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  <front>
    <journal-meta>
      <journal-id journal-id-type="ojs">aat</journal-id>
      <journal-id journal-id-type="publisher-id" xml:lang="en">
                       Acta Astrophys. Tau.
                </journal-id>
      <journal-title-group>
        <journal-title xml:lang="en">
                    Acta Astrophysica Taurica
                </journal-title>
      </journal-title-group>
      <issn pub-type="epub">2712-925X</issn>
      <publisher>
        <publisher-name>Kiselev Nikolai Nikolaevich,  Mosсow, settlement Moskovskii, Tat'yanin Park Str., 12, Moscow, Russia.</publisher-name>
        <publisher-loc>RU</publisher-loc>
      </publisher>
      <self-uri xlink:href="https://astrophysicatauricum.org/index.php/aat"/>
    </journal-meta>
    <article-meta>
      <article-id pub-id-type="publisher-id">15</article-id>
      <article-id pub-id-type="doi">10.31059/aat.vol1.iss2.pp6-12</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Reviewes</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">Crimean observations of the magnetic Sun: 1967–2018</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <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="en">Crimean Astrophysical Observatory, Nauchny, 298409</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2020-12-26">
        <day>26</day>
        <month>12</month>
        <year>2020</year>
      </pub-date>
      <volume>1</volume>
      <issue>2</issue>
      <fpage>6</fpage>
      <lpage>12</lpage>
      <history>
        <date date-type="received" iso-8601-date="2020-12-26">
          <day>26</day>
          <month>12</month>
          <year>2020</year>
        </date>
      </history>
      <permissions>
        <copyright-statement>
					Copyright (c) 2026 Kotov V.
				</copyright-statement>
        <copyright-year>
					2026
				</copyright-year>
        <copyright-holder>
					Valerii Kotov
				</copyright-holder>
        <license xlink:href="http://creativecommons.org/licenses/by/4.0">
          <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  Acta Astrophysica Taurica  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://astrophysicatauricum.org/index.php/aat/article/view/15"/>
      <abstract xml:lang="en">
        <p>  The magnetic field measurements of the Sun as a star initiated by academician A.B. Severny have been supported&amp;nbsp; 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 makes 27 semi-revolutions over one terrestrial year, and the Earth – the same number of its revolutions with the period   P   D    during one full solar rotation. The field changes 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="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="7"/>
      </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., Bizuar K., 2012. Izv. Krymsk. Astrofiz. Observ., vol. 108, no. 1, p. 57. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R17">
        <mixed-citation>Kotov V.A., Sanchez F.M., 2017. Astrophys. Space Sci., vol. 362, no. 1, p. 6.</mixed-citation>
      </ref>
      <ref id="R18">
        <mixed-citation>Kotov V.A., Severny 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 and 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>Sanchez 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.B., 1955. Izv. Krymsk. Astrofiz. Observ., vol. 15, p. 31. (In Russ.)</mixed-citation>
      </ref>
      <ref id="R32">
        <mixed-citation>Severny A., 1969. Nature, vol. 224, p. 53. Severny A.B., Kotov V.A., Tsap T.T., 1976. Nature, vol. 259, p. 87.</mixed-citation>
      </ref>
      <ref id="R33">
        <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="R34">
        <mixed-citation>Stefani F., Giesecke A., Weier T., 2019. Solar Phys., vol. 294, p. 60.</mixed-citation>
      </ref>
      <ref id="R35">
        <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>
