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Core-mantle boundary topography as a possible constraint on lower mantle chemistry and dynamics
被引:49
作者:
Lassak, Teresa Mae
[1
]
McNamara, Allen K.
[1
]
Garnero, Edward J.
[1
]
Zhong, Shijie
[2
]
机构:
[1] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA
[2] Univ Colorado, Dept Phys, Boulder, CO 80309 USA
基金:
美国国家科学基金会;
关键词:
mantle convection;
core-mantle boundary;
CMB topography;
thermochemical piles;
plume clusters;
LATERAL VARIATIONS;
STOCHASTIC-ANALYSIS;
AFRICAN SUPERPLUME;
VELOCITY STRUCTURE;
MGSIO3;
PEROVSKITE;
CONVECTION;
SHEAR;
TOMOGRAPHY;
PCP;
PKP;
D O I:
10.1016/j.epsl.2009.11.012
中图分类号:
P3 [地球物理学];
P59 [地球化学];
学科分类号:
0708 ;
070902 ;
摘要:
The origin of large low shear-wave velocity provinces (LLSVPs) in the lowermost mantle beneath the central Pacific and Africa is not well constrained. We explore numerical convection calculations for two proposed hypotheses for these anomalies, namely, thermal upwellings (e.g., plume clusters) and large intrinsically dense piles of mantle material (e.g., thermochemical piles), each of which uniquely affects the topography on Earth's core-mantle boundary (CMB). The thermochemical pile models predict a relatively flat but elevated CMB beneath piles (presumed LLSVPs), with strong upwarping along LLSVP margins. The plume cluster models predict CMB upwarping beneath upwellings that are less geographically organized. Both models display CMB depressions beneath subduction related downwelling. While each of the two models produces a unique, characteristic style of CMB topography, we find that seismic models will require shorter length scales than are currently being employed in order to distinguish between the end-member dynamic models presented here. (C) 2009 Elsevier B.V. All rights reserved.
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页码:232 / 241
页数:10
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