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Page 1: Carbon Dioxide Seal Capacity Study, Boggy...Otway Basin Pilot Project, Seal Capacity R. F. Daniel CO2CRC 3 Introduction The Otway Basin in the region of Boggy Creek in Victoria is
Page 2: Carbon Dioxide Seal Capacity Study, Boggy...Otway Basin Pilot Project, Seal Capacity R. F. Daniel CO2CRC 3 Introduction The Otway Basin in the region of Boggy Creek in Victoria is
Page 3: Carbon Dioxide Seal Capacity Study, Boggy...Otway Basin Pilot Project, Seal Capacity R. F. Daniel CO2CRC 3 Introduction The Otway Basin in the region of Boggy Creek in Victoria is

Carbon Dioxide Seal Capacity Study, Boggy Creek, Otway Basin, Victoria

Daniel, Dr. R.F.

September 2005 CO2CRC Report No: RPT05-0045

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Otway Basin Pilot Project, Seal Capacity

Cooperative Research Centre for Greenhouse Gas Technologies (CO2CRC) GPO Box 463 Level 3, 24 Marcus Clarke Street CANBERRA ACT 2601 Phone: +61 2 6200 3366 Fax: +61 2 6230 0448 Email: [email protected] Web: www.co2crc.com.au

Reference: Daniel, R.F., 2005, Boggy Creek Carbon Dioxide Seal Capacity Study, Otway Basin, Victoria, Australia. CO2CRC Publication No RPT05-0045, August 2005, 47pp

© CO2CRC 2005

Unless otherwise specified, the Cooperative Research Centre for Greenhouse Gas Technologies (CO2CRC) retains copyright over this publication through its commercial arm, Innovative Carbon Technologies Pty Ltd. You must not reproduce, distribute, publish, copy, transfer or commercially exploit any information contained in this publication that would be an infringement of any copyright, patent, trademark, design or other intellectual property right.

Requests and inquiries concerning copyright should be addressed to the Communication Manager, CO2CRC, GPO Box 463, CANBERRA, ACT, 2601. Telephone: +61 2 6200 3366.

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Table of Contents Executive Summary.......................................................................................................................................2 Introduction....................................................................................................................................................3 Methodology ...................................................................................................................................................4

Mercury Injection Capillary Pressure (MICP) .........................................................................................4 Pore Throat Size Distribution...................................................................................................................5 Determination of Seal Capacity................................................................................................................6 Otway Basin Subsurface fluid properties: ................................................................................................7

Results .............................................................................................................................................................8 Discussion and Conclusions ........................................................................................................................10 References.....................................................................................................................................................12 Appendix.......................................................................................................................................................13

Scanning Electron Microscopy...............................................................................................................13 XRD Mineralogy....................................................................................................................................22 Graphs of; (A) Injection Pressure vs. Hg Saturation and Incremental Pore Volume, (B) Pore Throat Size vs. Frequency and (C) CO2 Seal Capacity above FWL vs. Water Saturation................................28

Table of Figures Table 1 Data available on samples from Boggy Creek 1 and Flaxmans 1...................................................... 3 Table 2 Primary and derived data used to determine the carbon dioxide column height.............................. 8 Figure 1: Carbon dioxide retention heights for samples from Boggy Creek 1 and Flaxmans 1. Samples

analysed by the Australian School of Petroleum. ..................................................................................... 9 Table 3: Spatial distribution of depositional environment analogues for sealing lithologies (after R. Root,

2004)............................................................................................................................................................ 10 Figure 2 Analogue for Area / Thickness and Length / Width for sealing rock depositional environments

after Root in Daniel et al., 2003 and Root et al., 2004............................................................................. 11 Figure 3 – SEM of Boggy Creek 1 1673 – Waarre Formation ........................................................................ 14 Figure 4 - SEM of Boggy Creek 1 1674.1 – Waarre Formation...................................................................... 15 Figure 5 - SEM of Boggy Creek 1 1676.7 – Waarre Formation...................................................................... 16 Figure 6 - SEM of Flaxmans 1 1946.1 – Belfast Mudstone.............................................................................. 17 Figure 7 - SEM of Flaxmans 1 2020.8b – Flaxman Formation ....................................................................... 18 Figure 8 - SEM of Flaxmans 1 2083.3 – Flaxman Formation ......................................................................... 19 Figure 9 - SEM of Flaxmans 1 2194.9 – Waarre Formation ........................................................................... 20 Figure 10 - SEM of Flaxmans 1 2195.97 – Waarre Formation ....................................................................... 21 Table 4: Bulk mineralogy of sealing rock samples (M. Raven CSIRO) ......................................................... 22 Figure 11: XRD mineralogy Boggy Creek 1 1673 ............................................................................................ 23 Figure 12: XRD mineralogy Boggy Creek 1 1674.1 ......................................................................................... 23 Figure 13: XRD mineralogy Boggy Creek 1 1676.4 ......................................................................................... 24 Figure 14: XRD mineralogy Boggy Creek 1 1676.7 ......................................................................................... 24 Figure 15: XRD mineralogy Flaxmans 1 1946.1............................................................................................... 25 Figure 15: XRD mineralogy Flaxmans 1 2020.8............................................................................................... 25 Figure 16: XRD mineralogy Flaxmans 1 2083.3............................................................................................... 26 Figure 17: XRD mineralogy Flaxmans 1 2194.9............................................................................................... 26 Figure 18: XRD mineralogy Flaxmans 1 2195.97............................................................................................. 27

