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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-25-1721-2007</article-id>
<title-group>
<article-title>Anomalous behavior of cutoff rigidity variation in the region of the Mexico station during a magnetic superstorm on 20 November 2003</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pchelkin</surname>
<given-names>V. V.</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>Pchelkina</surname>
<given-names>E. V.</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>Golovchanskaya</surname>
<given-names>I. V.</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Polar Geophysical Institute RAS, Fersman Str. 14, Apatity, Murmansk region, 184200, Russia</addr-line>
</aff>
<pub-date pub-type="epub">
<day>29</day>
<month>08</month>
<year>2007</year>
</pub-date>
<volume>25</volume>
<issue>8</issue>
<fpage>1721</fpage>
<lpage>1725</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2007 V. V. Pchelkin et al.</copyright-statement>
<copyright-year>2007</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/25/1721/2007/angeo-25-1721-2007.html">This article is available from https://angeo.copernicus.org/articles/25/1721/2007/angeo-25-1721-2007.html</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/articles/25/1721/2007/angeo-25-1721-2007.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/articles/25/1721/2007/angeo-25-1721-2007.pdf</self-uri>
<abstract>
<p>The pioneering storm-time model of magnetospheric magnetic field T01S made
possible trajectory calculations for the events of giant magnetic storms. We
have performed such calculations for a unique magnetic storm on 20 November
2003. In our previous paper, Belov et al. (2005), dedicated to the
magnetospheric effects of cosmic rays (CR) during this storm, we revealed an
anomalous behavior of a cutoff rigidity variation at the Mexico station. Here,
by trajectory calculations, we demonstrate that this peculiarity persists in
the latitudinal and longitudinal curves of cutoff rigidity (Rc) for both
quiet and storm-time conditions and thus should be considered as physically
meaningful.</p>
</abstract>
<counts><page-count count="5"/></counts>
</article-meta>
</front>
<body/>
<back>
<ref-list>
<title>References</title>
<ref id="ref1">
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</back>
</article>