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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">71778</article-id>
   <article-id pub-id-type="doi">10.12737/stp-101202405</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">Intensity of the neutron component of cosmic rays and air humidity</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Intensity of the neutron component of cosmic rays and air humidity</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="2024-03-26T18:03:15+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>34</fpage>
   <lpage>39</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/71778/view">https://zh-szf.ru/en/nauka/article/71778/view</self-uri>
   <abstract xml:lang="ru">
    <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>
   </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>cosmic rays</kwd>
    <kwd>atmosphere</kwd>
    <kwd>neutrons</kwd>
    <kwd>monitor</kwd>
    <kwd>air humidity</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">The work was financially supported by the Ministry of Science and Higher Education of the Russian Federation (Project 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>
 <body>
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