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Executive Summary

Core samples from the Belfast Mudstone and Flaxman Formation regional seals and intraformational seals from the Waarre Formation are analysed for their capacity to retain or support a column carbon dioxide in the subsurface as part of the Otway Basin Pilot Project (OBPP). The samples are from Boggy Creek 1 and Flaxmans 1, which are in the region of the project and the closest wells, which are cored through the zones of interest. This report details the result of MICP (Mercury Injection Capillary Pressure) analyses, scanning electron microscopy (performed at the Australian School of Petroleum) and XRD mineral analyses (CSIRO) on these sealing samples.

Capillary pressure data are used to determine threshold or break through pressure, which is used in the calculation of the carbon dioxide retention height of sealing rocks. Pore throat size distributions are also plotted for the analysed samples and the laboratory mercury/air values are converted to subsurface supercritical carbon dioxide values to determine saturation versus height relationships.

The carbon dioxide seal retention column for the sample of the Belfast Formation is approximately 840 m, the Flaxman Formation CO2 column height varies between 713 to 987 m and the intraformational seal of the Waarre Formation column height between 0.16 and 1631 m.

Mudstones and claystones of the Belfast Mudstone, Flaxman and Waarre Fms in the Boggy Creek 1 and Flaxmans 1 area represent depositional environments from prodelta shelf to upper deltaic coastal shoreface to braided fluvial overbank (intraformational seal) (Faulkner 2000) and an indication of coverage of these depositional environments is provided by ancient and modern analogue data. The areal distribution of these depositional environment analogues vary from 350 to 5,000 km2 (Belfast Mudstone), 1 to 100 km2 (Flaxman Formation) and the analogue data for the Waarre Formation varies from 0.4 to 3 km2 .

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Introduction The Otway Basin in the region of Boggy Creek in Victoria is the subject of a pilot injection study to determine the viability of storing super critical carbon dioxide in the partially depleted Waarre C hydrocarbon reservoir. This reservoir is capped by regional sealing lithologies of the Belfast Mudstone and the Flaxman Formation and samples from these formations are the subject of MICP analysis to determine the carbon dioxide seal capacity or retention height. Intraformational seals from the upper Waarre Formation are also analysed to determine the potential for baffling the migration CO2. Background data for column height determination were obtained from the well completion reports of Boggy Creek 1 and Flaxmans 1. Super critical carbon dioxide saturation versus height and seal retention height were determined from the MICP analyses and these data.

An outline of mercury injection capillary porosimetry and the determination of pore throat size and seal capacity is presented under Methodology. Table 1 provides details of the samples analysed.

Table 1 Data available on samples from Boggy Creek 1 and Flaxmans 1

Well Depth (m) Formation Core/ Cuttings/ SWC

Boggy Creek 1 1673 Waarre Formation Core

Boggy Creek 1 1674.1 Waarre Formation Core

Boggy Creek 1 1676.4 Waarre Formation Core

Boggy Creek 1 1676.7 Waarre Formation Core

Flaxmans 1 1946.1 Belfast Mudstone Core

Flaxmans 1 2020.8b Flaxman Formation Core

Flaxmans 1 2083.3 Flaxman Formation Core

Flaxmans 1 2194.9 Waarre Formation Core

Flaxmans 1 2195.97 Waarre Formation Core

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Methodology

Mercury Injection Capillary Pressure (MICP)

The theory of the mercury porosimeter is based on the physical principle that a non-reactive, non-wetting liquid will not penetrate pores until sufficient pressure is applied to force its entrance. The relationship between the applied pressure and the pore throat size into which mercury will intrude is given by the Washburn equation (1921):

Pc D = 4 γ cos θ (1a)

More recently, however, this equation has developed into a more useful style for determining pore throat radius as suggested by Purcell (1949) and Schowalter (1979):

Pc r = 2 γ cos θ (1b)

Where Pc is the applied capillary pressure, D is the pore throat diameter, r is the pore throat radius, γ is the surface tension of mercury (480 dyne cm-1) and θ is the contact angle between mercury and the pore wall, usually near 140°. This equation assumes that all pores are right circular cylinders. As pressure increases, the instrument senses the intrusion volume of mercury by the change in capacitance between the mercury column and a metal sheath surrounding the stem of the penetrometer. As the mercury column shortens, the pressure and volume data are continuously acquired by an attached computer.

