Origin of clinopyroxene megacrysts in volcanic rocks from the North China Craton: a comparison study with megacrysts worldwide
Origin of clinopyroxene megacrysts in volcanic rocks from the North China Craton: a comparison study with megacrysts worldwide
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华北克拉通火山岩中单斜辉石巨晶的成因:与世界巨晶的对比研究
DOI:
10.1080/00206814.2019.1663766
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发表时间:
2019-09
影响因子:
2.6
通讯作者:
Ying Ji-Feng
中科院分区:
文献类型:
--
作者:
Liu Ya-Dong;Ying Ji-Feng
Clinopyroxene megacrysts in volcanic rocks can provide substantial information on the evolution of the magmatic system at depth. Although considerable attention has been paid to these crystals, their origin is not yet completely resolved. The clinopyroxene megacrysts worldwide can be divided into two major types in general: the green Cr-diopside type and the black Al-augite type. There is a consensus view that the Cr-diopside megacrysts are mantle xenocrysts, whereas two contrasting opinions exist regarding the origin of the black Al-augite megacrysts. One favours a cognate origin, viewing them as crystallization products of the host magmas under high-pressure; while the other argues that they are xenocrysts crystallized from previous alkali basalts or fragments of mantle peridotites, pyroxenites or pegmatite veins. A review study on the clinopyroxene megacrysts in Meso-Cenozoic volcanic rocks from the North China Craton (NCC) and their comparison with those worldwide provides new constraints on their origin, namely, the Cr-diopside megacrysts, as previously thought, are all xenocrysts, representing disaggregated clinopyroxene crystals from clinopyroxene-rich mantle rocks. Contrary to the formerly proposed cognate origin, the Al-augite megacrysts are also xenocrysts, having no direct genetic link to their host rocks. They crystallized from melts that have formed earlier than the host magmas, and probably accumulated in a magma chamber or occurred as sheets or veins filling a fracture network surrounding a magma chamber in the upper mantle. During the subsequent eruption of the host lavas, these previously formed crystals were incorporated into the magma and were brought up to the surface.
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影响因子:
3.5
作者:
A. Moore;G. Costin
通讯作者:
A. Moore;G. Costin
DOI:
10.1007/bf01829378
发表时间:
1991-06
期刊:
Geologische Rundschau
影响因子:
--
作者:
B. Marsh;B. Gunnarsson;R. Congdon;R. Carmody
通讯作者:
B. Marsh;B. Gunnarsson;R. Congdon;R. Carmody
DOI:
--
发表时间:
1969-11
期刊:
--
影响因子:
--
作者:
石橋 澄;K. Ishibashi;キヨシ イシバシ
通讯作者:
石橋 澄;K. Ishibashi;キヨシ イシバシ
影响因子:
3.1
作者:
Kevin S. Richter;I. Carmichael
通讯作者:
Kevin S. Richter;I. Carmichael
影响因子:
5
作者:
Jin-Ting Kang;Hong-Li Zhu;Yu-Fei Liu;Fang Liu;Fei Wu;Yan-Tao Hao;Xia-Chen Zhi;Zhao-Feng Zhang;Fang Huang
通讯作者:
Fang Huang