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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" article-type="к-75-летию-крао" xml:lang="ru">
  <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://jncrao.ru/index.php/izvcrao"/>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="publisher-id">941</article-id>
      <article-id pub-id-type="doi">10.31059/izcrao-vol116-iss1-pp14-23</article-id>
      <article-categories>
        <subj-group xml:lang="ru" subj-group-type="heading">
          <subject>К 75-летию КрАО</subject>
        </subj-group>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>To the 75th anniversary of CrAO</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="ru">Крымские наблюдения магнитного Солнца: 1967–2018 гг.</article-title>
        <trans-title-group xml:lang="en">
          <trans-title>Crimean observations of the magnetic Sun: 1967–2018</trans-title>
        </trans-title-group>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="ru" specific-use="primary">
              <surname>Котов</surname>
              <given-names>Валерий</given-names>
            </name>
            <name name-style="western" xml:lang="en" specific-use="">
              <surname>Kotov</surname>
              <given-names>Valerii</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="ru">ФГБУН "Крымская астрофизическая обсерватория РАН",  Научный, Крым, 298409</institution>
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory, Nauchny, 298409</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2020-07-15">
        <day>15</day>
        <month>07</month>
        <year>2020</year>
      </pub-date>
      <volume>116</volume>
      <issue>1</issue>
      <fpage>14</fpage>
      <lpage>23</lpage>
      <history>
        <date date-type="received" iso-8601-date="2020-06-10">
          <day>10</day>
          <month>06</month>
          <year>2020</year>
        </date>
      </history>
      <permissions>
        <copyright-statement xml:lang="ru">Copyright (c) 2020 Валерий Котов</copyright-statement>
        <copyright-statement xml:lang="en">Copyright (c) 2020 Kotov V.</copyright-statement>
        <copyright-year>
					2020
				</copyright-year>
        <copyright-holder xml:lang="ru">Валерий Котов</copyright-holder>
        <copyright-holder xml:lang="en">Kotov V.</copyright-holder>
        <license license-type="open-access" xlink:href="http://creativecommons.org/licenses/by/4.0" xml:lang="ru">
          <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>
        <license license-type="open-access" xlink:href="http://creativecommons.org/licenses/by/4.0" xml:lang="en">
          <license-p> The metadata for this submission is licensed under a  Creative Commons Attribution 4.0 International License.  
 Copyright and publishing rights for texts published in Izvestiya Krymskoi Astrofizicheskoi Observatorii is retained by the authors, with first publication rights granted to the journal.Texts are free to use with proper attribution and link to the licensing  (Creative Commons Attribution 4.0 International).  
     </license-p>
        </license>
      </permissions>
      <self-uri xlink:href="https://jncrao.ru/index.php/izvcrao/article/view/941"/>
      <abstract xml:lang="ru">
        <p>  Измерения магнитного поля Солнца как звезды, начатые по инициативе акад. А.Б. Северного, были поддержаны шестью другими обсерваториями. Кратко изложены история таких исследований в Крымской астрофизической обсерватории и основные результаты. По вариациям поля определен синодический период вращения солнечной гравитирующей массы   P   ⊙    = 27.027(6) сут. Обнаружено, что к нему привязаны движения Земли: за один земной год Солнце совершает 27 полуоборотов вокруг своей оси, а Земля – такое же число своих вращений с периодом   P  D   за полный солнечный оборот. Поле изменяется также с циклом Хейла   P   H    ≈   22   г. и циклом   P   7    ≈   7   лет, причем их отношение совпадает с приближением Архимеда, 22:7, для числа   π  , а временная шкала   (  π   -   3)  P   7    =   P   ⊙   2  /  2  P   D    – с орбитальным периодом Земли. Приведены аргументы в пользу космической природы обоих циклов и голографические выражения с участием   P   H   ,   P   7   ,   π   и универсальных констант.  </p>
