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<Article>
<Journal>
				<PublisherName>University of Tehran Press</PublisherName>
				<JournalTitle>Desert</JournalTitle>
				<Issn>2008-0875</Issn>
				<Volume>17</Volume>
				<Issue>2</Issue>
				<PubDate PubStatus="epublish">
					<Year>2012</Year>
					<Month>12</Month>
					<Day>01</Day>
				</PubDate>
			</Journal>
<ArticleTitle>Determining Area Affected by Dust Storms in Different Wind
Speeds, Using Satellite Images</ArticleTitle>
<VernacularTitle></VernacularTitle>
			<FirstPage>193</FirstPage>
			<LastPage>202</LastPage>
			<ELocationID EIdType="pii">32035</ELocationID>
			
<ELocationID EIdType="doi">10.22059/jdesert.2013.32035</ELocationID>
			
			<Language>EN</Language>
<AuthorList>
<Author>
					<FirstName>M.R.</FirstName>
					<LastName>Ekhtesasi</LastName>
<Affiliation>Associate professor, Yazd University, Yazd, Iran</Affiliation>

</Author>
<Author>
					<FirstName>Z.</FirstName>
					<LastName>Gohari</LastName>
<Affiliation>MSc. Graduate, Yazd University, Yazd, Iran</Affiliation>

</Author>
</AuthorList>
				<PublicationType>Journal Article</PublicationType>
			<History>
				<PubDate PubStatus="received">
					<Year>2011</Year>
					<Month>03</Month>
					<Day>02</Day>
				</PubDate>
			</History>
		<Abstract>The aim of this study is to determine the area affected by dust storms in different wind speeds using satellite&lt;br /&gt;images. In the first step, windy conditions of the Sistan plain were analyzed using wind statistics data. Next, five&lt;br /&gt;stormy days of Zabol city, indicating different wind speeds and horizontal visibilities during those storms, were&lt;br /&gt;selected. Then, high temporal resolution MODIS data was used as appropriate satellite data in this study. After that, a&lt;br /&gt;storm index was defined by means of analyses of storm radiance profile in bands with maximum and minimum storm&lt;br /&gt;reflection. The index is the square of difference between visible and thermal infrared bands, which is able to segment&lt;br /&gt;stormy confines with the range of reflection changes between 0 and 16. The reflection values were segmented in&lt;br /&gt;center of a 1 km2 network using usual interpolation methods such as Local Polynomial, Radial Basis Function,&lt;br /&gt;Inverse Distance Weighted, Ordinary Kriging and Universal Kriging. In order to assess the above mentioned&lt;br /&gt;interpolation methods, validation techniques were applied using ArcGIS 9.2 software. The result of these assessments&lt;br /&gt;such as standard deviation method indicates that the Ordinary Kriging had lower standard deviation. By analyzing the&lt;br /&gt;variograms and spatial analysis of the data using GS+ software, the best mathematic model able to fit the points was&lt;br /&gt;selected and classification was done by using this model. Finally, the stormy corridors with different dust densities&lt;br /&gt;were determined and by calculating the area and determining the villages located in these corridors, the critical&lt;br /&gt;regions were recognized. In this study the data from visible bands (4 and 9) and thermal band (21) of the MODIS&lt;br /&gt;sensor shows better results compared with the other bands, to segment and classify relative density of dust storms.&lt;br /&gt;Moreover, variographic analysis of the satellite data indicates that in most of the dust storms, power models with&lt;br /&gt;spherical threshold is the best for interpolation.</Abstract>
		<ObjectList>
			<Object Type="keyword">
			<Param Name="value">Dust Storm</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Dust density</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">remote sensing</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Geostatistics</Param>
			</Object>
			<Object Type="keyword">
			<Param Name="value">Kriging</Param>
			</Object>
		</ObjectList>
<ArchiveCopySource DocType="pdf">https://jdesert.ut.ac.ir/article_32035_361cd104e809ec1db56bcb6b311a8321.pdf</ArchiveCopySource>
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