4.1.Petrophysical modeling results
The initial stage for constructing 3D reservoir models is building the structural modeling, which relies on well-logs interpretations. The goal of 3D structural modeling is mainly to obtain a 3D interpretation and understanding of the geological structure. Structural model construction relies on main components, including faults patterns and horizons of oil and gas accumulation (Avseth et al. 2005). The structural model of the S1A reservoir, Sunah oilfield, is defined by the horizon and fault framework and creates the geometrical data for constructing the 3D grid. S1A oilfield is a sandstone reservoir interbedded with slight limestone, mudstone, and siltstone. Well correlation for S1A reservoir was conducted for 74 wells to present the significant variations in thickness and petrophysical properties in the four zones of the S1A reservoir. The S1A lithological units were subdivided into three units: upper shore, mid-shore, and low shore. The correlation was conducted by employing various logs, including Spontaneous potential (SP), Gamma Ray (GR), Resistivity (RT), and Acoustic impedance (AC). The S1A reservoir consists of four horizons, namely S1A-F1, S1A-F2, S1A-F3, S1A-F4, and S1B, which is divided sequentially from the tops to the bottom. Fig.5 presents the S1A reservoir result of surface modeling A, B, C, and D. The mapped horizons of the S1A reservoir indicated that formation units are laterally extended within the model area and influenced by the normal faults that were interpreted. The S1A shelf sands are crosscut by four main normal faults A-D. These four faults strike East-West and dip to the south. This has resulted in the formation of four S1A structural pools, A-D, on the footwall or northern side of the faults. Additionally, other faults affect trends to NW-SE influence the area of target study.
On the other hand, the S1A structural pools are isolated from other oilfields in the Masila Basin, including the North-East Sunah, Hemiar, and Camaal S1A structural pools, by water-filled structural low or spill point at approximately -2700 ft ss. The S1A structural pools are sealed by the overlying red Shale and Qishn Carbonate formations. The four Sunah structural pools, A–D, are separated by transmissive fault barriers. These “leaky” fault barriers indicate that the four Sunah pools may carry the exact initial reservoir pressure and the same initial oil/water contact. The lowest known oil (LKO) in the “A” pool is observed in the Sunah-41Z well at -2616 ft SS. The “B” pool has an LKO of –2640 ft ss observed in the Sunah-40 well. A LKO of –2643 ft SS has been established in the “C” pool by the Sunah-29 well. The lowest known oil (LKO) in the “D” pool is observed in the Sunah-43Z well at -2651 ft SS. (Fig.6) presents the S1A structural pools.
4.1.1. Facies Model
The lithofacies model has a significant contribution in controlling the distribution of petrophysical properties. The lithofacies model can be conducted by utilizing an appropriate technique, including stochastic and deterministic, which provides facilities to construct 3D spatial distributions of property models that can acquire from well datasets (Ali et al. 2020). The process of generating the facies log from the existing wells was the initial step for developing the facies model of the S1A reservoir (Abdel-Fattah et al. 2018; Rassas et al. 2020). However, before constructing the facies model, the lithofacies logs were created and upscaled to the grid model of the S1A reservoir. The facies model of the S1A reservoir was divided into four zones, namely S1A-F1, S1A-F2, S1A-F3, and S1A-F4. The S1A lithological units were subdivided into three units: upper shore, mid-shore, and low shore, with different proportions of 53.3%, 28.67%, and 18.03%, respectively.
Moreover, the S1A is a sandstone reservoir interbedded with slight limestone, mudstone, and siltstone. Furthermore, facies models are adapted to various facies techniques to populate the discrete facies model; however, the Simulation of Sequential Indicator (SIS) approach was employed to simulate the lithofacies model of S1A reservoir by a stochastic approach. A stochastic approach can integrate the volume fraction and variograms. Virtually, the stochastic approach is considered suitable with minimal data, specifically when the sand body is uncertain. Moreover, it facilitates the modeling of the sand body environment in which the facies volume ratio differs laterally and vertically. (Fig.7) presents the results of the S1A reservoir lithofacies model.
