the magnetic foliation perpendicular to the dyke plane. Lateral flow to the west and vertical flow is in evidence in the Shashe section. However, the overall analysis of normal and inverse magnetic fabric data supports that lateral flow to the west was dominant in the Shashe section. Across the Thune section, a poorly defined imbricated magnetic foliation also suggests lateral flow to the west. 相似文献
14.
Consideration of published anisotropy of magnetic susceptibility (AMS) studies on welded ignimbrites suggests that AMS fabrics are controlled by groundmass microlites distributed within the existing tuff fabric, the sum result of directional fabrics imposed by primary flow lineation, welding, and (if relevant) rheomorphism. AMS is a more sensitive indicator of fabric elements within welded tuffs than conventional methods, and usually yields primary flow azimuth estimates. Detailed study of a single densely welded tuff sample demonstrates that the overall AMS fabric is insensitive to the relative abundances of fiamme, matrix and lithics within individual drilled cores. AMS determinations on a welded-tuff dyke occurring in a choked vent in the Trans-Pecos Texas volcanic field reveals a consistent fabric with a prolate element imbricated with respect to one wall of the dyke, while total magnetic susceptibility and density exhibit axially symmetric variations across the dyke width. The dyke is interpreted to have formed as a result of agglutination of the erupting mixture on a portion of the conduit wall as it failed and slid into the conduit, followed by residual squeezing between the failed block and in situ wallrock. Irrespective of the precise mechanism, widespread occurrence of both welded-tuff dykes and point-welded, aggregate pumices in pyroclastic deposits may imply that lining of conduit walls by agglutionation during explosive volcanic eruptions is a common process. 相似文献
15.
G. Wadge 《Bulletin of Volcanology》1986,48(6):349-372
The orientations of dykes from many of the islands of the Lesser Antilles island arc have been mapped. Most of these dykes can be interpreted in terms of local or regional swarms derived from specific volcanoes of known age, with distinct preferred orientations. Dykes are known from all Cenozoic epochs except the Palaeocene, but are most common in Pliocene, Miocene and Oligocene rocks. A majority of the sampled dykes are basaltic, intrude volcaniclastic host rocks and show a preference for widths of 1–1.25 m. Locally, dyke swarms dilate their hosts by up to 9% over hundreds of metres and up to 2% over distances of kilometres. The azimuths of dykes of all ages show a general NE-SW preferred orientation with a second NW-SE mode particularly in the Miocene rocks of Martinique. The regional setting for these minor intrusions is a volcanic front above a subduction zone composed of three segments: Saba-Montserrat, Guadeloupe-Martinique, St. Lucia-Grenada. The spacing of volcanic centres along this front is interpreted in terms of rising plumes of basaltic magma spaced about 30 km apart. This magma is normally intercepted at crustal depths by dioritic plutons and andesitic/dacitic magma generated there. Plumes which intersect transverse fracture systems or which migrate along the front can avoid these crustal traps. Throughout its history the volcanic front as a whole has migrated, episodically, towards the backarc at an average velocity of about 1 km/Ma. The local direction of plate convergence is negatively correlated with the local preferred orientation of dykes. The dominant NE-SW azimuth mode corresponds closely to the direction of faulting in the sedimentary cover of the backarc and the inferred tectonic fabric of the oceanic crust on which the arc is founded. A generalised model of the regional stress field that controls dyke intrusion outside of the immediate vicinity of central volcanic vents is proposed, in which the maximum horizontal stress parallels the volcanic front except in the northern segment where subduction of the Barracuda Rise perturbs the stress field. There is also evidence of specific temporal changes in the stress field that are probably due to large scale plate kinematics. 相似文献
16.
《Earth and Planetary Science Letters》2006,241(1-2):307-322
Continental flood basalts consist of vast quantities of lava, sills and giant dyke swarms that are associated with continental break-up. The commonly radiating geometry of dyke swarms in these provinces is generally interpreted as the result of the stress regime that affected the lithosphere during the initial stage of continental break-up or as the result of plume impact. On the other hand, structures in the basement may also control dyke orientations, though such control has not previously been documented. In order to test the role of pre-dyke structures, we investigated four major putative Karoo-aged dyke swarms that taken together represent a giant radiating dyke swarm (the so-called “triple-junction”) ascribed to the Jurassic Karoo continental flood basalt (> 3 × 106 km2; southern Africa). One of the best tests to discriminate between neoformed and inherited dyke orientation is to detect Precambrian dykes in the Jurassic swarms. Accordingly, we efficiently distinguished between Jurassic and Precambrian dykes using abbreviated low resolution, 40Ar/39Ar incremental heating schedules.Save-Limpopo dyke swarm samples (n = 19) yield either apparent Proterozoic (728–1683 Ma) or Mesozoic (131–179 Ma) integrated ages; the Olifants River swarm (n = 20) includes only Proterozoic (851–1731 Ma) and Archaean (2470–2872 Ma) dykes. The single age obtained on one N–S striking dyke (1464 Ma) suggests that the Lebombo dyke swarm includes Proterozoic dykes in the basement as well. These dates demonstrate the existence of pre-Karoo dykes in these swarms as previously hypothesized without supporting age data. In addition, aeromagnetic and air-photo interpretations indicate that: (1) dyke emplacement was largely controlled by major discontinuities such as the Zimbabwe and Kaapvaal craton boundaries, the orientation of the Limpopo mobile belt, and other pre-dyke structures including shear zones and (2) considering its polygenetic, pre-Mesozoic origin, the Olif ants River dyke swarm cannot be considered part of the Karoo magmatic event.This study, along with previous results obtained on the Okavango dyke swarm, shows that the apparent “triple junction” formed by radiating dyke swarms is not a Jurassic structure; rather, it reflects weakened lithospheric pathways that have controlled dyke orientations over hundreds of millions of years. One consequence is that the “triple-junction” geometry can no longer be unambiguously used as a mantle plume marker as previously proposed, although it does not preclude the possible existence of a mantle plume. More generally, we suggest that most Phanerozoic dyke swarms (including triple junctions) related to continental flood basalts were probably controlled in part by pre-existing lithospheric discontinuities. 相似文献
17.
