冰冻的海洋水晶浆

IF 2.2 3区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY Terra Nova Pub Date : 2023-04-20 DOI:10.1111/ter.12655
V. Basch, C. Ferrando, A. Sanfilippo
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引用次数: 0

摘要

驱动晶浆演化的过程通常记录在复杂的系统中,在这些系统中,结晶、同化、岩浆补给和混合同时发生,并且通常因压实和变形而叠加。因此,记录未受干扰的晶浆的特性是最重要的;它强调了复杂的晶体糊状过程进行的初始条件。在这里,我们通过对大西洋中脊米级侵入体的详细岩石结构和化学研究,介绍了海洋晶浆的结构和组成。纹理、大块岩石和矿物成分表明原始熔体的闭合系统结晶,不受溶解-沉淀反应和随后变形的干扰。这些冻结的晶浆记录了小规模入侵的最简单可能的演化,可以用作确定晶浆过程对复杂系统演化影响的基线。与该参考文献的任何差异都是由于伴随岩浆系统逐渐闭合而发生的过程造成的。
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A frozen oceanic crystal mush
The processes driving the evolution of crystal mushes are often documented in complex systems where crystallization, assimilation, magma replenishment and mixing occur concurrently and are generally overprinted by compaction and deformation. Documenting the characteristics of an undisturbed crystal mush is thus of upmost importance; it highlights the initial conditions with which complex crystal mush processes proceed. We here present the structure and composition of an oceanic crystal mush through detailed petro‐structural and chemical study of metre‐scale intrusions from the Mid‐Atlantic Ridge. Textures, bulk‐rock and mineral compositions indicate closed‐system crystallization of primitive melts, undisturbed by dissolution–precipitation reactions and subsequent deformation. These frozen crystal mushes record the simplest possible evolution of small‐scale intrusions and can be used as a baseline to pinpoint the impact of crystal mush processes on the evolution of complex systems. Any divergence from this reference results from processes occurring concomitantly to the progressive closure of the magmatic system.
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来源期刊
Terra Nova
Terra Nova 地学-地球科学综合
CiteScore
4.80
自引率
8.30%
发文量
59
审稿时长
2.3 months
期刊介绍: Terra Nova publishes short, innovative and provocative papers of interest to a wide readership and covering the broadest spectrum of the Solid Earth and Planetary Sciences. Terra Nova encompasses geology, geophysics and geochemistry, and extends to the fluid envelopes (atmosphere, ocean, environment) whenever coupling with the Solid Earth is involved.
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