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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">46654</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">The effects of galactic cosmic rays, modulated by solar terrestrial magnetic fields, on the climate</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>The effects of galactic cosmic rays, modulated by solar terrestrial magnetic fields, on the climate</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Dergachev</surname>
       <given-names>V A</given-names>
      </name>
      <name xml:lang="en">
       <surname>Dergachev</surname>
       <given-names>V A</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Dmitriev</surname>
       <given-names>P B</given-names>
      </name>
      <name xml:lang="en">
       <surname>Dmitriev</surname>
       <given-names>P B</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Raspopov</surname>
       <given-names>O M</given-names>
      </name>
      <name xml:lang="en">
       <surname>Raspopov</surname>
       <given-names>O M</given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-3"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Van Geel</surname>
       <given-names>B </given-names>
      </name>
      <name xml:lang="en">
       <surname>Van Geel</surname>
       <given-names>B </given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-4"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Ioffe Physico-Technical Institute, Russian Academy of Science, Sankt-Petersburg, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Ioffe Physico-Technical Institute, Russian Academy of Science, Sankt-Petersburg, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Ioffe Physico-Technical Institute, Russian Academy of Science, Sankt-Petersburg, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Ioffe Physico-Technical Institute, Russian Academy of Science, Sankt-Petersburg, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Sankt-Petersburg Branch of the Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Science, Sankt-Petersburg, Russia</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Sankt-Petersburg Branch of the Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Science, Sankt-Petersburg, Russia</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-4">
    <aff>
     <institution xml:lang="ru">Amsterdam University, Holland</institution>
     <country>ru</country>
    </aff>
    <aff>
     <institution xml:lang="en">Amsterdam University, Holland</institution>
     <country>ru</country>
    </aff>
   </aff-alternatives>
   <volume>6</volume>
   <issue>5</issue>
   <fpage>323</fpage>
   <lpage>338</lpage>
   <history>
    <date date-type="received" iso-8601-date="2021-10-29T13:09:48+03:00">
     <day>29</day>
     <month>10</month>
     <year>2021</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/46654/view">https://rjes.ru/en/nauka/article/46654/view</self-uri>
   <abstract xml:lang="ru">
    <p>The results of analyzing the paleodata on solar activity variations (variations of cosmogenic 14 C and 10 Be isotopes in the terrestrial records, such as glaciers, tree rings, sea-floor marine and lacustrine sediments, loess, etc.), the paleomagnetic and archeomagnetic data, as well as the paleoclimatic data, prove that the flows of galactic cosmic rays, modulated by heliomagnetic and geomagnetic fields, affect the climate of the Earth. In this study we analyzed different periods of time, namely, the last millennium, the Holocene epoch (up to 10-12 thousand years ago), and the time interval of 10-50 thousand years ago. Our analysis suggested that the variations of the cosmic ray fluxes seemed to be the most effective factor responsible for long-term climate variations.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The results of analyzing the paleodata on solar activity variations (variations of cosmogenic 14 C and 10 Be isotopes in the terrestrial records, such as glaciers, tree rings, sea-floor marine and lacustrine sediments, loess, etc.), the paleomagnetic and archeomagnetic data, as well as the paleoclimatic data, prove that the flows of galactic cosmic rays, modulated by heliomagnetic and geomagnetic fields, affect the climate of the Earth. In this study we analyzed different periods of time, namely, the last millennium, the Holocene epoch (up to 10-12 thousand years ago), and the time interval of 10-50 thousand years ago. Our analysis suggested that the variations of the cosmic ray fluxes seemed to be the most effective factor responsible for long-term climate variations.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>cosmic rays</kwd>
    <kwd>solar and geomagnetic variations</kwd>
    <kwd>climate changes</kwd>
    <kwd>cosmogenic and stable nuclides.</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>cosmic rays</kwd>
    <kwd>solar and geomagnetic variations</kwd>
    <kwd>climate changes</kwd>
    <kwd>cosmogenic and stable nuclides.</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
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