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Dissociation Behavior of Methane-Ethane Mixed Gas Hydrate in Drilling Mud Fluid

Dissociation Behavior of Methane-Ethane Mixed Gas Hydrate in Drilling Mud Fluid
Dissociation Behavior of Methane-Ethane Mixed Gas Hydrate in Drilling Mud Fluid

Dissociation Behavior of Methane-Ethane Mixed Gas Hydrate in Drilling Mud Fluid Kawamura,T. a, Yamamoto, Y. b, Yoon, J.-H. b, Haneda, H. b, Ohga, K. a and Higuchi, K a

a Graduate School of Engineering, Hokkaido University, Sapporo, Hokkaido, Japan

b National Institute of Advanced Industrial Science and Technology, Tsukuba, Ibaraki, Japan

ABSTRACT

Dissociation kinetics of gas hydrates has been investigated experimentally. The artificial natural gas hydrates were made from pure methane or methane-ethane mixed gas, and then its composition and the structure were examined. These samples were dissociated under various conditions. Obtained dissociation rates were discussed with analytical model. As a result, it seemed that generated gas by hydrate dissociation affects heat flux and changes dissociation rate. Especially in case of methane-ethane mixed gas hydrate, generated gas seemed to affect thermal stability by changing environmental gas composition. In “drilling mud fluid”, the dissociation rate have almost proportional relation with the “mud” concentration.

KEY WORDS: Gas hydrate; methane; ethane; dissociation; model; drilling mud.

INTRODUCTION

Natural gas hydrates existing under sea ground have been widely known as a large natural gas reservoir, and then expected to be a future energy resource (Okuda, 1993). In order to recover natural gas from them commercially, in-situ dissociation of hydrate under sea ground is needed (Ji-Ahmadi and Smith, 2001). Therefore the dissociation rate, which depends on T-P condition and other environmental conditions, are essential parameter to evaluate gas recovery from hydrate layer. Like methane hydrate (C1 Hyd), a considerable amount of methane-ethane mixed hydrate (C1-C2 Hyd), which contains methane and ethane molecules as guests, is also found in ocean deposits. When comparing with comparing with C1 Hyd, C1-C2 Hyd can be considered to be more stable (Sloan and Fleyfel, 1992). However, there have been a few information on the dissociation kinetics and dynamic behavior under practical condition is not well understood.

In this study dissociation rates of C1 Hyd and C1-C2 Hyd are determined at a variety of experimental conditions. Both of C1 Hyd

and C1-C2 Hyd are synthesized by an ice-gas interface method. Raman spectrometry and gas chromatograph are used to examine the structure and composition of C1-C2 Hyd, respectively. Obtained information were used to estimate dissociation temperature, heat of dissociation and density of hydrate, which are needed in model calculations below. Then, these samples were dissociated under isothermal, isobaric condition in pure water, and the dissociation rates are determined. Based on one-dimensional thermal conduction theory, an analytical model is used to describe the dissociation behavior of gas hydrates. Moreover, the dissociation behavior of C1-C2 Hyd in viscous fluids such as drilling mud (Berthezene-Hemptinne-Audibert and Argillier, 1999) is also investigated.

EXPERIMENTAL

Determination of Hydrate Composition and the Structure The gases used in this work are pure methane (C1) and

methane?ethane (C1-C2) mixture. The initial composition of C1-C2 mixture used to make C1-C2 Hyd is 0.901(C1)/0.099(C2). All hydrate samples are synthesized in a high-pressure vessel at 270 K and 8.5-10 MPa by ice-gas interface method. To confirm the complete hydration it is necessary to keep the hydrate samples in the vessel at least for 2 days. After the hydration, each sample is quickly transferred to a cold-vessel at 139 K under atmospheric pressure. At this condition, it is reasonable that the hydrate sample can maintain its composition constant without a large change. Recently, some workers reported that more than 98 % of cavities in methane hydrates were filled with methane molecules (Hirai-Kondo-Hasegawa-Yagi-Yamamoto-Komai-Nagashima-Sakashita-Fujihisa and Aoki, 2000). For the measurement of composition of C1-C2 Hyd samples, the temperature of vessel is steadily increased to initiate the dissociation of hydrate. The gases generated from hydrates are instantly collected and used to analyze the composition by a gas chromatograph. A laser Raman microprobe spectrometer (Jobin Yvon Ramanor T6400) with beam spot size of 1 m is used for the structural identification of the mixed hydrates. The refraction right is detected by triple monochrometer and CCD detector. μ

