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      <ref-type name="Journal Article">17</ref-type>
      <work-type>ACL : Articles dans des revues avec comité de lecture répertoriées par l'AERES</work-type>
      <contributors>
        <authors>
          <author>
            <style face="normal" font="default" size="100%">Antonio, P. Y. J.</style>
          </author>
          <author>
            <style face="bold" font="default" size="100%">Baratoux, Lenka</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Trindade, R. I. F.</style>
          </author>
          <author>
            <style face="bold" font="default" size="100%">Rousse, Sonia</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Ayite, A.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Lana, C.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Macouin, M.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Adu, E. W. K.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Sanchez, C.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Silva, M. A. L.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Firmin, A. S.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Dopico, C. I. M.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Proietti, A.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Amponsah, P. O.</style>
          </author>
          <author>
            <style face="normal" font="default" size="100%">Sakyi, P. A.</style>
          </author>
        </authors>
      </contributors>
      <titles>
        <title>West Africa in Rodinia : high quality paleomagnetic pole from the similar to 860 Ma Manso dyke swarm (Ghana) [+ corrigendum, 2021, vol. 95, p. 10-13]</title>
        <secondary-title>Gondwana Research</secondary-title>
      </titles>
      <pages>28-43 [+ corrigendum, 2021, vol. 95,  10-13]</pages>
      <keywords>
        <keyword>West Africa</keyword>
        <keyword>Neoproterozoic</keyword>
        <keyword>Tonian</keyword>
        <keyword>Rodinia</keyword>
        <keyword>Paleomagnetism</keyword>
        <keyword>GHANA</keyword>
      </keywords>
      <dates>
        <year>2021</year>
      </dates>
      <call-num>fdi:010081291</call-num>
      <language>ENG</language>
      <periodical>
        <full-title>Gondwana Research</full-title>
      </periodical>
      <isbn>1342-937X</isbn>
      <accession-num>ISI:000643562600002</accession-num>
      <electronic-resource-num>10.1016/j.gr.2021.02.010</electronic-resource-num>
      <urls>
        <related-urls>
          <url>https://www.documentation.ird.fr/hor/fdi:010081291</url>
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          <url>https://www.documentation.ird.fr/intranet/publi/2021-05/010081291.pdf</url>
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      <volume>94</volume>
      <remote-database-provider>Horizon (IRD)</remote-database-provider>
      <abstract>The paleogeography of the Meso-Neoproterozoic Rodinia supercontinent remains debated partly because many stable cratons still lack reliable paleomagnetic data for this period. A new geochronological and paleomagnetic study was conducted on the NNW-trending Manso dyke swarm of southern West Africa (Ghana) to clarify the position of this unconstrained continent in Rodinia. Two U\\Pb apatite ages of 857.2 +/- 8.5 Ma and 855 +/- 16 Ma agree with one previous baddeleyite age, indicating a -860 Ma emplacement age for the Manso dykes. A characteristic remanent magnetization (ChRM) was isolated in stable single to pseudo-single domain (SD-PSD) magnetite. Well constrained site mean directions obtained for 13 dykes lead to a mean direction for the Manso dyke swarm of Dm = 181.9 degrees, Im = -77.2 degrees (N = 13, alpha 95 = 7.6 degrees, k = 30.6), yielding a paleomagnetic pole at 177.6 degrees E, 28.3 degrees S, (A95 = 12.7 degrees K = 11.6). Two directional clusters of opposite inclination passa reversal test (C-class) and the primary origin is supported by a positive baked contact test, satisfying all the seven R-criteria to provide the first West African Tonian key paleomagnetic pole. This key pole indicates a high latitude for the West Africa Craton during the emplacement of the-860 Manso dykes. A compilation of reliable paleomag-netic poles for West Africa, Baltica, Amazonia and Congo-S &amp; atilde;o Francisco cratons suggests that these cratons were together between-1200 and 800 Ma in a long-lived WABAMGO configuration. We suggest that the collision of this block with Laurentia along the Grenvillian-Sunsas orogens closed the external Nuna Ocean and formed Rodinia by extroversion.</abstract>
      <custom6>064 ; 066</custom6>
      <custom1>UR234</custom1>
      <custom7>Argentine / Brésil / Ghana</custom7>
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