      </abstract>
      <abstract xml:lang="en">
        <p>  The magnetic field measurements of the Sun as a star initiated by academician A.B. Severny have been supported by six other observatories. The history of such investigations at CrAO and the basic results are briefly described. The synodic spin period of the gravitating solar mass   P   ⊙    = 27.027(6) days is determined; the latter is shown to be linked to the Earth’s motion: the Sun performs 27 semi-revolutions over one terrestrial year, and the Earth – the same number of its revolutions with period   P  D   during one full solar rotation. The field is also changing with the Hale cycle   P   H    ≈   22   years and the cycle   P   7    = 7 years, whereas their ratio coincides with the Archimedes approximation, 22:7, for the   π   number, the timescale   (  π   -   3)  P   7    =   P   ⊙   2  /  2  P   D    – with the Earth’s orbital period. We provide arguments in favour of the cosmic origin of both cycles and holographic expressions, including   P   H   ,   P   7   ,   π  , and universal constants  </p>
      </abstract>
      <kwd-group xml:lang="ru">
        <kwd>история КрАО</kwd>
        <kwd>Солнце</kwd>
        <kwd>магнитное поле</kwd>
        <kwd>вращение</kwd>
        <kwd>11-летний цикл</kwd>
      </kwd-group>
      <kwd-group xml:lang="en">
        <kwd>CrAO history</kwd>
        <kwd>Sun</kwd>
        <kwd>magnetic field</kwd>
        <kwd>rotation</kwd>
        <kwd>11-year cycle</kwd>
      </kwd-group>
      <counts>
        <page-count count="10"/>
      </counts>
    </article-meta>
  </front>
  <body/>
  <back>
    <ref-list>
      <ref id="R1">
        <mixed-citation>Carr B.J., Rees M.J., 1979. Nature, vol. 278, p. 605.</mixed-citation>
      </ref>
      <ref id="R2">
        <mixed-citation>Chaplin W.J., Dumbill A.M., Elsworth Y., et al., 2003. Mon. Not. Roy. Astron. Soc., vol. 343, p. 813.</mixed-citation>
      </ref>
      <ref id="R3">
        <mixed-citation>Demidov M.L., Grigor’ev V.M., Peshcherov V.S., 2005. Astron. zhurn., vol. 82, no. 7, p. 628. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R4">
        <mixed-citation>Dicke R.H., 1978. Nature, vol. 276, p. 676.</mixed-citation>
      </ref>
      <ref id="R5">
        <mixed-citation>Gnevyshev M.N., Ohl A.I., 1948. Astron. zhurn., vol. 25, no. 1, p. 18. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R6">
        <mixed-citation>Gorobets B., 2004. Nauka i zhizn, no. 2, p. 64. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R7">
        <mixed-citation>Gough D.O., 2017. Solar Phys., vol. 292, p. 70.</mixed-citation>
      </ref>
      <ref id="R8">
        <mixed-citation>Haneychuk V.I., Kotov V.A., Tsap T.T., 2003. Astron. Astrophys., vol. 403, p. 1115.</mixed-citation>
      </ref>
      <ref id="R9">
        <mixed-citation>Kotov V.A., 2007. Izv. Krymsk. Astrofiz. Observ., vol. 103, no. 2, p. 245. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R10">
        <mixed-citation>Kotov V.A., 2013. Izv. Krymsk. Astrofiz. Observ., vol. 109, no. 1, p. 232. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R11">
        <mixed-citation>Kotov V.A., 2018. Astron. Nachr., vol. 339, no. 6, p. 513.</mixed-citation>
      </ref>
      <ref id="R12">
        <mixed-citation>Kotov V.A., 2019a. Adv. Space Res., vol. 63, p. 3385.</mixed-citation>
      </ref>
      <ref id="R13">