Measurement of dissociation Rate

The hydrate and ice pellets with a size of 12 mm-o.d. and 6 mm-thickness are prepared for the dissociation measurement. The photograph of these pellets used in this work is shown in Fig. 1. The drilling mud mainly consists of water, electrolytes and viscous media such as biopolymer. In this work, XANVIS supplied from TELNITE

Proceedings of The Twelfth(2002)International Offshore and Polar Engineering Conference Kitakyushu,Japan,May26–31,2002

Copyright?2002by The International Society of Offshore and Polar Engineers

ISBN1-880653-58-3(Set);ISSN1098-6189(Set)

CO. LTD. is used as a model mixture of viscous media. The concentration of aqueous XANVIS solutions ranges from 0.2 to 1.2 wt %. A schematic illustration of experimental apparatus used in this work is shown in Fig. 2. The optical cell covered with a sapphire window has an inner volume of about 2ml and maximum pressure of 15 MPa. The gas inlet, outlet and a

thermocouple are also equipped with the cell. Under isothermal and isobaric conditions, water or

XANVIS solutions are injected into the optical cell to initiate the

dissociation. The dissociation rate is determined directly by measuring the time required for complete

dissociation of the hydrates through optical window.

RESULTS AND DISCUSSION

Hydrate Composition and Structure

The experimental results obtained by gas analysis are compared with the model calculation results using CSMHYD (Sloan, 1998). Table 1 shows the difference between these two results. As previously stated, the initial gas composition to make C 1-C 2 Hyd is

0.901(C 1)/0.099(C 2). As can be seen from Table 1, the composition of hydrate phase is found to be 0.714(C 1)/0.286(C 2). It is very close to the model calculation result that this mixture forms only the structure II

hydrate. The Raman spectroscopy is also used to check the result of composition analysis of hydrate phase and depicted in Fig. 3. Each

dotted line shows the spectra intensities obtained from C 1-C 2 mixed gas. As shown in Fig. 3 (b), the peak intensity of methane in large cavity (I L ) has five times large value compared with that in small cavity (I S ) (Sum, Burrus and Sloan, 1997). Moreover, the spectrum obtained at 993.3 cm ?1 can be identified to ethane molecule of the hydrate structure II (Subramanian-Kini-Dec and Sloan, 2000) as shown in Fig. 3 (a). Therefore, it is reasonable to conclude that this C 1-C 2 gas mixture

forms the structure II hydrate. These obtained information were used to estimate dissociation temperature, heat of dissociation and density of hydrate, which are needed in model calculations below.

5 mm

Fig. 1 Photograph of hydrate pellet used in this work Height: 6mm, Diameter: 12mm, Weight: 0.48 to 0.52g, Porosity: 0.17 to 0.25 Table 1. Experimental and calculated results of composition analysis of C 1-C 2 Hyd sample. Mixed gas

CH 4/C 2H 6

Experimental Calculated Calculated

Structure - I II Temperature (K) 270 270 270 Pressure (MPa)

8.5

1.42

1.63

Initial gas composition 0.901/0.099 0.900/0.100 0.900/0.100 Mole fraction of hydrate guest 0.714/0.286 0.574/0.426 0.719/0.281

Liquid Cell

Coolant

980

985

990

995

1000

1005

1010

I n t e n s i t y

(a)

993.3cm -1

995.1cm -1

Raman shift (cm-1)

(b)

I S

Fig. 2 Schematic illustration of experimental apparatus 2870

2890

2910

2930

2950

2970

Raman shift (cm-1)

I n t e n s i t y

I L

Fig. 3 Raman spectra of C 1-C 2 Hyd at (a), C ?C starch reason and (b), C ?H starch reason

