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    A

    Robust Iterative Method

    for

    Flash Calculations

    Using

    the

    Soave Redlich Kwong or

    the

    Peng Robinson

    quation o

    State

    L.X. Nghiem,

    SPE, Computer Modelling Group

    K Aziz,*

    SPE, Computer Modelling Group

    Y.K. Li,

    SPE, Computer Modelling Group

    Abstract

    A robust algorithm for flash calculations that uses an

    equation of state (EOS) is presented. t first uses a

    special version

    of

    the successive substitution (SS)

    method and switches

    to

    Powell s method if poor con

    vergence is observed. Criteria are established for an effi

    cient switch from one method to the other. Experience

    shows that this method converges near the critical point

    and also detects the single-phase region without com

    puting the saturation pressure. The Soave-Redlich

    Kwong

    1

    (SRK) and the Peng-Robinson

    2

    (PR) EOS s are

    used in this work, but the method is general and applies

    to any EOS.

    Introduction

    The calculation

    of

    vaporlliquid equilibrium using an

    EOS

    in

    multi component systems yields a system

    of

    nonlinear equations that must be solved iteratively. The

    SS method is commonly used, but it exhibits poor rate of

    convergence near the critical point. To overcome con

    vergence problems, Newton s method has been used by

    Fussell and Yanosik

    3

    to solve the equations. The

    drawback of Newton s method is the necessity

    of

    com

    puting a complicated Jacobian matrix and its inverse at

    every iteration. Hence, for systems removed from their

    critical point it involves more work to arrive at the solu

    tion than the

    SS

    method. Furthermore, the radius

    of

    con

    vergence of Newton s method is relatively small when

    compared to that of the SS method; hence, a good initial

    Now with Stanford

    u

    01977520/83/00068285 00.25

    Copyright 1983 Society of Petroleum Engineers of AIME

    JUNE 1983

    guess is required before convergence can be achieved.

    The single-phase region usually

    is

    determined

    by

    com

    puting the saturation pressure and comparing

    it

    with the

    pressure

    of

    the system. This requires additional work,

    and it is sometimes difficult to decide whether a dew

    point or bubblepoint pressure, which involve different

    equations, should be computed.

    This paper presents a robust iterative method for flash

    calculations using either the SRK or the PR EOS, both

    of

    which have received much interest in recent years. The

    proposed method combines SS with Powell s iteration,

    which

    is

    a hybrid algorithm consisting

    of

    a quasi-Newton

    method and a steepest-descent method.

    4

    The SS method

    is

    used initially and

    is

    replaced

    by

    Powell s method if

    it

    demonstrates poor convergence, thus taking advantage

    of the simplicity of the former method and the robustness

    of

    the latter. The

    SS

    method has been modified so that

    the single-phase region can be detected without having to

    compute the saturation pressure.

    The nonlinear equations to be solved by

    an

    iteration

    scheme could behave differently, depending on their

    form and the variables for which they are solved. In this

    paper three different approaches are considered with

    Powell s method. One

    of

    the three approaches

    is

    based

    on the minimization of the Gibbs free energy.

    The convergence properties

    of

    the proposed schemes

    are demonstrated by three example problems.

    Equations in Flash Calculations

    At a given pressure and temperature, flash calculations

    yield the number

    of

    moles

    of

    component

    in

    the liquid

    phase, NiL and

    in

    the vapor phase,

    N

    w

    given that

    N

    i

    =1 nc represents the number of moles of each com-

    521

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    ponent

    in

    the feed. The thermodynamic criterion

    of

    vaporlliquid equilibrium is that the Gibbs free energy,

    G be minimized, which gives the following necessary

    conditions.

    aG

    aG

    --=--=0 i=1...ne ................

    1)

    aN

    iL

    aN

    iV

    Since NiL

    +

    NiV = N

    i

    , it easily can be shown

    5

    that

    aG aG

    --=---=G

    iL

    iV

    ,

    i=l.

