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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">100194</article-id>
   <article-id pub-id-type="doi">10.12737/stp-112202506</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">Studying the radial structure of the poloidal Alfvén resonator by the method of phase portraits from Van Allen Probes satellite data</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Studying the radial structure of the poloidal Alfvén resonator by the method of phase portraits from Van Allen Probes satellite data</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Власов</surname>
       <given-names>Александр Александрович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Vlasov</surname>
       <given-names>Aleksandr Aleksandrovich</given-names>
      </name>
     </name-alternatives>
     <email>a.vlasov@iszf.irk.ru</email>
     <xref ref-type="aff" rid="aff-1"/>
    </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>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2025-06-26T16:59:55+03:00">
    <day>26</day>
    <month>06</month>
    <year>2025</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2025-06-26T16:59:55+03:00">
    <day>26</day>
    <month>06</month>
    <year>2025</year>
   </pub-date>
   <volume>11</volume>
   <issue>2</issue>
   <fpage>60</fpage>
   <lpage>68</lpage>
   <history>
    <date date-type="received" iso-8601-date="2024-11-25T00:00:00+03:00">
     <day>25</day>
     <month>11</month>
     <year>2024</year>
    </date>
    <date date-type="accepted" iso-8601-date="2025-03-24T00:00:00+03:00">
     <day>24</day>
     <month>03</month>
     <year>2025</year>
    </date>
   </history>
   <self-uri xlink:href="https://zh-szf.ru/en/nauka/article/100194/view">https://zh-szf.ru/en/nauka/article/100194/view</self-uri>
   <abstract xml:lang="ru">
    <p>In the paper, we examine the spatial structure of eigenharmonics of the poloidal Alfvén resonator recorded by the RBSP-B satellite on 23 October 2012 at 19:12–20:24 UT. We employ the method of phase portraits, which is a set of plots of magnetic/electric field components of oscillations as well as the phase shift between transverse components, to interpret the data. Based on the theoretical description of magnetospheric MHD waves, an analytical solution for eigenharmonics of the poloidal Alfvén resonator is framed. The phase shift of individual harmonics of the observed oscillations is shown to have a quasi-periodic structure, which allows us to confirm that they have resonator modes, and the magnetic field components analytically calculated along the satellite trajectory qualitatively coincide with the satellite data. From comparison of theoretical calculations of the structure of transverse magnetic field components with observational data, we put forward an assumption that the second and fourth harmonics of the poloidal resonator make the main contribution to the observed oscillations.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>In the paper, we examine the spatial structure of eigenharmonics of the poloidal Alfvén resonator recorded by the RBSP-B satellite on 23 October 2012 at 19:12–20:24 UT. We employ the method of phase portraits, which is a set of plots of magnetic/electric field components of oscillations as well as the phase shift between transverse components, to interpret the data. Based on the theoretical description of magnetospheric MHD waves, an analytical solution for eigenharmonics of the poloidal Alfvén resonator is framed. The phase shift of individual harmonics of the observed oscillations is shown to have a quasi-periodic structure, which allows us to confirm that they have resonator modes, and the magnetic field components analytically calculated along the satellite trajectory qualitatively coincide with the satellite data. From comparison of theoretical calculations of the structure of transverse magnetic field components with observational data, we put forward an assumption that the second and fourth harmonics of the poloidal resonator make the main contribution to the observed oscillations.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>Alfvén waves</kwd>
    <kwd>poloidal resonator</kwd>
    <kwd>ULF waves</kwd>
    <kwd>satellite observations</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>Alfvén waves</kwd>
    <kwd>poloidal resonator</kwd>
    <kwd>ULF waves</kwd>
    <kwd>satellite observations</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">The work was financially supported by RSF (Grant No. 22-77-10032)</funding-statement>
    <funding-statement xml:lang="en">The work was financially supported by RSF (Grant No. 22-77-10032)</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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  <p></p>
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