<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">OJG</journal-id><journal-title-group><journal-title>Open Journal of Geology</journal-title></journal-title-group><issn pub-type="epub">2161-7570</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/ojg.2017.76059</article-id><article-id pub-id-type="publisher-id">OJG-77337</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Earth&amp;Environmental Sciences</subject></subj-group></article-categories><title-group><article-title>
 
 
  Reservoir Characterization and Pore Type Systems of Carbonate Low Resistivity Pay in Persian Gulf
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bita</surname><given-names>Arbab</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Davod</surname><given-names>Jahani</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Bahram</surname><given-names>Movahed</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Geology, Basic Science Faculty, North Tehran Branch, Islamic Azad University, Tehran, Iran</addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>bitaarbab@yahoo.com(BA)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>02</day><month>06</month><year>2017</year></pub-date><volume>07</volume><issue>06</issue><fpage>859</fpage><lpage>870</lpage><history><date date-type="received"><day>March</day>	<month>24,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>June</month>	<year>27,</year>	</date><date date-type="accepted"><day>June</day>	<month>30,</month>	<year>2017</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  The main focus of study is to characterize lower and upper cretaceous carbonate deposits with Low Resistivity Pay, in Persian Gulf. Four oil reservoirs in the Cretaceous including the Zubair, Buwaib, Shuaiba and Khatiyah Formations of Southern fields have been analyzed. Here is a look at that to determine main factors on decreasing resistivity in pay zone. In some intervals resistivity responses reach less than 6 to 1 ohm
  &amp;#183;m. Significant hydrocarbon accumulations are “hidden” in low resistivity Pay zone, (LRPZ). LRPZ reservoirs have been found in some formations in Persian Gulf. Causes of LRPZ reservoirs on the basis of experimental analysis include clay-coated grains, carbonate with interstitial dispersed clay. On the other side Smectite and Kaolinite of main clays types have high CEC and greater impact on lowering resistivity. Micritization and Pyritization of digenetic process have noticeable impact on LRPZ. It is mentioned that L
  &amp;#248;n
  &amp;#248;y method applied to address pore throat sizes which contain Inter crystalline porosity, Chalky Limestone, Mudstone micro porosity. Pore systems are classified at class 2 and 3 Lucia and pore size varies from 0.5 to 4 micron. NMR Core and Log results show different pore size distribution. NMR core and MRIL results explain that decreasing of resistivity in pay zone is related to texture and grain size variation not being existence of moved water. Irreducible water estimate for this reservoir was between 30% and 50%. T2 cut off estimates, for defining irreducible water saturation, 115 ms.
 
</p></abstract><kwd-group><kwd>Clay Types</kwd><kwd> CEC</kwd><kwd> Micritization</kwd><kwd> Low Resistivity Pay Zone</kwd><kwd> Lucia</kwd><kwd> L&amp;#248;n&amp;#248;y Method</kwd><kwd> NMR</kwd><kwd> Pore Size and Irreducible Water</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>This paper discusses the causes and location of LRLC pay zones, summarizes some of LRPZ examples. The examples are from Wells data of Balal, Salman and Reshadat fields from southern of Persian Gulf. Khatiyah (Cenomanian), Shuaiba (Aptian), Zubair and Buawib (Barreminan) formations have been selected for reservoir studying. The reservoir characterization of low resistivity pay has been challenging due to high reservoir heterogeneity [<xref ref-type="bibr" rid="scirp.77337-ref1">1</xref>] . The pay zone includes carbonate reservoirs that resistivity logs have a resistivity between 6 to 1 ohm-me- ters and even in some intervals reach less than 1 ohm・m. Due to influence of digenetic effects, determination of pore type size and pore distribution has significant impact. Current study shows that decreasing resistivity is related to texture changes not having movable water. In addition, the type of clay has a main role on resistivity response. Smectite is main clay types of mentioned formations. Smectite and Montmorillonite have high CEC (cation exchange capacity) and greater impact on lowering resistivity [<xref ref-type="bibr" rid="scirp.77337-ref2">2</xref>] . For each reservoirs microfacies analysis, digenetic process, rock fabric and pore systems have been defined.