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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">126</article-id>
      <article-id pub-id-type="edn">ASRHFV</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Instruments and Methods</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">Telescope for recording coronal mass ejections SPOT-CME</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Tlatov</surname>
              <given-names>Andrei</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-1"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Berezin</surname>
              <given-names>Ivan</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-2"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Shramko</surname>
              <given-names>Andrei</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-3"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Kirpichev</surname>
              <given-names>Roman</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-4"/>
        </contrib>
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname>Dormidontov</surname>
              <given-names>Denis</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-5"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Mountain Astronomical Station, Central Astronomical Observatory RAS, Gagarina 100, Kislovodsk 357700, Russia; Kalmyk State University, Pushkina 11, Elista 358000, Russia</institution>
      </aff>
      <aff id="aff-2">
        <institution content-type="orgname" xml:lang="en">Mountain Astronomical Station, Central Astronomical Observatory RAS, Gagarina 100, Kislovodsk 357700, Russia; Kalmyk State University, Pushkina 11, Elista 358000, Russia</institution>
      </aff>
      <aff id="aff-3">
        <institution content-type="orgname" xml:lang="en">Mountain Astronomical Station, Central Astronomical Observatory RAS, Gagarina 100, Kislovodsk 357700, Russia</institution>
      </aff>
      <aff id="aff-4">
        <institution content-type="orgname" xml:lang="en">Mountain Astronomical Station, Central Astronomical Observatory RAS, Gagarina 100, Kislovodsk 357700, Russia</institution>
      </aff>
      <aff id="aff-5">
        <institution content-type="orgname" xml:lang="en">Mountain Astronomical Station, Central Astronomical Observatory RAS, Gagarina 100, Kislovodsk 357700, Russia</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2026-06-26">
        <day>26</day>
        <month>06</month>
        <year>2026</year>
      </pub-date>
      <volume>7</volume>
      <issue>2</issue>
      <fpage>1</fpage>
      <lpage>3</lpage>
      <history>
        <date date-type="received" iso-8601-date="2026-06-15">
          <day>15</day>
          <month>06</month>
          <year>2026</year>
        </date>
      </history>
      <permissions>
        <copyright-statement xml:lang="en">Copyright (c) 2026 Andrei Tlatov, Ivan Berezin, Andrei Shramko, Roman Kirpichev, Denis Dormidontov</copyright-statement>
        <copyright-year>
					2026
				</copyright-year>
        <copyright-holder xml:lang="en">Andrei Tlatov, Ivan Berezin, Andrei Shramko, Roman Kirpichev, Denis Dormidontov</copyright-holder>
        <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  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/126"/>
      <abstract xml:lang="en">
        <p> We present a project of the new patrol telescope for regular solar observations with a cadence of about one minute. The instrument is intended to detect and determine parameters of coronal mass ejections and solar flares. It allows one to observe velocity fields in both the solar atmosphere and coronal ejections. The telescope is designed based on an air-proof single-volume scheme, may be mounted without a pavilion, and operates as a robotic telescope. It can be used within the Solar Service network. </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>Sun</kwd>
        <kwd>solar observations</kwd>
        <kwd>solar telescopes</kwd>
      </kwd-group>
      <funding-group>
        <funding-statement xml:lang="en">
                                                    The work was supported by the Ministry of Education and Science of the Russian Federation under state assignment No. 075-03-2026-375.
                                                </funding-statement>
      </funding-group>
      <counts>
        <page-count count="3"/>
      </counts>
    </article-meta>
  </front>
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  <back>
    <ref-list>
      <ref id="R1">
        <mixed-citation>Berezin I.A., Tlatov A.G., Pevtsov A.A., 2023. Astrophys. J., vol. 950, no. 2, p. 100.</mixed-citation>
      </ref>
      <ref id="R2">
        <mixed-citation>Tlatov A.G., Shramko A.D., Chernov Y.O., Strelkov M.A., Naga Varun E., 2017. Geomagnetism and Aeronomy, vol. 57, no. 7, pp. 854–858.</mixed-citation>
      </ref>
    </ref-list>
  </back>
</article>
