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<article article-type="research-article" dtd-version="1.3" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xml:lang="en"><front><journal-meta><journal-id journal-id-type="publisher-id">najo</journal-id><journal-title-group><journal-title xml:lang="en">Nanosystems: Physics, Chemistry, Mathematics</journal-title><trans-title-group xml:lang="ru"><trans-title>Наносистемы: физика, химия, математика</trans-title></trans-title-group></journal-title-group><issn pub-type="ppub">2220-8054</issn><issn pub-type="epub">2305-7971</issn><publisher><publisher-name>Университет ИТМО</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.17586/2220-8054-2016-7-3-479-481</article-id><article-id custom-type="elpub" pub-id-type="custom">najo-1254</article-id><article-categories><subj-group subj-group-type="heading"><subject>Research Article</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="en"><subject>PAPERS, PRESENTED AT NANO-2015</subject></subj-group><subj-group subj-group-type="section-heading" xml:lang="ru"><subject>PAPERS, PRESENTED AT NANO-2015</subject></subj-group></article-categories><title-group><article-title>Magnetic field dependent resonant light scattering by magnetic spheres in a magnetizable medium</article-title><trans-title-group xml:lang="ru"><trans-title>Magnetic field dependent resonant light scattering by magnetic spheres in a magnetizable medium</trans-title></trans-title-group></title-group><contrib-group><contrib contrib-type="author" corresp="yes"><name-alternatives><name name-style="eastern" xml:lang="ru"><surname>Bhatt</surname><given-names>Hem</given-names></name><name name-style="western" xml:lang="en"><surname>Bhatt</surname><given-names>Hem</given-names></name></name-alternatives><bio xml:lang="ru"><p>Sidsar, Bhavnagar. 364060</p></bio><bio xml:lang="en"><p>Sidsar, Bhavnagar. 364060</p></bio><email xlink:type="simple">drhembhatt@gmail.com</email><xref ref-type="aff" rid="aff-1"/></contrib></contrib-group><aff-alternatives id="aff-1"><aff xml:lang="ru"><institution>Shantilal Shah Engineering College</institution></aff><aff xml:lang="en"><institution>Shantilal Shah Engineering College</institution></aff></aff-alternatives><pub-date pub-type="collection"><year>2016</year></pub-date><pub-date pub-type="epub"><day>20</day><month>08</month><year>2025</year></pub-date><volume>7</volume><issue>3</issue><fpage>479</fpage><lpage>481</lpage><permissions><copyright-statement>Copyright &amp;#x00A9; Bhatt H., 2025</copyright-statement><copyright-year>2025</copyright-year><copyright-holder xml:lang="ru">Bhatt H.</copyright-holder><copyright-holder xml:lang="en">Bhatt H.</copyright-holder><license xml:lang="ru" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>Данная работа распространяется под лицензией Creative Commons Attribution 4.0.</license-p></license><license xml:lang="en" license-type="creative-commons-attribution" xlink:href="https://creativecommons.org/licenses/by/4.0/" xlink:type="simple"><license-p>This work is licensed under a Creative Commons Attribution 4.0 License.</license-p></license></permissions><self-uri xlink:href="https://nanojournal.ifmo.ru/jour/article/view/1254">https://nanojournal.ifmo.ru/jour/article/view/1254</self-uri><abstract><p>The anisotropy factor is a parameter from which one can determine preferential forward and backward light scattering. In the present study, we have calculated anisotropy factor hcos θi as a function of magnetic field for magnetic spheres in a magnetic medium. We have noticed resonances in hcos θi which indicate preferential enhanced scattering in forward and backward directions. Anisotropy factor is analyzed for various size parameters. The study clearly indicates that scattering can be modulated by means of size parameter of magnetic spheres as well as magnetic field. We have further confirmed the result by studying forward and backward intensity as a function of magnetic field. Resonances noticed in the intensity are in good agreement with the previous argument. This observation can be useful for the magnetic field dependent directional scattering and novel magneto-photonic devices.</p></abstract><trans-abstract xml:lang="ru"><p>The anisotropy factor is a parameter from which one can determine preferential forward and backward light scattering. In the present study, we have calculated anisotropy factor hcos θi as a function of magnetic field for magnetic spheres in a magnetic medium. We have noticed resonances in hcos θi which indicate preferential enhanced scattering in forward and backward directions. Anisotropy factor is analyzed for various size parameters. The study clearly indicates that scattering can be modulated by means of size parameter of magnetic spheres as well as magnetic field. We have further confirmed the result by studying forward and backward intensity as a function of magnetic field. Resonances noticed in the intensity are in good agreement with the previous argument. This observation can be useful for the magnetic field dependent directional scattering and novel magneto-photonic devices.</p></trans-abstract><kwd-group xml:lang="ru"><kwd>mie resonances</kwd><kwd>scattering</kwd><kwd>magnetic colloids</kwd><kwd>magneto-photonics</kwd></kwd-group><kwd-group xml:lang="en"><kwd>mie resonances</kwd><kwd>scattering</kwd><kwd>magnetic colloids</kwd><kwd>magneto-photonics</kwd></kwd-group></article-meta></front><back><ref-list><title>References</title><ref id="cit1"><label>1</label><citation-alternatives><mixed-citation xml:lang="ru">Yablonovitch E. Inhibited Spontaneous Emission in Solid-State Physics and Electronics. Phy. Rev. Lett., 1987, 58, P. 2059–2062.</mixed-citation><mixed-citation xml:lang="en">Yablonovitch E. Inhibited Spontaneous Emission in Solid-State Physics and Electronics. Phy. Rev. 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