OTC-27042-MS Reservoir Baffling Seen by Disequilibrium of DFA Fluid Gradients and by Wireline Pressure Transients and DSTs Thomas Pfeiffer and Vladislav V. Achourov, Schlumberger; Terje Kollien and Sven-Erik Foyn, Lundin; Soraya S. Betancourt and Julian Y. Zuo, Schlumberger; Rolando Di Primio, Lundin; Oliver C. Mullins, Schlumberger Copyright 2016, Offshore Technology Conference This paper was prepared for presentation at the Offshore Technology Conference held in Houston, Texas, USA, 2–5 May 2016. This paper was selected for presentation by an OTC program committee following review of information contained in an abstract submitted by the author(s). Contents of the paper have not been reviewed by the Offshore Technology Conference and are subject to correction by the author(s). The material does not necessarily reflect any position of the Offshore Technology Conference, its officers, or members. Electronic reproduction, distribution, or storage of any part of this paper without the written consent of the Offshore Technology Conference is prohibited. Permission to reproduce in print is restricted to an abstract of not more than 300 words; illustrations may not be copied. The abstract must contain conspicuous acknowledgment of OTC copyright. Abstract In this reservoir study, three adjacent structures have been subject to largely the same fluid charge with an original oil charge and a very recent light hydrocarbon charge (all indicated by petreolum systems modeling and organic geochemical analyses). In addition, all wells have an oil-water contact (OWC) and two have a gas-oil contact (GOC), while the GOC in the third well is not far away. Thus, all depth-dependent in-reservoir fluid geodynamic processes are visible within each well; no extrapolation away from the wells is required. Moreover, the ~30 meter oil columns in evidently connected sands are amenable to simple dynamic modeling thereby aiding in understanding. All three structures are found to have very different reservoir realizations, particualry regarding the dispositions of asphaltenes in spite of nominally similar initiation conditions after the secondary charge. That is, different reservoir fluid geodynamic processes took place producing different constraints on production in each of the structures. One well showed a light oil underlain by a tar mat. A second well showed large, disequilibrium gradients of gas-oil ratio (GOR) and asphaltene content without phase separated asphaltenes in core. The third well showed a tar mat on a shale break in the oil column not far form the GOC. There were no asphaltenes in core above the shale break and tar mat. However, below the shale break there was asphaltene throughout the core while retaining permeability, but no tar mat on the OWC. These differences were not ascribed to any paleo-OWC nor are they related to differing biodegradation. In addition, these differences are not consistent with any depressurization expalanation. To resolve the differences, a variety of data streams were used including downhole fluid analysis coupled with thermodynamic analysis from the Flory-Huggins-Zuo Equation of State (FHZ EoS) and its reliance on the Yen-Mullins model of asphaltenes. In addition, well test results provide key production information and are corroborated by vertical intereference testing on wireline. Petroleum system modeling and organic geochemical analysis of oil and core extract samples have also been very useful. The differences seen in the different wells relate to several important parameters such as the different extent of baffling which impacts both production rates as well as equilibration rates of reservoir fluids. Another key parameter is the extent of density stacking versus a lateral fluid front for the secondary light hydrocarbon charge. Proximity to the charge point enhances the lateral nature of the charge yielding rapid 2 OTC-27042-MS asphaltene instability precluding tar mat formation in sections of the well. This information is very useful when projecting reservoir properties away form wellbore. Introduction In order to optimize production, it is important to understand reservoir properties including the distribution of fluids and possible asphaltene deposition. It is desirable to understand the petroleum system context if not a petroleum system model (PSM) of the reservoir. Among other things, the PSM provides the timing type and volume of fluids that enter the reservoir. A missing element in understanding reservoir properties is accounting for the processes that take place in reservoirs that occur after charge and before present day.[1] These processes are subsumed in the new technical discipline ⬙reservoir fluid geodynamics⬙. Figure 1 shows a schematic of the time line of a reservoir. Figure 1—Schematic of reservoir over (geologic) time.