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Titlebook: Early Precambrian Basic Magmatism; R. P. Hall,D. J. Hughes Book 1990 Blackie & Son Ltd 1990 chemistry.classification.formation.geochemistr

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发表于 2025-3-21 16:04:10 | 显示全部楼层 |阅读模式
书目名称Early Precambrian Basic Magmatism
编辑R. P. Hall,D. J. Hughes
视频video
图书封面Titlebook: Early Precambrian Basic Magmatism;  R. P. Hall,D. J. Hughes Book 1990 Blackie & Son Ltd 1990 chemistry.classification.formation.geochemistr
描述Basic magmatic rocks make up approximately three-quarters of the crust ofthe present day Earth. Because we can observe and study the volcanic products of present day tectonic regimes comprehensively, we can shed light on ancient tectono-magmatic provinces, and thereby deduce the petrogenesis and evolution of the oldest basic rocks. This is the primary objective of this book. The book was conceived in order to provide a comprehensive review of the basic rocks produced during the first half of the Precambrian, i.e. the Archaean and early Proterozoic, to about 1.8 Ga years ago. Two major questions are addressed. First, what basic magmas were generated during the early Precambrian: were these magmas globally uniform, and to what extent were prevailing tectonic controls and compo­ sitions analogous to those of the present day? Clearly, this can be answered only by bringing together fundamental information about all relevant basic magmatic events. Second, is there any systematic temporal variation in the nature of basic suites, and what implications might such variations have on our interpretations of early Earth history? Are there important differences between early Archaean, late Archa
出版日期Book 1990
关键词chemistry; classification; formation; geochemistry; metamorphism; mineral; mineralogy; petrogenesis; petrogr
版次1
doihttps://doi.org/10.1007/978-94-009-0399-9
isbn_softcover978-94-010-6666-2
isbn_ebook978-94-009-0399-9
copyrightBlackie & Son Ltd 1990
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eProcurement in der Öffentlichen Logistikoleiites are chemically distinct from their more modern counterparts and they are the most abundant magma type represented in greenstone belts, and thus they warrant significant attention. Several magma types are not discussed in this chapter since, although they were erupted during the Archaean, th
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https://doi.org/10.1007/978-3-658-09447-8brian these suites comprise komatiites, komatiitic basalts (previously known as basaltic komatiites), siliceous high-Mg basalts (SHMB), norites and the parental magmas of the noritic portions of major layered, Bushveld-type intrusions (’U’-type magmas). However, of these, the petrology of norites ha
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Datengrundlage und Untersuchungsdesign,ng in the early mantle. Much of our knowledge is based on studies of the present mantle but the early Precambrian geological record, and in particular the sensitivity of the magmatic record to the thermal and chemical state of the mantle, places constraints on mantle evolution. These constraints, in
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https://doi.org/10.1007/978-3-658-15597-1has evolved from a distant object of curiosity to a natural laboratory for planetary geology. Because of the lack of tectonic recycling and chemical weathering, fresh rocks more than 4.0 Ga old still exist on the Moon and these rocks yield invaluable information about the early history of the solar
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https://doi.org/10.1007/978-3-658-03302-6, Cr, the platinum group elements (PGE), Cu, Au and asbestos are found in direct association with mafic and ultramafic magmatism. This chapter first considers Archaean metallogenesis associated with volcanic suites and reviews the classical association between Fe–Ni sulphide mineralisation and komat
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