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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">71777</article-id>
   <article-id pub-id-type="doi">10.12737/szf-101202405</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">Intensity of the neutron component of cosmic rays and air humidity</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Интенсивность нейтронной компоненты космических лучей и влажность воздуха</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>Калюжная</surname>
       <given-names>Марина Анатольевна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Kalyuzhnaya</surname>
       <given-names>Marina Anatolyevna</given-names>
      </name>
     </name-alternatives>
     <email>kalyuzhnayama@ipgg.sbras.ru</email>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Хисамов</surname>
       <given-names>Рашит Замалтдинович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Khisamov</surname>
       <given-names>Rashit Zamaltdinovich</given-names>
      </name>
     </name-alternatives>
     <email>khisamovrz@ipgg.sbras.ru</email>
     <xref ref-type="aff" rid="aff-3"/>
    </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">A.A. Trofimuk Institute of Oil and Gas Geology and Geophysics SB RAS</institution>
     <city>Novosibirsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <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>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2024-03-26T18:02:29+03:00">
    <day>26</day>
    <month>03</month>
    <year>2024</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2024-03-26T18:02:29+03:00">
    <day>26</day>
    <month>03</month>
    <year>2024</year>
   </pub-date>
   <volume>10</volume>
   <issue>1</issue>
   <fpage>37</fpage>
   <lpage>43</lpage>
   <history>
    <date date-type="received" iso-8601-date="2023-11-22T00:00:00+03:00">
     <day>22</day>
     <month>11</month>
     <year>2023</year>
    </date>
    <date date-type="accepted" iso-8601-date="2024-01-26T00:00:00+03:00">
     <day>26</day>
     <month>01</month>
     <year>2024</year>
    </date>
   </history>
   <self-uri xlink:href="https://zh-szf.ru/en/nauka/article/71777/view">https://zh-szf.ru/en/nauka/article/71777/view</self-uri>
   <abstract xml:lang="ru">
    <p>В настоящее время коррекция данных нейтронных мониторов осуществляется только на барометрический эффект. Однако нельзя исключать также воздействие изменений влажности воздуха на интенсивность нейтронной компоненты космических лучей (КЛ), регистрируемой нейтронными мониторами. В связи с этим были выполнены непрерывные измерения влажности и температуры воздуха при наблюдениях за вариациями интенсивности КЛ с помощью нейтронного монитора в Новосибирске. Анализ результатов наблюдений метеорологических параметров и интенсивности КЛ в Новосибирске, а также данных мировой сети нейтронных мониторов позволил выявить вариации интенсивности нейтронной компоненты, вызванные изменениями влажности воздуха. Сделанные оценки эффекта влажности свидетельствуют о необходимости его регулярного учета в данных нейтронного монитора. Для этого наряду с измерениями атмосферного давления следует проводить регулярные измерения влажности и температуры воздуха.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>Neutron monitor data is currently corrected only for the barometric effect. We cannot, however, exclude that changes in air humidity affect the intensity of the cosmic-ray neutron component recorded by neutron monitors. In this regard, we have carried out continuous measurements of air humidity and temperature when observing variations in the cosmic ray intensity with a neutron monitor in Novosibirsk. Analysis of the results of observations of meteorological parameters and cosmic ray intensity in Novosibirsk, as well as data from the global network of neutron monitors, made it possible to identify neutron component intensity variations caused by changes in air humidity. The estimated humidity effect indicates the need to regularly take it into account in the neutron monitor data. To do this, along with atmospheric pressure, regular measurements of humidity and air temperature should be performed.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>космические лучи</kwd>
    <kwd>атмосфера</kwd>
    <kwd>нейтроны</kwd>
    <kwd>монитор</kwd>
    <kwd>влажность воздуха</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>cosmic rays</kwd>
    <kwd>atmosphere</kwd>
    <kwd>neutrons</kwd>
    <kwd>monitor</kwd>
    <kwd>air humidity</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">Работа выполнена при финансовой поддержке Минобрнауки РФ (проект FWZZ-2022-0019)</funding-statement>
    <funding-statement xml:lang="en">The work was financially supported by the Ministry of Science and Higher Education of the Russian Federation (Project FWZZ-2022-0019)</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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