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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">20781</article-id>
   <article-id pub-id-type="doi">10.12737/szf-43201810</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">Atmospheric effects of the cosmic-ray mu-meson component</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Атмосферные эффекты мюонной компоненты космических лучей</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Янчуковский</surname>
       <given-names>Валерий Леонидович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Yanchukovsky</surname>
       <given-names>Valery Leonidovich</given-names>
      </name>
     </name-alternatives>
     <email>vjanch@gs.nsc.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 contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Кузьменко</surname>
       <given-names>Василий Сергеевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Kuzmenko</surname>
       <given-names>Vasiliy Sergeevich</given-names>
      </name>
     </name-alternatives>
     <email>mp3.87@mail.ru</email>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт нефтегазовой геологии и геофизики им. А.А. Трофимука СО РАН</institution>
     <city>Новосибирск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Trofimuk Institute of Petroleum Geology and Geophysics SB RAS</institution>
     <city>Novosibirsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Институт нефтегазовой геологии и геофизики им. А.А. Трофимука СО РАН</institution>
     <city>Новосибирск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Trofimuk Institute of Petroleum Geology and Geophysics SB RAS</institution>
     <city>Novosibirsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <volume>4</volume>
   <issue>3</issue>
   <fpage>95</fpage>
   <lpage>102</lpage>
   <self-uri xlink:href="https://zh-szf.ru/en/nauka/article/20781/view">https://zh-szf.ru/en/nauka/article/20781/view</self-uri>
   <abstract xml:lang="ru">
    <p>Вариации интенсивности космических лучей, наблюдаемые в глубине атмосферы, включают атмосферную составляющую вариаций. Мюонные телескопы космических лучей наряду с барометрическим обладают значительным температурным эффектом, обусловленным нестабильностью регистрируемых частиц. Для учета в данных мюонных телескопов атмосферных эффектов по экспериментальным данным с использованием различных методов факторного анализа найдены метеорологические коэффициенты интенсивности регистрируемых в глубине атмосферы мюонов. Полученные по экспериментальным данным результаты сопоставлены с результатами теоретических расчетов.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>Variations in the intensity of cosmic rays observed in the depth of the atmosphere include the atmospheric component of the variations. Cosmic-ray muon telescopes, along with the barometric effect, have a significant temperature effect due to the instability of detected particles. To take into account atmospheric effects in muon telescope data, meteorological coeffi-cients of muon intensity are found. The meteorological coefficients of the intensity of muons recorded in the depth of the atmosphere are estimated from experi-mental data, using various methods of factor analysis. The results obtained from experimental data are com-pared with the results of theoretical calculations.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>космические лучи</kwd>
    <kwd>мюоны</kwd>
    <kwd>температура</kwd>
    <kwd>атмосфера</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>cosmic rays</kwd>
    <kwd>muons</kwd>
    <kwd>temperature</kwd>
    <kwd>atmosphere</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
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