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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>1</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2014</Year>
					<Month>06</Month>
					<Day>18</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Solar Mini-Dimming Kinematics and Their Positive Correlations with Coronal Mass Ejections and Prominence</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>57</FirstPage>
			<LastPage>63</LastPage>
			<ELocationID EIdType="pii">5</ELocationID>
			
<ELocationID EIdType="doi">10.22128/ijaa.2014.5</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Nasibe </FirstName>
					<LastName>Alipour</LastName>
<Affiliation>Department of Physics, University of Zanjan, Zanjan, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Hossein </FirstName>
					<LastName>Safari</LastName>
<Affiliation>Department of Physics, University of Zanjan, Zanjan, Iran</Affiliation>
<Identifier Source="ORCID">0000-0003-2326-3201</Identifier>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2014</Year>
					<Month>06</Month>
					<Day>18</Day>
				</PubDate>
			</History>
		<Abstract>Solar mini-dimmings can be detect in the Extreme Ultra-Violet coronal eruptions. Here, sequences of 171_A images taken by Solar Dynamic Observatory/Atmospheric Imaging Assembaly on 13 June 2010 are used. In this special day, both of coronal mass ejection and prominence were observed. The average velocities and accelerations of 500 mini-dimmings which were detected using on feature based classifier (Alipour et al 2012) [1] are studied. The large number of mini-dimmings shows positive accelerations in the beginning times as similar as Coronal Mass Ejections. On the the start time of prominence eruptions, the number of mini-dimmings is increased to a maximum values. There is a positive correlation between the kinematics of mini-dimmings and both CME and prominences. This study can be extended to understand the exact relationship of CMEs and mini-dimmings.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Sun: CMEs</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">mini-dimming</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">prominence</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijaa.du.ac.ir/article_5_df04addb0c4c296bd3f2c6d2b553b020.pdf</ArchiveCopySource>
</Article>
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