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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="magnetism-and-activity-of-the-sun-and-stars--–-2021-conference-proceedings" xml:lang="en">
  <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">88</article-id>
      <article-categories>
        <subj-group xml:lang="en" subj-group-type="heading">
          <subject>Magnetism and activity of the Sun and stars  – 2021 Conference proceedings</subject>
        </subj-group>
      </article-categories>
      <title-group>
        <article-title xml:lang="en">Scattering properties of spherical ice particles</article-title>
      </title-group>
      <contrib-group content-type="author">
        <contrib>
          <name-alternatives>
            <name name-style="western" xml:lang="en" specific-use="primary">
              <surname> Petrov</surname>
              <given-names>Dmitry</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> Zhuzhulina</surname>
              <given-names>Elena</given-names>
            </name>
          </name-alternatives>
          <xref ref-type="aff" rid="aff-2"/>
        </contrib>
      </contrib-group>
      <aff id="aff-1">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory, Nauchny 298409</institution>
      </aff>
      <aff id="aff-2">
        <institution content-type="orgname" xml:lang="en">Crimean Astrophysical Observatory, Nauchny 298409</institution>
      </aff>
      <pub-date date-type="pub" iso-8601-date="2024-09-30">
        <day>30</day>
        <month>09</month>
        <year>2024</year>
      </pub-date>
      <volume>5</volume>
      <issue>3</issue>
      <fpage>1</fpage>
      <lpage>5</lpage>
      <history>
        <date date-type="received" iso-8601-date="2024-09-27">
          <day>27</day>
          <month>09</month>
          <year>2024</year>
        </date>
      </history>
      <permissions>
        <copyright-statement xml:lang="en">Copyright (c) 2024 Dmitry  Petrov, Elena  Zhuzhulina</copyright-statement>
        <copyright-year>
					2024
				</copyright-year>
        <copyright-holder xml:lang="en">Dmitry  Petrov, Elena  Zhuzhulina</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/88"/>
      <abstract xml:lang="en">
        <p>  Water ice is widespread in the Solar system. The sizes of water ice particles are distributed over a fairly wide range. However, computer modeling of light scattering by sufficiently large ice particles at the present stage of development of computer technology can only be realized in the approximation of geometrical optics. The question of the limiting size remains open, starting from which geometric optics begins to describe scattering properties well. In view of this, for a qualitative study of the scattering properties of ice particles, the Mie theory was used, which describes the scattering of light by an ideal sphere. In this work, we investigate the features of light scattering characteristics, such as intensity and polarization as well as photometric color, by large particles of water ice with a size of about 0.7 mm. The effect of the scattering particle size and the phase angle on the scattering properties of ice particles is studied. We determine&amp;nbsp;  the minimum size of an ice spherical particle at which scattering can be described by the laws of geometric optics.  </p>
      </abstract>
      <kwd-group xml:lang="en">
        <kwd>water ice</kwd>
        <kwd>light scattering</kwd>
        <kwd>Mie’s theory</kwd>
        <kwd>polarization</kwd>
        <kwd>photometric color</kwd>
      </kwd-group>
      <counts>
        <page-count count="5"/>
      </counts>
    </article-meta>
  </front>
  <body/>
  <back>
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</article>