    ..

    ne

    aN

    iL

    aN

    iV

    ............................. 2)

    where iL is the partial molar Gibbs free energy of com

    ponent i in the liquid phase. When an EOS is used to

    compute_the pa.Itial molar Gibbs free energy, the dif

    ference GiL - G V is related to the fugacities fiL and fiV

    as follows.

    - - fiL.

    GiL -GiV=RT In , 1=

    1.. .ne ..........

    (3)

    fiV

    The expressions for the fugacities using the SRK and

    PR EOS s are given in Appendix A.

    The equilibrium conditions of Eq. I yield

    InfiL

    =0

    i=1...nc

    .......................

    4)

    fiV

    or

    Fi - I =0 i= 1...ne> ....................... (5)

    where Fi is the fugacity ratio,fiLlfiV Eq. 5 represents a

    system of ne nonlinear equations that must be solved

    iteratively for NiL or N

    iV

    .

    Instead of solving directly for NiL or N

    iV

    ,

    it

    is often

    more convenient to solve for mole fractions, which are

    combinations

    of

    N

    i

    , NiL, and N

    iV

    .

    The definitions of mole fractions are given in Appen

    dix B. We also define moles of component

    i

    in liquid

    phase per mole

    of

    feed as

    niL =/LXi

    =NiLIN,

    ........................

    6)

    and moles of component

    i in

    vapor phase per mole of

    feed as

    niV=fvYi

    = N/ N

    . .........................

    7)

    Eq. 5 can be solved for one of the following sets of

    variables.

    /L,x i i= 1...n c - I (LX iteration).

    /v,Yi,

    i=

    1...ne

    - I

    (VY iteration).

    niL, i=1...nc

    (NLiteration).

    niV,

    i=

    1...ne

    (NV iteration).

    It easily can be shown that the variables in each of

    these sets are independent and completely define the

    system. Later in this paper, we will show how Powell s

    method is used to solve Eq. 5 for these sets of variables.

    LX or NL iterations will be used for predominantly liq

    uid systems.

    522

    The equilibrium-phase compositions also can be ob

    tained by minimizing the Gibbs free energy. It is shown

    below how Powell s method readily can be used to ob

    tain the solution from this approach.

    Since niL =NiLIN and niV=NiVIN, we obtain from

    Eqs. 2 and 3:

    I aG I aG fiL

    - In ......... 8)

    NRT an iL NRT an iV fiV

    We see from Eq. 8 that In(jiLlfiV) is equal to the gra

    dient

    of

    GINRT with respect to niL and the gradient of

    -GINRT with respect to niV. Hence, by applying

    Powell s method to solve Eq. 4 instead of Eq. 5, we are

    minimizing

    GINRT

    by using the quasi-Newton method.

    However, in doing so, we do not take advantage of the

    fact that

    In(IiLlfiV), i= 1...n

    e

    ,

    form the gradient of

    GINRT(-GINRT) with respect to niL(niV), i=1...ne

    since we merely were trying to reduce the values of

    In(fiLlfiV) to O. Hence, the refinements that could

    be

    ob

    tained from this additional information

    6

    were not in

    troduced. We define the iterations on

    niL

    and

    niV,

    i = 1...n e as NLM iteration and NVM iteration, respec

    tively. NLM iteration will be used for predominantly

    vapor systems and NVM iteration for predominantly liq

    uid systems.

    In practice, the equilibrium ratios K = Y/x

    i= 1...ne> are introduced. The following equations can

    be derived.

    xi=Z/[I+fv(Ki- l )] , i=1...ne . . . . . . . . . 9)

    Yi=Kiz/[I+fv(Ki-l)], i=1...ne

    . . . . . .

    10)

    ne

    zi(K

    i

    -I

    g(fv)=

    =0. . . . . . . . . . . . . . (11)

    i=i

    I +fv(K

    i

    - I

    Eq. 5 also can be solved iteratively for K

    i

    , i=1...ne

    Once a set

    of

    values has been determined,

    fv

    is

    ob

    tained by solving Eq. II and x i and Y are obtained

    from Eqs. 9 and

    10.

