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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">35377</article-id>
   <article-id pub-id-type="doi">10.12737/szf-63202011</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">Manifestation of solar activity and dynamics of the atmosphere in variations of 577.7 and 630.0 nm atmospheric emissions in solar cycle 24</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Проявление солнечной активности и динамики атмосферы в вариациях интенсивности эмиссий ночного неба 557.7 и 630.0 нм в 24-м солнечном цикле</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Михалев</surname>
       <given-names>Александр Васильевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Mikhalev</surname>
       <given-names>Aleksandr Vasilyevich</given-names>
      </name>
     </name-alternatives>
     <email>mikhalev@iszf.irk.ru</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 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>
   <volume>6</volume>
   <issue>3</issue>
   <fpage>99</fpage>
   <lpage>104</lpage>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/35377/view">https://naukaru.ru/en/nauka/article/35377/view</self-uri>
   <abstract xml:lang="ru">
    <p>В работе выполнен анализ вариаций интенсивности эмиссий атомарного кислорода [OI] 557.7 и 630 нм в 2011–2019 гг. Использовались данные наблюдений, полученные в Геофизической обсерватории ИСЗФ СО РАН. Интенсивности эмиссий сопоставлялись с атмосферными, солнечными и геофизическими параметрами. Получены высокие коэффициенты корреляции между среднемесячными и среднегодовыми значениями интенсивности эмиссии 630.0 нм и индексов солнечной активности F10.7, что указывает на определяющую роль солнечной активности в вариациях этой эмиссии в анализируемый период. В вариациях эмиссии 557.7 нм в большей степени проявляется корреляция с квазидвухлетними колебаниями зонального ветра в стратосфере (индекс QBO.U30). Обсуждаются причины слабой зависимости интенсивности эмиссии 557.7 нм от солнечной активности в текущем 24-м солнечном цикле.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>In the paper, variations of the night emission intensities in the 557.7 and 630 nm atomic oxygen lines [OI] in 2011–2019 have been analyzed. The analysis is based on data from the ISTP SB RAS Geophysical Observatory. The emission intensities are compared with atmospheric, solar, and geophysical parameters. High correlation coefficients between monthly average and annual average 630.0 nm emission intensities and solar activity indices F10.7 have been obtained. This suggests a key role of solar activity in variations of this emission in the period of interest. Variations of the 557.7 nm emission demonstrate to a greater extent the correlations of the stratospheric zonal wind (QBO.U30 index) with quasi-biennial oscillations. The causes of the weak dependence of the 557.7 nm emission intensity on solar activity in solar cycle 24 are discussed.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>верхняя атмосфера</kwd>
    <kwd>эмиссии 557.7 и 630.0 нм</kwd>
    <kwd>солнечная активность</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>upper atmosphere</kwd>
    <kwd>557.7 and 630.0 nm emissions</kwd>
    <kwd>solar activity</kwd>
   </kwd-group>
  </article-meta>
 </front>
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 </back>
</article>
