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    <responseDate>2026-10-14T15:23:16Z</responseDate>
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    <identifier>10.57760/sciencedb.space.02978</identifier>
    <datestamp>2026-02-11T10:32:58Z</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>2026-02-11</dc:date>
  <dc:title>Solar Activity AI Forecaster Database</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.space.02978</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>SA-AI Forecaster Dataset Structure==================================Data used in SA-AI Forecaster modeling is stored in the &amp;quot;dataset&amp;quot; folder, which consists of four subfolders:&amp;nbsp;- &amp;quot;Observation_image&amp;quot;- &amp;quot;SPNet_data&amp;quot;- &amp;quot;IATools_data&amp;quot;- &amp;quot;FPNet_data&amp;quot;1. Observation_image--------------------Observational image data (JPG format) used in modeling, categorized into:&amp;bull; Magnetograms: Solar photospheric magnetic field observations&amp;nbsp;- SDO_HMI&amp;nbsp;- SOHO_MDI&amp;nbsp;- ASO-S_FMG&amp;bull; Coronal EUV images: Solar coronal atmospheric observations&amp;nbsp;- SDO_AIA&amp;nbsp;- SOHO_EIT&amp;nbsp;- GOES-16_SUVI&amp;nbsp;(Images of different wavelengths stored in separate subfolders)&amp;bull; H&amp;alpha;: Solar chromospheric H&amp;alpha; observations&amp;nbsp;- BBSO&amp;nbsp;- KSO&amp;nbsp;- HSOS2. SPNet_data-------------Files for SPNet module input/output:&amp;bull; Labeling_data: Manually annotated ground truth&amp;bull; output_data: Module recognition outputBoth contain three feature subfolders:&amp;nbsp;- AR (Active Region)&amp;nbsp;- CH (Coronal Hole)&amp;nbsp;- FL (Filament)3. IATools_data---------------TXT output from IATools module (Jan 2023 - May 2024):&amp;bull; AR_parameters: Active Region parameters&amp;nbsp;- Daily_flare_events: Identified/located flare events&amp;nbsp;- flare_index: Calculated flare indices&amp;nbsp;- parameters: Other AR parameters&amp;bull; CH_parameters: Coronal Hole parameters&amp;bull; FL_parameters: Filament parameters4. FPNet_data-------------Training/testing data for FPNet module:&amp;bull; F10.7_index: Daily solar radio flux observations&amp;bull; FPNet-independent_data: Data from SWPC daily reports&amp;nbsp;▪ flare_index: Flare indices (Formula 1)&amp;nbsp;▪ label_M_class: M-class+ flare labels (24hr forecast)&amp;nbsp;▪ mag_type: Mount Wilson magnetic classification&amp;nbsp;▪ AR_parameters: Active region parameters (R-value, location, etc.)&amp;bull; Output: The output of the FPNet and FPNet*&amp;nbsp;▪ Full-disk_FPNet-independent: Full-disk forecasting result of FPNet*&amp;nbsp;▪ AR_FPNet-independent: AR forecasting result of FPNet*&amp;nbsp;▪ Full-disk_FPNet: Full-disk forecasting result of FPNet&amp;nbsp;▪ AR_FPNet: AR forecasting result of FPNetThe data used in the SA-AI forecaster modeling process is stored in the dataset folder, which consists of four subfolders: &amp;quot;Observation_image&amp;quot;, &amp;quot;SPNet_data&amp;quot;, &amp;quot;IATools_data&amp;quot;, and &amp;quot;FPNet_data&amp;quot;.