<?xml version="1.0" encoding="utf-8"?>
<ags:resources xmlns:ags="http://purl.org/agmes/1.1/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:agls="http://www.naa.gov.au/recordkeeping/gov_online/agls/1.2" xmlns:dcterms="http://purl.org/dc/terms/">
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[مرادی, علی سیاهکالی]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[میرزایی, نوربخش]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[رضاپور, مهدی]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[Attenuation relationships]]></dc:subject>
				<dc:subject><![CDATA[Epicentral distance]]></dc:subject>
				<dc:subject><![CDATA[Iran]]></dc:subject>
				<dc:subject><![CDATA[Isoseismal map]]></dc:subject>
				<dc:subject><![CDATA[Seismic intensity]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[The isoseismal maps for 22 earthquakes in different regions of Iran were analyzed to study the attenuation of seismic intensity with the distance from the epicentre under a certain surface wave magnitude (Ms). The attenuation relationships were derived by using an iterative least squares fit procedure. These equations were derived from more basic concepts assuming that the intensity is proportional to the logarithm of seismic energy density at any location empirically. The isoseismal maps are elongated in the direction of local structural trend of causative faults. Therefore, attenuation relationships for the main direction of fault, transverse to it and average attenuation were derived. 
Ia =11.564 + 0.943M — 2.508Ln(Ra + 33) a = 0.79 Ra]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10873_483505f348b9b17287c787c2e715e950.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[امامی, کسری]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[ریاحی, محمد علی]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[Complex structures]]></dc:subject>
				<dc:subject><![CDATA[Depth migration]]></dc:subject>
				<dc:subject><![CDATA[Lateral velocity]]></dc:subject>
				<dc:subject><![CDATA[Prestack]]></dc:subject>
				<dc:subject><![CDATA[Seismic image]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[The migration process removes the effect of wave propagation from the recorded seismic data. As an application of this operator, seismic events will move towards their correct positions, diffractions have to collapse and dipping events have to move to their correct subsurface locations. 
In this article different algorithms of the migration operator have been considered and applied on real data. Based on the results, the Kirchhoff migration, which is the most common algorithm, was chosen and used to apply for pre-stack depth migration on real data. The data obtained from an oil field in the southern part of Iran. Subsequently the obtained results were compared]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10874_ec698306c39c2fb225e5d03803195d1e.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[نادری, اصغر]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[جواهریان, عبدالرحیم]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[زاده, علیرضا گلال]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[Common offset records]]></dc:subject>
				<dc:subject><![CDATA[Dip move out]]></dc:subject>
				<dc:subject><![CDATA[Dipping reflector]]></dc:subject>
				<dc:subject><![CDATA[Normal move out]]></dc:subject>
				<dc:subject><![CDATA[Shot records]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[In conventional seismic reflection technique to improve the signal to noise ratio processing steps perform in common midpoint (CDP) gathers. To remove the effects of the offset normal move out correction, the operator does not perform well through reflectors which have intersecting dips beneath the surface. In this case, the dip move out operator will be able to remove the effect of the dip. All the known dip-move out (DM0) algorithms that are not integral methods require seismic data to be sorted in regularly sampled constant-offset sections. Sometimes sorting data is time consuming and difficult. In contrast, DM0 in shot profiles can be applied directly to shot records. The shot-DMO operator is space- variant and time-variant. After a logarithmic transformation the time and the space coordinates, the operator becomes time-invariant and space-invariant. In this paper, shot-DMO operator was used for a 2-D seismic line of central Iran. Field data show that the shot-DMO method yields stacked sections better than stacked sections with f-k DM0 for constant- offset sections.]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10875_5508c827fd828aafcaf5916e8eaa30e3.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[بیدحتی, عباسعلی علی اکبری]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[د, فاطمه مالکی فر]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[Boussinesq approximation]]></dc:subject>
				<dc:subject><![CDATA[Entertainment and gravity current]]></dc:subject>
				<dc:subject><![CDATA[Froude number]]></dc:subject>
				<dc:subject><![CDATA[Negative buoyancy]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10876_47cb9892a61163945dfc0a10206f8504.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[الحجه, علیرضا محب]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[مشایخی, رباب]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[barotropic primitive]]></dc:subject>
				<dc:subject><![CDATA[Imbalanced part]]></dc:subject>
				<dc:subject><![CDATA[Numerical algorithm]]></dc:subject>
				<dc:subject><![CDATA[Potential enstrophy]]></dc:subject>
				<dc:subject><![CDATA[Potential vorticity]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[In quantitative and qualitative assessment of the numerical algorithms for barotropic primitative equations, comparision with the real atmosphere can not be used as the main criterion to determine the accuracy of the algorithms. This holds particularly for limited-area applications when boundary conditions add to the difficulties of determining the true solution. The complexity comes from a combinations of the barotropic primitive model error, the numerical algorithm error, and errors in the way data are assimilated to the model. It is thus necessary to use ever increasingly our dynamical knowledge of the behavior of the solutions of the barotropic primitive, or shallow water, equations in the process of determining the accuracy of numerical algorithms. A useful approach here is to study balanced (vortical) and imbalanced (gravity waves) parts of the flows, and their