贾正元1,,,
张贵宾1,
张刚1,
张昌榕1,
孙仁斌2,
陈涛1
1. 中国地质大学(北京)地球物理与信息技术学院, 北京 100083
2. 中国地质调查局发展研究中心, 北京 100037
基金项目: 国家重点研发计划(2016YFC0600301,2017YFC0602204-01,2016YFC0600201)和中央高校基本科研业务费专项资金(2652016127)联合资助
详细信息
作者简介: 胡斌, 男, 1992年生, 中国地质大学(北京)博士生研究生, 主要从事重磁反演理论及深部探测等方面的研究.E-mail:759785247@qq.com
通讯作者: 贾正元, 男, 1981年生, 实验师, 主要从事地球物理反演、重磁电勘探等研究.E-mail:jzy@cugb.edu.cn
中图分类号: P541;P631收稿日期:2018-07-31
修回日期:2019-01-08
上线日期:2019-04-05
Three-dimensional inversion of gravity and magnetic data and its application in the study on the characteristics of magmatic rocks in the Gangdise belt and adjacent areas, Tibetan Plateau
HU Bin1,,JIA ZhengYuan1,,,
ZHANG GuiBin1,
ZHANG Gang1,
ZHANG ChangRong1,
Sun RenBin2,
CHEN Tao1
1. School of Geophysics and Information Technology, China University of Geosciences, Beijing 100083, China
2. Development and Research Center, China Geological Survey, Beijing 100037, China
More Information
Corresponding author: JIA ZhengYuan,E-mail:jzy@cugb.edu.cn
MSC: P541;P631--> Received Date: 31 July 2018
Revised Date: 08 January 2019
Available Online: 05 April 2019
摘要
摘要:岩浆岩在青藏高原的大陆动力学研究中有着重要的作用,它既是构造演化的记录,又是重要构造-岩浆-成矿带的指示.本文主要基于冈底斯带及邻区的地面重力和航磁数据,首先进行地质-地球物理先验信息约束下的重磁2.5维交互式反演,再将2.5维反演结果作为参考模型加入到三维反演计算中,得到地下三维密度和磁化率结构.结合岩浆岩密度、磁化率统计资料和岩浆岩地球化学成果,推断研究区基性岩、Ⅰ型花岗岩和S型花岗岩的三维分布图,得到如下结论:S型花岗岩主要分布在冈底斯东带和冈底斯弧背断隆带以北;北冈底斯的西部无明显的岩浆活动,而在其南侧和北侧,发现大量的隐伏基性岩和零散分布的Ⅰ型花岗岩;中生代Ⅰ型花岗岩在南冈底斯和冈底斯弧背断隆带广泛分布,且到新生代才出现大量的S型花岗岩.上述结果为中生代班公湖-怒江洋壳和新特提斯洋壳的双向剪刀式俯冲模式的观点提供了重要佐证,并认为班公湖-怒江洋壳在北冈底斯西部约84°E-88°E的范围内先后存在向北和向南俯冲的可能,北向羌塘地体下俯冲,南向冈底斯地体下俯冲.
关键词: 冈底斯带/
地质-地球物理先验信息/
重磁三维反演/
岩浆岩三维分布/
俯冲模式
Abstract:Magmatic rocks play an important role in research on continental dynamics in the Tibetan Plateau, which are records of tectonic evolution as well as the indications of major tectonic-magmatic-metallogenic belts. In this paper, we used large-scale ground gravity and aeromagnetic data to study the characteristics of magmatic rocks in the Gangdise belt and adjacent areas. To obtain the 3D density and susceptibility models of the study area, we carried out 2.5D interactive inversion of gravity and magnetic data based on geological-geophysical prior information. The 2.5D inversion results were then regarded as the reference model for the three-dimensional inversion. Integrating the inversion results with physical property statistics and geochemical data, we mapped the three-dimensional distribution of basic rocks, Ⅰ type granites and S type granites in the study area. The resulting maps show that S type granites which are related to the Mesozoic collision are mainly distributed in the eastern Gangdise belt and the north of Gangdise back-arc fault uplift. No remarkable intrusive rocks are found west of northern Gangdise. While a large number of hidden basic rocks are present in the south and north sides of the northern Gangdise, and a few Ⅰ type granites which are related to subduction are scattered there. In the southern Gangdise and Gangdise back-arc fault uplift, Mesozoic Ⅰ type granites are widely distributed, but the large number of S type granites did not appear till the Cenozoic era. The above results provide important evidence to support the bi-directional scissors-style subduction model of the Mesozoic Bangong Co-Nujiang oceanic crust southward and the Neo-Tethys oceanic crust northward subduction. We consider that the Bangong Co-Nujiang oceanic crust may have subducted northward and southward subsequently in the west of the northern Gangdise in the range of 84°E-88°E. The oceanic crust subducted northward to the Qiangtang terrane and southward to the Gangdise terrane.
Key words:Gangdise belt/
Geological-geophysical prior information/
3D inversion of gravity and magnetic data/
3D distribution of magmatic rocks/
Subduction model
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