日本地球惑星科学連合2016年大会

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インターナショナルセッション(口頭発表)

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT08] Structure and Dynamics of Suboceanic Mantle

2016年5月24日(火) 13:45 〜 15:15 201A (2F)

コンビーナ:*是永 淳(イェール大学地球科学科)、川勝 均(東京大学地震研究所)、Gaherty James(Lamont Doherty Earth Observatory)、馬場 聖至(東京大学地震研究所)、座長:川勝 均(東京大学地震研究所)、Gaherty James(Lamont Doherty Earth Observatory)

13:45 〜 14:00

[SIT08-01] Toward the reconciliation of seismological and petrological perspectives on oceanic lithosphere heterogeneity

★招待講演

*Kennett Brian2古村 孝志1 (1.東京大学地震研究所、2.オーストラリア国立大学地球科学研究所)

キーワード:Oceanic Mantle, Heterogeneity, Scattering of seismic wave, Po/So phases

The character of the high-frequency seismic phases Po and So, observed after propagation for long distances in the oceanic lithosphere, requires the presence of scattering from complex structure in 3-D. Current models use stochastic representations of seismic structure in the oceanic lithosphere. The observations are compatible with quasi-laminate features with horizontal correlation length around 10 km and vertical correlation length 0.5 km, with a uniform level of about 2% variation through the full thickness of the lithosphere. Such structures are difficult to explain with petrological models, which would favor stronger heterogeneity at the base of the lithosphere associated with underplating from frozen melts. Petrological evidence mostly points to smaller-scale features than suggested by seismology. The models from the different fields have been derived independently, with various levels of simplification. Fortunately, it is possible to gently modify the seismological model toward stronger basal heterogeneity, but there remains a need for some quasi-laminate structure throughout the mantle component of the oceanic lithosphere. The new models help to bridge the gulf between the different viewpoints, but ambiguities remain.