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<front>
<journal-meta>
<journal-id journal-id-type="publisher">EGUsphere</journal-id>
<journal-title-group>
<journal-title>EGUsphere</journal-title>
<abbrev-journal-title abbrev-type="publisher">EGUsphere</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">EGUsphere</abbrev-journal-title>
</journal-title-group>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/egusphere-2026-6656</article-id>
<title-group>
<article-title>Afternoon and nighttime differences in IRI-2026 electron-content partitioning over Hainan</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wang</surname>
<given-names>Zheng</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Li</surname>
<given-names>Quanhan</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wang</surname>
<given-names>Zehao</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Li</surname>
<given-names>Qinzeng</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Zhu</surname>
<given-names>Yajun</given-names>
<ext-link>https://orcid.org/0000-0002-8884-0885</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wang</surname>
<given-names>Guojun</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Tian</surname>
<given-names>Yusen</given-names>
<ext-link>https://orcid.org/0000-0002-2246-0919</ext-link>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Wang</surname>
<given-names>Xiao</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>State Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>National Field Observation and Research Station (Hainan) for Space Weather, Hainan, China</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>National Key Laboratory of Scattering and Radiation, China Aerospace Science and Technology Corporation, 365 Zhayin Road, Yangpu District, Shanghai, China</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Beijing Key Laboratory of Space Environment Exploration, National Space Science Center, Chinese Academy of Sciences, Beijing, China</addr-line>
</aff>
<pub-date pub-type="epub">
<day>09</day>
<month>11</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>23</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Zheng Wang et al.</copyright-statement>
<copyright-year>2026</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6656/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6656/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6656/egusphere-2026-6656.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-6656/egusphere-2026-6656.pdf</self-uri>
<abstract>
<p>Does replacing the modeled bottomside with a locally observed profile improve total electron content (TEC) estimates? We examine this question at Hainan using 1,666 manually traced ionosonde profiles from 852 dates in 2015&lt;span&gt;&amp;ndash;&lt;/span&gt;2018 and the International Reference Ionosphere (IRI-2026). We replace the modeled profile below the F2 density peak with the traced bottomside, retain the modeled topside to 1000 km, and compare the original and combined columns with contemporaneous GNSS vertical TEC. Replacement increases overall mean absolute error from 5.064 to 5.898 TECU, but the two sampled local times respond differently. Error rises from 6.305 to 8.440 TECU in the afternoon and falls from 3.808 to 3.325 TECU after midnight. Under their respective integration limits, the modeled afternoon bottomside contains 4.338 TECU more than the traced bottomside on average. This extra lower-column content partly offsets the positive GNSS-minus-combined difference, making the original total closer to GNSS. The opposite responses persist when the two integrals meet at the observed peak height. At Hainan, closer agreement in total TEC can therefore conceal a substantial difference in the lower profile, and introducing that observed profile can expose the discrepancy. These Hainan results show that regional TEC updating needs to assess the upper contribution alongside the observed bottomside, particularly in the afternoon, while accounting for GNSS electron content above 1000 km.</p>
</abstract>
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<funding-group>
<award-group id="gs1">
<funding-source>National Key Research and Development Program of China</funding-source>
<award-id>2025YFF0510703</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Chinese Academy of Sciences</funding-source>
<award-id>XDA0470301</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Chinese Academy of Sciences</funding-source>
<award-id>2023000116</award-id>
</award-group>
</funding-group>
</article-meta>
</front>
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