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    <identifier>10.57760/sciencedb.space.00584</identifier>
    <datestamp>2023-07-27T09:41:24Z</datestamp>
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  <dc:date>2023-07-27</dc:date>
  <dc:title>Figure of &amp;ldquo;Numerical Study of Divergence Cleaning and Coronal Heating/Acceleration Methods in the 3D COIN-TVD MHD Model. &amp;rdquo;</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.space.00584</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>&amp;nbsp;In this paper, we focus on the three-dimensional (3D) coronal solar wind simulation by using the Coronal Interplanetary-Total Variation Diminishing (COIN-TVD) magnetohydrodynamic (MHD) model. The volume heating source terms are included in the MHD equations to simulate the heating and acceleration of solar wind in coronal region.</dc:description>
  <dc:subject>COIN-TVD; MHD; Corona; Heating and acceleration</dc:subject>
  <dc:creator>沈芳</dc:creator>
  <dc:rights>RESTRICTED</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:relation>http://www.doi.org/10.3389/fphy.2021.705744</dc:relation>
  <dc:publisher>Science Data Bank</dc:publisher>
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