        <mixed-citation>Kotov V.A., 2019b. Astrophys. Space Sci., vol. 364, no. 3, p. 45.</mixed-citation>
      </ref>
      <ref id="R14">
        <mixed-citation>Kotov V.A., Haneychuk V.I., 2016. Izv. Krymsk. Astrofiz. Observ., vol. 112, p. 125. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R15">
        <mixed-citation>Kotov V.A., Haneychuk V.I., 2020. Astron. Nachr., doi:10.1002/asna.202013797.</mixed-citation>
      </ref>
      <ref id="R16">
        <mixed-citation>Kotov V.A., Sanchez F.M., 2017. Astrophys. Space Sci., vol. 362, no. 1, p. 6.</mixed-citation>
      </ref>
      <ref id="R17">
        <mixed-citation>Kotov V.A., Sanshez F.M., Bizuar K., 2012. Izv. Krymsk. Astrofiz. Observ., vol. 108, no. 1, p. 57. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R18">
        <mixed-citation>Kotov V.A., Severnyi A.B., 1983. The Total Magnetic Field of the Sun as a Star, Catalog 1968–1976. Moscow: Akad. Nauk SSSR. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R19">
        <mixed-citation>Kotov V.A., Severnyi A.B., Tsap T.T., 1982. Izv. Krymsk. Astrofiz. Observ., vol. 65, p. 3. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R20">
        <mixed-citation>Nikulin N.S., Severnyi A.B., Stepanov V.E., 1958. Izv. Krymsk. Astrofiz. Observ., vol. 19, p. 3. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R21">
        <mixed-citation>Obridko V.N., 2008. Plasma Heliophysics, vol. 1. Moscow: Fizmatlit. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R22">
        <mixed-citation>Quinn T., Speake C., Parks H., Davis R., 2014. Phil. Trans. R. Soc. A, vol. 372, p. 20140032.</mixed-citation>
      </ref>
      <ref id="R23">
        <mixed-citation>Rachkovskiy D.N., 1985. Izv. Krymsk. Astrofiz. Observ., vol. 71, p. 25. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R24">
        <mixed-citation>Rubakov V.A., Shtern B.E., 2020. Earth &amp; Universe, no. 1, p. 27. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R25">
        <mixed-citation>Sanchez F.M., Kotov V.A., Bizouard C., 2011. J. Cosmology, vol. 17, p. 7225.</mixed-citation>
      </ref>
      <ref id="R26">
        <mixed-citation>Sanshez F.M., Kotov V.A., Bizuar K., 2013. Izv. Krymsk. Astrofiz. Observ., vol. 109, no. 3, p. 181. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R27">
        <mixed-citation>Scafetta N., 2020. Solar Phys., vol. 295, no. 2, p. 33, doi:10.1007/s11207-020-1599-y.</mixed-citation>
      </ref>
      <ref id="R28">
        <mixed-citation>Scherrer P.H., Wilcox J.M., Kotov V., Severny A.B., Howard R., 1977a. Solar Phys., vol. 52, p. 3.</mixed-citation>
      </ref>
      <ref id="R29">
        <mixed-citation>Scherrer P.H., Wilcox J.M., Svalgaard L., 1980. Astrophys. J., vol. 241, p. 811.</mixed-citation>
      </ref>
      <ref id="R30">
        <mixed-citation>Scherrer P.H., Wilcox J.M., Svalgaard L., et al., 1977b. Solar Phys., vol. 54, p. 353.</mixed-citation>
      </ref>
      <ref id="R31">
        <mixed-citation>Severny A., 1969. Nature, vol. 224, p. 53.</mixed-citation>
      </ref>
      <ref id="R32">
        <mixed-citation>Severny A.B., 1955. Izv. Krymsk. Astrofiz. Observ., vol. 15, p. 31. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R33">
        <mixed-citation>Severny A.B., Kotov V.A., Tsap T.T., 1976. Nature, vol. 259, p. 87.</mixed-citation>
      </ref>
      <ref id="R34">
        <mixed-citation>Severny A.B., Kuvshinov V.M., Nikulin N.S., 1974. Izv. Krymsk. Astrofiz. Observ., vol. 50, p. 3. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R35">
        <mixed-citation>Stefani F., Giesecke A., Weier T., 2019. Solar Phys., vol. 294, p. 60.</mixed-citation>
      </ref>
      <ref id="R36">
        <mixed-citation>Tanabashi M., Hagiwara K., Hikasa K., et al., 2019. Phys. Rev. D, vol. 98, p. 030001.</mixed-citation>
      </ref>
    </ref-list>
  </back>
</article>