    The SS method usually

    is

    used in

    this case and is described

    in

    the next section.

    ethod o Successive Substitution

    It can be shown that values are related to the fugacity

    coefficients iL and iV as follows.

    = iL = fiLI(XiP) F . ~

    iV fiV1(YiP)

    Xi

    . . . . . . . . . .

    12)

    In this solution, estimated

    K

    values are used to flash

    the mixture at the specified pressure and temperature.

    The liquid and vapor fugacities then are determined from

    the phase compositions, and new estimates for values

    are obtained from Eq. 12. The procedure is assumed

    converged when

    (Fi

    _1 2

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    Solution of

    g(fv

    = 0

    Every time

    K

    values are determined, Eq.

    11

    has to be

    solved for

    Iv(O:5lv:5

    1).

    g O

    is a monotonically

    decreasing function of

    d g l d ~

    L and liquid

    otherwise.

    Criteria for Switching From

    SS

    to Powell s Method

    The important step of the proposed algorithm is the

    switch from

    SS

    to Powell s method. This should lead to

    a decrease in execution time; otherwise the switch is not

    necessary. The criteria for an efficient switch from one

    method to another were determined using a ternary

    system and were then tested on 10- and IS-component

    mixtures.

    The ternary system used was C0

    2

    /nC

    5

    /nC

    I6

    Fig. 2

    shows the calculated phase envelope at 1,500 psia (10.3

    523

  • 7/24/2019 00008285

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    85

    a Calculafed

    15

    mol nC

    1

    6

    Fig 2 Phase envelope of C0

    2

    /nC

    s

    /nC

    16

    system at 1,500 psia

    and 122F. Flash calculations

    in

    Table 1 are for points

    on

    Line

    A.

    MPa) and 122F (SOC). To determine the convergence

    behavior

    of

    the

    SS

    method for mixtures with different

    compositions, a series of flash calculations was per

    formed for mixtures containing 88 CO

    2

    and various

    mole percents of nC 5 and nC

    16.

    These mixtures lie

    along Line A in Fig. 2 and for notational convenience

    will be referred

    to

    using only their mole percent of

    nC

    5.

    This line contains mixtures in the fully developed two

    phase region (e.g.,

    0

    nC 5),

    mixtures near the critical

    point (e.g., 8 nC

    5

    ),

    and mixtures in single-phase

    region (e.g., 12

    nC

    s

    ).

    Plots

    of

    log

    ~ F i

    -1)2 vs. the number of SS iterations

    (SSI) for diffelrent mixtures are shown in Fig.

    3.

    The

    following can be observed.

    1. The convergence of the SS method deteriorates as

    the critical point

    is

    approached.

    2. After a few iterations the slope

    of

    each curve re

    mains almost constant for a l a r ~ e number of iterations.

    This implies that the ratio

    ~ [ F l

    )

    I F / ~ [ F l k - 1 ) I F

    1 1

    is also almost constant during that period and can be

    used as an indication of the rate

    of

    convergence

    of

    the SS

    method for a particular mixture.

    3. For the

    8

    nC

    s

    mixture, ~ F i _1)2 increases after

    44 iterations and then d e c r e s e ~ again after S6 iterations

    (not shown). This type of behavior of the

    SS

    method oc

    curs frequently in the critical region.

    4. For the 11

    nC

    5 mixture, the single-phase region

    is

    detected after 2S iterations.

    Fig. 4 shows the change of ~ F i _1)2 and

    v

    with

    the number of SSI for a mixturb in the fully developed

    524

    2

    \ 11 nC5

    \

    0

    1

    -2

    N

    ..-

    I

    -3

    u..

    1- 1 -

    5

    4

    01

    .2

    -5

    -6

    -7

    -8

    _ 9 L L_ _

    L L

    _ _

    L L

    _ _L L__L L__

    o

    5

    10

    15

    20

    25 30

    35 40 45 50

    No. of SST

    Fig.

