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    <responseDate>2026-10-14T23:38:40Z</responseDate>
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    <identifier>10.57760/sciencedb.space.00328</identifier>
    <datestamp>2026-09-29T11:19:05Z</datestamp>
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  <dc:date>2026-09-29</dc:date>
  <dc:title>The Deep Learning&amp;ndash;based Dual-branch Multimodal Fusion Model for Solar Flare  Prediction</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.space.00328</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>The dataset is associated with solar flare forecasting research. It includes SDO/HMI SHARP active-region magnetograms, the corresponding magnetic-field parameters, a supplemented solar flare catalog, and solar flare forecasting labels.The Magnetogram data include active-region magnetograms in the cylindrical equal-area (CEA) projection, recorded from May 2010 to May 2023 at a cadence of 96 minutes.The Flare-catalog was constructed from the NOAA/NCEI GOES X-ray Flare Catalog. For flare events without associated NOAA active-region numbers, the corresponding NOAA active-region numbers were supplemented using the SolarSoft event archive and corresponding SDO observations.The Flare label file was generated from the Flare-catalog using a predefined 24-hour forecasting window. Samples are labeled as flare or non-flare according to whether a C-class or stronger flare occurs within the subsequent 24 hours. For multiclass forecasting, flare samples are further categorized as C-, M-, or X-class according to the highest flare class within the forecasting window.</dc:description>
  <dc:subject>Solar flare; Solar activity; Solar forecasting; Deep learning</dc:subject>
  <dc:creator>Limin Zhao</dc:creator>
  <dc:creator>Xingyao Chen</dc:creator>
  <dc:creator>Xiaoshuai Zhu</dc:creator>
  <dc:creator>Dong Zhao</dc:creator>
  <dc:creator>Yihua Yan</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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