Diffusion Coefficients in Olivine, Wadsleyite and Ringwoodite

Abstract

Research Article| January 01, 2010 Diffusion Coefficients in Olivine, Wadsleyite and Ringwoodite Sumit Chakraborty Sumit Chakraborty Institut für Geologie, Mineralogie und Geophysik, Ruhr-Universität Bochum, Universitätsstraße 150, D-44780 Bochum, Germany, sumit.chakraborty@ruhr-uni-bochum.de Search for other works by this author on: GSW Google Scholar Reviews in Mineralogy and Geochemistry (2010) 72 (1): 603–639. https://doi.org/10.2138/rmg.2010.72.13 Article history first online: 09 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation Sumit Chakraborty; Diffusion Coefficients in Olivine, Wadsleyite and Ringwoodite. Reviews in Mineralogy and Geochemistry 2010;; 72 (1): 603–639. doi: https://doi.org/10.2138/rmg.2010.72.13 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyReviews in Mineralogy and Geochemistry Search Advanced Search (Fe,Mg)2SiO4 occurs in the polymorphic forms of olivine (orthorhombic), wadsleyite (orthorhombic) and ringwoodite (cubic). These are some of the most common minerals in the inner solar system. Olivine occurs in the mantles of the Earth, the Moon and Mars, in meteorites, in plutonic and volcanic igneous rocks as well as in some metamorphic rocks. The high pressure polymorphs wadsleyite and ringwoodite have been reported from shocked meteorites. Diffusion coefficients of different elements in these phases have been widely used in several areas of the Earth, planetary and materials-sciences (see below for examples). The relative simplicity of structure... You do not have access to this content, please speak to your institutional administrator if you feel you should have access.