The plume-dependent granite-rhyolite magmatism

Q4 Earth and Planetary Sciences
V. Puchkov
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引用次数: 12

Abstract

The plume-dependent magmatism is widespread and well justified. The bulk of it is represented by flood basalts, basalts of oceanic islands (OIB), and basalts of oceanic plateaus (OPB), though the whole scope of plume magmatism is very diverse. A noticeable role among them is played also by acid (silicic) magmatic rocks - rhyolites and granites. Two main types of plume magmatism are recognized. The first belongs to Large Igneous Provinces (LIP) and is thought to be born at the Core-Mantle boundary within structures, called superswells, that produce giant, short-living mantle upwellings, resulting in abundant volcanism on the Earth’s surface. The second type is represented by linear volcanic chains characterized by regular age progressions. They are formed by single plumes - thin ascending mantle flows, acting during longer periods of time. It is shown that the abundance of silicic magmatism strongly depends on the type of the earth’s crust. Among flood basalts of continents, silicic magmatism is usually present, subordinate in volume to basalts and belongs to a bimodal type of magmatism. But in some cases LIP in continents are formed predominantly by silicic rocks; they are given the name Silicic LIPS, or SLIPS. In oceans, LIP are fundamentally basaltic with no considerable volume of silicic volcanics, if any. The time-progressive volcanic chains in continents are rare and usually comprise a noticeable silicic component. In oceans, the chains are composed mostly of basalts (OIB type), though in the top parts of volcanoes more acid and alkaline differentiates are present; usually they lack rhyolites and granites, except the cases of a presence of some strips of continental crust or anomalously thick oceanic crust. This review can lead to a thought of an important role of melting of continental crust in formation of plume-dependent rhyolite-granite magmatism. As for the Urals, the proofs for a presence of plume-dependent magmatism in its history were presented only recently. Among the plume episodes, some are characterized by presence of silicic components, in particular: Mashak (1380-1385 Ma), Igonino (707-732 Ma), Man’khambo (mainly Cambrian), Ordovician Kidryasovo, Stepninsky (Permian) and Urals-Siberian (Triassic).
羽状花岗岩流纹岩岩浆作用
依赖于羽流的岩浆活动广泛存在,而且有充分的理由。尽管整个羽流岩浆活动范围非常多样,但其主要表现为洪水玄武岩、海洋岛屿玄武岩(OIB)和海洋高原玄武岩(OPB)。其中酸性(硅质)岩浆岩流纹岩和花岗岩也起着显著的作用。岩浆柱活动主要有两种类型。第一个属于大火成岩省(LIP),被认为诞生于核心-地幔边界内的结构,称为超级井,产生巨大的,短寿命的地幔上升流,导致地球表面丰富的火山活动。第二种类型为线性火山链,年龄递进规律。它们是由单一的地幔柱形成的——薄薄的上升的地幔流,在较长的时间内起作用。结果表明,硅质岩浆活动的丰度与地壳类型密切相关。在大陆洪泛玄武岩中,通常存在硅质岩浆作用,其体积从属于玄武岩,属于双峰型岩浆作用。但在某些情况下,大陆上的LIP主要由硅质岩石形成;它们被命名为硅唇,或slip。在海洋中,LIP基本上是玄武岩,没有相当数量的硅火山,如果有的话。大陆上随时间递进的火山链很少见,通常含有明显的硅成分。在海洋中,链条主要由玄武岩(OIB型)组成,尽管在火山的顶部存在更多的酸性和碱性差异;通常它们缺少流纹岩和花岗岩,除了一些大陆地壳带或异常厚的海洋地壳存在的情况。这一综述可以引出大陆地壳熔融在羽状流纹岩-花岗岩岩浆作用形成过程中的重要作用。至于乌拉尔山脉,其历史上存在羽状岩浆作用的证据直到最近才出现。其中,Mashak (1380 ~ 1385 Ma)、Igonino (707 ~ 732 Ma)、Man’khambo(主要为寒武系)、Kidryasovo(奥陶系)、Stepninsky(二叠纪)和Urals-Siberian(三叠纪)等地幔柱具有硅质成分。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Litosfera
Litosfera Earth and Planetary Sciences-Geophysics
CiteScore
0.70
自引率
0.00%
发文量
39
审稿时长
12 weeks
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