Cenozoic Volcanic Provinces and Shallow Asthenospheric Volumes in the Circum-Mediterranean: Evidence From Magmatic Geochemistry, Seismic Tomography, and Integrated Geophysical-Petrological Thermochemical Inversion

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Geochemistry Geophysics Geosystems Pub Date : 2024-09-07 DOI:10.1029/2023GC011017
A. El-Sharkawy, T. H. Hansteen, C. Clemente-Gomez, J. Fullea, S. Lebedev, T. Meier
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Abstract

We compile an extensive catalog comprising geochemistry and ages of Cenozoic volcanic provinces in the Mediterranean region, distinguishing between three groups according to the geochemistry of magmatic rocks: intraplate (IVP), subduction-related (SRVP), and mixed-origin volcanic provinces (MVP; intraplate with subduction imprint). In order to relate their spatial distribution to properties of the lithosphere-asthenosphere system, we determine temperature-depth profiles by integrated geophysical-petrological inversion at representative locations, using Rayleigh and Love wave phase velocities, heat flow, rock densities, and accounting for thermochemical conditions. The results confirm the occurrence of thin lithosphere (<100 km) above warm asthenosphere (>1,300°C) in areas of low shear-wave velocities in the shallow upper mantle. Nine shallow asthenospheric volumes (SAVs) between 70 and 300 km depths are identified, forming a partly interconnected belt across the Circum-Mediterranean. A remarkable colocation exists between the SAVs and the intraplate and mixed-origin volcanic provinces (IMVPs). Whereas dense networks of IMVPs have formed above the SAVs, IMVPs are absent in areas of thick mantle lithosphere. Magmatic activity in IMVPs at 60–70 Ma indicates that several SAVs existed already in the Paleogene (Central European, Adriatic, Western Mediterranean, and Moesian SAVs). The formation of SAVs is related either to asthenospheric upwelling caused by slab rollback and back-arc extension (Aegean-Anatolian, Moesian, Pannonian, Western Mediterranean SAVs), or to thermal upwelling (Adriatic, Central European, Middle East [MEA], North African, Rhine-Rhone SAVs), with some of the latter coupled partly with continental rifting (Central European, MEA, North African, Rhine Rhone SAVs).

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环地中海新生代火山群和浅成岩层体积:来自岩浆地球化学、地震层析和综合地球物理-岩石热化学反演的证据
我们编制了一份内容广泛的目录,包括地中海地区新生代火山群的地球化学和年龄,并根据岩浆岩的地球化学将其分为三类:板内火山群(IVP)、与俯冲有关的火山群(SRVP)和混合起源火山群(MVP;板内火山群,带有俯冲印记)。为了将它们的空间分布与岩石圈-热成层系统的特性联系起来,我们利用瑞利波和洛夫波相位速度、热流、岩石密度,并考虑热化学条件,通过综合地球物理-地球物理学反演,在具有代表性的地点确定了温度-深度剖面。结果证实,在浅上地幔剪切波速度较低的区域,温暖的岩石圈(1300°C)上方存在薄岩石圈(100 千米)。确定了深度在 70 至 300 千米之间的九个浅层星体层(SAVs),形成了一个横跨环地中海的部分相互连接的带。浅层星体与板内火山群和混合成因火山群(IMVPs)之间存在明显的同位现象。在狭长地带火山群上方形成了密集的板内火山群网络,而在厚地幔岩石圈地区则没有板内火山群。在 60-70 Ma 时,IMVPs 中的岩浆活动表明,在古近纪就已经存在多个 SAVs(中欧 SAVs、亚得里亚海 SAVs、西地中海 SAVs 和莫埃西亚 SAVs)。SAVs的形成要么与板块后退和弧后延伸引起的星体层上升流有关(爱琴海-安纳托利亚、摩埃西亚、潘诺尼亚、西地中海 SAVs),要么与热上升流有关(亚得里亚海、中欧、中东[MEA]、北非、莱茵河-罗纳河 SAVs),其中一些 SAVs 部分与大陆裂解有关(中欧、中东[MEA]、北非、莱茵河-罗纳河 SAVs)。
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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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