Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content

Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-or...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Banat, Khaled M. [verfasserIn] Basyoni, Mohammed H. Zeidan, Rashad H.

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	1997

Schlagwörter:	Dolomite Jurassic Anhydrite Evaporite Grainstone

Anmerkung:	© Springer 1997

Übergeordnetes Werk:	Enthalten in: Carbonates and evaporites - [Dordrecht [u.a.]] : Springer Netherlands, 1986, 12(1997), 1 vom: März, Seite 117-124
Übergeordnetes Werk:	volume:12 ; year:1997 ; number:1 ; month:03 ; pages:117-124

Links:	Volltext

DOI / URN:	10.1007/BF03175810

Katalog-ID:	SPR030654297

Internformat


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100	1		\|a Banat, Khaled M. \|e verfasserin \|4 aut
245	1	0	\|a Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content
264		1	\|c 1997
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520			\|a Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm.
650		4	\|a Dolomite \|7 (dpeaa)DE-He213
650		4	\|a Jurassic \|7 (dpeaa)DE-He213
650		4	\|a Anhydrite \|7 (dpeaa)DE-He213
650		4	\|a Evaporite \|7 (dpeaa)DE-He213
650		4	\|a Grainstone \|7 (dpeaa)DE-He213
700	1		\|a Basyoni, Mohammed H. \|4 aut
700	1		\|a Zeidan, Rashad H. \|4 aut
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773	1	8	\|g volume:12 \|g year:1997 \|g number:1 \|g month:03 \|g pages:117-124
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912			\|a GBV_ILN_95
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912			\|a GBV_ILN_105
912			\|a GBV_ILN_110
912			\|a GBV_ILN_120
912			\|a GBV_ILN_138
912			\|a GBV_ILN_150
912			\|a GBV_ILN_151
912			\|a GBV_ILN_152
912			\|a GBV_ILN_161
912			\|a GBV_ILN_170
912			\|a GBV_ILN_171
912			\|a GBV_ILN_187
912			\|a GBV_ILN_213
912			\|a GBV_ILN_224
912			\|a GBV_ILN_230
912			\|a GBV_ILN_250
912			\|a GBV_ILN_281
912			\|a GBV_ILN_285
912			\|a GBV_ILN_293
912			\|a GBV_ILN_370
912			\|a GBV_ILN_381
912			\|a GBV_ILN_602
912			\|a GBV_ILN_636
912			\|a GBV_ILN_702
912			\|a GBV_ILN_2001
912			\|a GBV_ILN_2003
912			\|a GBV_ILN_2004
912			\|a GBV_ILN_2005
912			\|a GBV_ILN_2006
912			\|a GBV_ILN_2007
912			\|a GBV_ILN_2008
912			\|a GBV_ILN_2009
912			\|a GBV_ILN_2010
912			\|a GBV_ILN_2011
912			\|a GBV_ILN_2014
912			\|a GBV_ILN_2015
912			\|a GBV_ILN_2020
912			\|a GBV_ILN_2021
912			\|a GBV_ILN_2025
912			\|a GBV_ILN_2026
912			\|a GBV_ILN_2027
912			\|a GBV_ILN_2031
912			\|a GBV_ILN_2034
912			\|a GBV_ILN_2037
912			\|a GBV_ILN_2038
912			\|a GBV_ILN_2039
912			\|a GBV_ILN_2044
912			\|a GBV_ILN_2048
912			\|a GBV_ILN_2049
912			\|a GBV_ILN_2050
912			\|a GBV_ILN_2055
912			\|a GBV_ILN_2057
912			\|a GBV_ILN_2059
912			\|a GBV_ILN_2061
912			\|a GBV_ILN_2064
912			\|a GBV_ILN_2065
912			\|a GBV_ILN_2068
912			\|a GBV_ILN_2088
912			\|a GBV_ILN_2093
912			\|a GBV_ILN_2106
912			\|a GBV_ILN_2107
912			\|a GBV_ILN_2108
912			\|a GBV_ILN_2110
912			\|a GBV_ILN_2111
912			\|a GBV_ILN_2112
912			\|a GBV_ILN_2113
912			\|a GBV_ILN_2118
912			\|a GBV_ILN_2129
912			\|a GBV_ILN_2143
912			\|a GBV_ILN_2144
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912			\|a GBV_ILN_2152
912			\|a GBV_ILN_2153
912			\|a GBV_ILN_2188
912			\|a GBV_ILN_2190
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912			\|a GBV_ILN_2336
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912			\|a GBV_ILN_4249
912			\|a GBV_ILN_4251
912			\|a GBV_ILN_4305
912			\|a GBV_ILN_4306
912			\|a GBV_ILN_4307
912			\|a GBV_ILN_4313
912			\|a GBV_ILN_4322
912			\|a GBV_ILN_4323
912			\|a GBV_ILN_4324
912			\|a GBV_ILN_4325
912			\|a GBV_ILN_4326
912			\|a GBV_ILN_4333
912			\|a GBV_ILN_4334
912			\|a GBV_ILN_4335
912			\|a GBV_ILN_4336
912			\|a GBV_ILN_4338
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951			\|a AR
952			\|d 12 \|j 1997 \|e 1 \|c 03 \|h 117-124

