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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">71169</article-id>
   <article-id pub-id-type="doi">10.12737/stp-101202403</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">Transfer of auroral kilometric radiation through low-density channels at the boundary of plasmasphere</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Transfer of auroral kilometric radiation through low-density channels at the boundary of plasmasphere</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Колпак</surname>
       <given-names>Валерия Игоревна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Kolpak</surname>
       <given-names>Valeria Igorevna</given-names>
      </name>
     </name-alternatives>
     <email>lera.kolpak@yandex.ru</email>
     <xref ref-type="aff" rid="aff-1"/>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Могилевский</surname>
       <given-names>Михаил Менделевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Mogilevsky</surname>
       <given-names>Michael Mendelevich</given-names>
      </name>
     </name-alternatives>
     <email>mogilevsky2012@gmail.com</email>
     <bio xml:lang="ru">
      <p>кандидат физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>candidate of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-3"/>
    </contrib>
    <contrib contrib-type="author">
     <contrib-id contrib-id-type="orcid">https://orcid.org/0000-0002-5809-0921</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Чугунин</surname>
       <given-names>Дмитрий Владимирович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Chugunin</surname>
       <given-names>Dmitriy Vladimirovich</given-names>
      </name>
     </name-alternatives>
     <email>dimokch@mail.ru</email>
     <xref ref-type="aff" rid="aff-4"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Чернышов</surname>
       <given-names>Александр Александрович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Chernyshov</surname>
       <given-names>Aleksandr Aleksandrovich</given-names>
      </name>
     </name-alternatives>
     <email>achernyshov@iki.rssi.ru</email>
     <xref ref-type="aff" rid="aff-5"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Моисеенко</surname>
       <given-names>Ирина Леонидовна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Moiseenko</surname>
       <given-names>Irina Leonidovna</given-names>
      </name>
     </name-alternatives>
     <email>moiseenko.irine@gmail.com</email>
     <xref ref-type="aff" rid="aff-6"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт космических исследований РАН</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Space Research Institute of RAS</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Национальный исследовательский университет «Высшая школа экономики»</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">National Research University “Higher School of Economics”</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Институт космических исследований РАН</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Space Research Institute of RAS</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-4">
    <aff>
     <institution xml:lang="ru">Институт космических исследований РАН</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Space Research Institute of RAS</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-5">
    <aff>
     <institution xml:lang="ru">Институт космических исследований РАН</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Space Research Institute of RAS</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-6">
    <aff>
     <institution xml:lang="ru">Институт космических исследований РАН</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Space Research Institute of RAS</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2024-03-26T18:03:15+03:00">
    <day>26</day>
    <month>03</month>
    <year>2024</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2024-03-26T18:03:15+03:00">
    <day>26</day>
    <month>03</month>
    <year>2024</year>
   </pub-date>
   <volume>10</volume>
   <issue>1</issue>
   <fpage>19</fpage>
   <lpage>28</lpage>
   <history>
    <date date-type="received" iso-8601-date="2023-10-11T00:00:00+03:00">
     <day>11</day>
     <month>10</month>
     <year>2023</year>
    </date>
    <date date-type="accepted" iso-8601-date="2023-12-28T00:00:00+03:00">
     <day>28</day>
     <month>12</month>
     <year>2023</year>
    </date>
   </history>
   <self-uri xlink:href="https://zh-szf.ru/en/nauka/article/71169/view">https://zh-szf.ru/en/nauka/article/71169/view</self-uri>
   <abstract xml:lang="ru">
    <p>We present the results of Auroral Kilometric Radiation (AKR) measurements near the plasmapause on the ERG (Arase) satellite. The apogee of the satellite's orbit is located near the ecliptic plane, at latitudes ±30°. According to the generally accepted point of view, AKR observation is impossible in this region since it is shielded by the plasmasphere. Simultaneous measurements of AKR and local plasma density made it possible to determine that AKR in near-equatorial regions occur in plasma channels — density inhomogeneities elongated along magnetic field lines. AKR from sources located in the auroral magnetosphere is transferred by these channels to the equatorial region. This work analyzes the conditions for the capture and propagation of AKR in low plasma density channels. In the geometrical optics approximation, we have simulated the conditions for the radiation capture and propagation. The calculation results show that the proposed scheme for AKR capture into plasma channels can explain the measurement results — the radiation transfer from the auroral region to the near-equatorial region.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>We present the results of Auroral Kilometric Radiation (AKR) measurements near the plasmapause on the ERG (Arase) satellite. The apogee of the satellite's orbit is located near the ecliptic plane, at latitudes ±30°. According to the generally accepted point of view, AKR observation is impossible in this region since it is shielded by the plasmasphere. Simultaneous measurements of AKR and local plasma density made it possible to determine that AKR in near-equatorial regions occur in plasma channels — density inhomogeneities elongated along magnetic field lines. AKR from sources located in the auroral magnetosphere is transferred by these channels to the equatorial region. This work analyzes the conditions for the capture and propagation of AKR in low plasma density channels. In the geometrical optics approximation, we have simulated the conditions for the radiation capture and propagation. The calculation results show that the proposed scheme for AKR capture into plasma channels can explain the measurement results — the radiation transfer from the auroral region to the near-equatorial region.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>auroral kilometric radiation</kwd>
    <kwd>radiation capture into the channel</kwd>
    <kwd>plasma inhomogeneities</kwd>
    <kwd>artificial Earth satellite</kwd>
    <kwd>space experiment</kwd>
    <kwd>upper hybrid resonance frequency</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>auroral kilometric radiation</kwd>
    <kwd>radiation capture into the channel</kwd>
    <kwd>plasma inhomogeneities</kwd>
    <kwd>artificial Earth satellite</kwd>
    <kwd>space experiment</kwd>
    <kwd>upper hybrid resonance frequency</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">The work of V.I. Kolpak and A.A. Chernyshov was financially supported by the Foundation for the Development of Theoretical Physics and Mathematics “BASIS”</funding-statement>
    <funding-statement xml:lang="en">The work of V.I. Kolpak and A.A. Chernyshov was financially supported by the Foundation for the Development of Theoretical Physics and Mathematics “BASIS”</funding-statement>
   </funding-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
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