</p></sec><sec id="s2"><title>2. Geological Setting</title><p>In Persian Gulf region the cretaceous succession are normally divided into three distinct parts. At the beginning of the Cretaceous global sea level was relatively high and consequently most of the Basin accumulated almost exclusively shallow-marine carbonates of Tamama group (<xref ref-type="fig" rid="fig1">Figure 1</xref>). The Basin was rapidly in filled, first bycarbonates and later by terrigenous clastic of Buwaib, Zubair and</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Stratigraphic column from the lower, middle, upper cretaceous</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x2.png"/></fig><p>Biyadh formations consequently. The Zubair carbonate (lithostratigraphic equivalents of Gadvan Formation) is considered to have good reservoir potential in Persian Gulf. This formation is one of subordinate reservoir rocks in the Persian Gulf Basin. Buwaib Formation is characterized by inter-bedded porous carbonate and tight argillaceous limestones or marls. The formation is lithostratigraphic equivalent of the Ratawi Formation of Kuwait and Gadvan Formation in Iran [<xref ref-type="bibr" rid="scirp.77337-ref3">3</xref>] . The Buwaib Formation and its equivalents host prolific oil reserves in a number of the Persian Gulf countries, particularly in Saudi Arabia, Kuwait, and UAE [<xref ref-type="bibr" rid="scirp.77337-ref4">4</xref>] . In Iran, the Gadvan Formation forms good oil reservoirs, mainly in the Abadan Plain (e.g., Azadegan, Jufair, Sepehr, and Yadavaran fields), southern Dezful Embayment (Chahar Bisheh, Gulkhari, and Chilingar fields) and northwest of the Persian Gulf (Arash, Soroosh, Nowruz, and Ferdowsi fields). In the Persian Gulf, the Hauterivian reservoirs are known as the Khalij member and Dictioconous carbonates [<xref ref-type="bibr" rid="scirp.77337-ref5">5</xref>] .</p><p>During middle Aptian carbonate platform were deposited with pellet bioclastic limestone in intershelf deeper water in south and north Persian Gulf in south pars this sediment are Shuaiba (dariyan) reservoir rock in cretaceous. After rising sea level at Aptian carbonate platform extended in early Albian with decline of water sediment extended in open marine as kazhdumi and Burgan. The Aptian carbonates Shuaiba Formation) forms prolific reservoirs in the eastern Persian Gulf, particularly in the UAE. This formation is overlain by the marls and clastics of NahrUmr Formation and underlain by the Kharaib carbonates, in this area. The Algal mounds and rudist buildup facies are the most productive zones, while karstified carbonates in the uppermost parts of the formation are other important oil-bearing intervals in the Shuaiba Formation [<xref ref-type="bibr" rid="scirp.77337-ref4">4</xref>] . In the UAE, the Shuaiba Formation, with thickness ranging from 45 to 145 m, consists of two informal and one formal member: the lower Shuaiba and upper Shuaiba members and the Bab Member, in ascending order. It is characterized as a prograding Orbitolina-dominated platform that surrounded the interior-shelf (Bab Basin) in the offshore of UAE.</p><p>During the middle cretaceous in late Albian-Cenomanian time the khatiyah (Sarvak of Iran) inter shelf basin formed in the southern part of Persian Gulf. The khatiyah consists of calcareous shales grading upward into argillaceous plagic lime mudstone with abundant calcisphere and planktonic formainifera. It overlies Maddud formation and locally is equivalent to upper Sarvak formation.</p></sec><sec id="s3"><title>3. Studying Method</title><p>We use available data such as thin sections, electrical well logs, NMR logs and core data to define quality of reservoir. Fully water saturated plugs were centrifuged in air using small capillary pressure steps, then the saturation profile along the length of the core was imaged using NMR. The NMR profiles clearly displayed a structural heterogeneity which influenced the fluid distribution. Along with additional data from formation pressure and down-Hole fluid sampling analysis were used. For pore size distribution, method L&#248;n&#248;y (2006) has been applied.