4.1.2. Porosity Model
Evaluation of hydrocarbons trapped in the oil reservoir is obtained by determining the reservoir's porosity (Agyare Godwill and Waburoko 2016; Rassas et al. 2020). The porosity model was constructed based on well-logs interpretations of the S1A reservoir. The well logs were scaled up utilizing the average arithmetic approach. Moreover, a Sequential Gaussian Simulation (SGS) algorithm was employed to distribute the porosity model within the S1A reservoir. Furthermore, the porosity value of the S1A reservoir ranges from 0% to 27%, with an average distribution of 22%. The lowest porosity values were found in the northern and eastern regions, while the highest values are situated in the central and northeastern areas. Approximately 60% of porosity values range between 0.10 to 0.20, while 40% range from 0.05 to 0.1. Vertically, a reversal relation between porosity values and depth was increasing. Overall, the result indicates that the porosity value within the S1A reservoir is a good sandstone reservoir. (Fig.8) represents the result of a porosity model in the S1A reservoir.
4.1.3.Permeability Model
The term permeability refers to the fluid movement's ability within the porous reservoir media (Agyare Godwill and Waburoko 2016; Rassas et al. 2020). Virtually, permeability plays a substantial role in determining the fluid flow trends and fluid flow rate. The permeability model was developed based on well-logs interpretations of the S1A reservoir. The well logs were scaled up utilizing the average arithmetic method. The (SGS) approach was utilized to distribute the permeability model within the S1A reservoir. The Permeability value ranges from 1 to 1000 md with an average distribution of 800 md within the S1A reservoir. The Permeability values centralized in with 2550 md. Approximately 90% of Permeability values range between 200 to 800 md, while 20% range more or less. Overall, the results indicate that the permeability value within the S1A reservoir is a good sandstone reservoir. (Fig.9) presents the permeability model of the S1A reservoir.
4.1.4 Water Saturation model
The ratio of oil, water, and gas in the pore media is known as the saturation distribution (Ali et al. 2020; Rassas et al. 2020; Islam et al. 2021). Saturation is a crucial form for specifying water areas with high potential. The average arithmetic method was employed to scale up the well logs. The (SGS) approach was used to distribute the water saturation model within the S1A reservoir. The water saturation value ranges from 0.1 to 0.7, with an average distribution of 0.75 within the S1A reservoir. The lowest water saturation values were found in the center, while the highest values were found in the boundary of the reservoir. Roughly, 80% of water saturation values range between 0.50 to 0.80, while 20% of them range from 0.1 to 0.3. Vertically, a proportional relation between water saturation values and depth increasing. (Fig.10) presented the result of water saturation within the S1A reservoir.
4.2. Geological uncertainty of petrophysical models
The uncertainties still exist in the model of the S1A reservoirs. Firstly, the structural model is still unconfident due to seismic interpretation from a geophysical aspect. Secondly, the facies model is not studying from a depositional conceptual model. The intermediate conceptual model has been referred to as for assumption of direction, location, and size of geological features distribution. Also, well log up-scale, and grid up-scaling themselves lead to model uncertainty, particularly Pore Volume. The Pore Volume is extremely important for static CO2 storage capacity in the subsurface.
On the other hand, the geological uncertainties could provide the uncertainties range (P10, P50, P90) for the porosity and permeability model. These plausible geological realizations are considered as rank models for dynamic CO2 storage capacity.
The uncertainty assessment was conducted from a geological package. In this paper, the global seed number is considered as the main parameter for finding the uncertainty values of Pore Volume. Also, the global seed number will be assigned to changed 100 porosity and permeability models. That means each pore volume calculation led to a change in each porosity and permeability. Then, the global seed number from P10, P50, and P90 pore volume was adapted as the global seed number for porosity and permeability models.