    3 Convergence

    rate of 55 for different mixtures of

    C0

    2

    /nC

    s

    /nC

    16

    at 1,500 psia and 122F.

    two-phase region (2 nC

    5),

    a mixture near the critical

    point (8

    nC s),

    and a single-phase mixture (11

    nC 5)

    For a two-phase mixture, ~ F i _1)2 decreases, n l

    v

    1

    reaches its ultimate value rapidly. For a mixture near the

    critical point, the change

    of

    ~ F i _1)2 and

    v is

    slow.

    1

    For a single-phase mixture, the change of v is very

    rapid and a value for

    v

    outside [0,1]

    is

    obtained after a

    few iterations. In this case, we set

    v

    to either zero or

    unity and proceed with the SS method as discussed

    earlier.

    Based on extensive testing

    of

    the flash program, the

    following criteria are proposed to switch from the SS

    method

    to

    Powell's method.

    ~ [ F l k ) - I F / ~ [ F l k - 1 ) - I F > E R (lSa)

    1 1

    Ilv k)

    -lv k-1)

    i =

    fugacity coefficient of component i in liquid

    phase

    Wi

    =

    acentric factor

    of

    component i

    JUNE 1983

    T BLE 5 FLASH C LCUL TIONS FOR THE RESERVOIR OIL

    Pressure

    SS Plus Powell

    Newton

    (psia)

    _ _v_

    SSI Plus

    FE

    SSI Plus FE Iterations

    4,950 0.0116 22 +

    111

    2+55

    2

    4,925 0.1144

    21

    + 56

    2+53

    4

    4,900 0.1770 21 + 49

    2+30

    4

    4,875 0.2206

    20+

    33

    2+28 3

    4,850 0.2536

    20+

    30

    2+27

    3

    4,800 0.3016 19+ 28

    2+27

    4

    4,750 0.3358

    18+

    26

    2+25

    4

    4,700 0.3623

    18+

    26

    2+26

    3

    4,650 0.3838

    17+

    25

    2+25

    3

    4,600 0.4019

    16+

    25

    2+24

    3

    4,550 0.4175

    16+

    25

    2+24 3

    4,500 0.4313

    15+

    25

    2+24 3

    -2

    ,{O 4875 psio

    1.2

    8{ 4875 psio

    fIR

    -1 t:J

    4750

    psio

    ...

    4750

    PSiO

    1.0

    -4

    C\I

    0.8

    .,....

    6

    LL

    .-

    0.6 t)

    c>

    -8

    0

    0.4

    -10

    0.2

    ~ 2 ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~ ~

    16 20 24 28 32 36

    No

    of

    FE

    Fig. 5-Convergence characteristics of Powell s method.

    Subscripts

    c = critical

    i,j,k = component number

    = subscript

    of

    largest equilibrium ratio

    L =

    liquid

    r

    =

    reduced

    s = subscript of smallest equilibrium ratio

    V

    = vapor

    Superscripts

    k) = iteration level

    k

    T

    =

    transpose

    - =

    results from SS method

    cknowledgments

    This research is supported

    by

    the general members of

    Computer Modelling Group and the Alberta/Canada

    527

  • 7/24/2019 00008285

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    Energy Resources Research Fund administered by the

    Dept.

    of

    Energy and Natural Resources of the Province

    of Alberta. We thank R.A. Heidemann and P.K.W. Vin

    some for their helpful comments on this work. The ver

    sions of the SRK and PR equations used are from the

    Hyprotech fluid properties program,

    HYPROP.

    References

    1. Soave, G.: Equil ibrium Constants from a Modified Redlich

    Kwong Equation of State, Chern Eng Sci. (1972) 27,

    1197-1203.

    2. Peng, D.Y. and Robinson, D.B.: A New Two-Constant Equa

    tion of State, Ind Eng. Chern Fund (1976) 59-64.

    3. Fussell, D.D. and Yanosik, J.L.: An Iterative Sequence for

    Phase-Equilibria Calculations Incorporating the Redlich-Kwong

    Equation of State, Soc Pet. Eng. J (June 1978) 173-82.