Dissociation Rate of Gas Hydrate (or Ice) in Water

The analytical model used in this work is based on simple one-dimensional thermal conduction (Kelker-Selim and Sloan, 1998). It is

assumed that the dissociation can occur only at the hydrate ?water

interface and the interface temperature is identical with the equilibrium

dissociation temperature at the system pressure. Thus, the movement of

the water-hydrate (or ice) interface X can be expressed as a function of

time t as follows

t X W 4αξ= (1) where ξ is given by

ξλρρπεξξ)()1(erf D 0W P,H W H

2

T T C e

??=? (2) where αW stands for thermal diffusivity of water, ρH for density of

hydrate (or ice), ρW for density of water, λH for heat of dissociation of

hydrate (or ice) (Sloan and Fleyfel, 1992), C P, W for heat capacity of

water, T 0 for the experimental temperature, and T D

for the hydrate (or

ice) dissociation temperature. The measured porosity of hydrate ε is

about 0.21 and T D is set by the applied pressure and its gas composition. To confirm the feasibility of the experimental method used in this work, the fusion behavior of pure ice pellet is first examined. As shown in Fig. 4, the time required for complete fusion of ice pellet decreases with increasing the dissociation temperature. In addition the

experimental data are found to be in good agreement with the model calculation results within a maximum deviation of 1.3 min.

0510152025303540273

275

277279281

283

Temperature (K)

T i m e (m i n )

The C 1 Hyd and C 1-C 2 Hyd pellets are also dissociated in pure water

under isothermal and isobaric conditions. The temperature is 279.15 K and the pressure ranges from 0.8 to 4.24 MPa. Fig. 5 shows the time required for complete dissociation of the pellets as a function of pressure. As can be easily seen from Fig. 5, the trend of time profile reveals an exponential fit. It must be noted that the limitation of

pressure is very close to the equilibrium pressure 4.67 MPa at 279.15 K. There is a little large deviation between the experimental and calculated results. It is also found that the experimental data are always larger than calculated values over a whole pressure condition. This may be caused by the influence of gas bubbles generated from gas hydrates on the dissociation rate. Since the existence of bubbles in water can resist the

heat transfer, it has a large influence on the overall dissociation reaction, resulting in the reduction of dissociation. For more accurate calculation by the model, it is necessary to modify and develop the analytical model for considering this bubble dynamics. As shown in Fig. 6, a lot of methane gas bubbles covers not only the surface of hydrates but also the optical window. For the C 1-C 2 Hyd, two different compositions of gas phase are considered in model calculation; 0.9 (C 1)/0.1(C 2) and 0.7(C 1)/0.3(C 2). In case of 0.9 (C 1)/0.1(C 2), it is assumed that the gas composition might not be changed through whole reaction. In contrast, for 0.7 (C 1)/0.3(C 2), it is assumed that the gas composition will be changed from initial

condition because of the gases generated from hydrate. As shown in

Fig. 5, it is evident that the change of gas composition plays a great role in model calculation. The slight changes of gas composition may make a large shift of time profile. In our model calculation, the result for the gas composition of 0.7 (C 1)/0.3(C 2) can reproduce the experimental

data better than the case of 0.9 (C 1)/0.1(C 2). It can be expected, therefore, that the calculated time profile agree well with experimentally observed results only when the gas composition is

almost identical with hydrate phase composition. This result indicates that the knowledge for the composition of hydrate phase would be a strong and essential factor to estimate the dissociation rate of gas

020

40

6080

1

234

Pressure (MPa)

T i m

e (m i n )

Fig. 5 Time variations of temperature required for complete dissociation of C 1 and C 1-C 2 Hyd pellets in water

Fig. 4 Time variations of temperature required for complete fusion of ice pellets

(a) Ice-Water (b) C 1 Hyd-Water

Fig. 6 Photograph of ice fusion and hydrate dissociation through optical window. Ice was at 275.15K, C 1 Hyd was at 279.15K, 3.8MPa respectively.

Dissociation Rate of Gas Hydrate in Aqueous XANVIS Solutions

The viscosity of aqueous XANVIS solutions is measured by using a rotary type viscometer at the temperature of 279.15 K and depicted in Fig. 7. The concentration of XANVIS solutions ranges from 0.2 to 1.2 wt %. As the concentration of XANVIS increases, the viscosity of aqueous XANVIS solutions increases dramatically. It is also clear that the XANVIS solutions have non-Newtonian flow behavior as shown in Fig. 7.

