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      <dc:title>Mg K-edge XANES of sepiolite and palygorskite</dc:title>
      <dc:creator>Sánchez del Río, Manuel</dc:creator>
      <dc:creator>Súarez Barrios, Mercedes</dc:creator>
      <dc:creator>García Romero, Emilia</dc:creator>
      <dc:creator>Alianelli, Lucia</dc:creator>
      <dc:creator>Felici, Roberto</dc:creator>
      <dc:creator>Martinetto, Pauline</dc:creator>
      <dc:creator>Dooryhée, Eric</dc:creator>
      <dc:creator>Reyes Valerio, Constantino</dc:creator>
      <dc:creator>Borgatti, Francesco</dc:creator>
      <dc:creator>Doyle, Bryan</dc:creator>
      <dc:creator>Giglia, Angelo</dc:creator>
      <dc:creator>Mahne, Nicola</dc:creator>
      <dc:creator>Pedio, Maddalena</dc:creator>
      <dc:creator>Nannarone, Stefano</dc:creator>
      <dc:description>We present a study of the Mg K-edge on sepiolite and palygorskite performed at the INFM BEAR beamline at Elettra
synchrotron light source (Trieste). These two clays, although having very similar structures, show some different
features in their near-edge. Mg is in octahedral coordination with oxygens, hydroxyl groups or water, for both palygorskite
and sepiolite. The differences found in the near-edge seem to reflect the fact that, on average, an Mg atom
in palygorskite ‘‘sees’’ less Mg in higher coordination shells than sepiolite.</dc:description>
      <dc:date>2023-06-20T09:30:06Z</dc:date>
      <dc:date>2023-06-20T09:30:06Z</dc:date>
      <dc:date>2005</dc:date>
      <dc:type>journal article</dc:type>
      <dc:identifier>0168-583X</dc:identifier>
      <dc:identifier>10.1016/j.nimb.2005.06.018</dc:identifier>
      <dc:identifier>https://hdl.handle.net/20.500.14352/49739</dc:identifier>
      <dc:identifier>http://www.elsevier.com/locate/nimb</dc:identifier>
      <dc:language>eng</dc:language>
      <dc:rights>open access</dc:rights>
      <dc:publisher>Elsevier</dc:publisher>
   </ow:Publication>
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