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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Solar-Terrestrial Physics</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Solar-Terrestrial Physics</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Solar-Terrestrial Physics</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">2500-0535</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">39951</article-id>
   <article-id pub-id-type="doi">10.12737/stp-72202108</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>Results of current research</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>Results of current research</subject>
    </subj-group>
    <subj-group>
     <subject>Results of current research</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">Signs of anomalous behavior of the ionosphere in 2003–2014 at F1-layer heights over Irkutsk</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Signs of anomalous behavior of the ionosphere in 2003–2014 at F1-layer heights over Irkutsk</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Кушнаренко</surname>
       <given-names>Галина Петровна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Kushnarenko</surname>
       <given-names>Galina Petrovna</given-names>
      </name>
     </name-alternatives>
     <email>kusch@iszf.irk.ru</email>
     <bio xml:lang="ru">
      <p>кандидат физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>candidate of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Яковлева</surname>
       <given-names>Ольга Евгеньевна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Yakovleva</surname>
       <given-names>Olga Evgenyevna</given-names>
      </name>
     </name-alternatives>
     <email>yakovleva@iszf.ru</email>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Кузнецова</surname>
       <given-names>Галина Михайловна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Kuznetsova</surname>
       <given-names>Galina Mihaylovna</given-names>
      </name>
     </name-alternatives>
     <email>kuz@iszf.irk.ru</email>
     <xref ref-type="aff" rid="aff-3"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт солнечно-земной физики СО РАН</institution>
     <city>Иркутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Solar Terrestrial Physics SB RAS</institution>
     <city>Irkutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Институт солнечно-земной физики СО РАН</institution>
     <city>Иркутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Solar Terrestrial Physics SB RAS</institution>
     <city>Irkutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Институт солнечно-земной физики СО РАН</institution>
     <city>Иркутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Solar Terrestrial Physics SB RAS</institution>
     <city>Irkutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <volume>7</volume>
   <issue>2</issue>
   <fpage>74</fpage>
   <lpage>80</lpage>
   <history>
    <date date-type="received" iso-8601-date="2020-10-19T00:00:00+03:00">
     <day>19</day>
     <month>10</month>
     <year>2020</year>
    </date>
    <date date-type="accepted" iso-8601-date="2021-05-17T00:00:00+03:00">
     <day>17</day>
     <month>05</month>
     <year>2021</year>
    </date>
   </history>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/39951/view">https://naukaru.ru/en/nauka/article/39951/view</self-uri>
   <abstract xml:lang="ru">
    <p>We have detected an anomalous electron density Ne increase in winter months in Irkutsk in some years of the period 2003–2014. This effect was manifested when we compared the experimental values obtained by the Irkutsk ionosonde with model calculations at F1-layer heights (120–200 km). Two anomalous time zones have been found. The first was observed in the period 2003–2006 near solar minimum. In this zone, 2003 is the year of maximum manifestation of the winter Ne increase over the entire research period. The second anomalous zone — 2012, 2013, 2014 — was detected during solar maximum. We have explored possible causes of the Ne change in winter at the F1-layer heights in all the years under study. We have found that the main factor causing the winter increase in Ne is significant geomagnetic disturbances in the above time periods.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>We have detected an anomalous electron density Ne increase in winter months in Irkutsk in some years of the period 2003–2014. This effect was manifested when we compared the experimental values obtained by the Irkutsk ionosonde with model calculations at F1-layer heights (120–200 km). Two anomalous time zones have been found. The first was observed in the period 2003–2006 near solar minimum. In this zone, 2003 is the year of maximum manifestation of the winter Ne increase over the entire research period. The second anomalous zone — 2012, 2013, 2014 — was detected during solar maximum. We have explored possible causes of the Ne change in winter at the F1-layer heights in all the years under study. We have found that the main factor causing the winter increase in Ne is significant geomagnetic disturbances in the above time periods.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>electron density</kwd>
    <kwd>winter increase in Ne</kwd>
    <kwd>geomagnetic activity</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>electron density</kwd>
    <kwd>winter increase in Ne</kwd>
    <kwd>geomagnetic activity</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">The work was financially supported by the Ministry of Science and Higher Education of the Russian Federation (project &quot;Study of the State and Dynamics of Earth's Atmosphere at Different Time Scales under the Influence of Geophysical, Cosmic, and Human Impacts&quot;)</funding-statement>
    <funding-statement xml:lang="en">The work was financially supported by the Ministry of Science and Higher Education of the Russian Federation (project &quot;Study of the State and Dynamics of Earth's Atmosphere at Different Time Scales under the Influence of Geophysical, Cosmic, and Human Impacts&quot;)</funding-statement>
   </funding-group>
  </article-meta>
 </front>
 <body>
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