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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">71117</article-id>
   <article-id pub-id-type="doi">10.2205/2024ES000903</article-id>
   <article-id pub-id-type="edn">ounmdd</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">Reversals and Large-Scale Variations of the Geomagnetic Field: Similarities and Differences</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Reversals and Large-Scale Variations of the Geomagnetic Field: Similarities and Differences</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-4909-6336</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Решетняк</surname>
       <given-names>Максим Юрьевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Reshetnyak</surname>
       <given-names>Maxim Yurievich</given-names>
      </name>
     </name-alternatives>
     <email>m.reshetnyak@gmail.com</email>
     <bio xml:lang="ru">
      <p>доктор физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>doctor of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт физики Земли им. О.Ю. Шмидта РАН</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Schmidt Institute of Physics of the Earth</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2024-04-22T00:00:00+03:00">
    <day>22</day>
    <month>04</month>
    <year>2024</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2024-04-22T00:00:00+03:00">
    <day>22</day>
    <month>04</month>
    <year>2024</year>
   </pub-date>
   <volume>24</volume>
   <issue>2</issue>
   <fpage>1</fpage>
   <lpage>8</lpage>
   <history>
    <date date-type="received" iso-8601-date="2023-10-20T00:00:00+03:00">
     <day>20</day>
     <month>10</month>
     <year>2023</year>
    </date>
    <date date-type="accepted" iso-8601-date="2023-12-29T00:00:00+03:00">
     <day>29</day>
     <month>12</month>
     <year>2023</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/71117/view">https://rjes.ru/en/nauka/article/71117/view</self-uri>
   <abstract xml:lang="ru">
    <p>It is shown that during reversals in geodynamo models the minimum amplitudes of the dipole, quadrupole and octupole coincide. Since the characteristic time of the reversal is close to the oscillations of the large-scale geomagnetic field, a similar analysis was carried out for the minima of the amplitude of the dipole magnetic field over the past 100 thousand years. It turned out that in this case such synchronization also occurs. It can be assumed that reversals and large scale variations of the geomagnetic field between the reversals have a lot in common. The wavelet analysis carried out indicates that the concept of the main geodynamo cycle is very arbitrary: the period of oscillation can vary from 8–10 thousand years to 20–30 thousand for a dipole. Analysis of the evolution of the Mauersberger spectrum allows us to conclude that magnetic field fluctuations observed at the Earth’s surface are associated with the transfer of the magnetic field to the surface of the liquid core and can hardly be described by functions periodic in time.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>It is shown that during reversals in geodynamo models the minimum amplitudes of the dipole, quadrupole and octupole coincide. Since the characteristic time of the reversal is close to the oscillations of the large-scale geomagnetic field, a similar analysis was carried out for the minima of the amplitude of the dipole magnetic field over the past 100 thousand years. It turned out that in this case such synchronization also occurs. It can be assumed that reversals and large scale variations of the geomagnetic field between the reversals have a lot in common. The wavelet analysis carried out indicates that the concept of the main geodynamo cycle is very arbitrary: the period of oscillation can vary from 8–10 thousand years to 20–30 thousand for a dipole. Analysis of the evolution of the Mauersberger spectrum allows us to conclude that magnetic field fluctuations observed at the Earth’s surface are associated with the transfer of the magnetic field to the surface of the liquid core and can hardly be described by functions periodic in time.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>geodynamo</kwd>
    <kwd>core-mantle boundary</kwd>
    <kwd>magnetic field modes synchronization</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>geodynamo</kwd>
    <kwd>core-mantle boundary</kwd>
    <kwd>magnetic field modes synchronization</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">The geodynamo modelling part of the work was supported by the Russian Science Foundation grant # 23-17-00112 and analysis of observational data was performed within the framework of a State Assignment of the Institute of Physics of the Earth of Russian Academy of Sciences.</funding-statement>
    <funding-statement xml:lang="en">The geodynamo modelling part of the work was supported by the Russian Science Foundation grant # 23-17-00112 and analysis of observational data was performed within the framework of a State Assignment of the Institute of Physics of the Earth of Russian Academy of Sciences.</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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