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  <front>
    <journal-meta>
      <journal-id journal-id-type="ojs">izvcrao</journal-id>
      <journal-id journal-id-type="publisher-id" xml:lang="ru">
                       Изв. Крымск. Астрофиз. Обсерв.
                </journal-id>
      <journal-id journal-id-type="publisher-id" xml:lang="en">
                        Izv. Krymsk. Astrofiz. Observ.
                    </journal-id>
      <journal-title-group>
        <journal-title xml:lang="ru">
                    Известия Крымской астрофизической обсерватории
                </journal-title>
        <trans-title-group xml:lang="en">
          <trans-title>Izvestiya Krymskoi Astrofizicheskoi Observatorii</trans-title>
        </trans-title-group>
      </journal-title-group>
      <issn pub-type="ppub">0367-8466</issn>
      <issn pub-type="epub">3034-4107</issn>
      <publisher>
        <publisher-name>Киселев Н.Н., пос. Московский, Москва, РФ</publisher-name>
        <publisher-loc>RU</publisher-loc>
      </publisher>
      <self-uri xlink:href="https://jn.craocrimea.ru/index.php/izvcrao"/>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="publisher-id">853</article-id>
      <article-categories>
        <subj-group xml:lang="ru" subj-group-type="heading">
          <subject>Материалы конференции</subject>
        </subj-group>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Сonference proceedings</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="ru">Regularities in the solar background magnetic field </article-title>
        <trans-title-group xml:lang="en">
          <trans-title>Regularities in the solar background magnetic field </trans-title>
        </trans-title-group>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="">
              <surname> Bumba</surname>
              <given-names>V.</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-1"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Astronomical Institute, Academy of Sciences of the Czech Republic, 25165, Ondřejov, Czech Republic</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2009-01-31">
        <day>31</day>
        <month>01</month>
        <year>2009</year>
      </pub-date>
      <volume>104</volume>
      <issue>6</issue>
      <fpage>87</fpage>
      <lpage>94</lpage>
      <history>
        <date date-type="received" iso-8601-date="2020-05-28">
          <day>28</day>
          <month>05</month>
          <year>2020</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>
					Copyright (c)   
				</copyright-statement>
        <copyright-year>
					
				</copyright-year>
        <copyright-holder>
					Bumba V.
				</copyright-holder>
        <license xlink:href="http://creativecommons.org/licenses/by/4.0">
          <license-p> Метаданные этой статьи доступны по лицензии  Creative Commons «Attribution» («Атрибуция») 4.0 Всемирная.  
 Авторское право и право на публикацию текстов, представленных в журнале  "Известия Крымской астрофизической обсерватории", сохраняются за авторами, при этом право первой публикации предоставляется журналу. Тексты могут свободно использоваться при условии правильного цитирования с указанием авторства в соответствии с лицензией  Creative Commons «Attribution» («Атрибуция») 4.0 Всемирная.  
     </license-p>
        </license>
      </permissions>
      <self-uri xlink:href="https://jn.craocrimea.ru/index.php/izvcrao/article/view/853"/>
      <abstract xml:lang="en">
        <p> We are searching for the physical cause of regular long periods of solar activity recurrences and regularities in the background magnetic field distribution. We use the Stanford synoptic maps of the magnetic field and of the source surface magnetic field divided into different longitudinal zones. We demonstrate that the longitudinal background field concentrations and their longitudinal shift with time in the individual zones run parallel with lines connecting points of projections of meetings of some planetary pairs into the same maps. 
 Further we show that very specific mutual positions of Jupiter and Saturn with respect to Venus and Earth during their oppositions and conjunctions principally differ during the phase of highest activity in the recent three odd cycles and two even cycles. Parallel with the sudden changes of the longitudinal field distribution, we again ascribe to Venus and Earth meetings, we characterize large-scale uni-polar magnetic structures, the development of which we also connect with these meetings. During the meetings, it is the positive polarity which predominates in the structures occupying the solar side facing the Earth, while the negative polarity is concentrated on the opposite side of the Sun. We suggest that another agent, possibly the magnetic and electric field acts parallel with the gravitational forces of the planetary system. </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>activity</kwd>
        <kwd>magnetic field</kwd>
        <kwd>planetary meetings</kwd>
      </kwd-group>
      <counts>
        <page-count count="8"/>
      </counts>
    </article-meta>
  </front>
  <body/>
  <back>
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</article>
