Based on a self-consistent thermodynamic-geophysical approach and xenolith-based constraints, we map the 2-D seismic, thermal and density structure of the mantle beneath the Siberian craton along the long-range profiles (Craton, Kimberlite, Rift and Meteorite) carried out in Russia with peaceful nuclear explosions. Structural peculiarities of the cratonic mantle are manifested by changes in seismic velocities, the degree and nature of layering and the relief of seismic boundaries. The results predict appreciable lateral temperature variations within the root to a depth of about 200 km, which are the main cause of seismic velocity variations. We find that the cratonic mantle is 300-400 degrees C colder than the tectonically younger surrounding mantle in this depth range. At greater depths, lateral changes in temperatures have little effect implying that thermal heterogeneity rapidly decreases. The present-day geotherms pass close to the 32.5-35 mW m(-2) conductive models and suggest low mantle heat flow. Within the model resolution, the thickness of the thermal boundary layer, TBL (defined as the depth of the 1300 degrees C adiabat) beneath Siberia does not depend significantly on the composition and can be estimated as 300 +/- 30 km; temperature at the base of the TBL is close to the 1450 +/- 100 degrees C isotherm. Changes in the composition from depleted to fertile material reveal a negligible effect on seismic velocities, which are practically unresolved by seismic methods, but remain the most important factor for the density increase of the cratonic root Density variations in the lower part of the root due to the chemical composition are greater than those caused by temperature. We find that both compositional and thermal anomalies are required to explain the Siberian mantle by a keel model consisting of depleted garnet peridotite at depths of 100 to 180 km and more fertile material at greater depths. (C) 2014 Elsevier B.V. All rights reserved.
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Tokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Akashi, Akihiko
Nishihara, Yu
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Tokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Tokyo Inst Technol, Res Ctr Evolving Earth & Planets, Tokyo 1528551, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Nishihara, Yu
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Takahashi, Eiichi
Nakajima, Yoichi
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Tokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Nakajima, Yoichi
Tange, Yoshinori
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Ehime Univ, Geodynam Res Ctr, Matsuyama, Ehime 7908577, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Tange, Yoshinori
Funakoshi, Ken-ichi
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Japan Synchrotron Radiat Res Inst, Hyogo 6795198, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
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Tokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Akashi, Akihiko
Nishihara, Yu
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h-index: 0
机构:
Tokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Tokyo Inst Technol, Res Ctr Evolving Earth & Planets, Tokyo 1528551, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Nishihara, Yu
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Takahashi, Eiichi
Nakajima, Yoichi
论文数: 0引用数: 0
h-index: 0
机构:
Tokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Nakajima, Yoichi
Tange, Yoshinori
论文数: 0引用数: 0
h-index: 0
机构:
Ehime Univ, Geodynam Res Ctr, Matsuyama, Ehime 7908577, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan
Tange, Yoshinori
Funakoshi, Ken-ichi
论文数: 0引用数: 0
h-index: 0
机构:
Japan Synchrotron Radiat Res Inst, Hyogo 6795198, JapanTokyo Inst Technol, Dept Earth & Planetary Sci, Tokyo 1528551, Japan