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Ora Shale Formation

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The <span class="search-highlight">Ora</span> <span class="search-highlight">Shale</span> <span class="search-highlight">Formation</span> in the type section (after R.  Wetzel, 1950 ) overl...
Published: 01 January 2007
Figure 19: The Ora Shale Formation in the type section (after R. Wetzel, 1950 ) overlies the Kaista Formation and underlies the Harur Formation. R. Wetzel considered the age of the Kaista Formation as either Late Devonian or early Carboniferous (Mississippian). More recent palynology studies
Journal Article
Journal: GeoArabia
Publisher: Gulf Petrolink
Published: 01 April 1998
GeoArabia (1998) 3 (2): 229–248.
... Devonian to Lower Carboniferous Ora Shale Formation, and the lower shaly beds of the Upper Permian Chia Zairi Formation. The main target reservoirs are of Ordovician, Silurian, Carboniferous and Permian ages. Similar reservoirs have recently been reported for the Western Desert of Iraq, eastern Jordan...
FIGURES | View All (8)
Image
The Harur <span class="search-highlight">Formation</span> in the type section (after R.  Wetzel, 1950 ) overlies ...
Published: 01 January 2007
Figure 22: The Harur Formation in the type section (after R. Wetzel, 1950 ) overlies the Ora Shale Formation and underlies the Permian Chia Zairi Formation. R. Wetzel considered the age of the Harur Formation as early Carboniferous (early Tournaisian). This is consistent with palynological
Journal Article
Journal: GeoArabia
Publisher: Gulf Petrolink
Published: 01 January 2007
GeoArabia (2007) 12 (1): 63–130.
...Figure 19: The Ora Shale Formation in the type section (after R. Wetzel, 1950 ) overlies the Kaista Formation and underlies the Harur Formation. R. Wetzel considered the age of the Kaista Formation as either Late Devonian or early Carboniferous (Mississippian). More recent palynology studies...
FIGURES | View All (41)
Image
Geologic column. Note the <span class="search-highlight">Ora</span> <span class="search-highlight">formation</span> (about 110 m thick) within a sedime...
Published: 01 August 2002
Figure 2 Geologic column. Note the Ora formation (about 110 m thick) within a sedimentary sequence (1500 m thick). As described in the right-hand column, the Ora formation includes an upper shale unit (~30 m thick), a middle carbonaceous unit (~20 m thick), and a lower shaly unit (~60 m thick
Journal Article
Journal: GeoArabia
Publisher: Gulf Petrolink
Published: 01 April 1998
GeoArabia (1998) 3 (2): 417–418.
... sequence is correctly translated from Al-Haba et al. (1994) to be 358 meters (m) thick in Akkas-1, and to correspond to the Kaista, Ora and Harur formations. In their original figure the section is shown as Tournaisian to Namurian and to consist of sandstone and shale. Also in Figure 2...
FIGURES
Journal Article
Journal: GSA Bulletin
Published: 01 August 1997
GSA Bulletin (1997) 109 (8): 1021–1035.
... differences in deformation style as a function of lithology, this study focuses on the progressive development of flexural-slip horizons and fabric development in extensional settings. Deformation in the intercalated shale, siltstone, carbonate, and gypsum beds of the Turonian Ora Formation is dominated...
Image
Thickness of the lower Carboniferous (Mississippian) Tournaisian <span class="search-highlight">Ora</span> <span class="search-highlight">Format</span>...
Published: 01 January 2007
Figure 21: Thickness of the lower Carboniferous (Mississippian) Tournaisian Ora Formation in northwest Iraq (after Al-Hadidy, 2001 ). The formation consists of marine shales and minor carbonates ( Figures 7 , 15 , 17 , 19 and 20 ). Towards Syria the formation may become dominated
Image
Cross section showing a conceptual model based on competency rather than li...
Published: 01 August 2002
to a duplex with internal complexities due to the competent units within the Ora formation.
Journal Article
Journal: AAPG Bulletin
Published: 01 August 2002
AAPG Bulletin (2002) 86 (8): 1367–1381.
...Figure 2 Geologic column. Note the Ora formation (about 110 m thick) within a sedimentary sequence (1500 m thick). As described in the right-hand column, the Ora formation includes an upper shale unit (~30 m thick), a middle carbonaceous unit (~20 m thick), and a lower shaly unit (~60 m thick...
FIGURES | View All (10)
Image
In the Khleisia-1 well the Silurian Akkas <span class="search-highlight">Formation</span> is 152 m thick and much...