Mercury porosimetry is a technique, which is rate limited, as predicted by the Darcy equation. This describes the general function of pressure drop vs. flowrate:

c

21

gV

Lαµρρ

=−

(2)

Where ρ1 is the upstream pressure, ρ2 is the downstream pressure, L is the pore length, 1/α is the permeability coefficient, µ is the fluid viscosity, V is the superficial velocity of fluid and gc is a dimensional constant. The velocity of flow in a viscous liquid such as mercury is proportional to the pressure drop and inversely proportional to the length and surface area of the pore. Hence, given a specific limited flow velocity, the complete filling of a porous network will be a function of time. The larger the volume of pores the more time is required to fill the total pore volume completely. Therefore mercury porosimetry is most accurate when mercury is allowed to fill all the available pores, at equilibration.

The mercury injection porosimetry analyses for this study were carried out using a Micromeritics Autopore 9410 instrument. This is composed of two separate systems, one for low pressure runs and the second for the high pressure runs. The low pressure run must always be done first, followed quickly by the high

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pressure run, to preclude the possibility of extra mercury intrusion into the sample by capillary action while the sample is held at atmospheric pressure at the conclusion of the low pressure run.

The system operates using the equilibration by time method - after the required pressure for a reading is attained it is held for twenty seconds to allow the amount of mercury entering the pores to stabilise. This is done because the process of mercury filling the pores is not an instantaneous one. Mercury begins entering the pores as soon as the pressure exceeds the value required for the pore throats' diameter, but the time required to fill the pores depends on the volume and shape of the pores. The equilibration by time process allows the pores to fill. If equilibration is not allowed, then the filling may not be complete when the reading is taken, which leads to estimation of lower pore volumes and smaller pore sizes than is actually the case. Readings of mercury intrusion are taken by measuring the electrical capacitance of the penetrometer. This varies as the mercury is intruded from the precision bore stem into the pore space of the sample by the increasing pressure.

Each sample is usually dried at 60oC for at least twenty four hours, weighed and placed into a penetrometer (a glass chamber attached to a precision bore glass tube, which has been nickel-plated) and the entire assembly is weighed. This is placed in the low pressure port and evacuated to 0.05 torr. This vacuum is held for thirty minutes to ensure that no vapour remains in the sample. After this time the penetrometer is filled with mercury and the low pressure run is carried out. The pressure is increased incrementally from 13.8 kPa (2 psia) to 199.5 kPa (28.94 psia), with a reading taken after 20 seconds of equilibration at each pressure. At the end of the low pressure run the penetrometer returns to atmospheric pressure. It is removed from the instrument and weighed to obtain its weight plus that of the mercury.

The penetrometer is then placed in the high pressure chamber, which uses hydraulic oil to take the pressure incrementally from 199.5 kPa (28.94 psia) to 413.7 MPa (60,000 psia). Again readings are taken after a twenty second equilibration period (see Graph A of the first three analyses). The pressure then decreases incrementally from 413.7 MPa (60,000 psia) to 139kPa (20 psia), with readings taken after the equilibration period. The sample is removed from the penetrometer and weighed. The specific gravity and porosity of the sample can be calculated when it is removed from the penetrometer and weighed.

Pore Throat Size Distribution

Using the following data for the air mercury system from (Vavra et al, 1992), capillary pressure data were converted to effective pore throat size:

Air/mercury contact angle (θa/m) = 140°, and

interfacial tension (σa/m) = 480 dynes/cm.

σ(a/m) cos θ(a/m) = 370

1 cm = 10,000 µ, 1 psi = 69035 dynes/cm2

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Solving for r in equation (1b) results in the following relationship of capillary pressure to pore throat size:

1 psi = (approx.) 100 microns

10 psi = (approx.) 10 microns

100 psi = (approx.) 1 micron

1000 psi = (approx.) 0.1 micron

(see Graph B of the first three analyses in the Appendix)

Determination of Seal Capacity

MICP studies done solely for the purpose of determining pore throat radius and pore throat size distribution are valuable. However, there is great benefit in using the MICP analytical data to relate the mercury saturation of the sedimentary rock to the intruding pressure as a function of height above the free water level (FWL). This function indicates the CO2 column height that a sealing rock will support. The processes of determining column height is described below.