</p></sec><sec id="s4"><title>4. Causes of LRLC Reservoirs</title><sec id="s4_1"><title>4.1. Clay Types</title><p>Clay minerals with their water-filled micro porosity and their ability to exchange cations contained within pore fluids are the most common causes of LRLC reservoirs [<xref ref-type="bibr" rid="scirp.77337-ref6">6</xref>] . Clays, in order of their highest to lowest exchange capacity and therefore their effect on suppression of electrical logs, are Smectite (Kaolinite), mixed-Layer Smectite (Kaolinite), Illite, Montmorillonite. Distribution clay minerals in cross plot Thorium potassium and XRD results (<xref ref-type="fig" rid="fig2">Figure 2</xref>, <xref ref-type="fig" rid="fig3">Figure 3</xref> and <xref ref-type="table" rid="table1">Table 1</xref>). The cause of the low resistivity is the presence of high cation exchange capacity clay minerals, which also have high irreducible water saturation Intervals. It can also be caused by features like Glauconitic pellets and more than 5 percent conductive materials such as pyrite. Digenetic Process like Micritization, emphasis that quality of the reservoir is influenced by various digenetic process such as Micrtization and Pyritization which have noticeable impact on declining resistivity. Porosity varies between interparticle, moldic and mudstone microporosity.</p></sec><sec id="s4_2"><title>4.2. Main Digenetic Features on Resistivity Response</title><p>Petrographic evidence indicated that Formation was subjected to different diagenetic processes with variable intensities. This formation has been buried to a</p><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Thorium potassium cross plot for clay types. Plot shows that a type of clay of mixed Illite, Montmorillonite and kaolinite for LRPZ formation</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x3.png"/></fig><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> XRD results of core sample data for Buwaib formation</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x4.png"/></fig><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> XRD results of Khatiyah formation shows a mixed layer Illite-Smectite is a randomly interstratified type with approximately 60% Smectite interlayers</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Depth (m)</th><th align="center" valign="middle" >Plug/Shale</th><th align="center" valign="middle" >Illite-Smectite</th><th align="center" valign="middle" >Kaolinite</th><th align="center" valign="middle" >Chlorite</th></tr></thead><tr><td align="center" valign="middle" >1317.4</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0</td><td align="center" valign="middle" >0</td></tr><tr><td align="center" valign="middle" >1321.8</td><td align="center" valign="middle" >shale</td><td align="center" valign="middle" >23</td><td align="center" valign="middle" >25</td><td align="center" valign="middle" >15</td></tr><tr><td align="center" valign="middle" >1322.81</td><td align="center" valign="middle" >30</td><td align="center" valign="middle" >26</td><td align="center" valign="middle" >15</td><td align="center" valign="middle" >13</td></tr><tr><td align="center" valign="middle" >1324.9</td><td align="center" valign="middle" >Shale</td><td align="center" valign="middle" >31</td><td align="center" valign="middle" >14</td><td align="center" valign="middle" >16</td></tr><tr><td align="center" valign="middle" >1326.18</td><td align="center" valign="middle" >36</td><td align="center" valign="middle" >39</td><td align="center" valign="middle" >trace</td><td align="center" valign="middle" >15</td></tr></tbody></table></table-wrap><p>depth of more than 2.4 km (intermediate burial realm) and has experienced micritization, bioturbation, cementation, dissolution and compaction as the main diagenetic alterations.</p><p>As an earlier diagenetic process, micritization has affected the carbonate grains in the studied formation (<xref ref-type="fig" rid="fig4">Figure 4</xref>(b), <xref ref-type="fig" rid="fig4">Figure 4</xref>(c) and <xref ref-type="fig" rid="fig4">Figure 4</xref>(e)). Micritized skeletal fragments are very common in the lagoonal and shoal facies (as reworked grains). Some of the uncertain grains (peloids) have formed during the complete micritization. It seems that after deposition, bioclasts were partially or completely micritized by endolithic and other microbes (micro-borer organisms) on the sea floor. This process commonly occurs in relatively low-energy, shallow-marine environments [<xref ref-type="bibr" rid="scirp.77337-ref7">7</xref>] [<xref ref-type="bibr" rid="scirp.77337-ref8">8</xref>] . Pyrite mineralization: Pyrite (FeS2) is present as barrow filling and authigenic diagenetic mineral (scattered opaque minerals both on the bioclasts and in the rock matrix). It occurs as cubic crystals with fine sizes (less than 0.3 mm). Pyritization is also seen in the bioclast grains (<xref ref-type="fig" rid="fig4">Figure 4</xref>(a), <xref ref-type="fig" rid="fig4">Figure 