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  <doi_batch_id>aspg-21-2230-1791475926</doi_batch_id>
  <timestamp>20261008161206</timestamp>
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  <registrant>American Scientific Publishing Group</registrant>
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  <journal>
   <journal_metadata language="en">
    <full_title>International Journal of Neutrosophic Science</full_title>
    <abbrev_title>IJNS</abbrev_title>
    <issn media_type="print">2692-6148</issn>
    <issn media_type="electronic">2690-6805</issn>
   </journal_metadata>
   <journal_issue>
    <publication_date media_type="online">
     <year>2024</year>
    </publication_date>
    <journal_volume>
     <volume>23</volume>
    </journal_volume>
    <issue>1</issue>
   </journal_issue>
   <journal_article publication_type="full_text">
    <titles>
     <title>Neutrosophic Control Chart for Rayleigh Quality with Applications To Wind Speed Data</title>
    </titles>
    <contributors>
     <person_name sequence="first" contributor_role="author">
      <given_name>Fuad S.</given_name>
      <surname>Alduais</surname>
      <affiliations>
       <institution>
        <institution_name>Mathematics Department, College of Humanities and Science in Al Aflaj, Prince Sattam Bin Abdulaziz University, Al-Kharj, Saudi Arabia; Business Administration Department, Administrative Scien</institution_name>
       </institution>
      </affiliations>
     </person_name>
     <person_name sequence="additional" contributor_role="author">
      <given_name>Zahid</given_name>
      <surname>Khan</surname>
      <affiliations>
       <institution>
        <institution_name>Department of Mathematics and Statistics, Hazara University Mansehra Pakistan</institution_name>
       </institution>
      </affiliations>
     </person_name>
     <person_name sequence="additional" contributor_role="author">
      <given_name>Muhammad</given_name>
      <surname>Waseem</surname>
      <affiliations>
       <institution>
        <institution_name>Department of Mathematics and Statistics, Hazara University Mansehra Pakistan</institution_name>
       </institution>
      </affiliations>
     </person_name>
    </contributors>
    <jats:abstract>
     <jats:p>The application of neutrosophic statistics provides a novel approach to dealing with uncertain and imprecise data problems. In this study, we present an improved method called neutrosophic Rayleigh exponential weighted moving average</jats:p>
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     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
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     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;REWMA</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;N chart. The</jats:p>
     <jats:p>style='font-size:10.0pt;mso-ansi-font-size:10.0pt;mso-bidi-font-size:10.0pt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
     <jats:p>mso-hansi-font-family:&quot;Times New Roman&quot;;mso-bidi-font-family:&quot;Times New Roman&quot;;</jats:p>
     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;REWMA</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;N chart is an extension of the traditional</jats:p>
     <jats:p>style='font-size:10.0pt;mso-ansi-font-size:10.0pt;mso-bidi-font-size:10.0pt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
     <jats:p>mso-hansi-font-family:&quot;Times New Roman&quot;;mso-bidi-font-family:&quot;Times New Roman&quot;;</jats:p>
     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;V</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;NR model and can be applied in various fields. The proposed</jats:p>
     <jats:p>style='font-size:10.0pt;mso-ansi-font-size:10.0pt;mso-bidi-font-size:10.0pt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
     <jats:p>mso-hansi-font-family:&quot;Times New Roman&quot;;mso-bidi-font-family:&quot;Times New Roman&quot;;</jats:p>
     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;REWMA</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;N scheme is designed to enhance the detection capability of the traditional</jats:p>
     <jats:p>style='font-size:10.0pt;mso-ansi-font-size:10.0pt;mso-bidi-font-size:10.0pt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
     <jats:p>mso-hansi-font-family:&quot;Times New Roman&quot;;mso-bidi-font-family:&quot;Times New Roman&quot;;</jats:p>
     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;V</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;NR chart. The key features of the suggested chart are discussed, highlighting its capability to handle vague, indeterminate, and fuzzy data situations. We evaluate the performance of the proposed scheme by analyzing the designated limits and charting parameters for different sample sizes. Moreover, we establish the performance metrics of the</jats:p>
     <jats:p>style='font-size:10.0pt;mso-ansi-font-size:10.0pt;mso-bidi-font-size:10.0pt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
     <jats:p>mso-hansi-font-family:&quot;Times New Roman&quot;;mso-bidi-font-family:&quot;Times New Roman&quot;;</jats:p>
     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;REWMA</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;N chart such as neutrosophic run length (</jats:p>
     <jats:p>style='font-size:10.0pt;mso-ansi-font-size:10.0pt;mso-bidi-font-size:10.0pt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
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     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;ARL</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;N ) and neutrosophic power curve (</jats:p>
     <jats:p>style='font-size:10.0pt;mso-ansi-font-size:10.0pt;mso-bidi-font-size:10.0pt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
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     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;PC</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;N ).Performance metrics demonstrate that the</jats:p>
     <jats:p>style='font-size:10.0pt;mso-ansi-font-size:10.0pt;mso-bidi-font-size:10.0pt;</jats:p>
     <jats:p>font-family:&quot;Cambria Math&quot;,serif;mso-ascii-font-family:&quot;Cambria Math&quot;;</jats:p>
     <jats:p>mso-hansi-font-family:&quot;Times New Roman&quot;;mso-bidi-font-family:&quot;Times New Roman&quot;;</jats:p>
     <jats:p>font-style:italic;mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;REWMA</jats:p>
     <jats:p>style='mso-bidi-font-style:normal'&gt;</jats:p>
     <jats:p>&quot;Cambria Math&quot;,serif;mso-bidi-font-family:&quot;Times New Roman&quot;'&gt;N chart is highly sensitive to persistent shifts in the scaling parameter of the neutrosophic Rayleigh distribution. Monte Carlo simulations are conducted to compare the suggested scheme with the existing model. A comparative study indicates that the proposed chart outperforms the competing design, particularly in detecting smaller shifts. Finally, we provide a charting structure for the proposed design using daily average wind speed data, which can be used as a practical implementation guideline for real-world applications.</jats:p>
    </jats:abstract>
    <publication_date media_type="online">
     <year>2024</year>
    </publication_date>
    <pages>
     <first_page>59</first_page>
     <last_page>72</last_page>
    </pages>
    <publisher_item>
     <item_number item_number_type="article-number">2230</item_number>
    </publisher_item>
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     <ai:license_ref applies_to="vor">https://creativecommons.org/licenses/by/4.0/</ai:license_ref>
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    <doi_data>
     <doi>10.54216/IJNS.230105</doi>
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