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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Russian Journal of Earth Sciences</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Russian Journal of Earth Sciences</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Russian Journal of Earth Sciences</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">1681-1208</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">47004</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>ORIGINAL ARTICLES</subject>
    </subj-group>
    <subj-group>
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">From the geophysical to heliophysical year: The results of the CORONAS-F project</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>From the geophysical to heliophysical year: The results of the CORONAS-F project</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Kuznetsov</surname>
       <given-names>V D</given-names>
      </name>
      <name xml:lang="en">
       <surname>Kuznetsov</surname>
       <given-names>V D</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Pushkov Institute of the Earth Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences IZMIRAN, Troitsk, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Pushkov Institute of the Earth Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences IZMIRAN, Troitsk, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <volume>9</volume>
   <issue>3</issue>
   <fpage>1</fpage>
   <lpage>14</lpage>
   <history>
    <date date-type="received" iso-8601-date="2021-11-10T19:21:13+03:00">
     <day>10</day>
     <month>11</month>
     <year>2021</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/47004/view">https://rjes.ru/en/nauka/article/47004/view</self-uri>
   <abstract xml:lang="ru">
    <p>The main and most significant results of the CORONAS-F space project are presented. In the scope of this project observations of solar activity and its impact on the Earth were carried out from July 2001 to December 2005. The remote observation devices studied the localization and morphology of solar activity in the second half of the 23rd solar cycle. High-temperature plasma formations are found and studied in the solar corona, eruptive phenomena, processes of particle acceleration, and atomic and nuclear processes in solar flares are investigated. The devices of the &quot;Solar Cosmic Ray'' complex studied manifestations of solar activity in the near-Earth environment, dynamics of the radiation belts of the Earth, and rebuilding of the magnetosphere structure in the periods of magnetic storms caused by active events on the Sun. Results related to the upper atmosphere of the Earth and helioseismology are also presented.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The main and most significant results of the CORONAS-F space project are presented. In the scope of this project observations of solar activity and its impact on the Earth were carried out from July 2001 to December 2005. The remote observation devices studied the localization and morphology of solar activity in the second half of the 23rd solar cycle. High-temperature plasma formations are found and studied in the solar corona, eruptive phenomena, processes of particle acceleration, and atomic and nuclear processes in solar flares are investigated. The devices of the &quot;Solar Cosmic Ray'' complex studied manifestations of solar activity in the near-Earth environment, dynamics of the radiation belts of the Earth, and rebuilding of the magnetosphere structure in the periods of magnetic storms caused by active events on the Sun. Results related to the upper atmosphere of the Earth and helioseismology are also presented.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>heliophysical year</kwd>
    <kwd>CORONAS-F project</kwd>
    <kwd>near-Earth environment</kwd>
    <kwd>helioseismology.</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>heliophysical year</kwd>
    <kwd>CORONAS-F project</kwd>
    <kwd>near-Earth environment</kwd>
    <kwd>helioseismology.</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
 <back>
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</article>
