Stress regime analysis for the transition to a stagnant-lid convection regime in the terrestrial mantle

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Masaki Yoshida
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Abstract

A series of numerical simulations of terrestrial mantle convection with temperature-dependent viscosity in a three-dimensional spherical geometry was performed to investigate the thermal structure of the mantle interior and the mechanical condition of the lithosphere. The common “sluggish-lid” convection regime has the thermal structure of the mantle interior with a slowly mobile lid under a moderately temperature-dependent viscosity of mantle rocks, whereas the “stagnant-lid” convection regime has a convection pattern in which the entire surface is covered by a highly viscous lid due to the strongly temperature-dependent viscosity. This study focused not only on the thermal structure of the mantle but also on the mechanical conditions in the lithosphere on an intermediate, transitional convection regime between these end-member convections both under the standard- and the extended-Boussinesq approximations. In this “quasi-stagnant-lid” convection regime, the entire surface of the planet is covered by a highly viscous stagnant-lid that moves slowly, whereas the mantle interior is dominated by a long-wavelength (i.e., degree-one) thermal structure. The stress regime analyses revealed that the strike-slip regime is highly restricted spatially in the lid. If the constitutive laws allow the formation of faults in the future numerical model, the time-dependent formation of weak faults that can initiate plate tectonics may differ among the three convection regimes (i.e., degree-one, quasi-stagnant-lid, and stagnant-lid convection regimes). The range of viscosity contrast of the lid required to realize the “quasi-stagnant-lid” convection regime in the model under the extended-Boussinesq approximation was wider than under the standard Boussinesq approximation, because the adiabatic heating of the mantle increased the mantle temperature with the depth and enhanced the formation of stagnant-lid owing to the strong mechanical decoupling between the cold lid and the underlying hot mantle.

陆幔向滞盖对流过渡的应力状态分析
为了研究地幔内部的热结构和岩石圈的力学状况,在三维球面几何中进行了一系列具有温度依赖黏度的陆地地幔对流数值模拟。常见的“缓盖”对流是地幔内部的热结构,在地幔岩石的温度依赖粘度适中的情况下,地幔内部有一个缓慢移动的盖子,而“滞盖”对流是由于温度依赖粘度很强,整个表面被一个高粘性的盖子覆盖的对流模式。本文不仅研究了地幔的热结构,而且研究了在标准和扩展的boussinesq近似下这些端元对流之间的中间过渡对流状态下岩石圈的力学条件。在这种“准滞盖”对流状态下,行星的整个表面都被一个移动缓慢的高粘性滞盖覆盖,而地幔内部则被一个长波长(即一级)的热结构所主导。应力状态分析表明,井盖内走滑状态在空间上受到高度限制。如果本构律在未来的数值模型中允许断层的形成,那么可以引发板块构造的弱断层的时间依赖性形成可能在三种对流机制(即一级对流、准滞盖对流和滞盖对流)中有所不同。在扩展Boussinesq近似下,模型中实现“准滞盖”对流状态所需的地幔黏度对比范围比标准Boussinesq近似下更宽,这是由于地幔的绝热加热使地幔温度随深度升高,并且由于冷盖与下垫热地幔之间强烈的力学解耦,促进了滞盖的形成。
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来源期刊
Planetary and Space Science
Planetary and Space Science 地学天文-天文与天体物理
CiteScore
5.40
自引率
4.20%
发文量
126
审稿时长
15 weeks
期刊介绍: Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered: • Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics • Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system • Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating • Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements • Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation • Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites • Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind • Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations • Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets • History of planetary and space research
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