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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Solnechno-Zemnaya Fizika</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Solnechno-Zemnaya Fizika</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Солнечно-земная физика</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">2712-9640</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">100193</article-id>
   <article-id pub-id-type="doi">10.12737/szf-112202506</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>Результаты  исследований</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>Results of current research</subject>
    </subj-group>
    <subj-group>
     <subject>Результаты  исследований</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>Исследование радиальной структуры полоидального альфвеновского резонатора методом «фазовых портретов» по данным спутника Van Allen Probes</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="2025-06-26T00:00:00+03:00">
    <day>26</day>
    <month>06</month>
    <year>2025</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2025-06-26T00:00:00+03:00">
    <day>26</day>
    <month>06</month>
    <year>2025</year>
   </pub-date>
   <volume>11</volume>
   <issue>2</issue>
   <fpage>69</fpage>
   <lpage>78</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://naukaru.ru/en/nauka/article/100193/view">https://naukaru.ru/en/nauka/article/100193/view</self-uri>
   <abstract xml:lang="ru">
    <p>В работе исследована пространственная структура собственных гармоник полоидального альфвеновского резонатора, зарегистрированных спутником RBSP-B 23 октября 2012 г. в 19:12–20:24 UT. Для интерпретации данных использован метод фазовых портретов, представляющих собой совокупность графиков компонент магнитного/ электрического поля колебаний и разности фаз между поперечными компонентами. На основе теоретического описания магнитосферных МГД-волн построено аналитическое решение для собственных мод полоидального альфвеновского резонатора. Показано, что разности фаз отдельных монохроматических гармоник наблюдаемых колебаний имеют квазипериодическую структуру, что позволило подтвердить их резонаторную природу, а аналитически рассчитанные компоненты магнитного поля вдоль траектории движения спутника качественно совпадают с данными спутниковых наблюдений. На основе сопоставления теоретических расчетов структуры поперечных компонент магнитного поля с данными наблюдений выдвинуто предположение, что основной вклад в наблюдаемые колебания вносят вторая и четвертая собственные гармоники полоидального резонатора.</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>альфвеновские волны</kwd>
    <kwd>полоидальный резонатор</kwd>
    <kwd>УНЧ-волны</kwd>
    <kwd>спутниковые наблюдения</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">Работа была выполнена при поддержке гранта РНФ № 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>
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