Before the mercury injection data can be applied to seal capacity they must be converted to a subsurface CO2/brine system using the following equation (after Schowalter, 1979):

( )( )m/am/a

CO/bbCOm/abCO cos

cosPP 22

2 θσθσ

= (3)

Where 2bCOP is the capillary pressure in the brine/CO2 system, m/aP is the capillary pressure in the

air/mercury system, 2bCOσ and m/aσ are the interfacial tensions of the brine/CO2 and the air mercury

systems respectively, 2CO/bθ and m/aθ are the contact angles of the brine/CO2/solid and air/mercury/solid

systems respectively.

The initial pressure at which the mercury first displaces the air is referred to as the "displacement pressure" (Pd). In the subsurface, buoyancy pressure drives CO2 (the non-wetting phase) movement and forces it into the pore throats of a rock, displacing water (the wetting phase). Buoyancy is simply the density difference between CO2 and brine multiplied by the column height and a constant (k) gravitational factor, which is 0.433. The greater the column thickness, the greater the buoyancy pressure driving the CO2.

Pd in the reservoir system is the pressure at which CO2 first entered the pore system by displacing the water. Different rocks with different pore throat sizes will have different displacement pressures and different saturations as a function of height (h) above the free water level (FWL). Thus, in any given

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reservoir section, the lowest indication of live (vs. residual) CO2 in a particular rock type approximates the displacement pressure (Pd) for that rock. The Pd can thus be considered as the CO2 – water contact for that particular rock type. It should be remembered that a reservoir may have several CO2 water contacts (as a function of pore properties controlled by rock type), but will have only one FWL. It is therefore of significance to determine the FWL.

In order to do this, capillary pressure data must first be converted to height above free water level information by using the equation:

Pcb/co2 = h(ρb-ρco2) x 0.433 (4)

Where: Pcb/co2 = Capillary Pressure (psi) reservoir brine/CO2 system

h = height (in ft.)

ρb = brine density (gm/cc)

ρco2 = CO2 density (gm/cc)

Otway Basin Subsurface fluid properties: Super critical CO2 Density - 0.65 to 0.70 gm/c3 (variable )

Brine Density- variable in the range of 1.01 to 1.004 gm/c3.

Interfacial Tensions were determined from the CO2CRC web-site carbon dioxide calculator (see Table 2 for the parameters of each sample). Generally the interfacial tension for brine/CO2 is approximately 26 dynes/cm and the contact angle is 0° as shown below.

System Contact angle ( � Interfacial tension ( �)

Brine/CO2 0° 26 dynes/cm (variable)

Air/mercury 140° 485 dynes/cm

Once the capillary pressure values have been converted to h (height in metres), a plot of height versus mercury (non-wetting phase) saturations can be constructed. However, conversion of mercury (non-wetting phase) to CO2 (non-wetting phase) will now result in a height versus CO2 saturation plot. Since water (wetting phase) saturation is more commonly used in the oil and gas industry, the non-wetting phase saturation needs to be converted to water (wetting-phase) saturation (Schowalter, 1979). This is done using the simple conversion:

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Sw = 1 – Snw (5)

Where: Sw = wetting phase (water) saturation

Snw = non-wetting phase (CO2) saturation

Combining equations (4) and (5) result in a plot of height (above FWL) versus water saturation as highlighted in the third graph (C) shown of each sample (see Graph C of the first three analyses in the Appendix)

Results

The carbon dioxide seal retention column of the Belfast Formation is calculated to be approximately 840 m from MICP analysis in Flaxmans 1. The Flaxman Formation CO2 column height varies between 713 to 987 m in Flaxmans 1. The Waarre Formation column height varies between 0.16 and 1631 m in Boggy Creek 1 and 15 to 101 m in Flaxmans 1 (Table 2 and Figure 1).

Table 2 Primary and derived data used to determine the carbon dioxide column height.

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Figure 1: Carbon dioxide retention heights for samples from Boggy Creek 1 and Flaxmans 1. Samples analysed by the Australian School of Petroleum.

0.16 m

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Discussion and Conclusions CO2 retention heights in these samples vary with relative clay vs sand content and the presence of partially dissolved feldspars. The four samples with lower retention values all featured a significant medium to very fine grain sand fraction with partial dissolution of feldspar grains. The surfaces of these comparatively larger grains and the partially dissolved grains may act as larger capillary conduits for fluids moving through the formation leading to a reduced retention height. These reductions are occurring only in the Waarre Formation and not the regional seals and hence will act as baffles and increase the potential for mineralogical storage of carbon dioxide.

