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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">51702</article-id>
   <article-id pub-id-type="doi">10.2205/2022ES000825</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">Wavelet analysis of geomagnetically induced currents during the strong geomagnetic storms</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Wavelet analysis of geomagnetically induced currents during the strong geomagnetic storms</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <contrib-id contrib-id-type="orcid">https://orcid.org/0000-0001-5380-713X</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Аксенович</surname>
       <given-names>Татьяна Валерьевна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Aksenovich</surname>
       <given-names>Tatyana Valerievna</given-names>
      </name>
     </name-alternatives>
     <email>t.aksenovich@ksc.ru</email>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Билин</surname>
       <given-names>Владислав Андреевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Bilin</surname>
       <given-names>Vladislav Andreevich</given-names>
      </name>
     </name-alternatives>
     <email>bilinvlad@gmail.com</email>
     <xref ref-type="aff" rid="aff-2"/>
     <xref ref-type="aff" rid="aff-3"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Сахаров</surname>
       <given-names>Ярослав Алексеевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Sakharov</surname>
       <given-names>Yaroslav Alekseevich</given-names>
      </name>
     </name-alternatives>
     <email>sakharov@pgia.ru</email>
     <bio xml:lang="ru">
      <p>кандидат физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>candidate of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-4"/>
     <xref ref-type="aff" rid="aff-5"/>
     <xref ref-type="aff" rid="aff-6"/>
    </contrib>
    <contrib contrib-type="author">
     <contrib-id contrib-id-type="orcid">https://orcid.org/0000-0001-5681-065X</contrib-id>
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Селиванов</surname>
       <given-names>Василий Николаевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Selivanov</surname>
       <given-names>Vasiliy Nikolaevich</given-names>
      </name>
     </name-alternatives>
     <email>v.selivanov@ksc.ru</email>
     <bio xml:lang="ru">
      <p>кандидат технических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>candidate of technical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-7"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Центр физико-технических проблем энергетики Севера КНЦ РАН</institution>
     <city>Апатиты</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Northern Energetics Research Centre KSC RAS</institution>
     <city>Apatity</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Полярный геофизический институт РАН</institution>
     <city>Апатиты</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Polar Geophysical Institute, RAS</institution>
     <city>Apatity</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-3">
    <aff>
     <institution xml:lang="ru">Центр физико-технических проблем энергетики Севера КНЦ РАН</institution>
     <city>Апатиты</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Nothern Energetics Research Centre KSC RAS</institution>
     <city>Apatity</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-4">
    <aff>
     <institution xml:lang="ru">Полярный Геофизический Институт</institution>
     <city>Апатиты</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Polar Geophysical Institute</institution>
     <city>Apatity</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-5">
    <aff>
     <institution xml:lang="ru">Центр физико-технических проблем энергетики Севера КНЦ РАН</institution>
     <city>Апатиты</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Nothern Energetics Research Centre KSC RAS</institution>
     <city>Apatity</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-6">
    <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>
   <aff-alternatives id="aff-7">
    <aff>
     <institution xml:lang="ru">Центр физико-технических проблем энергетики Севера КНЦ РАН</institution>
     <city>Апатиты</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Northern Energetics Research Centre KSC RAS</institution>
     <city>Apatity</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2022-12-31T00:00:00+03:00">
    <day>31</day>
    <month>12</month>
    <year>2022</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2022-12-31T00:00:00+03:00">
    <day>31</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="2022-07-12T00:00:00+03:00">
     <day>12</day>
     <month>07</month>
     <year>2022</year>
    </date>
    <date date-type="accepted" iso-8601-date="2022-12-20T00:00:00+03:00">
     <day>20</day>
     <month>12</month>
     <year>2022</year>
    </date>
   </history>
   <self-uri xlink:href="https://rjes.ru/en/nauka/article/51702/view">https://rjes.ru/en/nauka/article/51702/view</self-uri>
   <abstract xml:lang="ru">
    <p>The main problem of electric utilities around the world is to ensure continuous power supply to consumers. One of the causes of power outages and blackouts can be geomagnetic storms during periods of the increased solar activity. They arouse geomagnetically induced currents (GICs) flowing in the long-distance high-voltage power grids on Earth’s surface. The history of this phenomenon investigation shows that GICs during strong geomagnetic storms had led to blackouts in certain regions of Canada, Sweden and the USA. To study these phenomena and assess the risks of such accidents for the regional system, a GICs registration system in 330 kV autotransformers neutrals of the Kola-Karelian power transit was developed in northwestern Russia. During 11 years of monitoring numerous cases of the flow of high values of quasi-dc currents with different time durations, induced by variations of the geomagnetic field, have been registered. In order to analyze the currents a wavelet transform was chosen, since this method allows to define not only the frequency composition but also changes in spectral characteristics over time, which is significant in the study of GIC. The paper presents a discussion of GIC scalograms obtained for four events of Solar Cycle 24: 13-14 November 2012, 17-18 March 2015, 7-8 September 2015 and 7-8 September 2017. The analysis showed that the characteristic duration of the peak of the considered GICs is from 4.6 to 11.1 min.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>The main problem of electric utilities around the world is to ensure continuous power supply to consumers. One of the causes of power outages and blackouts can be geomagnetic storms during periods of the increased solar activity. They arouse geomagnetically induced currents (GICs) flowing in the long-distance high-voltage power grids on Earth’s surface. The history of this phenomenon investigation shows that GICs during strong geomagnetic storms had led to blackouts in certain regions of Canada, Sweden and the USA. To study these phenomena and assess the risks of such accidents for the regional system, a GICs registration system in 330 kV autotransformers neutrals of the Kola-Karelian power transit was developed in northwestern Russia. During 11 years of monitoring numerous cases of the flow of high values of quasi-dc currents with different time durations, induced by variations of the geomagnetic field, have been registered. In order to analyze the currents a wavelet transform was chosen, since this method allows to define not only the frequency composition but also changes in spectral characteristics over time, which is significant in the study of GIC. The paper presents a discussion of GIC scalograms obtained for four events of Solar Cycle 24: 13-14 November 2012, 17-18 March 2015, 7-8 September 2015 and 7-8 September 2017. The analysis showed that the characteristic duration of the peak of the considered GICs is from 4.6 to 11.1 min.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>geomagnetically induced currents</kwd>
    <kwd>geomagnetic storm</kwd>
    <kwd>autotransformer</kwd>
    <kwd>continuous wavelet transform</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>geomagnetically induced currents</kwd>
    <kwd>geomagnetic storm</kwd>
    <kwd>autotransformer</kwd>
    <kwd>continuous wavelet transform</kwd>
   </kwd-group>
   <funding-group>
    <funding-statement xml:lang="ru">This study is supported by the grant no. 22-29-00413 from the Russian Science Foundation (https://rscf.ru/project/22-29-00413/).</funding-statement>
    <funding-statement xml:lang="en">This study is supported by the grant no. 22-29-00413 from the Russian Science Foundation (https://rscf.ru/project/22-29-00413/).</funding-statement>
   </funding-group>
  </article-meta>
 </front>
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