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<front>
<journal-meta>
<journal-id journal-id-type="publisher">ANGEOD</journal-id>
<journal-title-group>
<journal-title>Annales Geophysicae Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ANGEOD</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Ann. Geophys. Discuss.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">2568-6402</issn>
<publisher><publisher-name></publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>
<article-meta>
<article-id pub-id-type="doi">10.5194/angeo-2019-155</article-id>
<title-group>
<article-title>Geomagnetic pulsations in the Pc5/Pi3 frequency range and fluctuations of foF2 frequency</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yagova</surname>
<given-names>Nadezda</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>Kozlovsky</surname>
<given-names>Alexander</given-names>
<ext-link>https://orcid.org/0000-0003-1468-7600</ext-link>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Fedorov</surname>
<given-names>Evgeny</given-names>
<ext-link>https://orcid.org/0000-0001-5516-3155</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Kozyreva</surname>
<given-names>Olga</given-names>
<ext-link>https://orcid.org/0000-0003-0825-151X</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Schmidt Institute of Physics of the Earth, Moscow, Russia</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Sodankylä Geophysical Observatory, Sodankylä, Finland</addr-line>
</aff>
<funding-group>
<award-group id="gs1">
<funding-source></funding-source>
<award-id>298578 and  310348</award-id>
</award-group>
</funding-group>
<pub-date pub-type="epub">
<day>03</day>
<month>12</month>
<year>2019</year>
</pub-date>
<volume>2019</volume>
<fpage>1</fpage>
<lpage>36</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2019 Nadezda Yagova et al.</copyright-statement>
<copyright-year>2019</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://angeo.copernicus.org/preprints/angeo-2019-155/">This article is available from https://angeo.copernicus.org/preprints/angeo-2019-155/</self-uri>
<self-uri xlink:href="https://angeo.copernicus.org/preprints/angeo-2019-155/angeo-2019-155.pdf">The full text article is available as a PDF file from https://angeo.copernicus.org/preprints/angeo-2019-155/angeo-2019-155.pdf</self-uri>
<abstract>
<p>&lt;p&gt;Using data of the ionosonde in Sodankyla, (SOD, 67&amp;deg;&amp;thinsp;N, 27&amp;deg;&amp;thinsp;E, Finland), parameters of 
variations of foF2 critical
frequency in the Pc5/Pi3 (1&amp;ndash;5&amp;thinsp;mHz) frequency range are studied.
For that, a technique of automatic detection of critical frequency
from an ionogram is developed. The variations of foF2  are
compared with the Pc5/Pi3 geomagnetic pulsations on the ground and
in the magnetosphere. The variations of foF2 are in the majority
of cases decoupled from the Pc5/Pi3 on the ground. Meanwhile, the
analysis of geomagnetic and foF2 variations at SOD show intervals
with noticeable coherence for both horizontal components. These
coherent pulsations are predominantly registered in the afternoon
MLT sector. Statistically, their spectral content, polarization
and spatial distribution differs from those of background
variations. Coherent pulsation tend to occur under moderate
geomagnetic and auroral activity, SW speed, and dynamic pressure
fluctuations. The fraction of coherent geomagnetic and foF2
pulsations is higher for the geomagnetic pulsations registered in
the magnetosphere, than on the ground.&lt;/p&gt;</p>
</abstract>
<counts><page-count count="36"/></counts>
</article-meta>
</front>
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