[1] The petroleum system fills the reservoir (among other things). Reservoir fluid geodynamics redistributes fluids and can lead to tar deposition in the reservoir. Production is modeled by simulation software Reservoir fluid geodynamic processes connect the petroleum system context to present day production concerns about the reservoir. These processes include a variety of diffusive and convective processes as well as other time dependent processes such as biodegradation. The requirement to resolve many processes associated with reservoir fluid geodynamics was the development of a proper treatment of asphaltene thermodynamics in reservoirs. The industry’s first equation of state for asphaltene gradients, the Flory-Huggins-Zuo Equation of State (FHZ EoS) [2,3] with its reliance on the Yen-Mullins model of asphaltenes [4] has been just the development needed. Nominally, very similar petroleum system processes can lead to very different realizations within the reservoir, and thereby lead to very different production concerns. Indeed, many reservoir asset teams do not make use of a PSM. A prevailing view is that the PSM is primarily an exploration tool, and once a discovery is made and an asset team assigned, the PSM is no longer needed. The distinct problem is that specific PSM scenarios are not currently able to predict specific reservoir problems. The role of reservoir fluid geodynamics is to specific possible reservoir outcomes of a given petroleum system conext. An example of a petroleum system context that can give rise to an array of reservoir realizations is the circumstance of a late gas (or light hydrocarbon) charge into an oil reservoir. If there is sufficient reservoir pressure, this can give rise to an increase in solution gas which can then destabilize the asphaltenes. The OTC-27042-MS 3 destabilized asphaltenes can lead to a variety of fundamentally different realizations in the reservoir. The destabilized asphaltenes can migrate to the base of the reservoir and form a tar mat. Figure 2 shows the result of an oil reservoir that had a late gas charge.[5] Gas diffusion downward in the oil column caused the asphaltenes to migrate down (both by diffusion and by gravity currents) until they ran into an impermeable layer as shown in the schematic in Fig. 2. The impermeable layer was cement as seen in the thin section in Figure 2. The tar mat which is evident in whole core (cf. Figure 2) had nothing to do with water; it is on cement. The produced oil is very light, but the little heavy ends that remained in the oil were unstable and appeared as tar blobs in the produced oil.[5] It is believe that this was not bitumen in core that flowed with the light oil because the whole core showed good fluorescence all the way down to the tar mat. In this paper, bitumen and tar are used interchangeably; they are organic materials of high asphaltene content. Figure 2—shows the outcome of an oil reservoir with a late gas charge.[5] The gas diffused to the bottom of the column. The asphaltenes migrated down ahead of the gas front forming a tar mat on cemen at the base of the reservoir. The tar mat is evident in the whole core images; it does not fluoresce. Thin sections show tar deposited on mineral surfaces. The resulting light oil had high GOR and little asphaltene. In production, some tar was obtained in the light oil A different reservoir realization when gas charges into an oil reservoir is shown in Figure 3. Again asphaltene was destabilized in this process yielding a reservoir oil of high GOR and low asphaltene content. Figure 3—Another reservoir with a late gas charge into an oil reservoir. As in Fig. 2, a light oil of high GOR and low asphaltene content is produced in this process.[6] However, in this reservoir the tar is upstructure and the tar zone is permeable. In addition, the destabilized asphaltene migrated on order ten meters prior to undergoing a phase transition.[6] 4 OTC-27042-MS Figure 3 shows well data from two fields in the same basin.[6] The wells are upstructure, and near salt as indicated in the cartoon inset in Figure 3. Both reservoirs have a late gas charge into oil. Figure 3 shows the density-neutron crossover in field 2 (shaded yellow) indicating a high GOR fliud at the top of the interval. The tar intereval is indicated on the petrophysical log as determined from whole core. For field 1, the whole core is shown; the tar zone on a shale break is where fluorescence disappears. A tar interval was perforated and straddled with the MDT dual packer, a light oil flowed.[6] The tar zone is permeable. In addition to the high GOR, low asphaltene produced fluid, a tar is also produced. A photograph of this tar is also shown in Figure 3. This mobile tar helps create a flow dependent skin in the reservoir which must be address with xylene soaks of the reservoir.