Modeling velocity dispersion In Gypsy site, Oklahoma

Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2010. Cataloged from PDF version of thesis. Includes bibliographical references (p. 73-76). Discrepancies in interval velocities estimated from vertical well measurements made with different so...

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Main Author: Alsaadan, Sami Ibrahim
Other Authors: M. Nafi Toksöz and Daniel R. Burns., Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences.
Format: Thesis
Language:English
Published: Massachusetts Institute of Technology 2010
Subjects:
Online Access:http://hdl.handle.net/1721.1/62484
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spelling ftmit:oai:dspace.mit.edu:1721.1/62484 2023-06-11T04:16:24+02:00 Modeling velocity dispersion In Gypsy site, Oklahoma Alsaadan, Sami Ibrahim M. Nafi Toksöz and Daniel R. Burns. Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences. n-us-ok 2010 91 p. application/pdf http://hdl.handle.net/1721.1/62484 eng eng Massachusetts Institute of Technology http://hdl.handle.net/1721.1/62484 712066297 M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582 Earth Atmospheric and Planetary Sciences Thesis 2010 ftmit 2023-05-29T08:22:22Z Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2010. Cataloged from PDF version of thesis. Includes bibliographical references (p. 73-76). Discrepancies in interval velocities estimated from vertical well measurements made with different source central frequencies at Gypsy site could be primarily explained in terms of intrinsic attenuation. Four intervals were chosen for this study based on varying rock properties. The first interval is predominantly shale, second interval is mostly sandstone, and the third interval is made up of shale and sandstone. The fourth interval is the second and third intervals combined. The data used are acquired from three seismic sources; Full Wave Sonic (FWS), Bender log, and Vertical Seismic Profile (VSP) with estimated central frequencies 10kHz, 1kHz, and 100Hz, respectively. The modeling was done using the Discrete Wavenumber (DWN) method and the Logarithmic Dispersion Relation (LDR) to calculate a constant Quality Factor (Q) that best explains the observed velocity dispersion for each of the intervals of interest. The elastic scattering component of the dispersion is negligible. Intrinsic quality factors of 54,35,28, and 30 best explain the field data for first, second, third, and fourth intervals, respectively. The identification and subsequent modeling of velocity dispersion and its components provide key information for integrated reservoir characterization and better enable the prediction of the seismic response at different frequencies. by Sami Ibrahim Alsaadan. S.M. Thesis sami DSpace@MIT (Massachusetts Institute of Technology)
institution Open Polar
collection DSpace@MIT (Massachusetts Institute of Technology)
op_collection_id ftmit
language English
topic Earth
Atmospheric
and Planetary Sciences
spellingShingle Earth
Atmospheric
and Planetary Sciences
Alsaadan, Sami Ibrahim
Modeling velocity dispersion In Gypsy site, Oklahoma
topic_facet Earth
Atmospheric
and Planetary Sciences
description Thesis (S.M.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2010. Cataloged from PDF version of thesis. Includes bibliographical references (p. 73-76). Discrepancies in interval velocities estimated from vertical well measurements made with different source central frequencies at Gypsy site could be primarily explained in terms of intrinsic attenuation. Four intervals were chosen for this study based on varying rock properties. The first interval is predominantly shale, second interval is mostly sandstone, and the third interval is made up of shale and sandstone. The fourth interval is the second and third intervals combined. The data used are acquired from three seismic sources; Full Wave Sonic (FWS), Bender log, and Vertical Seismic Profile (VSP) with estimated central frequencies 10kHz, 1kHz, and 100Hz, respectively. The modeling was done using the Discrete Wavenumber (DWN) method and the Logarithmic Dispersion Relation (LDR) to calculate a constant Quality Factor (Q) that best explains the observed velocity dispersion for each of the intervals of interest. The elastic scattering component of the dispersion is negligible. Intrinsic quality factors of 54,35,28, and 30 best explain the field data for first, second, third, and fourth intervals, respectively. The identification and subsequent modeling of velocity dispersion and its components provide key information for integrated reservoir characterization and better enable the prediction of the seismic response at different frequencies. by Sami Ibrahim Alsaadan. S.M.
author2 M. Nafi Toksöz and Daniel R. Burns.
Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences.
format Thesis
author Alsaadan, Sami Ibrahim
author_facet Alsaadan, Sami Ibrahim
author_sort Alsaadan, Sami Ibrahim
title Modeling velocity dispersion In Gypsy site, Oklahoma
title_short Modeling velocity dispersion In Gypsy site, Oklahoma
title_full Modeling velocity dispersion In Gypsy site, Oklahoma
title_fullStr Modeling velocity dispersion In Gypsy site, Oklahoma
title_full_unstemmed Modeling velocity dispersion In Gypsy site, Oklahoma
title_sort modeling velocity dispersion in gypsy site, oklahoma
publisher Massachusetts Institute of Technology
publishDate 2010
url http://hdl.handle.net/1721.1/62484
op_coverage n-us-ok
genre sami
genre_facet sami
op_relation http://hdl.handle.net/1721.1/62484
712066297
op_rights M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission.
http://dspace.mit.edu/handle/1721.1/7582
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