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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>9</Volume>
				<Issue>2</Issue>
				<PubDate PubStatus="epublish">
					<Year>2022</Year>
					<Month>10</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Recent Data of Extensive Air Showers Recorded by Alborz I Array and Their Detailed Analysis</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>135</FirstPage>
			<LastPage>147</LastPage>
			<ELocationID EIdType="pii">342</ELocationID>
			
<ELocationID EIdType="doi">10.22128/ijaa.2022.698.1151</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>Mahmud </FirstName>
					<LastName>Bahmanabadi</LastName>
<Affiliation>Physics Department, Sharif University of Technology, Tehran, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Mostafa </FirstName>
					<LastName>Heydarizad</LastName>
<Affiliation>Alborz Observatory‎, ‎Sharif University of Technology‎, ‎PO Box 11155-9161‎, ‎Tehran‎, ‎Iran</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2023</Year>
					<Month>07</Month>
					<Day>15</Day>
				</PubDate>
			</History>
		<Abstract>An array of five scintillation detectors has been installed in Sharif University of Technology to record extensive air showers. ‎‎‎By using the time lags of the secondary particles of air showers relative to each other and the location of each of these ‎particles‎ relative to the core of the shower, the arrival direction of the primary particle producing each air shower has been ‎obtained.‎&lt;br /&gt;&lt;br /&gt;‎‎These data show that the distribution of time intervals of successive events in all directions of arrival into‎ the atmosphere is a random distribution‎. The distribution of the time intervals between successive events in different ‎seasons‎ has also been obtained and the seasonal effect has been ‎investigated‎. The effects of the environment‎, ‎including temperature and pressure‎, on the cosmic ray count rate have been investigated‎. ‎The distribution of zenith and azimuth angles‎, ‎as well as‎ the ‎solar,‎ sidereal, and antisidereal time distributions of cosmic rays‎, ‎have been obtained‎.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">‎ Cosmic rays‎ Extensive air shower‎</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">‎ R‎ andom ‎ events</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://ijaa.du.ac.ir/article_342_122d6959964c024de4eae7f9c4f3c6c7.pdf</ArchiveCopySource>
</Article>
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