&amp;quot;Observation_image&amp;quot; contains observational image data in JPG format used for modeling, categorized into three types: &amp;quot;magnetograms&amp;quot;, &amp;quot;Coronal EUV images&amp;quot;, and &amp;quot;H&amp;alpha;&amp;quot;. The &amp;quot;magnetograms&amp;quot; subfolder stores solar photospheric magnetic field observation images from different sources: &amp;quot;SDO-HMI&amp;quot;, &amp;quot;SOHO-MDI&amp;quot;, and &amp;quot;ASO-S-FMG&amp;quot;. The &amp;quot;Coronal EUV images&amp;quot; subfolder contains solar coronal atmospheric observation images from various sources: &amp;quot;SDO-AIA&amp;quot;, &amp;quot;SOHO-EIT&amp;quot;, and &amp;quot;GOES-16-SUVI&amp;quot;, with images of different wavelengths stored in separate subfolders. The &amp;quot;H&amp;alpha;&amp;quot; subfolder preserves solar chromospheric H&amp;alpha; observation images from different institutions: &amp;quot;BBSO&amp;quot;, &amp;quot;KSO&amp;quot;, and &amp;quot;HSOS&amp;quot;.The &amp;quot;SPNet_data&amp;quot; folder contains input and output files for building the SPNet module, with two subfolders: manually annotated ground truth data &amp;quot;Labeling data&amp;quot; and module recognition output data &amp;quot;output_data&amp;quot;. Each subfolder is further divided into three feature-based subfolders: &amp;quot;AR&amp;quot;, &amp;quot;CH&amp;quot;, and &amp;quot;FL&amp;quot;.The &amp;quot;IATools_data&amp;quot; folder stores output data (TXT format) from the IATools module between January 2023 and May 2024. The &amp;quot;AR_parameters&amp;quot; subfolder contains three subfolders: daily identified and located flare events &amp;quot;Daily_flare_events&amp;quot;, flare indices calculated using formulas &amp;quot;flare_index&amp;quot;, and other AR parameters &amp;quot;parameters&amp;quot;. The &amp;quot;CH_parameters&amp;quot; and &amp;quot;FL_parameters&amp;quot; subfolders store CH and FL parameters respectively.The &amp;quot;FPNet_data&amp;quot; folder contains training and testing data for building the FPNet module. It includes &amp;quot;F10.7_index&amp;quot; (daily F10.7 index observation data required for modeling), &amp;quot;FPNet_data&amp;quot; (data obtained from daily reports provided by SWPC for building the flare prediction module FPNet), and &amp;quot;Output&amp;quot;(forecasting results of the FPNet and FPNet*). The &amp;quot;FPNet_data*&amp;quot; contains four subfolders: &amp;quot;flare_index&amp;quot; (flare indices calculated using formula 1 based on SWPC event list), &amp;quot;label_M_class&amp;quot; (M-class flare eruption labels for the next 24 hours derived from SWPC event lists), &amp;quot;mag_type&amp;quot; (AR Mount Wilson magnetic classifications obtained from SWPC solar active region summaries), and &amp;quot;AR_parameters&amp;quot; (AR parameters including R-values and locations, obtained from SWPC and manual annotations). The &amp;quot;Output&amp;quot; contains four files in .xlsx format, which are forecasting results of the FPNet and FPNet* on the full-disk and AR, respectively.</dc:description>
  <dc:subject>Solar activity; Large model; AI forecaster; Space weather; Artificial intelligence</dc:subject>
  <dc:creator>Jingjing Wang</dc:creator>
  <dc:creator>Pengyu Liang</dc:creator>
  <dc:creator>Tingyu Wang</dc:creator>
  <dc:creator>Ming Li</dc:creator>
  <dc:creator>Yanmei Cui</dc:creator>
  <dc:creator>Siwei Liu</dc:creator>
  <dc:creator>Xin Huang</dc:creator>
  <dc:creator>Yunshi Zeng</dc:creator>
  <dc:creator>Zhu Cao</dc:creator>
  <dc:creator>Xiang Li</dc:creator>
  <dc:creator>Jiekang Feng</dc:creator>
  <dc:creator>Minghui Zhang</dc:creator>
  <dc:creator>Qinghua Hu</dc:creator>
  <dc:creator>Bingxian Luo</dc:creator>
  <dc:creator>Bing Cao</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>
</oai_dc:dc>

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