The Monte Carlo Simulation with Latin Hyper Sampling was used to determine the probability distribution of reservoir pore volume. The P10, P50, P90 pore volume was used for risk assessment of static CO2 storage capacity. (Fig.11) represents the result of uncertainty analysis of pore volume in the S1A reservoir.
Furthermore, the ranked porosity and permeability model was also obtained from the geological uncertainties process. (Fig.12) illustrates the three realizations (P10, P50, P90) of porosity and permeability models. These 3D images showed the significant difference between three realizations (porosity and permeability) that represents the overall geological uncertainty in the reservoir.
4.3 Theoretical CO2 storage capacity
The static CO2 storage capacity evaluates from petrophysical data of the potential candidate sites. There are many ways for determining the potential of CO2 storage capacity for structural trapping, capillary trapping, and dissolution trapping (Bradshaw et al. 2007; Zhong and Carr 2019)
This paper emphasizes on static CO2 storage capacity by using the equation below:

where MCO2 is estimated CO2 storage capacity (Mt), A is trap area (m2), h is the average thickness (m), ϕ is the porosity of storage site (%), Swiir is known as irreducible water saturation (%), B knows as a formation volume factor in the storage site (m3/m3), ρCO2 is the CO2 density (kg/m3), and E is the capacity coefficient (IEA GHG 2008; Vo Thanh et al. 2019a).
However, the trap area, porosity, and thickness can be included in many uncertainties in the geological modeling process. Therefore, we consider the sum of grid pore volumes (Vpv=∑iAi×hi×ϕi) to swap A×h×ϕ (Vo Thanh et al., 2019a). The new formula can be replaced as follows:

where Vpv is the pore volume of a reservoir (m3)
Thus, the static CO2 storage capacity can be computed by considering Equation (2) and (Table-2).
Table 2 Uncertainty assessment for theoretical storage capacity in S1A reservoir
Parameters
|
Symbol
|
Unit
|
P10
|
P50
|
P90
|
Pore volume
|
Vpv
|
Mm3
|
60.24
|
78.83
|
97.51
|
Irreducible water saturation
|
Swiir
|
%
|
0.34
|
0.24
|
0.11
|
Formation volume factor
|
B
|
Bbl/STB
|
1.35
|
1.35
|
1.35
|
Average CO2 density
|
ρCO2
|
Kg/m3
|
769
|
769
|
769
|
Capacity coefficient
|
E
|
%
|
0.11
|
0.51
|
0.91
|
CO2 storage capacity
|
MCO2
|
Mt
|
4.54
|
31.72
|
81.98
|
(Table 2) illustrates the three probability of static CO2 storage in the S1A reservoir. The amount of P90 CO2 storage achieves the highest values compared with P10 and P50 CO2 storage capacity. There has been a strong increase of CO2 storage amount from 4.54 Mt P10 to just over 31.71 Mt P50. Overall, it is clear that the least likely, P10, storage capacity was 4.54 million tons, and the most likely, P90, storage capacity was 81.98 million tons
In this context, we consider that this sandstone reservoir is potential CO2 storage. Also, this evaluation is just for structural/stratigraphic trapping. The dynamic CO2 simulation will further investigate the other type of CO2 trapping using MRST_CO2lab. This open-source code was used to simulate the CO2 trapping mechanism in the Sunah field. The next section will elaborate on the CO2 behavior inside the reservoir.
4.4 Dynamic CO2 storage capacity
The results of the dynamic CO2 storage capacity were applied for three realizations (P10, P50, P90). The reservoir properties and injection rate were considered as the sensitivity impact of dynamic CO2 storage. MRST-VE open-source MATLAB code could perform the quick CO2 injection process in the subsurface. Thus, this source could be considered for this study. All simulation scenarios will be conducted in 10 years of injection and 90 post-injection periods. The grid simulation cell with 188×144×20 (391040 grid cells). A large number of grid cells could produce a reliable simulation in the subsurface.
