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作 者:徐新文[1,2] 强小科[1] 符超峰[1,3] 赵辉[1,2] 陈艇[1,2] 孙玉芳[1,2]
机构地区:[1]中国科学院地球环境研究所黄土与第四纪地质国家重点实验室,西安710075 [2]中国科学院研究生院,北京100049 [3]长安大学西部矿产资源与地质工程教育部重点实验室,西安710075
出 处:《第四纪研究》2012年第4期812-819,共8页Quaternary Sciences
基 金:国家重点基础研究发展规划项目(973项目)(批准号:2010CB833400);国家自然科学基金项目(批准号:40572109和40872114);中国科学院地球环境研究所黄土与第四纪国家重点实验室开放基金项目(批准号:SKLLQG0913);自主部署项目(批准号:LQ0701)共同资助
摘 要:鹤庆盆地位于我国西南地区,受印度季风影响。在盆地内获取的665.83m的湖相岩芯具有沉积连续,时间跨度长的特点,是研究印度季风在第四纪以来发展演化特征的理想材料。在岩芯的下部(1.8Ma以前),磁化率大幅度降低,而烧失量则较高。通过对这部分沉积物详细的岩石磁学测试和扫描电镜分析可知,岩芯下部(2.5~1.8Ma)磁性矿物含量较低,低磁化率值与沉积后的还原溶解作用密切相关。在岩芯下部有自形程度较高的单畴(SD)胶黄铁矿存在,可能为早期还原成岩过程的产物。Heqing Basin(26°27' -26°46'N, 100°08' -100°17'E) is a Late Cenozoic north-south oriented pull-apart basin near the northwestern margin of the Yunnan-Guizhou Plateau. The Basin is located at the southeastern margin of the Tibetan Plateau and belongs to the terminal of Hengduan Mountains. The local climate is dominated by Indian monsoon. Therefore, the continuous and thick sediments in the basin make it a perfect continental record for evolution of Indian summer monsoon. The Heqing drill core was obtained in the centre of the Heqing Basin. Using the internal lining method, recovery of the HQ drill core (26°33'43. I"N, 100°10'14.2"E;2200m) which has an accumulative depth of 665.83m reaches up to 96.7%. The lake sediments mainly consist of horizontally laminated greyish-green calcareous clay and silty clay with thin-bedded silt and fine sand layers,except two intervals of sand layers with fine gravels. With the equal interval of 50em,we obtained 1368 samples from the drill core and chose 108 from different depositional units for detailed rock magnetic measurements. Based on detailed rock magnetic measurements like magnetic susceptibility versus high/low temperature curves, thermal demagnetization curve, hysteresis loops and FORC diagrams, we have investigated the magnetic properties of Heqing core lacustrine sediments. Magnetic measurements showed that sediments from the lower section (before 1.8Ma) of the core contain both magnetite and greigite while sediments from the upper section ( after 1.8Ma)contain magnetite only. The abrupt decrease at about 580℃ in %-T curves revealed that magnetite could be the dominant magnetic minerals in the upper section. FORC diagram displayed a characteristic PSD distribution. Hysteresis loop of low % units in upper sections showed a wasp waist shape which is due to admixture of different eoercivity and different domain state. This could be attributed to magnetic dissolution which decrease ferromagnetic component like magnetite and maghemi
分 类 号:P318.41[天文地球—固体地球物理学] P941.78[天文地球—地球物理学]
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