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HYDRATE FORMATION AND
CONTROL
MR. KWAME SARKODIE
OUTLINE
GAS HYDRATE FORMATION
CONDITIONS FOR HYDRATE FORMATION
HYDRATE PROPERTIES
GAS HYDRATE FORMATION PREDICTION
HYDRATE INHIBITION METHODS
GAS HYDRATE FORMATION
Natural gas hydrates are solid crystalline
compounds formed by the chemical combination
of natural gas and water under pressure and at
temperatures considerably above the freezing
point of water.
In the presence of free water, hydrates would form
when the temperature is below a certain degree
(hydrate temperature).
Chemical formulae of gas hydrates :
Methane CH4.7H2O
Ethane C2H6.8H2O
Propane C3H8.18H2O
Carbon dioxide CO2.7H2O
CONDITIONS FOR HYDRATES FORMATION
• Natural gas at or below its water dew point with
liquid water present.
• Temperature below the hydrate formation
temperature for the pressure and gas
composition considered.
• High operating pressures that increase the
hydrate formation temperature.
• High velocity or agitation through piping or
equipment.
• Presence of a small seed crystal of hydrate.
• Presence of H2S and CO2 since these gases are
more soluble in water than in hydrocarbons
HYDRATE BUILD-UP INSIDE A PIPE
PROPERTIES
Gas hydrates are a class of solid, non-stoichiometriccompounds called clathrates.
They form when a host material, water for hydrates through hydrogen bonding, forms a caged structure that contains guest molecules, such as methane.
Both host and guest must be present for the solid to form, but not all of the cages will be occupied.
HYDRATE FORMATION CONDITIONS FOR
PURE METHANE, ETHANE, AND PROPANE
The Figure above shows a break in all of the
curves at 32°F (0°C) because the hydrates are in
equilibrium with gas and ice at the lower
temperatures, and with gas and liquid water at
the higher temperatures.
For the ethane hydrate line, an abrupt change
occurs at 57°F (14°C).
At this point, the hydrate is in equilibrium with
gaseous ethane and both liquid ethane and liquid
water
At higher temperatures, the ethane hydrate is in
equilibrium with liquid ethane and liquid water
GAS HYDRATE FORMATION
PREDICTION
There are three methods basically used in the
prediction of hydrate formation, they are:
K-values method
The gas gravity correlation
The use of computer programs.
In this lecture the gas gravity method would be
discussed.
The figure below shows hydrate formation prediction
curves for natural gases as a function of gas specific
gravity. For below 1,000 psi (70 bar), the figure can
be
t(°F) = −16.5 − 6.83/(SpGr)2 + 13.8 ln[P(psia)]
t(°C) = −6.44 – 3.79/(SpGr)2 + 7.68 ln[P(bara)]
GAS HYDRATE FORMATION
PREDICTION
EXAMPLE
Estimate the hydrate-formation temperature at
325 psia (22.4 bar) for the gas with the
composition in the Table. Compare the results
from curve above and the Equation.
Solution
1. The specific gravity of the gas is calculated as
molar massgas /molar massair = 20.08/28.96 = 0.693.
2. Using the equation,
t = −16.5 − 6.83/(0.693)2 + 13.8 × ln(325) = 49°F.
3. The figure gives 50oF
GAS COMPOSITION
HYDRATE INHIBITION
Three ways exist to avoid hydrate formation in
natural gas streams:
Operate outside the hydrate formation region.
Dehydrate the gas.
Add hydrate inhibitors.
HYDRATE INHIBITORS.
The proper inhibitor dosage must be known to
avoid plugging or needless chemical costs, but
oftentimes it is determined empirically.
The chemical cost, although it is usually a small
fraction of overall operating costs
The reliability of inhibitor injection can be a
problem because of malfunctioning injection
pumps and depleted inhibitor reservoirs,
especially at remote sites.
The possible interaction between hydrate
inhibitors and other additives reduces the
effectiveness of some of additives, an effect that
is usually determined empirically.
HYDRATE INHIBITORS
Chemical hydrate inhibitors come in three types:
1. Antiagglomerates (AA)
2. Kinetic (KHI)
3. Thermodynamic
ANTIAGGLOMERATES
Antiagglomerates
prevent small hydrate particles from
agglomerating into larger sizes to produce a plug.
The inhibitors reside in the liquid hydrocarbon
phase and are most often used in pipelines where
gas is dissolved in oil.
They require testing to ensure proper
concentrations.
KINETIC INHIBITORS
Kinetic inhibitors slow crystal formation by
interfering with the construction of the cages.
advantage is that they can be used at
concentrations in the 1 wt% range in the aqueous
phase, and they are nonvolatile
disadvantage is that the proper dosage must be
determined empirically, as too much inhibitor
may enhance hydrate formation rates
THERMODYNAMIC INHIBITORS
Thermodynamic inhibitors, mainly methanol and
ethylene glycol, are widely used.
They are essentially antifreeze. Inorganic salts
are effective but rarely used, and further
discussion relates only to methanol and ethylene
glycol.
