<?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>Joseph Meert</dc:contributor>
  <dc:contributor>Anthony Francis Pivarunas</dc:contributor>
  <dc:contributor>Anup K. Sinha</dc:contributor>
  <dc:contributor>Manoj K. Pandit</dc:contributor>
  <dc:contributor>Paul A. Mueller</dc:contributor>
  <dc:contributor>George Kamenov</dc:contributor>
  <dc:creator>Scott R Miller</dc:creator>
  <dc:date>2023</dc:date>
  <dc:description>&lt;div id="ab010" class="abstract author"&gt;&lt;div id="as010"&gt;&lt;p id="sp0010"&gt;&lt;span&gt;Coupled paleomagnetic and geochronologic data derived from mafic dykes provide valuable records of continental movement. To reconstruct the Proterozoic paleogeographic history of Peninsular India, we report paleomagnetic directions and U-Pb&amp;nbsp;zircon&amp;nbsp;ages from twenty-nine mafic dykes in the Eastern Dharwar Craton near Hyderabad. Paleomagnetic analysis yielded clusters of directional data that correspond to&amp;nbsp;dyke swarms&amp;nbsp;at 2.37&amp;nbsp;Ga, 2.22&amp;nbsp;Ga, 2.08&amp;nbsp;Ga, 1.89–1.86&amp;nbsp;Ga, 1.79&amp;nbsp;Ga, and a previously undated dual polarity magnetization. We report new positive baked contact tests for the 2.08&amp;nbsp;Ga swarm and the 1.89–1.86&amp;nbsp;Ga swarm(s), and a new inverse baked contact test for the 2.08&amp;nbsp;Ga swarm. Our results promote the 2.08&amp;nbsp;Ga Dharwar Craton paleomagnetic pole (43.1° N, 184.5° E; A95&amp;nbsp;=&amp;nbsp;4.3°) to a reliability score of&amp;nbsp;&lt;/span&gt;&lt;i&gt;R&lt;/i&gt;&lt;span&gt;&amp;nbsp;=&amp;nbsp;7 and suggest a position for the Dharwar Craton at 1.79&amp;nbsp;Ga based on a&amp;nbsp;virtual geomagnetic pole&amp;nbsp;(VGP) at 33.0° N, 347.5° E (a95&amp;nbsp;=&amp;nbsp;16.9°,&amp;nbsp;&lt;/span&gt;&lt;i&gt;k&lt;/i&gt;&amp;nbsp;=&amp;nbsp;221,&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;i&gt;N&lt;/i&gt;&amp;nbsp;=&amp;nbsp;2). The new VGP for the Dharwar Craton provides support for the union of the Dharwar, Singhbhum, and Bastar Cratons in the Southern India Block by at least 1.79&amp;nbsp;Ga. Combined new and published northeast-southwest moderate-steep dual polarity directions from Dharwar Craton dykes define a new paleomagnetic pole at 20.6° N, 233.1° E (A95&amp;nbsp;=&amp;nbsp;9.2°,&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;i&gt;N&lt;/i&gt;&amp;nbsp;=&amp;nbsp;18;&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;i&gt;R&lt;/i&gt;&amp;nbsp;=&amp;nbsp;5). Two dykes from this group yielded 1.05–1.01&amp;nbsp;Ga&lt;span&gt;&amp;nbsp;&lt;/span&gt;&lt;sup&gt;207&lt;/sup&gt;Pb/&lt;sup&gt;206&lt;/sup&gt;Pb zircon ages and this range is taken as the age of the new paleomagnetic pole. A comparison of the previously published poles with our new 1.05–1.01&amp;nbsp;Ga pole shows India shifting from equatorial to higher (southerly) latitudes from 1.08 Ga to 1.01&amp;nbsp;Ga as a component of Rodinia.&lt;/p&gt;&lt;/div&gt;&lt;/div&gt;</dc:description>
  <dc:format>application/pdf</dc:format>
  <dc:identifier>10.1016/j.gsf.2023.101581</dc:identifier>
  <dc:language>en</dc:language>
  <dc:publisher>Elsevier</dc:publisher>
  <dc:title>The drift history of the Dharwar Craton and India from 2.37 Ga to 1.01 Ga with refinements for an initial Rodinia configuration</dc:title>
  <dc:type>article</dc:type>
</oai_dc:dc>