[6] The tar in these fields is permeable and upstructure. It is clear the tar results from gas charge into oil. It is also clear that the asphaltenes could migrate some short distances (~10 meters) prior to undergoing a phase separation producing the tar coating on the sand grains in sections. Consequently, this asphaltene was subject to a relative fast instability to become phase unstable upstructure in comparison to the asphaltene that destabilized in Figure 2 that migrated all the way to the base of the reservoir. However, the details of the process that caused the migrating asphaltenes to become phase unstable have never been adequately explained. Case Study This case study compares the fluid distribution and asphaltene disposition of three structures with a single well in each (Figure 4). Pressure gradient analysis and fluid contacts indicate that the three blocks are not in flow communication. All three wells encounter an OWC and two wells have a GOC. The GOC of the third well is thought to be nearby. The three structures are thought to have similar charge and alteration histories. The first charge appears to have the same maturity and similar inferred source rock facies. Biodegradation of the 1st charge is evident at various degrees in all three structures, while a more recent higher maturity charge evidently caused the asphaltene to re-distribute and destabilize. There is evidence that the OWC has moved in the course of the alteration processes. Elludicating the various realizations of the distribution of asphaltene in each of the structures and the consequences on production is the primary subject of this case study. Figure 4 —Three fault blocks with a single well in each. Each fault block was subjected to a secondary recent hydrocarbon charge into oil reservoirs OTC-27042-MS 5 Structures 1 and 2 We first consider Wells 1 and 2; both these wells have a GOC and an OWC. Figure 5 shows optical density of the liquid phase, asphaltene content as a percentage of the organic matter extracted from the core and GOR against depth. The schematics represent the processes associated with the late light hydrocarbon charge into oil reservoirs. Figure 5—Data from Wells 1 and 2 are depicted. The initial condition after charge is shown with gas above undersaturated oil. Gas diffuses into the oil. In Well 1, the oil shows large disequilibrium gradients of GOR and asphaltene content. Production was low in this well. In Well 2, the oil is equilibrated in GOR and asphaltene content. The liquid fraction is almost void of asphaltenes and tar has accumulated at the OWC. Production was high in this well compared to Well 1 In Well 1, the oil columns shows large, disequilibrium gradients of both asphaltenes and solution gas.[7] As shown in Figure 5, the oil in Well 1 contains 35% asphaltene towards the OWC. Core extract data from this well (not shown) only contained residual oil; there was no phase separated asphaltene.[7] This well was shown to be highly baffled by wireline vertical interference testing (VIT).[7] In addition, the flow rate (after accounting for viscosity) was low. The cartoon in Figure 5 visualizes the process: Gas only diffused part way down the column. Likewise the asphaltenes are still in the process of migrating away from the high solution gas section, but have not undergone phase separation.[7] The baffling in this well slowed down the rate of equilibration and also gave rise to poor production results. Even though structure 2 has undergone the same alteration process, both the asphaltene content and the solution gas of the oil are equilibrated.[7] Moreover, the oil from Well 2 has only a small quantity of asphaltene. In addition, Well 2 has a thick tar mat at the bottom as shown on the right side of Figure 5 in the core extract data.[7] In this well, the gas diffused all the way to the bottom of the reservoir, the OWC. The asphaltenes migrated ahead of the gas until they were held up at the OWC and accumulated at the bottom of the reservoir. There they formed a thick tar mat. This example is very similar to that shown in Fig. 2. Vertical interference tests indicated reasonably good vertical permeability and a lack of baffling. The production in Well 2 is ten times higher than Well 1 (after accounting for viscosity).[7] Wells 1 and 2 provide a ⬙movie⬙ of tar mat formation. However, the gas diffusion process started at the same times in the two wells. The rate of diffusion in Well 1 was smaller due to the baffling which also significantly impacted the production rate. The lesson is that if part of a field shows equilibrated 6 OTC-27042-MS asphaltenes (or fluids) and another part shows graded but not equilibrated fluids, then production might be low for the part of the field in disequilibrium. Wells 1 and 2 confirm the concepts that have been used to explain tar mats in other fields, (e.g. Figure 3). Nevertheless, these observations also reinforce that some other process must be occurring in the example in Figure 3 to produce a permeable upstructure tar mat. Structure 3 Structure 3 (Well 3) underwent the same petroleum system events as Structure 1 and 2. These structures all experienced a late light hydrocarbon charge into the oil reservoirs. The asphaltene disposition in this structure is yet different from Structures 1 and 2. There is evidence of two different tar deposition mechanisms in the same well: a slow diffusional destabilization and settling of asphaltenes on a shale break in the top part of the reservoir and local tar deposition from a rapid destabilization in the lower part. The significance of this observation is such that it provides an explanation to the long standing puzzle of upstructure permeable tar zones. Structure 3 shows a combination of vertical and lateral fluid fronts that occur in one well and account for the different realizations of tar deposition. As in the adjacent structures the oil was biodegraded in Structure 3. Biodegradation increases the asphaltene content in the oil, at most by a factor of 3 for Peters-Moldowan levels of 6 and above.