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<!DOCTYPE ArticleSet PUBLIC "-//NLM//DTD PubMed 2.7//EN" "https://dtd.nlm.nih.gov/ncbi/pubmed/in/PubMed.dtd">
<ArticleSet>
<Article>
<Journal>
				<PublisherName>University of Tehran</PublisherName>
				<JournalTitle>Journal of Solar Energy Research</JournalTitle>
				<Issn>2588-3097</Issn>
				<Volume>4</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2019</Year>
					<Month>01</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>CFD analysis of solar chimney power plant: Effect of chimney height, shape and collector size</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>61</FirstPage>
			<LastPage>71</LastPage>
			<ELocationID EIdType="pii">70911</ELocationID>
			
<ELocationID EIdType="doi">10.22059/jser.2019.70911</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>R.</FirstName>
					<LastName>Bhoraniya</LastName>
<Affiliation>Marwadi Education Foundation Group of Institutions, Rajkot, India</Affiliation>

</Author>
<Author>
					<FirstName>M.</FirstName>
					<LastName>Jiren</LastName>
<Affiliation>Marwadi Education Foundation Group of Institutions, Rajkot, India</Affiliation>

</Author>
<Author>
					<FirstName>A.</FirstName>
					<LastName>Harichandan</LastName>
<Affiliation>Marwadi Education Foundation Group of Institutions, Rajkot, India</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2019</Year>
					<Month>04</Month>
					<Day>22</Day>
				</PubDate>
			</History>
		<Abstract>This paper presents computational fluid dynamics (CFD) simulation of the solar&lt;br /&gt; chimney power plant to analyze to analyze buoyancy-nature of heated air by har-&lt;br /&gt; nessing solar energy. ANSYS Fluent a finite volume code has been used for axisym-&lt;br /&gt; metric model of the solar chimney power plant (SCPP) prototype in Manzanares,&lt;br /&gt; Spain considering updraft tower. A standard k- turbulence model and Boussinesq&lt;br /&gt; approximation for buoyancy driven flow is considered. Small pressure difference because of natural draft inside the chimney during day time has been observed due&lt;br /&gt; to solar radiation. The numerical results obtained for average velocity and temper-&lt;br /&gt; ature at chimney inlet are validated with the experimental results of the prototype.&lt;br /&gt; It has been observed that both the velocity and temperature of air inside the SCPP&lt;br /&gt; increases significantly with the increment in solar radiation. Increase in the chimney&lt;br /&gt; height and collector radius also increases the power output of the plant. The effect&lt;br /&gt; of chimney convergence with different area ratio on the power output of SCCPs have&lt;br /&gt; been analyzed</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Solar chimney</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">CFD</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">collector, area ratio</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">turbulence model</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Solar radiation</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://jser.ut.ac.ir/article_70911_2c28d223baab3f21a96ce4b643e18299.pdf</ArchiveCopySource>
</Article>
</ArticleSet>