The required dosage of thermodynamic inhibitors
is predictable, but the concentrations can be high,
over 50 wt% of the water phase
THERMODYNAMIC INHIBITORS
A number of empirical correlations, on the basis
of thermodynamic properties of solutions,
predict the amount of any hydrate inhibitor
required to depress hydrate formation
temperatures.
The two most commonly used are discussed
here).
Hammerschmidt (1939) proposed the following
equation:
THERMODYNAMIC INHIBITORS
where
t is the hydrate-depression temperature,°F,
Xi is the mass fraction of inhibitor in the free-water phase,
and MWi is the molecular weight of the inhibitor.
• It is recommended to use this equation for methanol concentrations of 20 to 25 wt% of the water phase;
• It is also recommended to use the equation
for ethylene glycol concentrations up to 60 to 70 wt%.
THERMODYNAMIC INHIBITORS
Nielsen and Bucklin (1983) proposed
Δt(°F) = −129.6 ln Xw,
where Xw is the mole fraction of water in the
aqueous phase
METHANOL VS. ETHYLENE GLYCOL
METHANOL ETHYLENE GLYCOL
More volatile Less volatile
Less viscous (high vapour pressure) More viscous (lower vapour
pressure)
Difficult to recover (requires distillation) Easy to recover (evaporation by
water)
Widely used Less widely used
CONTRASTS
SIMILARITES
Both inhibitors
are hydrophilic and remain predominantly with a
condensed water phase, even if
a condensed hydrocarbon phase is present
Both toxic compounds and must be well treated and before
disposal.
EXAMPLE
A sweet gas with a specific gravity of 0.73 leaves
a gas−liquid separator at 100°F and 600 psia
saturated with water.
The gas drops to 35°F before reaching the next
booster station at 500 psia.
Assume no hydrocarbon condensate has formed
in the line.
Calculate how much methanol must be added to
prevent hydrate formation between the separator
and the booster station per MMscf.
Repeat the calculation for ethylene glycol, which
is added in an 80 wt% mixture with water.
SOLUTION
If the formation of hydrate is probable, then;
Determination of the inhibitor rate requires:
1. Determination of the amount of liquid water
formed
2. Calculation of the required amount of inhibitor
in the water phase
3. Calculation of the required amount of inhibitor
in the gas phase
PROBABLE HYDRATE FORMATION
Use of Equation or chart to predict probable
hydrate formation
Shows that the hydrate formation temperature at
600 psia is 59oF.
This value means a 59°F – 35°F = 24°F sub-
cooling into the hydrate region, and hydrate
formation is probable without inhibition.
THUS WE CARRY ON TO DETERMINE THE
INHIBITOR RATE
DETERMINATION OF THE AMOUNT OF
LIQUID WATER FORMED
From the chart below,
the water content of the gas leaving the separator is
95lb/MMScf and
13lb/MMScf at 35°F and 600 psia
Thus
95 lb – 13 lb = 82 lb of water per MMscf drops out in the
line, assuming worse-case conditions
DETERMINATION OF THE AMOUNT OF LIQUID
WATER FORMED
METHANOL REQUIREMENT
To estimate the concentration of methanol, rearrange
Nielsen and Bucklin Equation to give
ln Xw = −t(°F)/129.6 = −24/129.6 = −0.185
Xw = 0.831 or
XMeOH = 0.169 mole fraction.
In Wt %
= (0.169 × 32)/(0.831× 18 + 0.169 × 32) = 26.6 wt%
or 0.362 lb methanol/lb water
Thus, the methanol needed in the water phase is
0.362 × 82 = 29.7 lb/MMscf.
METHANOL IN THE VAPOR PHASE
To estimate the methanol in the vapor phase use the figure below which at 35oF and 600 psia, gives 1.22 lb methanol vaporized per wt% methanol in the aqueous phase,
or 1.22 × 26.6 = 32 lb methanol per MMscf
Thus, the vapor phase consumes more methanol than does the aqueous phase.
The total amount of methanol required
is (29 + 32) = 61 lb/ MMscf.
If a condensate phase was present as well, the losses estimated by use of the solubility chart would have to be added into that phase.
This amount of methanol will be much less than what goes into the aqueous and vapor phase in gas lines.
RATIO OF METHANOL-VAPOR COMPOSITION TO METHANOL-
LIQUID COMPOSITION.
SOLUBILITY OF METHANOL IN PARAFFINIC HYDROCARBONS AS A FUNCTION OF
TEMPERATURE AT VARIOUS METHANOL CONCENTRATIONS.
ETHYLENE GLYCOL REQUIREMENT
Use the Hammerschmidt Equation with the 2235
constant and a molar mass of ethylene glycol of
62 to obtain the mass fraction of pure glycol
required:
However, the glycol is diluted to 80 wt%. To
obtain the mass of inhibitor solution added per
unit mass of free water present to obtain the
desired concentration,
we use X0 /(X0 – Xi), where X0 is the weight
fraction of inhibitor in the solution to be added.
The amount of inhibitor solution added per
pound of free water initially present is then
0.8/(0.8 – 0.40) = 2.00,
and the total amount of ethylene glycol solution
added is 2.00 × 82 = 164 lb/MMscf.
At these conditions, glycol loss into the vapor
phase is negligible, so the total amount of
solution required is 164 lb/MMscf.