Published: 01 January 2007
Figure 7: In the Khleisia-1 well the Silurian Akkas Formation is 152 m thick and much thinner than in Akkas-1 where it is 864 m thick ( Figure 6 . As in Akkas-1, the GR log shows the two hot shales in the Hoseiba Member (API > 100). Also seen in Khleisia-1 are the Pirispiki, Kaista, Ora
Image
Waterfall exposures (see  Figures 3a  and  4  for locations). (a) Northern ...
Published: 01 August 2002
of the lower member of the Ora formation has been reduced to less than 0.5 m in a few localities. The marly limestone layers within the carbonate-bearing unit have been faulted and jointed. The faults are of both reverse and normal types. Some isolated layers at the bottom of the sequence show boudinage
Image
Waterfall exposures (see  Figures 3a  and  4  for locations). (a) Northern ...
Published: 01 August 2002
of the lower member of the Ora formation has been reduced to less than 0.5 m in a few localities. The marly limestone layers within the carbonate-bearing unit have been faulted and jointed. The faults are of both reverse and normal types. Some isolated layers at the bottom of the sequence show boudinage
Image
Index of the intersection of the NW Zagros Trend with the Aziz-Bashiqa Inve...
Published: 01 October 2010
Formation, (b) Cambrian Sosink Formation, (c) Ordovician Bedinan Formation, (d) Ordovician Khabour Formation, (e) Lower Carboniferous Kaista Formation, (f) Upper Devonian Pirispiki Formation and the Lower Carboniferous Ora Shale and Harur Limestone, and (g) Permian Chia Zairi Limestone. Despite
Journal Article
Journal: AAPG Bulletin
Published: 01 June 2014
AAPG Bulletin (2014) 98 (6): 1071–1090.
... grainstone (IRb), (3) fossiliferous wackestone-packstone (MRa), (4) massive to bedded chert (MRb), (5) spiculitic wackestone-packstone (MRc), (6) silty mudstone-wackestone (ORa), (7) glauconitic siltstone-sandstone (ORb), and (8) shale (ORc). The eight lithofacies are grouped into three facies associations...
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Journal Article
Journal: Palynology
Published: 01 January 2008
Palynology (2008) 32 (1): 183–204.
... with carbonaceous clays and muds (Text-Figures 2 , 3 ). These sediments span the boundary between the Nanafalia and Tuscahoma formations of the Wilcox Group. There are no diagnostic marine fossils such as calcareous nannoplankton or planktonic foraminifera to date these deposits. If the Red Hills Mine succession...
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Journal Article
Published: 01 April 2004
Mineralogical Magazine (2004) 68 (2): 255–277.
.... It lies near the base of a major cycle of mafic to ultramafic volcanics, which is separated from underlying cycles by thin units of banded iron formation, carbonaceous shale and chert ( Hronsky et al. , 1990 ). Locally the deposit is hosted by carbonaceous schist and minor basalt and dolerite...
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Journal Article
Journal: AAPG Bulletin
Published: 01 January 1991
AAPG Bulletin (1991) 75 (1): 108–120.
... ) in the Jauf, Qasim, and Tabuk areas in Saudi Arabia, Oman, and southwestern and central Iran. Lithology key boundary ages as in Figure 5 . The Lower Silurian shales of the Ghakum Formation ( Figure 7 , Appendix 1) occur at Kuh-e-Faraghan near Bandar Abbas in the Zagros Mountains (A. Allison, 1937...
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Journal Article
Journal: Clay Minerals
Published: 01 June 2006
Clay Minerals (2006) 41 (2): 637–658.
... of 1st bed below GYP 53 L. Cenomanian 94±3 GYP 53 13280/00815 yellow marl Hazera Tamar 2 m below top of Mbr. L. Cenomanian 94±3 GYP 54 13275/00845 light coloured clayey 1st Ora Shale Lower 1 m above base of Mbr. L. Cenomanian 94±3 There was no significant difference...
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Journal Article
Journal: AAPG Bulletin
Published: 01 April 2015
AAPG Bulletin (2015) 99 (4): 617–637.
... of clastic sediments, that is, sandstone and shale. Possible source rocks of the Paleozoic petroleum system consist of several dark-shale intervals, including the regionally widespread Silurian Akkas hot shale, in addition to those of the Ordovician Khabour and Ora formations ( Al-Juboury and Al-Hadidy, 2009...
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