Indexfelder

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matchkey_str	article:18785212:1997----::aeuascaeemadlmtsnetasuirbaagti
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publishDate	1997
allfields	10.1007/BF03175810 doi (DE-627)SPR030654297 (SPR)BF03175810-e DE-627 ger DE-627 rakwb eng Banat, Khaled M. verfasserin aut Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content 1997 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Springer 1997 Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm. Dolomite (dpeaa)DE-He213 Jurassic (dpeaa)DE-He213 Anhydrite (dpeaa)DE-He213 Evaporite (dpeaa)DE-He213 Grainstone (dpeaa)DE-He213 Basyoni, Mohammed H. aut Zeidan, Rashad H. aut Enthalten in Carbonates and evaporites [Dordrecht [u.a.]] : Springer Netherlands, 1986 12(1997), 1 vom: März, Seite 117-124 (DE-627)617505799 (DE-600)2533885-7 1878-5212 nnns volume:12 year:1997 number:1 month:03 pages:117-124 https://dx.doi.org/10.1007/BF03175810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 12 1997 1 03 117-124
spelling	10.1007/BF03175810 doi (DE-627)SPR030654297 (SPR)BF03175810-e DE-627 ger DE-627 rakwb eng Banat, Khaled M. verfasserin aut Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content 1997 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Springer 1997 Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm. Dolomite (dpeaa)DE-He213 Jurassic (dpeaa)DE-He213 Anhydrite (dpeaa)DE-He213 Evaporite (dpeaa)DE-He213 Grainstone (dpeaa)DE-He213 Basyoni, Mohammed H. aut Zeidan, Rashad H. aut Enthalten in Carbonates and evaporites [Dordrecht [u.a.]] : Springer Netherlands, 1986 12(1997), 1 vom: März, Seite 117-124 (DE-627)617505799 (DE-600)2533885-7 1878-5212 nnns volume:12 year:1997 number:1 month:03 pages:117-124 https://dx.doi.org/10.1007/BF03175810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 12 1997 1 03 117-124
allfields_unstemmed	10.1007/BF03175810 doi (DE-627)SPR030654297 (SPR)BF03175810-e DE-627 ger DE-627 rakwb eng Banat, Khaled M. verfasserin aut Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content 1997 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Springer 1997 Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm. Dolomite (dpeaa)DE-He213 Jurassic (dpeaa)DE-He213 Anhydrite (dpeaa)DE-He213 Evaporite (dpeaa)DE-He213 Grainstone (dpeaa)DE-He213 Basyoni, Mohammed H. aut Zeidan, Rashad H. aut Enthalten in Carbonates and evaporites [Dordrecht [u.a.]] : Springer Netherlands, 1986 12(1997), 1 vom: März, Seite 117-124 (DE-627)617505799 (DE-600)2533885-7 1878-5212 nnns volume:12 year:1997 number:1 month:03 pages:117-124 https://dx.doi.org/10.1007/BF03175810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 12 1997 1 03 117-124
allfieldsGer	10.1007/BF03175810 doi (DE-627)SPR030654297 (SPR)BF03175810-e DE-627 ger DE-627 rakwb eng Banat, Khaled M. verfasserin aut Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content 1997 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Springer 1997 Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm. Dolomite (dpeaa)DE-He213 Jurassic (dpeaa)DE-He213 Anhydrite (dpeaa)DE-He213 Evaporite (dpeaa)DE-He213 Grainstone (dpeaa)DE-He213 Basyoni, Mohammed H. aut Zeidan, Rashad H. aut Enthalten in Carbonates and evaporites [Dordrecht [u.a.]] : Springer Netherlands, 1986 12(1997), 1 vom: März, Seite 117-124 (DE-627)617505799 (DE-600)2533885-7 1878-5212 nnns volume:12 year:1997 number:1 month:03 pages:117-124 https://dx.doi.org/10.1007/BF03175810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 12 1997 1 03 117-124
allfieldsSound	10.1007/BF03175810 doi (DE-627)SPR030654297 (SPR)BF03175810-e DE-627 ger DE-627 rakwb eng Banat, Khaled M. verfasserin aut Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content 1997 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Springer 1997 Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm. Dolomite (dpeaa)DE-He213 Jurassic (dpeaa)DE-He213 Anhydrite (dpeaa)DE-He213 Evaporite (dpeaa)DE-He213 Grainstone (dpeaa)DE-He213 Basyoni, Mohammed H. aut Zeidan, Rashad H. aut Enthalten in Carbonates and evaporites [Dordrecht [u.a.]] : Springer Netherlands, 1986 12(1997), 1 vom: März, Seite 117-124 (DE-627)617505799 (DE-600)2533885-7 1878-5212 nnns volume:12 year:1997 number:1 month:03 pages:117-124 https://dx.doi.org/10.1007/BF03175810 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_381 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 AR 12 1997 1 03 117-124