4</xref>(d) and <xref ref-type="fig" rid="fig4">Figure 4</xref>(g)). Occurrence of pyrite in organic-rich sediments indicate that this mineral may be formed by sulfate reducing bacteria (SRB), under anaerobic condition, although most of the pyrites in sedimentary rocks are of diagenetic origin [<xref ref-type="bibr" rid="scirp.77337-ref8">8</xref>] . Compaction: On the basis of its burial depth (&gt;2 km) and evident compaction features, it seems that the Buwaib Formation has affected by compaction with various degrees in shallow to deep burial realms. Compaction features, such as solution seams, stylolites and compaction</p><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Digenetic features on reservoir carbonate</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x5.png"/></fig><p>gash fractures, are recorded in the both core samples and thin sections of the formation (<xref ref-type="fig" rid="fig4">Figure 4</xref>(f) and <xref ref-type="fig" rid="fig4">Figure 4</xref>(h)). Our observations have revealed that lithology (particularly clay content) exert the main control on the distribution of stylolite and seam solutions in the studied intervals. Stylolites are very common in the limestone and porous facies, particularly lithocodium-bearing facies, whereas solution seams are commonly seen in the argillaceous limestone facies these features are mostly parallel to the bedding planes. Horse-tail structures are also present. The evidence indicated that main parts of the porosity were destroyed during burial and compaction (and also through cementation). Development of pressure solution features requires a depth of more than 500 m. This process reflects the compaction due to the heavy sedimentary cover (&gt;1 km thickness), which indicating burial diagenesis.</p></sec><sec id="s4_3"><title>4.3. Pore Type System</title><p>The most widely used pore-type classification systems for carbonate reservoirs are limited by the fact that the relation between porosity and permeability is poorly defined. Existing classification schemes for porosity-permeability data do not, in many cases, optimally integrate sedimentology, diagenesis, and flow-re- lated properties. In many carbonate reservoirs, it is therefore difficult to generate predictive models for reservoir-quality distribution, resulting insignificant uncertainty in hydrocarbon reserve calculations. Porosity distribution is a major new element in the classification. Winland and Lucia’s subdivision of inter particle porosity has been partly incorporated into the new classification system [<xref ref-type="bibr" rid="scirp.77337-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.77337-ref10">10</xref>] (<xref ref-type="fig" rid="fig5">Figure 5</xref>), but is now based on pore size instead of grain size and sorting. L&#248;n&#248;y method [<xref ref-type="bibr" rid="scirp.77337-ref11">11</xref>] applied to address pore throat sizes which contain Inter crystalline porosity, Chalky Limestone, Mudstone micro porosity. Pore systems are classified at class 2 and 3 Lucia and pore size varies from 0.5 to 4 micron. Pore types, are introduced: mudstone microporosity Interparticle, micromoldic and micromoldic. Mudstone micropores have extremely small pore sizes, commonly a few micrometers in diameter. Individual pores cannot be seen with a standard petrographic microscope.</p><p>However, because of the extremely small pore sizes and variable pore structure (interparticle), these pores were classified as a separate pore-type class (<xref ref-type="fig" rid="fig6">Figure 6</xref> and <xref ref-type="fig" rid="fig7">Figure 7</xref>). Mudstone microporosity includes both true chalks and chalky microporosity. Chalk micropores are primary in origin and occur between grains of planktonic calcareous algae (coccospheres) or their component crystal plates (coccoliths). Chalky micropores are not related to chalk, but the pore structure is similar [<xref ref-type="bibr" rid="scirp.77337-ref10">10</xref>] . These pores occur between recrystallized mud particles and may be formed either during early meteoric leaching or deeper burial diagenesis. The pores typically form in low-energy, muddy, platform-interior facies.</p></sec><sec id="s4_4"><title>4.4. Reservoir Characterization</title><p>Examples of petrophysical evaluation for Khatiyah, Shuiaba and Buawib formations, Mineral responses defines based on petrophysical tools (<xref ref-type="table" rid="table2">Table 2</xref>). Base on core data and NMR data these formations should be controlled to define precisely water saturation. 