Sound velocity and density of magnesiowüstites: Implications for ultralow‐velocity zone topography

  • June K. Wicks
    Division of Geological and Planetary Sciences California Institute of Technology Pasadena California USA
  • Jennifer M. Jackson
    Division of Geological and Planetary Sciences California Institute of Technology Pasadena California USA
  • Wolfgang Sturhahn
    Division of Geological and Planetary Sciences California Institute of Technology Pasadena California USA
  • Dongzhou Zhang
    Division of Geological and Planetary Sciences California Institute of Technology Pasadena California USA

書誌事項

公開日
2017-03-04
権利情報
  • http://onlinelibrary.wiley.com/termsAndConditions#vor
DOI
  • 10.1002/2016gl071225
公開者
American Geophysical Union (AGU)

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説明

<jats:title>Abstract</jats:title><jats:p>We explore the effect of Mg/Fe substitution on the sound velocities of iron‐rich (Mg<jats:sub>1 − <jats:italic>x</jats:italic></jats:sub>Fe<jats:sub><jats:italic>x</jats:italic></jats:sub>)O, where <jats:italic>x</jats:italic> = 0.84, 0.94, and 1.0. Sound velocities were determined using nuclear resonance inelastic X‐ray scattering as a function of pressure, approaching those of the lowermost mantle. The systematics of cation substitution in the Fe‐rich limit has the potential to play an important role in the interpretation of seismic observations of the core‐mantle boundary. By determining a relationship between sound velocity, density, and composition of (Mg,Fe)O, this study explores the potential constraints on ultralow‐velocity zones at the core‐mantle boundary.</jats:p>

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