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    <identifier>10.57760/sciencedb.space.01652</identifier>
    <datestamp>2024-01-26T15:02:44Z</datestamp>
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  <dc:date>2024-01-26</dc:date>
  <dc:title>Modeling energetic particle transport in a corotating intercation region</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.space.01652</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>An energetic particle event related to a corotating interaction region (CIR) structure was observed by the Solar-Terrestrial Relations Observatory-A (STEREO-A) from 21 to 24 August 2016. We developed a coupled model composed of a data-driven analytical background model providing solar wind configuration and a particle transport model represented by the focused transport equation (FTE). We simulated particle transport in the CIR region of interest in order to obtain the evolution of proton fluxes and derive the spectra.</dc:description>
  <dc:subject>Simulation ; Solar Wind; particle</dc:subject>
  <dc:creator>Xinyi Tao</dc:creator>
  <dc:creator>Fang Shen</dc:creator>
  <dc:creator>Wenwen Wei</dc:creator>
  <dc:creator>Yuji Zhu</dc:creator>
  <dc:creator>Xi Luo</dc:creator>
  <dc:creator>Xushang Feng</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/publicdomain/zero/1.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
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