The mudstones and claystones of the Belfast Mudstone represent a prodelta to open shelf depositional environment. Sediments of the Flaxman Formation is attributed to a lower delta to restricted shallow marine depositional environment and the Waarre Formation to a braided fluvial complex with overbank deposits acting as intraformational seals (Faulkner 2000). An indication of coverage of the above depositional environments is provided by ancient and modern analogue data of varying depositional environments (Figure 2). These depositional environment analogues have areal distributions of 350 to 5,000 km2 (Belfast Mudstone), 1 to 100 km2 (Flaxman Formation) and the analogue data for the Waarre Formation intraformational seals vary from 0.4 to 3 km2 (Table 3).

Table 3: Spatial distribution of depositional environment analogues for sealing lithologies (after R. Root, 2004)

Lithology Spatial Distribution Depositional Environment Area km2 Package Thickness m

Prodelta Mudstone - claystone

1 – 5,000 ~2

Upper Delta Plain Very fine sand to silty

mudstone

3 - 100 3 - 15

Fluvial Overbank Vfg sandstone -mudstone

0.4 - 3 4 - 10

Previous investigations of seal capacities within the Otway Basin in the Shipwreck Trough area show that the Belfast Formation can support columns of SC CO2 between 580 and 1100 m (5 samples). The Flaxman Formation retention column varies between 20 and 1400 m (5 samples) and the Waarre Formation intraformational seals between 180 and 1900 (2 samples).

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Figure 2 Analogue for Area / Thickness and Length / Width for sealing rock depositional environments after Root in Daniel et al., 2003 and Root et al., 2004.

0.01 0.1 1 10 100 1,000 10,000 100,000

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References Boyd, G.A. and Gallagher, S.J., 2001. The sedimentology and palaeoenvironments of the late Cretaceous Sherbrook Group in the Otway Basin. PESA Eastern Australian Basins Symposium p.475 - 483

Buffin, A.J., 1989. Waarre Sandstone development within the Port Campbell embayment. APEA Journal, 1989, p., 299-311.

Dewhurst, D.N., Jones, R.M., and Raven, M.D., 2002. Microstructural and petrophysical characterisation of Muderong Shale; application to top seal risking. Petroleum Geoscience V 8, p. 371 – 383.

Daniel, R.F., and Kaldi, J.G., 2004. Atlas of Australian and New Zealand Hydrocarbon Seals. Volume 3, APCRC Technical Workshop Proceedings, Program 1; Hydrocarbon Sealing Potential of Faults and Cap Rocks. Perth, WA, June 2004. 220p

Faulkner, A., 2000. Sequence stratigraphy of the late Cretaceous Sherbrook Group, Shipwreck Trough, Otway Basin. Honours Thesis, National Centre for Petroleum Geology and Geophysics, The University of Adelaide.

Kaldi, J.G., O’Brien, G., and Kivior, T., 1999. Seal capacity and hydrocarbon accumulation history in dynamic petroleum systems: the East Java Sea, Indonesia, and the Timor Sea, Australia. APPEA Journal V.39.

Kivior, T., Kaldi, J.G. and Lang, S.C., 2002. Seal potential in Cretaceous and late Jurassic rocks of the Vulcan Sub-Basin, northwest shelf Australia. APPEA Journal V 42, p. 203-224

Purcell, W.R., 1949. Capillary pressures – their measurement using mercury and the calculation of permeability therefrom. Petroleum transactions, American Institute of Mining, Metallurgical and Petroleum Engineers, v. 186, p. 39 – 48.

Root, R.S., Gibson-Poole, C.M., Lang, S.C., Streit, J.E., Underschultz, J. and Ennis-King, J., 2004. Opportunities for geological storage of carbon dioxide in the offshore Gippsland Basin, SE Australia: An example from the upper Latrobe Group. In Boult, P.J., Johns, D.R. and Lang, S.C. (Eds), Eastern Australasian Basins Symposium II, Petroleum Exploration Society of Australia, Special Publication , p. 367-388.

Schowalter, T.T., 1979. Mechanics of secondary hydrocarbon migration and entrapment. AAPG Bulletin v. 63, p. 723 – 760.

Sneider, R.M., 1987. Practical petrophysics for exploration and development. AAPG Continuing Education Short Course Notes.

Wardlaw, N.C., 1980. The effects of pore structure on displacement efficiency in reservoir rocks and in glass micromodels. In: 1st joint SPE/DOE Symposium on Enhanced Oil Recovery, SPE no. 8843, p. 345 – 352.

Wardlaw, N.C., and M. McKellar, 1981. Mercury porosimetry and the interpretation of pore geometry in sedimentary rocks and artificial models. Powder Technology v. 29, p. 127 – 143.

