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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>7</Volume>
				<Issue>1</Issue>
				<PubDate PubStatus="epublish">
					<Year>2020</Year>
					<Month>04</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Omori’s Law in the Occurrence of Solar Flare : Approach of Hybrid Model</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>11</FirstPage>
			<LastPage>18</LastPage>
			<ELocationID EIdType="pii">180</ELocationID>
			
<ELocationID EIdType="doi">10.22128/ijaa.2020.399.1079</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Amin </FirstName>
					<LastName>Najafi</LastName>
<Affiliation>Department of Basic Science, Faculty of Shahid Mofateh, Hamedan Branch, Technical &amp;amp;amp;amp;amp;amp;amp; Vocational University (TVU), Hamedan, Iran</Affiliation>
<Identifier Source="ORCID">0000-0002-0496-8743</Identifier>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2021</Year>
					<Month>04</Month>
					<Day>05</Day>
				</PubDate>
			</History>
		<Abstract>Solar flares are large-scale phenomena that have a significant effect on the&lt;br /&gt;Earth’s climate. Using the solar flare time series from January 1, 2006 to July 21, 2016,&lt;br /&gt;we develop a complex network for predicting solar flares. In the work, hybrid model&lt;br /&gt;is employed to construct complex network. In addition to the position of the flares&lt;br /&gt;and their occurrence times, the energy of events based on the Telesca-lovallo model&lt;br /&gt;is also used to develop solar flare network. Using constructed complex network, the&lt;br /&gt;Omori’s law for fore flare and after flares associated with a main flare are retrieved. The&lt;br /&gt;frequency of occurrence of solar flares decreases over time as a power law. Statistical&lt;br /&gt;analysis of flaring events catalogues indicates that a power-law dependence characterizes&lt;br /&gt;the occurrence of both fore flares and after flares corresponding to a main flare. The&lt;br /&gt;hybrid model reconstructs the Omori’s law for fore flare–after flare process associated&lt;br /&gt;with a main event.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Solar Flare</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Complex Network</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Hybrid Model</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Omori’s Law</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijaa.du.ac.ir/article_180_ff54f8b8df9ccefc5c4ef0fb519cd8ee.pdf</ArchiveCopySource>
</Article>
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