TY - JOUR
T1 - Linking lowermost mantle structure, core-mantle boundary heat flux and mantle plume formation
AU - Li, Mingming
AU - Zhong, Shijie
AU - Olson, Peter
N1 - Funding Information:
We would like to acknowledge high performance computing support from Yellowstone (ark:/85065/d7wd3xhc) provided by NCAR's Computational and Information Systems Laboratory, sponsored by the National Science Foundation. We thank Takashi Nakagawa and two anonymous reviewers for their constructive comments. This work is supported by National Science Foundation through Grants 1135382 and 1645245.
Funding Information:
We would like to acknowledge high performance computing support from Yellowstone (ark:/85065/d7wd3xhc) provided by NCAR ’s Computational and Information Systems Laboratory, sponsored by the National Science Foundation. We thank Takashi Nakagawa and two anonymous reviewers for their constructive comments. This work is supported by National Science Foundation through Grants 1135382 and 1645245 .
Publisher Copyright:
© 2018 Elsevier B.V.
PY - 2018/4
Y1 - 2018/4
N2 - The dynamics of Earth's lowermost mantle exert significant control on the formation of mantle plumes and the core-mantle boundary (CMB) heat flux. However, it is not clear if and how the variation of CMB heat flux and mantle plume activity are related. Here, we perform geodynamic model experiments that show how temporal variations in CMB heat flux and pulses of mantle plumes are related to morphologic changes of the thermochemical piles of large-scale compositional heterogeneities in Earth's lowermost mantle, represented by the large low shear velocity provinces (LLSVPs). We find good correlation between the morphologic changes of the thermochemical piles and the time variation of CMB heat flux. The morphology of the thermochemical piles is significantly altered during the initiation and ascent of strong mantle plumes, and the changes in pile morphology cause variations in the local and the total CMB heat flux. Our modeling results indicate that plume-induced episodic variations of CMB heat flux link geomagnetic superchrons to pulses of surface volcanism, although the relative timing of these two phenomena remains problematic. We also find that the density distribution in thermochemical piles is heterogeneous, and that the piles are denser on average than the surrounding mantle when both thermal and chemical effects are included.
AB - The dynamics of Earth's lowermost mantle exert significant control on the formation of mantle plumes and the core-mantle boundary (CMB) heat flux. However, it is not clear if and how the variation of CMB heat flux and mantle plume activity are related. Here, we perform geodynamic model experiments that show how temporal variations in CMB heat flux and pulses of mantle plumes are related to morphologic changes of the thermochemical piles of large-scale compositional heterogeneities in Earth's lowermost mantle, represented by the large low shear velocity provinces (LLSVPs). We find good correlation between the morphologic changes of the thermochemical piles and the time variation of CMB heat flux. The morphology of the thermochemical piles is significantly altered during the initiation and ascent of strong mantle plumes, and the changes in pile morphology cause variations in the local and the total CMB heat flux. Our modeling results indicate that plume-induced episodic variations of CMB heat flux link geomagnetic superchrons to pulses of surface volcanism, although the relative timing of these two phenomena remains problematic. We also find that the density distribution in thermochemical piles is heterogeneous, and that the piles are denser on average than the surrounding mantle when both thermal and chemical effects are included.
KW - CMB heat flux
KW - Geomagnetic superchrons
KW - Large igneous provinces
KW - Mantle plume
KW - Thermochemical piles
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U2 - 10.1016/j.pepi.2018.01.010
DO - 10.1016/j.pepi.2018.01.010
M3 - Article
AN - SCOPUS:85044649981
SN - 0031-9201
VL - 277
SP - 10
EP - 29
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
ER -