Superplumes, plates, and mantle magmatism in two‐dimensional numerical models
Superplumes, plates, and mantle magmatism in two‐dimensional numerical models
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DOI:
10.1029/2006jb004533
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发表时间:
2007-06
影响因子:
--
通讯作者:
Masaki Ogawa
中科院分区:
文献类型:
--
作者:
Masaki Ogawa
[1] Two-dimensional numerical models are systematically presented for magmatism in a convecting mantle internally heated by incompatible radioactive elements. Plate tectonics is self-consistently modeled as a part of convection of Newtonian fluid with temperature- and stress-history-dependent viscosity driven by thermal and compositional buoyancy, while magmatism is modeled as an upward migration of basaltic magma generated by decompression melting. Ridge magmatism actively takes place to chemically differentiate the mantle, and a superplume is well developed in the lowermost mantle as a broad hot region enriched in basaltic component, provided that the lithosphere is mechanically strong enough to inhibit spontaneous initiation of subduction by its own weight and that the internal heating rate is sufficiently high. Hot narrow plumes frequently rise up from the superplume to induce deep magma generation and hot spot magmatism, which in turn frequently induces new plate margins. The frequent plate margin formation keeps the activity of plate tectonics rather steady. The thermal and chemical state of the mantle remains rather steady, too. As the internal heating rate becomes lower, however, the narrow plumes from superplume become sporadic and significantly colder, deep magma generation becomes rare; and new plate margin formation becomes less frequent. As a consequence, the activity of plate tectonics and the thermal and chemical state of the mantle become fluctuating much with time. The mantle structure and plume behavior modeled here match with many observations for those of the Earth from the Archean to the present.