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<ArticleSet>
<Article>
<Journal>
				<PublisherName>Amirkabir University of Technology</PublisherName>
				<JournalTitle>AUT Journal of Mechanical Engineering</JournalTitle>
				<Issn>2588-2937</Issn>
				<Volume>10</Volume>
				<Issue>4</Issue>
				<PubDate PubStatus="epublish">
					<Year>2026</Year>
					<Month>10</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Thermal-Dependent 2-D Magneto-Micropolar Fluid Flow over Stretching Surfaces in Porous Media: OHAM-Based Analysis with Viscous Dissipation and Radiation Effects</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage></FirstPage>
			<LastPage></LastPage>
			<ELocationID EIdType="pii">6055</ELocationID>
			
<ELocationID EIdType="doi">10.22060/ajme.2026.24746.6228</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Hussain</FirstName>
					<LastName>Basha</LastName>
<Affiliation>Department of Mathematics, Government First Grade College, Zalaki-586204, Vijayapur, Karnataka, India</Affiliation>
<Identifier Source="ORCID">0000-0003-4470-2074</Identifier>

</Author>
<Author>
					<FirstName>V.</FirstName>
					<LastName>Ramanjini</LastName>
<Affiliation>Department of Mathematics, Government First Grade College, Lingasuguru, Raichur –584 122, Karnataka, India</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>09</Month>
					<Day>15</Day>
				</PubDate>
			</History>
		<Abstract>In this study, the convective transport of a temperature-dependent magneto-micropolar fluid over a stretching surface embedded in a porous medium is examined. The formulation accounts for viscous dissipation, internal heat generation or absorption, and radiative heat transfer modeled through the Rosseland diffusion approximation, which is appropriate for optically thick media. The governing equations, developed without the use of similarity transformations, are solved using the Optimal Homotopy Analysis Method (OHAM). The resulting velocity, microrotation, and temperature fields are illustrated through graphical and tabulated data across a broad range of physical parameters. Validation against existing literature demonstrates the reliability of the present approach. Quantitative analysis shows that the microrotation boundary layer decreases by approximately 18–25% with increasing micropolar parameter, while thermal boundary layer thickness increases by about 10–14% under stronger radiative effects. Moreover, micropolar fluids exhibit a thinner momentum boundary layer compared to Newtonian fluids under identical conditions. Specifically, the Newtonian case yields a thinner layer relative to the micropolar case . Overall, the results provide valuable insights into micropolar fluid behavior with practical implications in porous and radiative flow systems.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">magneto-micropolar fluid</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">viscous dissipation</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Thermal Radiation</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">heat generation or absorption</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">OHAM</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ajme.aut.ac.ir/article_6055_5cd7edbe7a1a668fdc63c138002cc43a.pdf</ArchiveCopySource>
</Article>
</ArticleSet>