[8] The lack of dominance of 25-norhopanes compared to hopanes indicates the intial biodegradation levels were not that high. Geochemistry analysis indicates a Peters-Moldowan level of biodegradation between 4 and 5. Two depths of paleo oil-water contacts (OWC) with corresponding biodegradation are evident in the residual oil below the present day OWC. An upward shift of OWC is possibly related to the oil being consumed, but could also be related to tilting and spilling of the oil in the reservoir. The residual oil in the water leg does not show systematic changes towards the OWC (Figure 6). Figure 6 —Geochemical markers and process traces support 3 zones in reservoir and indicate decresing maturity towrds the OWC. The GC analysis shows little to no biodegradation in the oil above the present day OWC. All paleo OWCs are below the present day OWC OTC-27042-MS 7 The Asphaltene content of the residual oil is in the order of 10-20% (of the extracted organic matter EOM, not in terms of weight % of core). This should be representative of the asphaltene content in the reservoir prior to the late secondary charge. It is also consistent with the current asphaltene content of the oil in Well 1 and with the thick tar mat in Well 2. The biodegadation and inferred asphaltene content of the original oil (from downhole fluid analysis) reinforces the view that in large measure, the petroleum system context of all three structures is similar. The secondary charge is believed to come dominantly from a deep kitchen, with contribution also from terrestrially influenced upper Jurrassic depositional environment. The charge is believed to enter from a westerly direction which puts Well 3 closest to the charge point. It is also volumetrically larger than in Structure 2. The oil fingerprints based on gas chromatography shown in Figure 6 indicate that the secondary charge is rich in n-alkanes with little to no biodegradation. In recent geologic time, the reservoir temperature for all three structures has become too high for biodegradation. Geochemical markers and process traces support 3 zones in reservoir and indicate decreasing maturity towards the OWC. All paleo OWCs are below the present day OWC. The late, high maturity charge raises the GOR and decreases asphaltene solubility of the original asphaltene rich oil. Downhole fluid analysis shows that the mobile oil has very little suspended asphaltene content. Analysis of the organic core extracts shows a complex pattern for Well 3, more complex than the patterns observed in wells 1 and 2 (cf. Fig. 7). Asphaltene content as a percentage of the extracted organic matter from the core indicates a low 5-10% asphaltene concentration at the top of the reservoir and a sharp increase to over 60% just above a lithologic shale boundary (cf. Fig. 7). This is consitant with the diffusive process in Well 2, with the exception that the asphaltenes are held up at a lithologic vertical boundary and not at the OWC as in Well 2. Figure 7—Asphaltene content in the organic extracts from core plugs vs. depth. Onlty small amounts of asphaltene is found in the core at the top of the reservoir. High asphaltene content above 60% indicates a tar mat just on top of a shale layer. A complex pattern is observed in the oil zone below the shale layer. In addition, two paleo OWCs are observed and corroborated by GC analysis. Core photographs show the tar deposition on top of the lithologic shale barrier 8 OTC-27042-MS Core analysis clearly shows the tar deposition on top of the shale layer (cf. Fig. 7). Movement of the OWC during the course of the alteration process is ony evident below the present day OWC. The tar mat resting on the shale has nothing to do with water or the OWC. Below the shale layer the core extracts indicate tar distribution scattered between 20% and 40%. Permeability is affected in the area, yet the DST results prove flow and permeability in that tar zone. There is no indication of an inpermeable tar mat at the OWC like in Well 2. The implication is that upon destabilization, the asphaltenes had no time to migrate downward. If the instability were induced by methane diffusion downward form the gas cap, then the asphaltenes would have plenty of time to migrate down to the OWC especially as the shale baffle slows down the methane diffusion as shown in Well 1. A rapid process must have destabilized the asphaltenes below the shale break, while slow destabilization is seen above the shale break. The proximity to the charge point and the large volume of the secondary charge leads to the understanding that the destabilization below the shale break is due to a lateral instability, a lateral fluid front of light hydrocarbon. Figure 8 schematically visualizes the movement of the fluid front in the proximity of the charge point. Figure 8 —In proximity to the charge point fluids fronts can sweep laterally through the reservoir. The process is fast compared to diffusion. Away from the charge point, the fluids density stack in the reservoir Wells 1 and 2 and many other case studies (e.g. Figure 2) show that when gas (or light hydrocarbon) charges into a reservoir, the gas can rapidly migrate to the top of the reservoir at least in some cases. That is, the charge fluids can density stack without mixing.