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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>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">122589</article-id>
   <article-id pub-id-type="doi">10.12737/szf-122202606</article-id>
   <article-id pub-id-type="edn">ybsgms</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">The mid-altitude atmosphere of the European-Asian Region during Forbush decreases in cosmic rays</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Среднеширотная атмосфера Европейско-Азиатского региона  в период форбуш-понижений 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 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">Trofimuk Institute of Petroleum 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>
   <volume>12</volume>
   <issue>2</issue>
   <fpage>54</fpage>
   <lpage>62</lpage>
   <history>
    <date date-type="received" iso-8601-date="2025-09-08T00:00:00+03:00">
     <day>08</day>
     <month>09</month>
     <year>2025</year>
    </date>
    <date date-type="accepted" iso-8601-date="2025-11-25T00:00:00+03:00">
     <day>25</day>
     <month>11</month>
     <year>2025</year>
    </date>
   </history>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/122589/view">https://naukaru.ru/en/nauka/article/122589/view</self-uri>
   <abstract xml:lang="ru">
    <p>Выполнен анализ реакции среднеширотной атмосферы на форбуш-понижения галактических космических лучей, для чего были привлечены результаты многолетних наблюдений вариаций космических лучей и изменений атмосферных параметров на семи среднеширотных станциях космических лучей за период с 1966 по 2024 г. Во время форбуш-понижений (на спаде и в минимуме интенсивности) наблюдается увеличение атмосферного давления на всех среднеширотных станциях космических лучей. При восстановлении интенсивности космических лучей после форбуш-понижения происходит уменьшение давления. Продолжительность этого отклика атмосферы совпадает с продолжительностью форбуш-понижения. Эффект более четко проявляется в холодный период года, а также для станций космических лучей с небольшими значениями жесткости геомагнитного обрезания. Вариации среднемассовой и приземной температур во время форбуш-понижения наблюдаются на всех станциях космических лучей и существенно различаются для холодного и теплого времени года. Полученные результаты позволяют предположить, что изменения облачности и прозрачности атмосферы, вызванные изменениями скорости ионизации во время форбуш-понижений, являются причиной наблюдаемых эффектов.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The response of the mid-latitude atmosphere to Forbush decreases in galactic cosmic rays is analyzed. We use the results of long-term observations of cosmic ray variations and changes in atmospheric parameters at seven mid-latitude cosmic ray stations for the period from 1966 to 2024. During Forbush decreases (at the decline and minimum of intensity), an increase in atmospheric pressure is observed at all mid-latitude cosmic ray stations. When the cosmic ray intensity is restored after a Forbush decrease, the pressure decreases. The duration of this atmospheric response coincides with the duration of the Forbush decrease. The effect is more pronounced in the cold season, as well as for cosmic ray stations with small geomagnetic cutoff rigidity values. Variations in mean mass and surface temperatures during a Forbush decrease are observed at all cosmic ray stations and differ significantly for the cold and warm seasons. The obtained results suggest that changes in cloudiness and atmospheric transparency caused by changes in the ionization rate during Forbush decreases are a possible cause of the observed effects.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>космические лучи</kwd>
    <kwd>атмосфера</kwd>
    <kwd>форбуш-понижения</kwd>
    <kwd>давление</kwd>
    <kwd>температура</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>cosmic rays</kwd>
    <kwd>atmosphere</kwd>
    <kwd>Forbush decreases</kwd>
    <kwd>pressure</kwd>
    <kwd>temperature</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). The results were obtained using the equipment of Unique Research Facility 85 “Russian National Network of Cosmic Ray Stations” [http://www.ckp-rf.ru/usu/433536]</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). The results were obtained using the equipment of Unique Research Facility 85 “Russian National Network of Cosmic Ray Stations” [http://www.ckp-rf.ru/usu/433536]</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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