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    <identifier>10.57760/sciencedb.25466</identifier>
    <datestamp>2025-05-23T10:11:09Z</datestamp>
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  <dc:date>2025-05-23</dc:date>
  <dc:title>The inversion ionosphere parameters based on the automatic model for tweek atmospherics (Zhang et al., 2023) recorded by the VLF sensor in Duke Forest during January to April, 2010.</dc:title>
  <dc:identifier>doi:10.57760/sciencedb.25466</dc:identifier>
  <dc:language>en</dc:language>
  <dc:description>48395 1st-order tweeks in total, the variables are:dt, Occurrence time for each tweek signal h, Reflection height of the tweek signal (Unit: [km])Ne, The electron density at the reflection height (Unit: [cm-3])D, Horizontal propagation distance of the tweek signal (Unit: [km])pos, The source lightning location [latitude, longitude](Note: to trace the source lightning, the NLDN lists are used to compare the lightning stroke time and the start time of the tweek signals)Reference:Zhang, M., Lu, G. P., Huang, H. L., Cheng, Z. W., Chen, Y. Z., Cummer, S. A., Zheng, J. Y., and Lei, J. H. (2023). Automatic recognition of tweek atmospherics and plasma diagnostics in the lower ionosphere with the machine learning method. Earth Planet. Phys., 7(3), 1&amp;ndash;7. http://doi.org/10.26464/epp2023039</dc:description>
  <dc:subject>tweek atmospherics; nighttime lower ionosphere; electron density</dc:subject>
  <dc:creator>Mao Zhang</dc:creator>
  <dc:creator>Gaopeng Lu</dc:creator>
  <dc:rights>PUBLIC</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by-nc/4.0/</dc:rights>
  <dc:type>dataset</dc:type>
  <dc:publisher>Science Data Bank</dc:publisher>
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