2 samples of MICP results for Khatiyah formation show water saturation is 20% to 45% (<xref ref-type="fig" rid="fig8">Figure 8</xref>).</p><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Porosity permeability plots shows with Winland method class 2 and 3 Lucia for reservoirs with low resistivity pay zones</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x6.png"/></fig><fig-group id="fig6"><label><xref ref-type="fig" rid="fig6">Figure 6</xref></label><caption><title> Pore systems of Buwaib formation. Interparticle Lucia 2 and 3 have been defined.</title></caption><fig id ="fig6_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x7.png"/></fig><fig id ="fig6_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x8.png"/></fig></fig-group><fig-group id="fig7"><label><xref ref-type="fig" rid="fig7">Figure 7</xref></label><caption><title> Pore systems of Zubair formation in interparticle microporosity class 3 Lucia.</title></caption><fig id ="fig7_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x9.png"/></fig><fig id ="fig7_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x10.png"/></fig></fig-group><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Real responses for petrophysical evaluation to define precisely porosity and water saturation</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >Mineral responses</th><th align="center" valign="middle" >RHOB</th><th align="center" valign="middle" >NPHI</th><th align="center" valign="middle" >DT</th><th align="center" valign="middle" >U</th><th align="center" valign="middle" >CGR</th><th align="center" valign="middle" >GR</th></tr></thead><tr><td align="center" valign="middle" >Kaolinite (wet clay)</td><td align="center" valign="middle" >2.43</td><td align="center" valign="middle" >0.58</td><td align="center" valign="middle" >98</td><td align="center" valign="middle" >4.99</td><td align="center" valign="middle" >100</td><td align="center" valign="middle" >200</td></tr><tr><td align="center" valign="middle" >Illite (wet clay)</td><td align="center" valign="middle" >2.5</td><td align="center" valign="middle" >0.25</td><td align="center" valign="middle" >101.3</td><td align="center" valign="middle" >10</td><td align="center" valign="middle" >150</td><td align="center" valign="middle" >160</td></tr><tr><td align="center" valign="middle" >Montmoriollinte (wet clay)</td><td align="center" valign="middle" >2.2</td><td align="center" valign="middle" >0.45</td><td align="center" valign="middle" >105</td><td align="center" valign="middle" >4</td><td align="center" valign="middle" >150</td><td align="center" valign="middle" >160</td></tr></tbody></table></table-wrap><fig-group id="fig8"><label><xref ref-type="fig" rid="fig8">Figure 8</xref></label><caption><title> MICP results of LRP show water saturation between 20 to 60 percent.</title></caption><fig id ="fig8_1"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x12.png"/></fig><fig id ="fig8_2"><label></label><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x11.png"/></fig></fig-group><p>It should be noted resistivity response these formations are very low (<xref ref-type="fig" rid="fig9">Figure 9</xref> and <xref ref-type="fig" rid="fig1">Figure 1</xref>0).</p><p>Nuclear magnetic resonance (NMR) refers to the response of atomic nuclei to magnetic fields. NMR measurements show pore-size distribution; the presence of clay, vugs; hydrocarbon properties such as viscosity; and grain-size. Knowing the value of T2 cutoff enables the amount of mobile and bound fluids to be calculated from log data. The T2 cutoff is the size boundary between small pores containing bound fluid and larger pores where the fluid is free. While various rock types have standard T2 cutoff values, the geometry of the pores and the rock’s mineralogy may shift the T2 spectrum, so laboratory core analysis experiments are used to determine the value of T2 cutoff.</p><p>MRIL (Magnetic Resolution Imager Log) spectrums indicate high volume of irreducible bound water; there is also some free fluid porosity which is mainly water with a little oil in some interval oil and water are identified [<xref ref-type="bibr" rid="scirp.77337-ref12">12</xref>] . Porosity spectrum also show that the total porosity is about 20% - 25% in the reservoir intervals as well as permeability varies between 5 to 200 md. In order to define water saturation precisely for the reservoir, T2 Cut off define 115 microseconds related to micro porosity carbonate to define. Irreducible water saturation defined 30% to 50% in reservoir interval. Combination between full set logs and NMR logs with NMR core results (<xref ref-type="fig" rid="fig1">Figure 1</xref>0). Water saturation varies between 35% to 50% results extract based on 15 core samples selected for NMR analysis in oil brine and air brine condition to get information about pore size Clay bound water, Moved oil and water and residual water saturation.