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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ANGEO</journal-id>
<journal-title-group>
<journal-title>Annales Geophysicae</journal-title>
<abbrev-journal-title abbrev-type="publisher">ANGEO</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Ann. Geophys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1432-0576</issn>
<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/angeo-21-2323-2003</article-id>
<title-group>
<article-title>Study of mid-latitude nighttime enhancement in F-region electron density using tomographic images over the UK</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dabas</surname>
<given-names>R. S.</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>Kersley</surname>
<given-names>L.</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Radio and Atmospheric Sciences Division, National Physical Laboratory, New Delhi-110012, India</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Department of Physics, University of Wales, Aberystwyth, SY23, 3BZ, UK</addr-line>
</aff>
<pub-date pub-type="epub">
<day>31</day>
<month>12</month>
<year>2003</year>
</pub-date>
<volume>21</volume>
<issue>12</issue>
<fpage>2323</fpage>
<lpage>2328</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2003 R. S. Dabas</copyright-statement>
<copyright-year>2003</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/3.0/">https://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://angeo.copernicus.org/articles/21/2323/2003/angeo-21-2323-2003.html">This article is available from https://angeo.copernicus.org/articles/21/2323/2003/angeo-21-2323-2003.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/21/2323/2003/angeo-21-2323-2003.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/21/2323/2003/angeo-21-2323-2003.pdf</self-uri>
<abstract>
<p>Nighttime enhancements in ionospheric electron content (IEC)/peak
 electron density &lt;i&gt;(Nm&lt;/i&gt;F2) have been studied by various workers in the
 equatorial anomaly and mid-latitude regions. Such studies give an idea about
 their enhancement over that location only. In the present study tomographic
 images over the UK, which give a latitudinal versus height distributions of
 ionospheric electron density in a much wider area, have been used to study the
 anomalous increases in nighttime F-region electron density at mid-latitudes.
 From the analysis of four seasonal representative months (November 1997, March,
 June and October 1998) data it was noted that the majority of the cases of
 nighttime enhancements were observed after local midnight, with a maximum
 between 03:00–04:00 LT in the month of November 1997. Enhancements were
 observed mostly between 45–50° N latitudes, and their positions are not
 affected by magnetic activity (&lt;i&gt;K&lt;sub&gt;p &lt;/sub&gt;&lt;/i&gt;) variations, whereas the
 separation between the mid-latitude trough and enhancement decreases with
 increases in magnetic activity. This finding shows that only the trough moves
 equatorward with the increase in magnetic activity. It is also noted that the
 electron density gradient from the trough to the enhancement increases with an
 increase in &lt;i&gt;K&lt;sub&gt;p&lt;/sub&gt;&lt;/i&gt;. Results are discussed in terms of downward plasma
 transport from the protonosphere to the ionosphere and the nighttime neutral
 winds.&lt;br&gt;&lt;br&gt;&lt;b&gt;Key words. &lt;/b&gt;Ionosphere (mid-latitude
 ionosphere; modeling and forecasting; instruments and techniques)</p>
</abstract>
<counts><page-count count="6"/></counts>
</article-meta>
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