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    <responseDate>2026-10-14T13:20:47Z</responseDate>
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    <identifier>10.57760/sciencedb.space.03111</identifier>
    <datestamp>2026-02-28T13:44:00Z</datestamp>
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<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" 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:date>2026-02-28</dc:date>
  <dc:title>Evolution of Three-Dimensional Interplanetary CMEs under Three Different Polar Magnetic Field Strengths</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.space.03111</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>The polar magnetic field can have an impact on the evolution of CMEs. We changed three different polar magnetic field strengths to study their effects on the evolution of CMEs in interplanetary space. Case 1 corresponds to the original polar magnetic map, case 2 corresponds to enhancing the polar magnetic field by 3G, and case 3 corresponds to enhancing the polar magnetic field by 6G.&amp;nbsp;</dc:description>
  <dc:subject>Solar coronal mass ejections; Solar polar magnetic field; Magnetohydrodynamic numerical simulation</dc:subject>
  <dc:creator>zhang xiao</dc:creator>
  <dc:creator>Yang Liping</dc:creator>
  <dc:creator>Feng Xueshang</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
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