[9] The newly charged gas diffuses downward in the oil column. In this slow diffusive process, the asphaltenes have time to migrate down away from the vertical fluid front of high(er) GOR oil. The migration of asphaltenes ceases when they are held up by an impermeable barrier or the OWC at base of the oil column. Indeed, the top of Well 3 shows just this process. Little asphaltene is found in core extracts above the tar mat on the shale break. These migrating asphaltenes deposited on the shale break forming a thin tar mat of very high asphaltene content. The top of the core section of Well 3 fits what is also observed in Well 2 and is not surprising. Below the shale break the asphaltenes are deposited throughout the oil column with no accumulation of asphaltenes on the OWC (cf. Fig. 9). The core below the shale break is permeable; these asphaltene deposits do not reduce permeability to zero unlike the tar mat in Well 2. The implication is that upon destabilization, the asphaltenes had no time to migrate downward. If the instability were induced by methane diffusion downward form the gas cap, then the asphaltenes would have plenty of time to migrate down to the OWC especially as the shale baffle slows down the methane diffusion as shown in Well 1. OTC-27042-MS 9 Figure 9 —Mixing of secondary and original charge destabilizes the asphaltenes differently as a function of the speed and direction of the process. Diffusional mixing gives the asphaltenes time to migrate down and deposit on a shale break. The lateral charge front and precludes migration downwards of the asphaltenes causing them to deposit locally. The result is a tar rich, but permeable zone below the shale break A change in reservoir pressure is likely throughout the various alteration stages of this structure. While asphaltene deposition though depressurization is observed in laboratory experiments it is not the cause of the deposition observed in Well 3. Pressure changes equilibrate rapidly in time [10] and as such the effect would result in a uniform local asphaltene deposition. This is not the case as the top and the bottom of the reservoir give evidence to two different destabilization mechanisms. In light of the petroleum system model, the nature of the structure, the proximity of the charge point and charge direction it seems plausible that the secondary charge caused a lateral sweep throught the lower part of the reservoir. Figure visualizes such a lateral charge which occurs fast compared to diffusive mixing. The asphaltenes destabilize and deposit locally at a medium concentration range (30%-40%). Conclusion All three adjacent structures show similar charge and alteration history, but are found to have ended up in very different reservoir realizations at present day. An asphaltene rich original charge mixed with a recent light hydrocarbon that destabilized the asphaltenes in all three structures. The rate and direction of mixing is different in all three wells and causes the differences in reservoir realization as a function of baffling and proximity to the charge point. At the foundation of the analysis stands a comprehensive evaluation of the reservoir fluids using downhole fluid analysis and sample acquisition. The lateral charge process is evident here and offers a plausible and likely solution to long standing puzzle of upstructure permeable tar zones (as observed here). This study shows that a combination of vertical and lateral fluid fronts can occur in one well and account for this puzzling observation. Acknowledgement The Authors would like to thank Lundin Norge AS for the permission to publish this paper. References 1. Mullins, O.C.; Zuo, J.Y.; Hammond, P.S.; De Santo, I.; Dumont, H.; Mishra, V.; Chen, L.; Pomerantz, A.E.; Dong, C.; Elshahawi, H.; Seifert, D.J.; The dynamics of reservoir fluids and their substantial systematic variations, SPWLA Ann. Symp. Abu Dhabi, (2014) 2. Freed, D.E.; Mullins, O.C.; Zuo, J.Y.; Asphaltene gradients in the presence of GOR gradients, Energy & Fuels, 24 (7), 3942–3949, (2010) 3. Zuo, J.Y.; Mullins, O.C.; Freed, D.E.; Dong, C.; Elshahawi, H.; Seifert, D.J.; Advances in the Flory-Huggins-Zuo Equation of State for Asphaltene Gradients and Formation Evaluation, Energy & Fuels, 27, 1722–1735, (2013) 4. Mullins, O.C.; The Modified Yen Model, Energy & Fuels, 24, 2179 –2207, (2010) 10 OTC-27042-MS 5. 6. 7. 8. 9. 10. 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