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Appendix

Scanning Electron Microscopy

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Figure 3 – SEM of Boggy Creek 1 1673 – Waarre Formation

a) General view of an intraformational seal within the upper Waarre Formation showing coarse quartz and remnant feldspar grains in a matrix of smectite, muscovite and kaolinite View – oblique to bedding. Scale – 50 µm

b) Microporous framboids of pyrite are common throughout the matrix (see insert) View – oblique to bedding. Scale – 20 µm

c) The matrix is composed of dominantly smectite, illite and kaolinite. Framboids of pyrite upper left. Rhomb of siderite arrowed View – oblique to bedding. Scale – 10 µm

d) Rhombs of siderite encapsulated in a smectite / kaolinite matrix View – oblique to bedding. Scale – 10 µm

e) EDS spectrum indicates abundant clays with silica and trace anatase (Ti) with siderite and pyrite (Fe).

f) Larger grains of muscovite and occasional quartz are highlighted along the bedding plane. View – parallel to bedding. Scale – 20 µm

q

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Figure 4 - SEM of Boggy Creek 1 1674.1 – Waarre Formation

a) General view of an intraformational seal within the upper Waarre Formation highlighting a matrix of kaolinite and muscovite View – perpendicular to bedding. Scale – 100µm

b) Very fine silty grains of quartz throughout the kaolinite and muscovite matrix. View – perpendicular to bedding. Scale – 50µm

c) Detail of muscovite within the clay matrix View – perpendicular to bedding. Scale – 20µm

d) EDS spectrum indicates silica, kaolinite, minor pyrite. High sulphur due to jarosite (see XRD)

e) Elongate grains of mica in a kaolinitic matrix View – oblique to bedding. Scale – 20µm

f) Very fine grained matrix of kaolinite and jarosite with minor pyrite View – oblique to bedding. Scale – 50µm

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Figure 5 - SEM of Boggy Creek 1 1676.7 – Waarre Formation

a) General view of an intraformational seal within the upper Waarre Formation highlighting fine grained quartz in a kaolinite matrix View – oblique to bedding. Scale – 100µm

b) Quartz with partially dissolved feldspar and pyrite molds in the matrix. View – oblique to bedding. Scale – 50µm

c) Detail of partially dissolved K feldspar showing intra granular microporosity (see insert) View – oblique to bedding. Scale – 20µm

d) EDS spectrum indicating silica, clays, feldspar and pyrite (NB high sulphur)

e) General view of overlapping platelets of clay indicating a good sealing lithology View – perpendicular to bedding. Scale – 50µm

f) Detail of overlapping platelets highlighting very low microporosity. View – perpendicular to bedding. Scale – 5µm

f p

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Figure 6 - SEM of Flaxmans 1 1946.1 – Belfast Mudstone

a) General view of the Belfast Mudstone, regional seal, highlighting tightly packed matrix View – perpendicular to bedding. Scale – 50µm

b) Detail showing large overlapping clay platelets with little microporosity visible. View – perpendicular to bedding. Scale – 20µm

c) Detail of smectite, illite and kaolinite in the matrix View – perpendicular to bedding. Scale – 2µm

d) EDS spectrum indicates clays with silica and trace feldspar and pyrite.

e) View parallel to the bedding shows more micro-porosity and also that the overlapping clay platelets would inhibit flow across the bedding (arrow direction) View – parallel to bedding. Scale – 20µm

f) Detail a large flake of mica with small pyrite framboids in the clay packages. View – parallel to bedding. Scale – 5µm

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Figure 7 - SEM of Flaxmans 1 2020.8b – Flaxman Formation

a) General view of Flaxmans Formation sample showing coarse quartz sand in a very fine matrix Scale - 500µm

b) Detail of a rounded quartz grains with very fine grained matrix. Scale – 20µm

c) Detail of the matrix highlighting a combination of berthierine and siderite with fine grained mica Scale – 2µm

d) EDS spectrum indicates silica and clay/mica with siderite and berthierine (XRD).

e) Microporosity is abundant in areas where there is a lack of siderite and berthierine is common Scale – 5µm

f) Foliated muscovite platelets among berthierine and rhombs of siderite Scale – 2µm

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Figure 8 - SEM of Flaxmans 1 2083.3 – Flaxman Formation

a) General view of Flaxmans Formation seal showing fine quartz sand and mica flakes in a very fine matrix. View – oblique to bedding. Scale – 50µm

b) EDS spectrum indicates silica, clays/mica, pyrite and calcite with trace anatase (Ti).

c) Detail of common quartz and mica grains throughout the matrix. View – oblique to bedding. Scale – 10µm

d) Matrix detail of kaolinite smectite and mica with View – oblique to bedding. Scale – 5µm

e) Large grains of muscovite in clay matrix with microporosity evident between the platelets View – perpendicular to bedding. Scale – 20µm

f) Detail of smectite / kaolinite matrix with vfg berthierine and pyrite between the clay platelets View – perpendicular to bedding. Scale – 10µm