interaction. In spite of the limitations faced when working with real-atmosphere data, such study can uncover some important information on the working of the algorithms. Having this objective in mind, the present paper is devoted to the study of spatio-temporal behavior of balanced and imbalanced parts in three numerical algorithms for the regional barotropic primitive equation. The algorithms are: the potential enstrophy conserving Eulerian algorithm of Sadoumy (1975), and two algorithms derived from Sadoumy’s algorithm by simply changing the prognostic variables from :momentum-geopotential height to (i) Rossby potential vorticity (PV), divergence, geopotential height, (ii) PV, divergence, and ageostrophic vorticity. In the latter two algorithms, PV is solved by a standard semi-Lagrangian method using piecewise bicubic interpolation and the other prognostic variables are solved by the proper use of Sadoumy’s algorithm for momentum components and geopotential height. Compared with the Eulerian algorithm of Sadourny, the PV-based algorithm shows a marked improvement in the representation of both balanced and imbalanced parts of the flow.]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10877_0865fd19f407149e3a6a70c6ab86434a.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[مرید, سعید]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[ا.ک.گوساین, ]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[و.ا.ک‘کشاری, ]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[Snowmelt simulation]]></dc:subject>
				<dc:subject><![CDATA[SWAT Model]]></dc:subject>
				<dc:subject><![CDATA[Synthetic climate data]]></dc:subject>
				<dc:subject><![CDATA[Ungauged catchments]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[Snowmelt-runoff simulation is an important concern in different aspects of snowy watershed management. But data scarcity is often an obstacle in such a simulation. Inadequate data has restricted the modelers to employ simpler methods. The present paper is aimed at modeling ungauged snowy catchments with more complicated methods, wherein the required data has been generated. For this objective the SWAT (Soil and Water Assessment tool), Degree-Day, SRM, and SNOW17 are identified for detailed evaluations, which are combinations of temperature, temperature-radiation and energy budget based methods. These methods have been programmed and linked with the SWAT model so as to take advantage of SWAT weather data generation capability, and also to ensure uniformity in evaluation of the snowmelt algorithms. Off line performance evaluation of these selected modules has been carried out for the Ammameh watershed in Iran. The results show better performance of the energy budget method using synthesized data, compared with solely simple temperature-based method.]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10878_69b16b84b7bd0417c15a39d9d0977198.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[اردستانى., وحید ابراهیم زاده]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[Anomaly detection]]></dc:subject>
				<dc:subject><![CDATA[depth estimation]]></dc:subject>
				<dc:subject><![CDATA[Microgravity]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[A microgravity investigation was conducted on an excavated foundation located in the Technical University of Tehran. The aim was the detection of subsurface cavities or other anomalous conditions that threaten the stability of the foundation. The survey consists of 420 gravity stations. The positive coarse grain alluvium saturated by surplus water and negative cavity anomalies have been detected based on the Bouguer and second vertical derivative maps. The depth of the sources have also been determined. To confirm the results an inversion 2D-modelling is also applied to residual anomalies. Some of the shallow accessible anomalies have been confirmed in the field by excavation.]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10879_61a552855b8b20819ab3c9a1baaded2b.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[آقایی, امید]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[ریاحی, محمد علی]]></ags:creatorPersonal>
<ags:creatorPersonal><![CDATA[ندری, داریوش]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[Depth migration]]></dc:subject>
				<dc:subject><![CDATA[modeling]]></dc:subject>
				<dc:subject><![CDATA[Picking phase]]></dc:subject>
				<dc:subject><![CDATA[Travel time inversion]]></dc:subject>
				<dc:subject><![CDATA[Velocity model]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[Travel time inversion has been used in this study in order to obtain a velocity model. This velocity model has been used in a depth migration algorithm afterwards. 
To achieve this purpose three main steps are as follows: picking phases, forward modeling, inverse modeling and finally using an appropriate depth migration algorithm to apply to the data.]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10880_064810850b276e23c3b2ecc5705172b7.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>
<ags:resource>
					<dc:title><![CDATA[-]]></dc:title>
					<dc:creator>
					<ags:creatorPersonal><![CDATA[قیطانچی, محمد رضا]]></ags:creatorPersonal>

			</dc:creator>
			<dc:publisher>
				<ags:publisherName><![CDATA[Institute of Geophysics, University of Tehran]]></ags:publisherName>
			</dc:publisher>
			<dc:date><dcterms:dateIssued><![CDATA[2004]]></dcterms:dateIssued></dc:date>
				<dc:subject><![CDATA[active faults]]></dc:subject>
				<dc:subject><![CDATA[Changoureh-Avaj (southern Qazvin) earthquake]]></dc:subject>
				<dc:subject><![CDATA[Rupture process]]></dc:subject>
				<dc:subject><![CDATA[source mechanism]]></dc:subject>
				<dc:subject><![CDATA[Source parameters]]></dc:subject>
				<dc:subject><![CDATA[Waveform modeling]]></dc:subject>
			<dc:description>
				<ags:descriptionNotes><![CDATA[Includes references]]></ags:descriptionNotes>
				<dcterms:abstract><![CDATA[]]></dcterms:abstract>
			</dc:description>
            <dc:identifier scheme="dcterms:URI"><![CDATA[https://jesphys.ut.ac.ir/article_10881_7b66328e94a0f3af7a759f5d2f74da9d.pdf]]></dc:identifier>
			<dc:identifier scheme="ags:DOI"><![CDATA[]]></dc:identifier>
			<dc:type><![CDATA[Journal Article]]></dc:type>
			<dc:format><dcterms:medium><![CDATA[text]]></dcterms:medium></dc:format>
			<dc:language><![CDATA[فارسی]]></dc:language>
			<dc:source><![CDATA[https://jesphys.ut.ac.ir/]]></dc:source>
			<dc:source><![CDATA[Journal of the Earth and Space Physics]]></dc:source>
		</ags:resource>

</ags:resources>