共查询到20条相似文献，搜索用时 15 毫秒
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Maria Irene Bartolomeu Raposo 《Geophysical Journal International》1997,131(1):159-170
Magnetic fabric was determined by applying the anisotropy from the low-field magnetic susceptibility (AMS) technique in 62 mafic dykes from the Mesozoic Florianópolis (Santa Catarina Island) dyke swarm, southern Brazil. These dykes cut the crystalline basement rocks, which are mainly Proterozoic. They are vertical or subvertical in dip and trend mainly NE, although NW-trending dykes are also found. Dykes are tholeiitic in composition and are geochemically similar to those from the Ponta Grossa swarm. Thicknesses vary from 0.3 to 60 m. Polished sections show that titanomagnetites carry the AMS in these dykes. Hysteresis parameters show that the magnetic minerals fall in the PSD range. Two types of magnetic fabric are recognized. Type I is characterized by K 1 - K 2 parallel to the dyke wall, representing magma flow within the dykes; type II, with K 1 - K 3 parallel to the dyke wall, was found in four dykes. Type I is found in 94 per cent of the dykes, and approximately 20 per cent of these have K 1 inclinations of less than 30°, suggesting horizontal or subhorizontal flow. About 80 per cent have K 1 inclinations of greater than 30°, due to inclined to vertical flow. The comparison of AMS studies from both the Florianópolis and the Ponta Grossa dykes suggests a source position closer to Santa Catarina Island than the Ponta Grossa arch. 相似文献
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Magnetic properties of the profiles of polluted and non-polluted soils. A case study from Ukraine 总被引：7，自引：0，他引：7
Maria Jele&#;ska Agata Hasso-Agopsowicz Barbara Kopcewicz Anatoliy Sukhorada Ksenija Tyamina Magdalena K&#;dzia&#;ko-Hofmokl Zhanna Matviishina 《Geophysical Journal International》2004,159(1):104-116
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Summary. An exact equation is derived for the magnetic field lines of the general axisymmetric magnetic multipole of arbitrary degree ( n ). This new result has important applications in studies of the possible nature of solarterrestrial physics during geomagnetic polarity reversals. In the limiting case of a magnetic dipole ( n=1 ), the equation for the magnetic field lines of the general axisymmetric magnetic multipole simplifies correctly to the well-known dipolar form, which is used extensively in geomagnetism, magnetospheric physics and cosmic-ray physics as a first-order approximation to the actual configuration of the geomagnetic field.
It is also shown theoretically that suites of similar magnetic field lines of the general axisymmetric multipole attain their maximum radial distances from the origin on a set of circular conical surfaces, with coincident vertices at the centre of the Earth; this set includes the equatorial plane if the degree ( n ) of the multipole is odd. The magnetic field is horizontal everywhere on all these surfaces.
Palaeomagnetic studies have suggested that during some polarity reversals the magnetic field in the inner magnetosphere can be represented approximately either by a single, non-dipolar, low-degree (2 < n < 4), axisymmetric magnetic multipole or by a linear combination of such multipoles. In this situation, the equation for the field lines of an axisymmetric magnetic multipole of low degree (2 < n < 4) would be as fundamental to a proper understanding of magnetospheric, ionospheric and cosmic-ray physics during polarity reversals as is the equation for dipolar field lines in the case of the contemporary geomagnetic field. 相似文献
It is also shown theoretically that suites of similar magnetic field lines of the general axisymmetric multipole attain their maximum radial distances from the origin on a set of circular conical surfaces, with coincident vertices at the centre of the Earth; this set includes the equatorial plane if the degree ( n ) of the multipole is odd. The magnetic field is horizontal everywhere on all these surfaces.