    4. Powell, M.J.D.: A Hybrid Method for Nonlinear Equations,

    Numerical Methods for Nonlinear Algebraic Equations, P.

    Rabinowitz (ed.), Gordon and Breach, London (1970).

    5. Sandler, S.I.: Chemical and Engineering Thermodynamics, John

    Wiley

    Sons Inc., New York City (1977) 300-04.

    6. Broyden, C.G.: Quasi-Newton Methods and their Application to

    Function Minimization,

    Math

    Compo (1967) 368-81.

    7. Wilson, G.: A Modified Redlich-Kwong Equation

    of

    State, Ap

    plication to General Physical Data Calculations, paper 15C

    presented at the 1968 AIChE National Meeting, Cleveland, OH,

    May

    4-7.

    8. Jarrat, P.:

    A

    Review of Methods for Solving Non-linear

    Algebraic Equations in One Variable, Numerical Methods for

    Nonlinear Algebraic Equations, P. Rabinowitz (ed.), Gordon and

    Breach, London (1970).

    9. Nghiem, L.X. and Heidemann, R.A.: General Acceleration Pro

    cedure for Multiphase Flash Calculation with Application to Oil

    Gas-Water System s, paper presented at the 1982 European Sym

    posium on Enhanced Oil Recovery, Paris, Nov. 8-10.

    10. Michelsen, M.L.:

    The

    Isothermal Flash Problem, Parts I and

    II,

    Fluid Phase Equilibria (1982) 1-40.

    11. Baker, L.E., Pierce, A.C., and Luks, K.D.: Gibbs Energy

    Analysis

    of

    Phase Equilibria,

    Soc Pet. Eng

    J (Oct. 1982)

    731-42.

    12. Broyden, C.G.: A Class

    of

    Methods for Solving Nonlinear

    Simultaneous Equations,

    Math Camp.

    (1965) 577-93.

    13. Peng, D.Y. and Robinson, D.B.: A Rigorous Method for Pre

    dicting the Critical Properties of Multicomponent Systems from an

    Equation

    of State,

    AIChE

    J

    (1977) 23, 137-44.

    14. Bergman, D.F.: Predicting the Phase Behavior of Natural Gas in

    Pipelines, PhD dissertation, U.

    of

    Michigan, Ann Arbor (1976).

    15. Katz, D.L. and Firoozabadi, A.: Predicting Phase Behavior

    of

    Condensate/Crude-Oil Systems Using Methane Interaction Coeffi

    cients,

    J

    Pet.

    Tech

    (Nov. 1978) 1649-55.

    16. Young, L.C. and Stephenson, R.E.: A Generalized Composi

    tional Approach for Reservoir Simulation, paper SPE 10516

    presented at the 1982 SPE Symposium on Reservoir Simulation,

    New Orleans, Feb. 1-3.

    PPENDIX A

    The SRK and PR EOS s

    The details of the development of the SRK and PR

    EOS's are given in Refs. 1 and 2. The final results are

    the following.

    SRK

    528

    RT a T)

    P

    v-b v v+b)

    RTc

    b=0.08664-

    Pc

    and

    PR

    and

    R2T2

    a Tc)

    =0.42747-_

    c

    -

    Pc

    m

    =0.480

    +1.574w

    -0.176w

    2

    .

    RT a T)

    p

    v-b

    v(v+b)+b(v-b)

    RTc

    b=0.07780-

    Pc

    R2Tl

    a(T

    c

    =0 . 45724 - -

    Pc

    m=0.37464+ 1.54226w-0.26992w

    2

    .

    f the compressibility factor, Z =pvIR1), is intro

    duced, the following cubic equations are obtained. For

    SRK,

    Z3 -Z2

    + A -B -B

    2

    )z-AB=0.

    . (A-1a)

    For PR,

    Z3 _(1-B)Z2

    + A

    -3B

    2

    -2B)z-(AB-B

    2

    -B3)=0

    ,

    . (A-1b)

    where A=apIR

    2

    T

    2

    and B=bpIRT.

