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 <front>
  <journal-meta>
   <journal-id journal-id-type="publisher-id">Russian Journal of Earth Sciences</journal-id>
   <journal-title-group>
    <journal-title xml:lang="en">Russian Journal of Earth Sciences</journal-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Russian Journal of Earth Sciences</trans-title>
    </trans-title-group>
   </journal-title-group>
   <issn publication-format="online">1681-1208</issn>
  </journal-meta>
  <article-meta>
   <article-id pub-id-type="publisher-id">56090</article-id>
   <article-id pub-id-type="doi">10.2205/2022ES000803</article-id>
   <article-categories>
    <subj-group subj-group-type="toc-heading" xml:lang="ru">
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
    <subj-group subj-group-type="toc-heading" xml:lang="en">
     <subject>ORIGINAL ARTICLES</subject>
    </subj-group>
    <subj-group>
     <subject>ОРИГИНАЛЬНЫЕ СТАТЬИ</subject>
    </subj-group>
   </article-categories>
   <title-group>
    <article-title xml:lang="en">&quot;Danjon Effect&quot;, Solar-Triggered Volcanic Activity, and Relation to Climate Change</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>&quot;Danjon Effect&quot;, Solar-Triggered Volcanic Activity, and Relation to Climate Change</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Комитов</surname>
       <given-names>Борис </given-names>
      </name>
      <name xml:lang="en">
       <surname>Komitov</surname>
       <given-names>Boris </given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Кафтан</surname>
       <given-names>Владимир </given-names>
      </name>
      <name xml:lang="en">
       <surname>Kaftan</surname>
       <given-names>Vladimir </given-names>
      </name>
     </name-alternatives>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт астрономии Болгарской академии наук</institution>
     <city>София</city>
     <country>Болгария</country>
    </aff>
    <aff>
     <institution xml:lang="en">1Institute of Astronomy and National Astronomical Observatory, Bulgarian Academy of Sciences</institution>
     <city>Sofia</city>
     <country>Bulgaria</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Геофизический центр РАН</institution>
     <city>Москва</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Geophysical Center of the Russian Academy of Sciences</institution>
     <city>Moscow</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2022-12-23T00:00:00+03:00">
    <day>23</day>
    <month>12</month>
    <year>2022</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2022-12-23T00:00:00+03:00">
    <day>23</day>
    <month>12</month>
    <year>2022</year>
   </pub-date>
   <volume>22</volume>
   <issue>6</issue>
   <fpage>1</fpage>
   <lpage>12</lpage>
   <history>
    <date date-type="received" iso-8601-date="2022-07-10T00:00:00+03:00">
     <day>10</day>
     <month>07</month>
     <year>2022</year>
    </date>
    <date date-type="accepted" iso-8601-date="2022-09-09T00:00:00+03:00">
     <day>09</day>
     <month>09</month>
     <year>2022</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/56090/view">https://rjes.ru/en/nauka/article/56090/view</self-uri>
   <abstract xml:lang="ru">
    <p>The “Danjon effect” is a phenomenon that presents a tendency to concentrate the so-called “dark” total lunar eclipses (DTLE) near solar sunspot cycle minimum phases. It was a starting point for the present study, whose main subject is a statistical analysis of relationship between solar and volcanic activity for the maximum long time. To this end, the Smithsonian National Museum of Natural History's volcanic activity catalog was used. On its basis, a time series of the total annual volcanic eruptions for the period 1551–2020 AD has been built and explored for cycles of possible solar origin. Cycles with duration of 10–11, 19–25, ∼60, and ∼240 years (all with possible solar origin) has been established. It has also been found that there are two certain peaks of volcanic activity during the sunspot activity cycle: the first one is close to or after the sunspot minimum (sunspot cycle phase 0.9 ≤ Φ ≤1.0 and 0.1 ≤ Φ ≤ 0.2), and the second is wider – close to the sunspot cycle maximum (0.3 ≤ Φ ≤ 0.5). A third maximum is detected about 3–4 years after the sunspot cycle maximum (0.7 ≤ Φ ≤ 0.8) for the “moderate strong” volcanic eruptions with volcanic eruptive index VEI = 5. It corresponds to the geomagnetic activity secondary maximum, which usually occurs 3–4 years after the sunspot maximum. Φ is calculated separately on the basis of each sunspot cycle length. Finally, without any exclusions, all most powerful volcanic eruptions for which VEI ≥ 6 are centered near the ∼11-year Schwabe-Wolf cycle extremes. Trigger mechanisms of solar and geomagnetic activity over volcanic events, as well as their relation to climate change (in interaction with galactic cosmic rays (GCR) and/or solar energetic particles (SEP)), are discussed. The Pinatubo eruption in 1991 as an example of a “pure” strong solar–volcanism relationship has been analyzed in detail.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The “Danjon effect” is a phenomenon that presents a tendency to concentrate the so-called “dark” total lunar eclipses (DTLE) near solar sunspot cycle minimum phases. It was a starting point for the present study, whose main subject is a statistical analysis of relationship between solar and volcanic activity for the maximum long time. To this end, the Smithsonian National Museum of Natural History's volcanic activity catalog was used. On its basis, a time series of the total annual volcanic eruptions for the period 1551–2020 AD has been built and explored for cycles of possible solar origin. Cycles with duration of 10–11, 19–25, ∼60, and ∼240 years (all with possible solar origin) has been established. It has also been found that there are two certain peaks of volcanic activity during the sunspot activity cycle: the first one is close to or after the sunspot minimum (sunspot cycle phase 0.9 ≤ Φ ≤1.0 and 0.1 ≤ Φ ≤ 0.2), and the second is wider – close to the sunspot cycle maximum (0.3 ≤ Φ ≤ 0.5). A third maximum is detected about 3–4 years after the sunspot cycle maximum (0.7 ≤ Φ ≤ 0.8) for the “moderate strong” volcanic eruptions with volcanic eruptive index VEI = 5. It corresponds to the geomagnetic activity secondary maximum, which usually occurs 3–4 years after the sunspot maximum. Φ is calculated separately on the basis of each sunspot cycle length. Finally, without any exclusions, all most powerful volcanic eruptions for which VEI ≥ 6 are centered near the ∼11-year Schwabe-Wolf cycle extremes. Trigger mechanisms of solar and geomagnetic activity over volcanic events, as well as their relation to climate change (in interaction with galactic cosmic rays (GCR) and/or solar energetic particles (SEP)), are discussed. The Pinatubo eruption in 1991 as an example of a “pure” strong solar–volcanism relationship has been analyzed in detail.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>volcanic activity</kwd>
    <kwd>solar activity</kwd>
    <kwd>geomagnetism</kwd>
    <kwd>Sun–climate relationships</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>volcanic activity</kwd>
    <kwd>solar activity</kwd>
    <kwd>geomagnetism</kwd>
    <kwd>Sun–climate relationships</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">This work was supported within the framework of a state assignment at the Institute of Astronomy and National Astronomic Obsrvatory, Bulgarian Academy of Sciences, and the Geophysical Center, Russian Academy of Sciences approved by the Ministry of Education and Science of the Russian Federation.</funding-statement>
    <funding-statement xml:lang="en">This work was supported within the framework of a state assignment at the Institute of Astronomy and National Astronomic Obsrvatory, Bulgarian Academy of Sciences, and the Geophysical Center, Russian Academy of Sciences approved by the Ministry of Education and Science of the Russian Federation.</funding-statement>
   </funding-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
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