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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">28055</article-id>
   <article-id pub-id-type="doi">10.12737/stp-51201908</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">Estimated nitric oxide density in auroras from ground-based photometric data</article-title>
    <trans-title-group xml:lang="ru">
     <trans-title>Estimated nitric oxide density in auroras from ground-based photometric data</trans-title>
    </trans-title-group>
   </title-group>
   <contrib-group content-type="authors">
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Дашкевич</surname>
       <given-names>Жанна Владимировна</given-names>
      </name>
      <name xml:lang="en">
       <surname>Dashkevich</surname>
       <given-names>Zhanna Vladimirovna</given-names>
      </name>
     </name-alternatives>
     <email>zhanna@pgia.ru</email>
     <bio xml:lang="ru">
      <p>кандидат физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>candidate of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-1"/>
    </contrib>
    <contrib contrib-type="author">
     <name-alternatives>
      <name xml:lang="ru">
       <surname>Иванов</surname>
       <given-names>Владимир Евгеньевич</given-names>
      </name>
      <name xml:lang="en">
       <surname>Ivanov</surname>
       <given-names>Vladimir Evgenievich</given-names>
      </name>
     </name-alternatives>
     <email>ivanov@pgia.ru</email>
     <bio xml:lang="ru">
      <p>доктор физико-математических наук;</p>
     </bio>
     <bio xml:lang="en">
      <p>doctor of physical and mathematical sciences;</p>
     </bio>
     <xref ref-type="aff" rid="aff-2"/>
    </contrib>
   </contrib-group>
   <aff-alternatives id="aff-1">
    <aff>
     <institution xml:lang="ru">Полярный геофизический институт</institution>
     <city>Апатиты</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Polar Geophysical Institute</institution>
     <city>Apatity</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <aff-alternatives id="aff-2">
    <aff>
     <institution xml:lang="ru">Полярный геофизический институт РАН</institution>
     <city>Апатиты</city>
     <country>Россия</country>
    </aff>
    <aff>
     <institution xml:lang="en">Polar Geophysical Institute, RAS</institution>
     <city>Apatity</city>
     <country>Russian Federation</country>
    </aff>
   </aff-alternatives>
   <volume>5</volume>
   <issue>1</issue>
   <fpage>58</fpage>
   <lpage>61</lpage>
   <self-uri xlink:href="https://naukaru.ru/en/nauka/article/28055/view">https://naukaru.ru/en/nauka/article/28055/view</self-uri>
   <abstract xml:lang="ru">
    <p>In this paper, we numerically estimate the nitric oxide density in auroras, using photometric data on 427.8, 557.7, and 630.0 nm emission intensities. The data were obtained at midnight at observatories of the Polar Geophysical Institute. These estimates were made using a numerical modeling procedure with a time-dependent model of the auroral ionosphere [Dashkevich et al., 2017]. It is shown that the NO density in the maximum of the altitude profile is between (1÷3.3)∙10^8 cm–3. The obtained estimates indicate the absence of a correlation between the [NO]max values and 427.8 nm emission intensities.</p>
   </abstract>
   <trans-abstract xml:lang="en">
    <p>In this paper, we numerically estimate the nitric oxide density in auroras, using photometric data on 427.8, 557.7, and 630.0 nm emission intensities. The data were obtained at midnight at observatories of the Polar Geophysical Institute. These estimates were made using a numerical modeling procedure with a time-dependent model of the auroral ionosphere [Dashkevich et al., 2017]. It is shown that the NO density in the maximum of the altitude profile is between (1÷3.3)∙10^8 cm–3. The obtained estimates indicate the absence of a correlation between the [NO]max values and 427.8 nm emission intensities.</p>
   </trans-abstract>
   <kwd-group xml:lang="ru">
    <kwd>nitric oxide</kwd>
    <kwd>ionosphere component densities</kwd>
    <kwd>auroras</kwd>
    <kwd>emission intensity</kwd>
    <kwd>modeling</kwd>
    <kwd>electron precipitation</kwd>
   </kwd-group>
   <kwd-group xml:lang="en">
    <kwd>nitric oxide</kwd>
    <kwd>ionosphere component densities</kwd>
    <kwd>auroras</kwd>
    <kwd>emission intensity</kwd>
    <kwd>modeling</kwd>
    <kwd>electron precipitation</kwd>
   </kwd-group>
  </article-meta>
 </front>
 <body>
  <p></p>
 </body>
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