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<ArticleSet>
<Article>
<Journal>
				<PublisherName>Damghan University Press</PublisherName>
				<JournalTitle>Iranian Journal of Astronomy and Astrophysics</JournalTitle>
				<Issn>2322-4924</Issn>
				<Volume>12</Volume>
				<Issue>2</Issue>
				<PubDate PubStatus="epublish">
					<Year>2025</Year>
					<Month>09</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Numerical Study of Magnetoacoustic Wave Interaction with Null Points: Plasma Beta Modulation in Solar Atmospheres</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>143</FirstPage>
			<LastPage>161</LastPage>
			<ELocationID EIdType="pii">1913</ELocationID>
			
<ELocationID EIdType="doi">10.22128/ijaa.2025.2992.1216</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Naser </FirstName>
					<LastName>Karimi</LastName>
<Affiliation>Department of Physics Education, P.O. Box 14665-889, Frahangian  University, Tehran, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Mahdi </FirstName>
					<LastName>Alizadeh</LastName>
<Affiliation>Independant researcher, Tabriz, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Zianab </FirstName>
					<LastName>Shajei</LastName>
<Affiliation>Physics Department, Payame Noor University, Tehran, 19395-3697, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Ehsan </FirstName>
					<LastName>Tavabi</LastName>
<Affiliation>Physics Department, Payame Noor University, Tehran, 19395-3697</Affiliation>
<Identifier Source="ORCID">0000-0001-9602-0767</Identifier>

</Author>
<Author>
					<FirstName>Navid </FirstName>
					<LastName>Elyasi</LastName>
<Affiliation>Department of Electrical Engineering, Chalmers University of Technology, Gothenburg, Sweden</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2025</Year>
					<Month>07</Month>
					<Day>15</Day>
				</PubDate>
			</History>
		<Abstract>This investigation examines the interaction of magnetoacoustic pulses with a two-dimensional magnetic null point, explicitly accounting for variations in plasma β arising from spatial fluctuations in the magnetic field strength. The analysis employs the PLUTO code to solve the magnetohydrodynamic (MHD) equations, enabling a detailed exploration of nonlinear effects associated with plasma β modulation across distinct stratified layers. The results demonstrate temporal evolution in the system’s response, characterized by periodic fluctuations in amplitude and the emergence of pronounced peaks. These features indicate episodes of intensified coupling between the magnetoacoustic pulses and the magnetic topology. The observed variability in both amplitude and peak sharpness underscores the system’s inherent dynamism, with certain temporal phases exhibiting more vigorous interactions. Furthermore, the study reveals a correlation between plasma density alterations and radial velocity variations of the pulses, suggesting that these phenomena are closely tied to the redistribution of plasma β throughout the stratified magnetic environment.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Sun</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Magnetohydrodynamics</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Magnetoacoustic Wave Dynamics</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">2D Magnetic Null Point</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Plasma beta</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijaa.du.ac.ir/article_1913_41e2a3c0396c6d50fc7ad8898d244454.pdf</ArchiveCopySource>
</Article>
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