</p><fig id="fig9"  position="float"><label><xref ref-type="fig" rid="fig9">Figure 9</xref></label><caption><title> Petrophysical evaluation of Khatiyah formation based on well logs an. Track 1 displays Gamma ray and Caliper, track 2 shows resistivity track 3 for density and neutron response track 4 lithology calculation, track 6 and 7 display fluid calculation. Resistivity is near to 1 ohm meter. Intervals show hydrocarbon Pay zone. Water saturation calibrate with MICP results</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x13.png"/></fig></sec></sec><sec id="s5"><title>5. Conclusions</title><p>The lower and upper cretaceous carbonate Formations are of main producing oil carbonates in the Persian Gulf. Four oil reservoirs in the Cretaceous from the Zubair, Buwaib, Shuaiba and Khatiyah formations of Southern fields have susceptible for LRP formations. Majority of the response resistivity logs are between 1 to 6 ohm・m.</p><p>Geological core analysis (XRD) and standard petrophysical cross plots show that dispersed clay types and conductive minerals like pyrite are most reason for LRP reservoir. Smectite and Illite are main clay types that Smectite has high CEC (Cation exchange capacity) and greater impact on lowering resistivity.</p><p>Petrographic evidence indicated that Formation was subjected to different diagenetic processes with variable intensities. Reservoir quality is under digenetic process such as pyritization, micritization and bioturbation.</p><fig id="fig10"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref>0</label><caption><title> Combination between full set logs and NMR logs with NMR core results. Water saturation varies between 35% to 50% results extract based on 15 core samples selected for NMR analysis in oil brine and air brine condition to get information about pore size clay bound water, moved oil and water and residual water saturation</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/10-1210847x14.png"/></fig><p>L&#248;n&#248;y method addresses pore throat sizes which contain Inter crystalline porosity, Chalky Limestone, Mudstone micro porosity. Pore systems are classified at class 2 and 3 Lucia and pore size varies from 0.5 to 4 micron.</p><p>MRIL spectrums indicate high volume of irreducible bound water; there is also some free fluid porosity which is mainly water with a little oil; in some interval oil and water are identified. Porosity spectrums also show that the total porosity is about 20% - 25% in the reservoir intervals as well as permeability varies between 5 to 200 md. In order to define water saturation precisely for the reservoir, T2 Cut off defines 115 microseconds related to micro porosity carbonate to define.</p></sec><sec id="s6"><title>Acknowledgements</title><p>The authors would like to acknowledge, with deep appreciation and gratitude, invaluable help and give advices of the associate and assistant Professors of Department of Geology, Basic Science Faculty, North Tehran branch, Islamic Azad University, Tehran, Iran. This work is supported by Iranian offshore oil company and Research department that I am so grateful of experts of Iranian Offshore Oil Company for providing required data, and all facilities.</p></sec><sec id="s7"><title>Cite this paper</title><p>Arbab, B., Jahani, D. and Movahed, B. (2017) Reservoir Characterization and Pore Type Systems of Car- bonate Low Resistivity Pay in Persian Gulf. Open Journal of Geology, 7, 859-870. https://doi.org/10.4236/ojg.2017.76059</p></sec></body><back><ref-list><title>References</title><ref id="scirp.77337-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Adedapo, A. and Ayham, A. (2017) A Cohesive Approach at Estimating Water Saturation in a Low-Resistivity Pay Carbonate Reservoir and Its Validation. Journal of Petroleum Exploration and Production Technology, 57, 1-21.</mixed-citation></ref><ref id="scirp.77337-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Serra, O.L. (2004) Well Logging. Data Acquisition and Applications, 667.</mixed-citation></ref><ref id="scirp.77337-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Sharland, P.R., Archer, R., Casey, D.M., Davies, R.B., Hall, S.H., Heward, A.P., Horbury, A.D. and Simmons, M.D. (2001) Arabian Plate Sequence Stratigraphy. 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