The structure of Precambrian crust in sub-Saharan Africa: An AfricaArray synthesis and review

IF 2.2 4区 地球科学 Q2 GEOSCIENCES, MULTIDISCIPLINARY
Alexandra Sabattier , Andrew Nyblade , Raymond Durrheim , Fenitra Andriampenomanana , Andriamiranto Raveloson , Islam Fadel , Mark van der Meijde , Amanda Willet
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引用次数: 0

Abstract

We combine new estimates of crustal thickness and shear wave velocities from 48 broadband seismic stations in Mozambique, Namibia, South Africa and Uganda with previously published results to review and examine Precambrian crustal structure in sub-Saharan Africa for secular trends. The ensemble of crustal structure estimates used relies heavily on data obtained through the AfricaArray initiative, which is briefly reviewed. Whether or not Precambrian crustal structure exhibits notable changes from the Mesoarchean through the Neoproterozoic places a key constraint on continental crustal genesis and evolution. Our 48 new estimates of Moho depth and crustal shear wave velocity profiles, combined with results from similar previous studies, yield an average crustal thickness for all Precambrian terranes of 39 ± 4 km. We find that average crustal thicknesses are essentially identical for Mesoarchean (38 ± 3 km), Neoarchean (39 ± 4 km), Paleoproterozoic (40 ± 4 km), Mesoproterozoic (40 ± 4 km) and Neoproterozoic (39 ± 4 km) terranes. The average thickness of the mafic lower crust, identified by high velocity layering (Vs > 4.0 km/s), is also almost identical in Archean and Proterozoic terranes (7 ± 4 km and 6 ± 4 km, respectively). Finally, the average crustal shear wave velocities for all terranes fall within 1 standard deviation of a mean velocity of 3.7 km/s. These results are consistent with findings from other studies highlighting a lack of evidence for secular variation in crustal structure or composition within Precambrian terranes in sub-Saharan Africa, suggesting that secular trends, if they existed at the time of crust formation, have been obscured by crustal reworking during later orogenic and/or magmatic events.
撒哈拉以南非洲前寒武纪地壳结构:非洲阵列综合与评述
我们将来自莫桑比克、纳米比亚、南非和乌干达的48个宽带地震站的地壳厚度和横波速度的新估计与先前发表的结果相结合,以回顾和研究撒哈拉以南非洲的前寒武纪地壳结构的长期趋势。所使用的地壳结构估计的集合在很大程度上依赖于通过非洲阵列计划获得的数据。从中太古宙到新元古代,前寒武纪地壳结构是否有显著变化,是制约大陆地壳发生演化的关键因素。我们对莫霍深度和地壳横波速度剖面的48个新估计,结合以往类似研究的结果,得出所有前寒武纪地体的平均地壳厚度为39±4 km。中太古代(38±3 km)、新太古代(39±4 km)、古元古代(40±4 km)、中元古代(40±4 km)和新元古代(39±4 km)的平均地壳厚度基本相同。高速分层确定的基性下地壳平均厚度(Vs >;4.0 km/s),在太古宙和元古宙中也几乎相同(分别为7±4 km和6±4 km)。最后,所有地形的平均地壳横波速度落在平均速度3.7 km/s的1个标准差以内。这些结果与其他研究的发现一致,这些研究强调缺乏证据证明撒哈拉以南非洲前寒武纪地体中地壳结构或组成的长期变化,表明长期趋势,如果在地壳形成时存在,则被后来的造山和/或岩浆事件中的地壳改造所掩盖。
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来源期刊
Journal of African Earth Sciences
Journal of African Earth Sciences 地学-地球科学综合
CiteScore
4.70
自引率
4.30%
发文量
240
审稿时长
12 months
期刊介绍: The Journal of African Earth Sciences sees itself as the prime geological journal for all aspects of the Earth Sciences about the African plate. Papers dealing with peripheral areas are welcome if they demonstrate a tight link with Africa. The Journal publishes high quality, peer-reviewed scientific papers. It is devoted primarily to research papers but short communications relating to new developments of broad interest, reviews and book reviews will also be considered. Papers must have international appeal and should present work of more regional than local significance and dealing with well identified and justified scientific questions. Specialised technical papers, analytical or exploration reports must be avoided. Papers on applied geology should preferably be linked to such core disciplines and must be addressed to a more general geoscientific audience.
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