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Figure 9 - SEM of Flaxmans 1 2194.9 – Waarre Formation

a) General view of Waarre Formation intra-formational seal showing coarse quartz sand grains in a very fine matrix. View – parallel to bedding. Scale – 500µm

b) Detail of the kaolinite and muscovite matrix between quartz grains View – parallel to bedding. Scale – 50µm

c) Detail of feldspar dissolution with chlorite / berthierine development View – parallel to bedding. Scale – 20µm

d) EDS spectrum indicates abundant silica with kaolinite chlorite/berthierine, mica and feldspar.

e) View of large flake of muscovite with kaolinite and minor quartz. View – perpendicular to bedding. Scale – 50µm

f) Detail of muscovite and kaolinite matrix highlighting large overlapping platelets View – perpendicular to bedding. Scale – 20µm

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Figure 10 - SEM of Flaxmans 1 2195.97 – Waarre Formation

a) General view of Waarre Formation intra-formational seal showing coarse quartz sand grains in a very fine matrix. View – oblique to bedding. Scale – 500µm

b) Detail of sub-laminar matrix between the quartz grains. View – oblique to bedding. Scale - 50µm.

c) Very fine clay matrix between the quartz provides sealing qualities although microporosity is present at the sub-micron level. View – oblique to bedding. Scale - 10µm.

d) Detail of muscovite (m), K feldspar (Kf) and berthierine/chlorite (b). View – oblique to bedding. Scale - 2µm.

e) EDS spectrum indicates silica, clays, feldspar and minor pyrite

f) Detail shows large overlapping platelets kaolinite and muscovite with small grains of feldspar View – perpendicular to bedding. Scale - 5µm.

Kf

m

b

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XRD Mineralogy Table 4: Bulk mineralogy of sealing rock samples (M. Raven CSIRO)

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46- 1045 QUARTZ, SYN 13- 135 MONTMORILLONITE-15A 29- 696 SIDERITE 42- 1340 PYRITE 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1

File Name: c:\...\13670blk.101

BC-1673 Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

5

10

15

20

25

Inte

nsity

(Cou

nts)

X 1

00

10.67910.0107.181

5.003

4.524

4.355

4.252

3.582

3.345

2.804

2.710

2.587

2.4562.4192.280

2.2342.212

2.128

1.9801.967

1.915

1.819

1.7351.671

1.6571.644

1.633

1.5421.5131.504

1.453

Figure 11: XRD mineralogy Boggy Creek 1 1673

46- 1045 QUARTZ, SYN 42- 1340 PYRITE 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1 22- 827 JAROSITE, SYN

File Name: c:\...\13672blk.103

BC-1674.1 Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

9

18

27

36

45

Inte

nsity

(Cou

nts)

X 1

00

9.974

7.142

4.979 4.466

4.354

4.253

3.8863.736

3.572

3.490

3.339

3.1973.121

2.9842.8572.790

2.7072.593

2.566

2.490

2.457

2.4242.3822.339

2.280

2.2342.212

2.128

1.991

1.980

1.915

1.817

1.7891.757

1.6711.6601.6471.634

1.542

1.5041.4881.453

1.430

Figure 12: XRD mineralogy Boggy Creek 1 1674.1

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46- 1045 QUARTZ, SYN 42- 1340 PYRITE 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1 33- 664 HEMATITE, SYN 33- 311 GYPSUM, SYN 22- 827 JAROSITE, SYN 19- 932 MICROCLINE, INTERMEDIATE

File Name: c:\...\13673blk.104

BC-1676.4 Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

3

6

9

12

15In

tens

ity (C

ount

s) X

100

0

9.971 7.542

7.1484.980

4.255

3.574

3.344

3.2363.0752.9902.863 2.7072.6942.5652.490

2.457

2.4382.4202.3832.337

2.281

2.235

2.2082.161

2.1281.980

1.914

1.817

1.7891.759

1.671

1.6581.6331.618

1.542

1.5041.4881.453

1.4311.418

Figure 13: XRD mineralogy Boggy Creek 1 1676.4

46- 1045 QUARTZ, SYN 42- 1340 PYRITE 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1 19- 932 MICROCLINE, INTERMEDIATE 33- 664 HEMATITE, SYN 22- 827 JAROSITE, SYN

File Name: c:\...\13674blk.105

BC-1676.7 Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

10

20

30

40

50

60

70

80

90

Inte

nsity

(Cou

nts)