The C 1-C 2 Hyd pellets are dissociated in aqueous XANVIS solutions. The temperature and pressure are 279.15 K and 0.1 MPa, respectively. As shown in Fig. 8, the dissociation rate decreases with increasing the concentration of XANVIS. Therefore, it can be concluded that the dissociation rate of gas hydrates in drilling mud fluids is almost

proportional to the concentration of mud fluid. In this study, the change of physical properties such as heat capacity and thermal conductivity by adding XANVIS has not been considered sufficiently. This change may have a considerable influence on the dissociation of gas hydrates. Therefore, our research should be further extended to more complicated system in order to get more accurate description on the dissociation behavior of gas hydrates.

05000

10000150002000025000300000

5

101520

25

Shear rate (rpm)

V i s c o s i t y (c P )

46

8

10

12

0.2

0.4

0.6

0.8

1

1.2

1.4

XANVIS Concentration (%)

T i m e (m i n )

CONCLUSION

The natural gas hydrates, C 1 Hyd and C 1-C 2 Hyd, have been prepared in a high-pressure vessel by ice-gas interface method. By using Raman spectroscopy and gas chromatograph, the structure and composition of C 1-C 2 Hyd are clearly identified. It is found that the composition of hydrate phase is 0.714(C 1)/0.286(C 2) and structure II hydrate can be stabilized by methane and ethane molecules even though they belong to only structure I hydrate-formers.

The dissociation rates of C 1 Hyd and C 1-C 2 Hyd are measured at several isothermal and isobaric conditions in pure water and aqueous XANVIS solutions. And then, they were discussed with analytical model. It has been found that the influence of gas bubbles generated from hydrate phase on the dissociation rate is very strong. The

existence of bubbles in water may resist the heat transfer, resulting in the reduction of dissociation. Especially in C 1-C 2 Hyd system, it can be expected that the calculated time profile agree well with experimentally observed results only when the gas composition is almost identical with hydrate phase composition. This result indicates that the knowledge for the composition of hydrate phase would be a strong and essential factor to estimate the dissociation rate of gas hydrate under sea ground. It is also found that the dissociation rate of gas hydrates in drilling mud fluids is almost proportional to the concentration of mud fluid then it can be suggested that in case of riser drilling, dissociation rate will be slow comparing with the case of no drilling mud.

REFERENCES

Berthezene, N., de Hemptinne, J. C., Audibert, A. and Argillier, J. F.

(1999). “Methane solubility in synthetic oil-based drilling muds.” J. Petro. Sci. Eng., Vol 23, pp 71-81

Hirai, H., Kondo, T., Hasegawa, M., Yagi, T., Yamamoto, Y., Komai,

T., Nagashima, K., Sakashita, M., Fujihisa, H. and Aoki, K. (2000). “Methane hydrate behavior under high pressure,” J. Phys. Chem. B , Vol 104, pp 1429-1433.

Ji, C., Ahmadi, G. and Smith, D.H. (2001). “Natural gas production

from hydrate decomposition by depressurization,” Chem. Eng. Sci., Vol 56, pp 5801-5814.

Kelker, S.K., Selim, M.S. and Sloan, E.D. (1998). “Hydrate

dissociation rates in pipelines,” Fluid Phase Equilibria , Vol 150, pp 371-382.

Fig. 7 Viscous property of aqueous XANVIS solutions

Okuda, Y. (1993). “Natural gas resources with sherbet like feature-Gas

Hydrate,” Petrotech, Vol 16, pp 300-305.

Sloan, E.D. (1998). Clathrate hydrates of natural gas (2nd ed.),

Marcel Dekker, New York.

Sloan, E.D. and Fleyfel, F. (1992). “Hydrate dissociation enthalpy and

guest size” Fluid Phase Equilibria , Vol 76, pp 123-140

Subramanian, S., Kini, R. A., Dec, S. F. and Sloan, E. D. (2000).

“Evidence of structure II hydrate formation from methane + ethane mixtures,” Chem. Eng. Sci., Vol 55, pp 1981-1999.

Sum, A.K., Burrus, R.C. and Sloan, E.D. (1997). “Measurement of

clathrate hydrates via Raman spectroscopy,” Journal of Physical Chemistry B , Vol 101, pp 7371-7377.

Fig. 8 Time variations of temperature required for complete dissociation of C 1-C 2 Hyd pellets in aqueous XANVIS solution

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uncivilized behavior

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