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Introduction to 'Magnetic iron minerals in sediments and their relation to geologic processes, climate, and the geomagnetic field'

机译:“沉积物中的磁性铁矿物及其与地质过程,气候和地磁场的关系”简介

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摘要

Iron is the fourth most common element on Earth and gives rise to the magnetic properties of rock-forming minerals. Magnetic iron minerals are, therefore, abundant and occur in almost every type of geological material. Scientific interest in the occurrence of magnetic minerals in sediments was triggered over 60 years ago by paleomagnetic and magnetostratigraphic applications that relate to the capability of these minerals to record the Earth's magnetic field shortly after deposition, and to store this information over geological timescales (e.g. Johnson et al., 1948; King, 1955; Irving and Major, 1964). Marine sediments are a key source of long and continuous paleomagnetic records, which are essential for reconstructing past geomagnetic field variations and for dating using global geomagnetic reversals (Ogg and Smith, 2004). Magnetic polarity stratigraphy, combined with other age determination methods, has become an essential tool in sedimentary geochronology. Important aspects of sedimentary paleomagnetism, such as the mechanism, efficiency and timing of acquisition of a natural remanent magnetization (NRM), its preservation during diagenetic processes, and possible overprinting by magnetic minerals that formed long after deposition, are intensively investigated and have not yet been fully explained (e.g. Tauxe, 2006; Roberts et al., 2013).
机译:铁是地球上第四大最常见的元素,并且会增加形成岩石的矿物的磁性。因此,磁性铁矿物质丰富,几乎存在于每种类型的地质材料中。六十多年前,古磁性和地层学的应用引发了人们对沉积物中磁性矿物发生的科学兴趣,这些应用与这些矿物在沉积后不久记录地球磁场的能力以及在地质时标上存储该信息的能力有关(例如Johnson等人,1948;金,1955;欧文和梅杰,1964)。海洋沉积物是长期和连续的古地磁记录的重要来源,这对于重建过去的地磁场变化和利用全球地磁逆转定年是必不可少的(Ogg和Smith,2004)。磁极地层学与其他年龄确定方法相结合,已成为沉积地球年代学中必不可少的工具。深入研究了沉积古磁性的重要方面,例如获得自然剩磁的机制,效率和时机,在成岩过程中的保存以及沉积后形成很长时间的磁性矿物可能的套印。充分解释(例如Tauxe,2006; Roberts等,2013)。

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  • 来源
    《Global and planetary change》 |2013年第ptac期|259-263|共5页
  • 作者单位

    Central Institute for Meteorology and Geodynamics, Hohe Warte 38, A-1190 Vienna, Austria;

    Istituto Nazionale di Geofisica e Vulcanologia, Via di Vigna Murata 605, 1-00143 Rome, Italy;

    Research School of Earth Sciences, The Australian National University, 61 Mills Road, Canberra, ACT 0200, Australia;

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