language	English
source	Enthalten in Carbonates and evaporites 12(1997), 1 vom: März, Seite 117-124 volume:12 year:1997 number:1 month:03 pages:117-124
sourceStr	Enthalten in Carbonates and evaporites 12(1997), 1 vom: März, Seite 117-124 volume:12 year:1997 number:1 month:03 pages:117-124
format_phy_str_mv	Article
institution	findex.gbv.de
topic_facet	Dolomite Jurassic Anhydrite Evaporite Grainstone
isfreeaccess_bool	false
container_title	Carbonates and evaporites
authorswithroles_txt_mv	Banat, Khaled M. @@aut@@ Basyoni, Mohammed H. @@aut@@ Zeidan, Rashad H. @@aut@@
publishDateDaySort_date	1997-03-01T00:00:00Z
hierarchy_top_id	617505799
id	SPR030654297
language_de	englisch
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author	Banat, Khaled M.
spellingShingle	Banat, Khaled M. misc Dolomite misc Jurassic misc Anhydrite misc Evaporite misc Grainstone Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content
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topic_title	Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content Dolomite (dpeaa)DE-He213 Jurassic (dpeaa)DE-He213 Anhydrite (dpeaa)DE-He213 Evaporite (dpeaa)DE-He213 Grainstone (dpeaa)DE-He213
topic	misc Dolomite misc Jurassic misc Anhydrite misc Evaporite misc Grainstone
topic_unstemmed	misc Dolomite misc Jurassic misc Anhydrite misc Evaporite misc Grainstone
topic_browse	misc Dolomite misc Jurassic misc Anhydrite misc Evaporite misc Grainstone
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title	Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content
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title_full	Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content
author_sort	Banat, Khaled M.
journal	Carbonates and evaporites
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container_start_page	117
author_browse	Banat, Khaled M. Basyoni, Mohammed H. Zeidan, Rashad H.
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format_se	Elektronische Aufsätze
author-letter	Banat, Khaled M.
doi_str_mv	10.1007/BF03175810
title_sort	late jurassic-late permian dolomites in central saudi arabia: ca:mg stoichiometry and sr-content
title_auth	Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content
abstract	Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm. © Springer 1997
abstractGer	Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm. © Springer 1997
abstract_unstemmed	Abstract A difference in the depositional environments of the Upper Permian and the Upper Jurassic carbonate rocks exposed in central Saudi Arabia led to a difference in the initial dolomite geochemistry; i.e. Ca: Mg stoichiometry and Sr-content. The Khuff dolomites are characterized by: (i) well-ordering (high R-value) (ii) stoichiometric nature (with an average $ CaCO_{3} $ of about 1 mole %) (iii) and low Sr-content (from 55 ppm to 183 ppm) relative to Holocene marine dolomites. The Khuff carbonates were deposited in a sabkha-like, hypersaline environment, where the increased salinity favored the precipitation of a better-ordered and more stoichiometric dolomite than would be expected to form had the dolomites formed in a normal marine environment. Later recrystallization of the Khuff dolomite also may have increased the degree of ordering in the dolomites. The low strontium content in the Khuff dolomite could have been due to depletion during diagenetic modification of the initially precipitated non-ideal Khuff dolomite. Jubaila carbonates were formed in a normal marine environment, where the source of $ Mg^{+2} $ responsible for the dolomitization of its upper part is related to the prograding of the supratidal sabkha front formed at the terminal Jubaila stages. The Jubaila dolomites are relatively poorly ordered with a $ CaCO_{3} $ content of 7 mole % and an average Sr-content of 241 ppm. © Springer 1997
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title_short	Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content
url	https://dx.doi.org/10.1007/BF03175810
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author2	Basyoni, Mohammed H. Zeidan, Rashad H.
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up_date	2024-07-03T19:21:31.002Z
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Late Jurassic-Late Permian dolomites in central Saudi Arabia: Ca:Mg stoichiometry and Sr-content

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