John S. Myers 《Earth and Planetary Science Letters》1980,46(3):407-418
The coastal dyke swarm and associated flexure, plutonic intrusions and volcanics are the products of a short episode of rifting between normal and thinned continental crust during initial opening of the Atlantic Ocean between Greenland and the Rockall Plateau 56–52 m.y. ago. They constitute a continental rift zone which provides deeply eroded onshore examples of phenomena which probably lie buried beneath the sea along major rifted continental margins.The dyke swarm occurs in a series of zones arranged en echelon, similar to dyke and fissure swarms in Iceland. Most dykes were intruded vertically before flexuring rather than as a fan during flexuring as postulated by Wager and Deer [1]. Layered gabbro plutons and basic cone sheets were emplaced during early stages of flexuring. Magma was tapped westwards along the upper limb of the developing flexure to form the Skaergaard and Kap Edvard Holm intrusions, but intrusions such as Imilik and Kap Gustav Holm in the steep limb show more complex histories of synplutonic tilting, slumping and deformation. Most flexuring occurred after consolidation of the gabbros and was followed by the intrusion of linear and radial swarms of intermediate dykes and ring dykes associated with the emplacement of syenite and granite plutons by cauldron subsidence. 相似文献
18.
Emplacement and arrest of sheets and dykes in central volcanoes 总被引：1，自引：0，他引：1
Sheet intrusions are of two main types: local inclined (cone) sheets and regional dykes. In Iceland, the inclined sheets form dense swarms of (mostly) basaltic, 0.5–1 m thick sheets, dipping either at 20–50° or at 75–90° towards the central volcano to which they belong. The regional dykes are (mostly) basaltic, 4–6 m thick, subvertical, subparallel and form swarms, less dense than those of the sheets but tens of kilometres long, in the parts of the volcanic systems that are outside the central volcanoes. In both types of swarms, the intrusion intensity decreases with altitude in the lava pile. Theoretical models generally indicate very high crack-tip stresses for propagating dykes and sheets. Nevertheless, most of these intrusions become arrested at various crustal depths and never reach the surface to supply magma to volcanic eruptions. Two principal mechanisms are proposed to explain arrest of dykes and sheets. One is the generation of stress barriers, that is, layers with local stresses unfavourable for the intrusion propagation. The other is mechanical anisotropy whereby sheet intrusions become arrested at discontinuities. Stress barriers may develop in several ways. First, analytical solutions for a homogeneous and isotropic crust show that the intensity of the tensile stress associated with a pressured magma chamber falls off rapidly with distance from the chamber. Thus, while dyke and sheet injection in the vicinity of a chamber may be favoured, dyke and sheet arrest is encouraged in layers (stress barriers) at a certain distance from the chamber. Second, boundary-element models for magma chambers in a mechanically layered crust indicate abrupt changes in tensile stresses between layers of contrasting Young’s moduli (stiffnesses). Thus, where soft pyroclastic layers alternate with stiff lava flows, as in many volcanoes, sheet and dyke arrest is encouraged. Abrupt changes in stiffness between layers are commonly associated with weak and partly open contacts and other discontinuities. It follows that stress barriers and discontinuities commonly operate together as mechanisms of dyke and sheet arrest in central volcanoes. 相似文献
19.
本文对"鲁科一井"(CCSD-LK-Ⅰ)768.9~1112.3m之间的上白垩统沉积岩样品进行了岩石磁学、磁化率各向异性(AMS)以及天然剩磁组分的研究.在此基础上,分析了利用特征剩磁(ChRM)和黏滞剩磁(VRM)方向恢复岩芯原始方位的可行性.三轴等温剩磁热退磁曲线、磁滞回线、反向场退磁曲线、一阶反转曲线等岩石磁学测量结果表明,沉积岩的主要载磁矿物为磁铁矿和赤铁矿.335块样品的AMS测量结果表明磁化率椭球主轴的最大轴K1和中间轴K2与水平面夹角较小,最小轴K3接近垂直于水平面分布,说明沉积岩保留了原始沉积磁组构特征.系统热退磁实验表明,多数样品在25~350℃和500~690℃温度段分别获得VRM和ChRM分量.利用ChRM偏角方向,并考虑构造旋转量校正,对VRM偏角方向进行恢复,Fisher统计得到DVRM=-1.3°,IVRM=59.6°,与当地现代地磁场方向(D=-6.7°,I=53.9°)基本一致.用ChRM偏角方向对磁化率主轴K1偏角方向进行校正,校正的结果为:D_(ch_K1)=349.2°,I_(ch_K1)=-0.7°.本文研究结果对于地质勘探中利用古地磁学方法恢复钻孔岩芯原始方位具有一定参考意义. 相似文献