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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">33971</article-id>
   <article-id pub-id-type="doi">10.12737/stp-54201913</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">Optical observations of small spacecraft and space debris at ISTP SB RAS Sayan Observatory</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Optical observations of small spacecraft and space debris at ISTP SB RAS Sayan Observatory</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Коробцев</surname>
       <given-names>Иван Владимирович</given-names>
      </name>
      <name xml:lang="en">
       <surname>Korobtsev</surname>
       <given-names>Ivan Vladimirovich</given-names>
      </name>
     </name-alternatives>
     <email>korobtsev@yandex.ru</email>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Мишина</surname>
       <given-names>Марина Николаевна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Mishina</surname>
       <given-names>Marina Nikolaevna</given-names>
      </name>
     </name-alternatives>
     <email>mmish@iszf.irk.ru</email>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Институт солнечно-земной физики СО РАН</institution>
     <city>Иркутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Solar Terrestrial Physics SB RAS</institution>
     <city>Irkutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Институт солнечно-земной физики СО РАН</institution>
     <city>Иркутск</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Institute of Solar Terrestrial Physics SB RAS</institution>
     <city>Irkutsk</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <volume>5</volume>
   <issue>4</issue>
   <fpage>97</fpage>
   <lpage>100</lpage>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/33971/view">https://naukaru.ru/en/nauka/article/33971/view</self-uri>
   <abstract xml:lang="ru">
    <p>Launch of several thousands of small spacecraft as part of satellite groups of various companies (OneWeb, SpaceX, etc.) is expected in the coming years. They will significantly increase the “population” in the low-orbit region. The spacecraft are designed mainly to provide telecommunications and remote sensing of Earth from space. They have a short lifetime. The use of high-speed sCMOS (scientific complementary metal-oxide-semiconductor) detectors in combination with medium diameter optical telescopes provides high temporal resolution, which allows us to get detailed brightness light curves and to estimate the state of small spacecraft. We present the technique and results of photometric measurements of small spacecraft obtained with the 1.6-meter AZT-33IK telescope of ISTP SB RAS Sayan Solar Observatory. Photometric measurements are shown to be an important source of information at various operational stages of satellites.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>Launch of several thousands of small spacecraft as part of satellite groups of various companies (OneWeb, SpaceX, etc.) is expected in the coming years. They will significantly increase the “population” in the low-orbit region. The spacecraft are designed mainly to provide telecommunications and remote sensing of Earth from space. They have a short lifetime. The use of high-speed sCMOS (scientific complementary metal-oxide-semiconductor) detectors in combination with medium diameter optical telescopes provides high temporal resolution, which allows us to get detailed brightness light curves and to estimate the state of small spacecraft. We present the technique and results of photometric measurements of small spacecraft obtained with the 1.6-meter AZT-33IK telescope of ISTP SB RAS Sayan Solar Observatory. Photometric measurements are shown to be an important source of information at various operational stages of satellites.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>small spacecraft</kwd>
    <kwd>low-Earth orbit</kwd>
    <kwd>photometry</kwd>
    <kwd>optical telescope</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>small spacecraft</kwd>
    <kwd>low-Earth orbit</kwd>
    <kwd>photometry</kwd>
    <kwd>optical telescope</kwd>
   </kwd-group>
  </article-meta>
 </front>
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