In this article, experimental data on methane hydrate formation in mixtures of water and acetone are presented. For eight different acetone-water mixtures, the phase transition hydrate + liquid + vapor f liquid + vapor (HLV f LV) was determined in the pressure range 2.50 < p/MPa < 11.25. In addition, the experimental data obtained were described by a model that takes into account the variation of the enthalpy of hydrate formation as a function of pressure and acetone concentration. The average absolute temperature difference in the representation of the hydrate formation temperatures of methane in the presence of acetone is less than 0.32 K.
ammerschmidt (1 934) developed an empirical method for predicting the hydrate formation temperature for natural gas H constituents in the presence of alcohol. ('Alcohol' is used here to describe alcohols and polyhhydroxy alcohols, or glycols.) Subsequently, several other models have been suggested, for example, Anderson and Prausnitz (1 986) and Moshfeghian and Maddox (1 993).In the presence of electrolytes, the method of Englezos and Bishnoi (1 988) is applicable. Their procedure uses the activity model developed by Pitzer and Mayorga (1 973) to predict the water activity coefficient in the presence of electrolytes. Their model is not recommended for hydrate forming gases with high solubility in the water phase. Javanmardi and Moshfeghian (1996) and later Javanamardi et al. (1 998) took a different approach and incremented the pure water hydrate formation temperature to predict conditions of incipient hydrate formation in the presence of electrolytes. Englezos (1 992), by using flash calculation algorithms and the fugacity model of Aasberg-Peterson et al.(1 991), predicted the temperature for incipient hydrate formation in single aqueous electrolyte solutions. Javanmardi and Moshfeghian (2000) used the same activity model to predict the hydrate formation temperature in mixed aqueous electrolyte solutions. Yousif and Young (1994), based on modification of the Hammerschmidt model, developed a simple model to predict the hydrate temperature suppression of aqueous mixtures of salts and a single alcohol. Their correlation is restricted to the prediction of the hydrate condition for a specified gas mixture; however, we used it to predict hydrate formation conditions for other systems. In the Nasrifar et al.( 1 998) work, the hydrate formation temperature in the presence of mixed electrolytes and alcohols is calculated by adding a correction to the hydrate formation temperature in the presence of inhibitors. Therefore, their method is a two-step procedure.In the present work, a new method is suggested for direct prediction of hydrate temperature in the presence of both aqueous electrolyte solutions and a single alcohol. The model is based on the extension of the water activity model to the above systems. The suggested method is A new thermodynamic model for calculating the hydrate formation temperature of different hydrate formers in aqueous solutions of both electrolytes and a single alcohol has been presented. This method uses a generalization of the Aasberg-Petersen model for water activity. For calculation of water activity in the presence of electrolytes, the effect of alcohols was taken into account without using any new fitting parameters. The results are in good agreement with published experimental data.
Experimental and thermodynamic results
for methane hydrate dissociation
conditions in the simultaneous presence of ethanol and 1-butyl-3-methylimidazolium
tetrafluoroborate (BMIM-BF4) ionic liquid (IL) in aqueous
solution are presented. Three different aqueous solutions including
solution 1 (0.0142 mole fraction of ethanol, 0.0060 mole fraction
of BMIM-BF4), solution 2 (0.0348 mole fraction of ethanol,
0.0059 mole fraction of BMIM-BF4) and solution 3 (0.0549
mole fraction of ethanol, 0.0058 mole fraction of BMIM-BF4) were used. An isochoric pressure-search method was used to perform
the measurements. The experimental pressure and temperature ranges
are (3.18 to 8.32) MPa and (273.6 to 283.3) K, respectively. The thermodynamic
inhibition effects of these solutions on methane hydrate dissociation
were observed and solution 3 leads to the strongest inhibition effect.
The average hydrate dissociation temperature reduction for methane
hydrate in the presence of solutions 1, 2, and 3 are approximately
1.0, 2.2, and 3.7 K, respectively, in comparison with the pure water
case. Furthermore, to predict methane hydrate dissociation conditions,
a van der Waals-Platteeuw (vdW-P) type model was used. The activity
of water in the liquid/aqueous phase is computed using the NRTL activity
coefficient model and the fugacity of the gas phase is accounted using
the Peng–Robinson equation of state (PR EoS). Results indicate
that there is a good agreement between the experimental and modeled
data.
In this work, experimental hydrate dissociation conditions
of methane
in the presence of 0.06, 0.10, and 0.20 mass fractions of methanol
and 0.10 and 0.25 mass fractions of ethane-1,2-diol in aqueous
solutions are reported. In addition, phase equilibria of a ternary
mixture of methane (0.9319 mole fraction) + ethane (0.0481 mole fraction) + propane (0.02 mole fraction) in the presence of 0.25 mass
fraction of ethane-1,2-diol aqueous solution is investigated. A high-pressure
equilibrium cell is used for measurement of hydrate dissociation conditions
in the temperature range of (265.4 to 282.0) K and pressure range
of (1.97 to 6.96) MPa. The experimental gas hydrate dissociation conditions
are modeled using the van der Waals and Platteeuw (vdW-P) solid
solution theory for dealing with the hydrate phase and the Valderrama–Patel–Teja
equation of state (VPT-EoS) along with the nondensity dependent (NDD)
mixing rules to account for the fluid phases. The obtained experimental
data are finally compared with selected experimental data from the
literature as well as the model predictions, and acceptable agreements are observed.
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