The injection rate is an important parameter for dynamic storage capacity. The injection rate will monitor the balance between buoyancy and CO2 horizontal spread. Also, the increasing injection rate will lead to improved sweep efficiency for well injection operation. However, the disadvantage of a large injection rate is CO2 leakage risk.
At the first step of the MRST-VE module, the 3D grid cell will be converted approximately to a 2D form shape. (Fig.13) illustrates the result of the processing grid cell for the S1A field to conduct the dynamic storage assessment.
(Fig.14) represents the CO2 saturation migration in three ranked geological realizations. The visualization of this CO2 saturation indicated that the injection rate improved the CO2 sweep efficiency in the storage sites. Besides, the large injection rate could be more suitable in the storage sites that have long horizontal sides. Also, (Fig.15) gives an idea about the petrophysical distribution effect on CO2 migration. Although, the increasing injection rate was improved sweep efficiency. However, the diversity of reservoir heterogeneity was strongly affected by changing the morphology of the CO2 plume in the S1A reservoir.
Also, the simulation results will suggest the CO2 leakage potential according to the injection rate analysis. (Fig.15) represents the comparison of P10, P50, and P90 realizations according to the percentage of different types of CO2 trapping with sensitivity injection rate.
This bar chart represents the amount of CO2 trapping in P10, P50, and P90 geological realizations. It also highlighted the potential CO2 leakage in three realizations. The green column illustrated the percentage of CO2 leakage with an injection rate varying from 5000 m3/day to 7000 m3/day.
There were 5 types of CO2 trapping obtained after 10-year injection and 90 years post-injection period in (Fig.15).
In terms of 5000 m3/day, the amount of residual CO2 trapping increased light from 32 % to 36%. Regarding the residual (traps) is stable in three realizations. In terms of residual (plume), the percentage of CO2 trapping has slightly decreased from 23% to 21%. Similarity with residual (traps), the movable (traps) of P90 realization slightly decreased 1% compared with P10 and P50 realizations.
Regarding the injection rate with 6000 m3/day, the five type trapping percentage is slightly increasing or decreasing. However, the CO2 will be leaked in three realizations if the injector operates with an injection rate equal to 6000 m3/day.
Moreover, the movable (plume) achieved the highest amount with the largest injection rate (7000 m3/day). The higher injection rate will supply a large amount in the injection period. This mechanism contributes to improving CO2 sweep efficiency in storage reservoirs. Even so, the CO2 leakage is strongly increased with the largest injection for three realizations.
Overall, the P50 geological realization with the lowest injection rate (5000 m3/day) was the best strategy for decision-making under geological uncertainty. Also, the dynamic CO2 storage capacity under geological uncertainty would provide a better plan for future development plans about geo-sequestration in the S1A reservoir.
Finally, the comparison between static and dynamic CO2 storage would be considered. This step will answer the question of why dynamic CO2 storage under geological uncertainties is important in CCS projects. (Fig.16) depicts the difference between static and dynamic CO2 storage capacity in the upper Qishn Clastics.
The bar chart represents how much static and dynamic CO2 storage capacity in P10, P50, and P90 realization. There was a slight difference between static and dynamic CO2 storage in P10 realization. A difference about half was evidence in static and dynamic in P50 realization where P50 static is 15.65 Mt and P50 dynamic is 31.72 Mt. Similarly, more static CO2 is stored than dynamic CO2 trapping (approximately 81.98 and 17.52).
The main reason for the difference between static and dynamic is the efficient storage factor in the static calculation. Also, the dynamic CO2 storage capacity is considered CO2 leakage during the simulation process. Therefore, the results will be different in terms of static and dynamic CO2 storage.
In addition, this study demonstrated the important role of CO2 storage capacity under geological uncertainty. The CO2 storage capacity will include a lot of uncertainty factors. Our work emphasizes the role of petrophysical modeling uncertainties from static to dynamic CO2 storage capacity. It could provide the template for future development about Carbon Capture Storage in Yemen.