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DOI | 10.1016/j.epsl.2019.115962 |
Evolution of cratons through the ages: A time-dependent study | |
Paul J.; Ghosh A. | |
发表日期 | 2020 |
ISSN | 0012821X |
卷号 | 531 |
英文摘要 | The viscosity of cratons is key to understanding their long term survival. In this study, we present a time-dependent, full spherical, three dimensional mantle convection model to investigate the evolution of cratons of different viscosities. The models are initiated from 409 Ma and run forward in time till the present-day. We impose a surface velocity boundary condition, derived from plate tectonic reconstruction, to drive mantle convection in our models. Cratons of different viscosities evolve accordingly with the changing velocity field from their original locations. Along with the viscosity of cratons, the viscosity of the asthenosphere also plays an important role in cratons' long term survival. Our results predict that for the long-term survival of cratons they need to be at least 100 times more viscous than their surroundings and the asthenosphere needs to have a viscosity of the order of 1020 Pa-s or more. © 2019 Elsevier B.V. |
关键词 | cratonsmantle convectionnumerical modelingstudy of deep earth interior |
英文关键词 | Numerical models; Velocity; cratons; Deep earths; Mantle convection; Mantle convection models; Surface velocity; Time dependent; Velocity field; Viscosity; asthenosphere; boundary condition; craton; mantle convection; numerical model; plate tectonics; reconstruction; viscosity |
语种 | 英语 |
来源期刊 | Earth and Planetary Science Letters |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/202825 |
作者单位 | Centre for Earth Sciences, Indian Institute of Science, Bangalore, 560012, India |
推荐引用方式 GB/T 7714 | Paul J.,Ghosh A.. Evolution of cratons through the ages: A time-dependent study[J],2020,531. |
APA | Paul J.,&Ghosh A..(2020).Evolution of cratons through the ages: A time-dependent study.Earth and Planetary Science Letters,531. |
MLA | Paul J.,et al."Evolution of cratons through the ages: A time-dependent study".Earth and Planetary Science Letters 531(2020). |
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