Palaeomagnetic studies have suggested that during some polarity reversals the magnetic field in the inner magnetosphere can be represented approximately either by a single, non-dipolar, low-degree (2 < n < 4), axisymmetric magnetic multipole or by a linear combination of such multipoles. In this situation, the equation for the field lines of an axisymmetric magnetic multipole of low degree (2 < n < 4) would be as fundamental to a proper understanding of magnetospheric, ionospheric and cosmic-ray physics during polarity reversals as is the equation for dipolar field lines in the case of the contemporary geomagnetic field. 相似文献
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K. Dimitropoulos 《Geophysical Journal International》1986,85(2):383-388
Summary . An elongated zone of positive magnetic anomalies extends from Northern Ireland to the Shetland Islands. From the total magnetization of the body causing the anomaly and published palaeomagnetic directions corresponding to a range of different possible ages for the remanent magnetization of this body, associated ranges of susceptibility are calculated. These ranges favour a Siluro–Devonian age as most plausible for the remanent magnetization. Such an age is compatible with the known geology of the area. 相似文献
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A simple new model for sudden lithospheric thinning that considers the crust to be stretched and the lower layer of the lithosphere to be partially stretched and partially mechanically eroded is proposed. This model allows calculation of the thermal field of the lithosphere during the initial warming phase and the surface uplift.
Application of this model to the Tuscan Basin explains the high regional heat flux density values (>100 mW m−2 ), the tectonic subsidence (about 1 km) and the average uplift (>400 m) observed in this region well. 相似文献
Application of this model to the Tuscan Basin explains the high regional heat flux density values (>100 mW m
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黄土磁化率各向异性（AMS）被认为是重建古风向变化重要的指标之一,在黄土高原地区得到广泛的应用。然而新疆地区的黄土磁化率各向异性研究相对薄弱。通过对新疆塔城盆地库尔托别剖面磁化率各向异性参数和磁化率分析古风向和风力强度的变化,结果表明：塔城地区末次冰期以来以东南风为主,剖面从下至上,可分为5个阶段：第1阶段（12~14 m）：对应MIS3c时期,磁组构特征受水流作用的影响明显,表现为东南风。第2阶段（6~12 m）：对应MIS3b时期,出现西南风,但主要还是以东南风为主。第3阶段（4~6 m）：对应MIS3a早中期,以东南风为主,西南风逐渐消失,并且风力强度逐渐减弱。第4阶段（0.5~4 m）：对应MIS3a晚期和MIS2早期,表现为东南风,风力强度波动较大。第5阶段（0~0.5 m）：磁组构特征受成壤作用影响强烈。 相似文献
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The quiet-day geomagnetic field variation data from the recently commissioned Nagpur geomagnetic observatory, which has augmented the currently active latitudinal chain of Indian magnetic observatories, are analysed for the year 1993- The variations for diurnal frequencies (Sq) recorded at Nagpur do not follow the expected trend with latitude. This is most conspicuous in the northward horizontal ( X ) component. The anomalous behaviour at Nagpur is also seen in the diurnal harmonic amplitudes when compared with those of the neighbouring stations Alibag (south of Nagpur) and Ujjain (north of Nagpur). This behaviour is attributed to the presence of electrically conducting anomalous sources in the vicinity of Nagpur. The anomalous internal source is inferred to be located at relatively shallower depths and is highly localized. 相似文献
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青藏高原东缘山地古冰川沉积物磁化率特点及其影响因素分析 总被引：1，自引：1，他引：0
湖泊、黄土与古土壤、深海沉积物等连续沉积体的磁化率变化作为环境变化的替代性指标被广泛应用,然而对于非连续、能够反映特定时段气候变化的沉积体,如冰川沉积物的磁化率却较少涉及.本文通过对青藏高原东缘8 个典型冰川发育山地冰碛物磁化率进行研究,并与黄土、湖泊、深海沉积物以及不同区域的表土磁化率进行对比,采用质量磁化率和频率磁化率探讨冰碛物的磁化率特点及其影响因素.结果表明：青藏高原东缘山地的冰碛物质量磁化率呈宽幅波动,介于(3.01~1808.80)×10-8 m3·kg-1,平均值147.84×10-8 m3·kg-1;频率磁化率值较低、且波动幅度小,介于0~6.89%,平均值为1.37%.不同时空条件下冰碛物的磁化率特点不同,即不同地点同一冰期磁化率的差异显著;同一地点不同冰期冰碛物的磁化率变化不明显.影响冰碛物磁化率的主导因素是母岩的岩性条件,气候因素起次要作用. 相似文献