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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">12014</article-id>
   <article-id pub-id-type="doi">10.12737/19877</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">North-south asymmetry of geomagnetic activity and solar wind electric field</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>North-south asymmetry of geomagnetic activity and solar wind electric field</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Макаров</surname>
       <given-names>Георгий Афанасьевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Makarov</surname>
       <given-names>Georgy Afanasyevich</given-names>
      </name>
     </name-alternatives>
     <email>gmakarov@ikfia.sbras.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-1"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт космофизических исследований и аэрономии им. Ю.Г. Шафера СО РАН</institution>
     <city>Якутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy SB RAS</institution>
     <city>Yakutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <pub-date publication-format="print" date-type="pub" iso-8601-date="2016-05-31T00:00:00+03:00">
    <day>31</day>
    <month>05</month>
    <year>2016</year>
   </pub-date>
   <pub-date publication-format="electronic" date-type="pub" iso-8601-date="2016-05-31T00:00:00+03:00">
    <day>31</day>
    <month>05</month>
    <year>2016</year>
   </pub-date>
   <volume>2</volume>
   <issue>1</issue>
   <fpage>44</fpage>
   <lpage>49</lpage>
   <self-uri xlink:href="https://zh-szf.ru/en/nauka/article/12014/view">https://zh-szf.ru/en/nauka/article/12014/view</self-uri>
   <abstract xml:lang="ru">
    <p>Geomagnetic activity asymmetry in the Northern and Southern hemispheres is studied. It is shown that the higher is the level of magnetic activity the greater is the asymmetry. It is found that the asymmetry in the hemispheres manifests itself in the 06–18-hour component of magnetic activity diurnal variation, while the asymmetry in the 00–12-hourly component is completely absent. The cause of geomagnetic north-south asymmetry is supposed to be meridional Pedersen current between high and middle latitudes in the ionosphere. A qualitative model of formation of asymmetry connected with the solar wind electric field is proposed.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>Geomagnetic activity asymmetry in the Northern and Southern hemispheres is studied. It is shown that the higher is the level of magnetic activity the greater is the asymmetry. It is found that the asymmetry in the hemispheres manifests itself in the 06–18-hour component of magnetic activity diurnal variation, while the asymmetry in the 00–12-hourly component is completely absent. The cause of geomagnetic north-south asymmetry is supposed to be meridional Pedersen current between high and middle latitudes in the ionosphere. A qualitative model of formation of asymmetry connected with the solar wind electric field is proposed.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>Geomagnetic activity</kwd>
    <kwd>Earth’s magnetosphere</kwd>
    <kwd>interplanetary magnetic field</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>Geomagnetic activity</kwd>
    <kwd>Earth’s magnetosphere</kwd>
    <kwd>interplanetary magnetic field</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
 <back>
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</article>
