<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:contributor>T. Lay</dc:contributor>
  <dc:contributor>Justin Revenaugh</dc:contributor>
  <dc:contributor>E.J. Garnero</dc:contributor>
  <dc:creator>Alexander R. Hutko</dc:creator>
  <dc:date>2008</dc:date>
  <dc:description>Earth's lowermost mantle has thermal, chemical, and mineralogical complexities that require precise seismological characterization. Stacking, migration, and modeling of over 10,000 P and S waves that traverse the deep mantle under the Cocos plate resolve structures above the core-mantle boundary. A small -0.07 ?? 0.15% decrease of P wave velocity (Vp) is accompanied by a 1.5 ?? 0.5% increase in S wave velocity (Vs) near a depth of 2570 km. Bulk-sound velocity [Vb = (V p2 - 4/3Vs2)1/2] decreases by -1.0 ?? 0.5% at this depth. Transition of the primary lower-mantle mineral, (Mg1-x-y FexAly)(Si,Al) O3 perovskite, to denser post-perovskite is expected to have a negligible effect on the bulk modulus while increasing the shear modulus by ???6%, resulting in local anticorrelation of Vb and Vs anomalies; this behavior explains the data well.</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1126/science.1155822</dc:identifier>
  <dc:language>en</dc:language>
  <dc:title>Anticorrelated seismic velocity anomalies from post-perovskite in the lowermost mantle</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>