X 1

00

9.978

7.147

4.980 4.466

4.254

3.845

3.573

3.345

3.2443.1973.1212.9912.8632.7892.707 2.5632.491

2.457

2.4232.3832.342

2.281

2.2382.212

2.1281.9911.980

1.9151.895

1.817

1.6711.6601.633

1.542

1.5051.4881.453

Figure 14: XRD mineralogy Boggy Creek 1 1676.7

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46- 1045 QUARTZ, SYN 42- 1340 PYRITE 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1 13- 135 MONTMORILLONITE-15A 7- 315 BERTHIERINE-1M

File Name: c:\...\13677blk.108

Fl-6385 Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

9

18

27

36

45In

tens

ity (C

ount

s) X

100

9.9677.136

4.983

4.512

4.253

4.051

3.572

3.525

3.345

3.1913.0572.991 2.810

2.706

2.5722.5722.457

2.419

2.280

2.2342.208

2.128

1.9941.980

1.819

1.6711.633

1.542

1.5121.502

1.4881.453

Figure 15: XRD mineralogy Flaxmans 1 1946.1

46- 1045 QUARTZ, SYN 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1 29- 696 SIDERITE 5- 586 CALCITE, SYN 19- 932 MICROCLINE, INTERMEDIATE 7- 315 BERTHIERINE-1M

File Name: c:\...\13678blk.109

Fl-6630a Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

10

20

30

40

50

60

70

Inte

nsity

(Cou

nts)

X 1

00

9.963

7.136

7.060

5.000 4.466

4.253

3.573

3.524

3.340

3.248 3.032

2.810

2.795

2.490

2.456

2.3472.280

2.2352.147

2.128

1.9771.964

1.817

1.7401.736

1.6711.658

1.542

1.505 1.453

Figure 15: XRD mineralogy Flaxmans 1 2020.8

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46- 1045 QUARTZ, SYN 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1 29- 696 SIDERITE 42- 1340 PYRITE 9- 466 ALBITE, ORDERED 19- 932 MICROCLINE, INTERMEDIATE 33- 311 GYPSUM, SYN

File Name: c:\...\13680blk.111

Fl-6835 Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

8

16

24

32

40

Inte

nsity

(Cou

nts)

X 1

00

9.9687.650

7.1374.484

4.253

4.0353.789

3.566

3.345

3.1963.0672.9992.8632.8012.706

2.5662.457

2.372

2.280

2.2342.128

1.980

1.819

1.6711.659

1.542

1.5021.488

1.428

Figure 16: XRD mineralogy Flaxmans 1 2083.3

46- 1045 QUARTZ, SYN 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1 42- 1340 PYRITE 19- 932 MICROCLINE, INTERMEDIATE 33- 311 GYPSUM, SYN 29- 701 CLINOCHLORE-1MIIB, FE-RICH 9- 466 ALBITE, ORDERED 7- 315 BERTHIERINE-1M

File Name: c:\...\13684blk.115

Fl-7201 Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

2

4

6

8

10

12

Inte

nsity

(Cou

nts)

X 1

000

14.276 9.966

7.137

7.088

6.465 4.979

4.253

4.0223.8463.776

3.572

3.5243.467

3.340

3.2363.188

2.9912.9022.7622.5652.490

2.456

2.3832.337

2.280

2.235

2.161

2.1271.980

1.817

1.800

1.6711.660

1.571

1.542

1.5021.4901.453

1.418

Figure 17: XRD mineralogy Flaxmans 1 2194.9

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46- 1045 QUARTZ, SYN 14- 164 KAOLINITE-1A 6- 263 MUSCOVITE-2M1 42- 1340 PYRITE 19- 932 MICROCLINE, INTERMEDIATE 29- 701 CLINOCHLORE-1MIIB, FE-RICH 9- 466 ALBITE, ORDERED 7- 315 BERTHIERINE-1M

File Name: c:\...\13685blk.116

Fl-7205 Bulk

2-Theta Angle (deg)10.00 20.00 30.00 40.00 50.00 60.00 70.00 80.00

10

20

30

40

50

60

70

80In

tens

ity (C

ount

s) X

100

14.1499.967

7.1347.082

4.9774.7154.466

4.253

4.0233.788

3.5723.524

3.478

3.340

3.2353.1882.9902.902 2.685

2.5652.495

2.456

2.3822.342

2.280

2.235

2.161

2.128

1.9941.980

1.817

1.7971.784

1.6711.658 1.552

1.542

1.490 1.4531.418

Figure 18: XRD mineralogy Flaxmans 1 2195.97

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Graphs of; (A) Injection Pressure vs. Hg Saturation and Incremental Pore Volume, (B) Pore Throat Size vs. Frequency and (C) CO2 Seal Capacity above FWL vs. Water Saturation

A A)

B)

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C)

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