DEFORMATION OF (MG0.9,FE0.1)SIO3 PEROVSKITE AGGREGATES UP TO 32 GPA

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dc.contributor.author Merkel S.
dc.contributor.author Wenk H.R.
dc.contributor.author Badro J.
dc.contributor.author Montagnac G.
dc.contributor.author Gillet P.
dc.contributor.author Mao H.K.
dc.contributor.author Hemley R.J.
dc.date.accessioned 2021-12-24T05:12:38Z
dc.date.available 2021-12-24T05:12:38Z
dc.date.issued 2003
dc.identifier https://www.elibrary.ru/item.asp?id=1472099
dc.identifier.citation Earth and Planetary Science Letters, 2003, 209, 3-4, 351-360
dc.identifier.issn 0012-821X
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/33794
dc.description.abstract Room temperature investigations on the shear stress and deformation mechanisms of (Mg0.9Fe0.1)SiO3 perovskite are performed in situ up to 32 GPa using radial X-ray diffraction and the diamond anvil cell as a deformation apparatus. The uniaxial stress supported by the perovskite aggregate is found to increase continuously with pressure up to 10.9(+/-1.9) GPa at 32(+/-1) GPa. Our measurements show no development of significant lattice preferred orientations in the sample, which indicates that deformation by dislocation glide is not the dominant deformation mechanism under these conditions. Assuming that the underlying cause for seismic anisotropy in the deep Earth is elastic anisotropy combined with lattice preferred orientation, our results indicate that silicate perovskite deformed under the conditions of this experiment would not be the source of seismic anisotropy.
dc.subject HIGH PRESSURE
dc.subject DEFORMATION
dc.subject PEROVSKITE
dc.subject SHEAR STRENGTH
dc.subject TEXTURE
dc.subject ANISOTROPY
dc.title DEFORMATION OF (MG0.9,FE0.1)SIO3 PEROVSKITE AGGREGATES UP TO 32 GPA
dc.type Статья


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