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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-2026-5205</article-id>
<title-group>
<article-title>Are drivers of northern lights in the ionosphere?</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Saka</surname>
<given-names>Osuke</given-names>
<ext-link>https://orcid.org/0000-0002-8382-7825</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Office Geophysik, Ogoori, 838-0141, Japan</addr-line>
</aff>
<pub-date pub-type="epub">
<day>30</day>
<month>09</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>18</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Osuke Saka</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-2026-5205/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5205/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5205/egusphere-2026-5205.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-5205/egusphere-2026-5205.pdf</self-uri>
<abstract>
<p>Within the first minute of Pi2 onset, macro-scale free vortices -characterized by two-cell, irrotational vortical flows- are excited in the midnight sector of the inner magnetosphere. This state persists for approximately 10 minutes. Rather than serving as a direct source of field-aligned current, these free vortex perturbations excite guided poloidal waves. As these waves transmit to the ionosphere, they create localized space charges. To maintain quasi-neutrality, ionosphere responds by generating parallel potential drops and outflows. These parallel potential drops subsequently produce a forced vortex that propagates down to the polar ionosphere. Within this forced vortex, electron fluids composed of primary and secondary electrons (which manifest as the aurora) undergo ExB drifts. Ultimately, the primary driver for the generation of these parallel potential drops resides within the polar ionosphere itself.</p>
</abstract>
<counts><page-count count="18"/></counts>
</article-meta>
</front>
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