    Eqs. A 1a and A 1b yield one

    or

    three real roots

    depending on the number

    of

    phases in the system. In the

    two-phase region, the largest root

    is

    the compressibility

    factor of the vapor, while the smallest positive root cor

    responds to that of the liquid.

    For mixtures, the following mixing rules are

    recommended.

    2

    b=

    2. >ibi, (A-2)

    a= ~ i j a i j

    , A-3)

    i

    and

    where 0 j are binary interaction coefficients obtained by

    fitting the predicted binary bubblepoint pressures to ex

    perimental data.

    SOCIETY

    OF

    PETROLEUM ENGINEERS JOURNAL

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    The fugacity coefficient of component

    k

    in a mixture

    can be calculated from the following equations.

    . . . . . . . . . . . . . . . . . . . . . . (A-5a)

    For PR,

    b

    k

    In k=- z - I ) - ln z -B)

    b

    __

    [

    2: . Xiaik

    ~ B a - :kJ

    . In Z+2.414B) , (A-5b)

    z-0.414B

    APPENDIX B

    Mole Fractions Definitions

    Let

    The mole fractions are defined as follows.

    Global mole fraction of component i,

    i

    =N;lN. .

    (B-1)

    Liquid mole fraction of component

    i,

    xi=NiLIN

    L

    .

    (B-2)

    Vapor mole fraction of component i,

    Yi =NiVIN

    v

    . B-3)

    Liquid mole fraction

    of

    the system,

    fL

    =N

    LIN.

    . B-4)

    Vapor mole fraction

    of

    the system,

    fv=NvIN. . (B-5)

    From these definitions we obtain

    i

    =fLXi +fVYi, B-6)

    fL = f v =

    1 , B-7)

    JUNE 1983

    and

    2 :

    Z

    i=

    2:Xi=

    2:Yi=1 .

    i i

    B-8)

    APPENDIX C

    Powell s Hybrid Method

    Consider the problems of finding the root x* of a system

    of

    n

    nonlinear equations in

    n

    unknowns .

    f x)=O

    C-l)

    given a starting iterate x 0) .

    Various methods have been studied and shown to be

    quadratically or superlinearly convergent if x 0) is close

    enough to x*. For many problems, however, a good in

    itial estimate

    is

    not available and therefore a more robust

    algorithm is needed.

    Two well-known methods for solving Eq. C-l are

    Newton s method and the steepest-descent method .

    Newton s method is based on a linear approximation

    of f around the kth iterate x k) .

    f[X k) +a k)] =f[x k)] +J k)a k) ,

    (C-2)

    where

    (

    af ) k)

    J k)=

    -

    ax

    is the Jacobian matrix

    of

    f at

    x k).

    The Newton s step, a k) =x k +

    I)

    -x k), is obtained

    by setting the left side of Eq. C-2 to 0 and solving for

    a k) .

    a k)

    = - J -I k)f k) ,

    (C-3)

    where f k) denotes f x

    k)]

    for convenience. Newton s

    method is quadratically convergent if x k) is close to x*.

    I f

    x k)

    is

    not close to x*, there

    is no

    guarantee that

    x k+ I)

    will be any better than

    x

    k) and Newton s method

    need not converge. A method that guarantees that

    is the steepest-descent method where

    11 11

    denotes the

    Euclidian norm.

    Consider the functional equation

    F x) = z

    T

    x ) f x). . (C-4)

    The steepest-descent direction g is

    g= -

    \ l F x)

    =

    -JTf x) .

    .

    (C-5)

    Given the kth iterate x k) , the steepest -descent step

    p

    k)

    =

    x k+I)

    - x k) is defined by

    p k)

    =J1. k)g k)

    ,

    C-6)

    with J1 k) chosen so that the functional C-4 with f x)

    replaced by f k) + J k)p k) is minimized.

    5 9

  • 7/24/2019 00008285

    10/10

    It can be shown that the value of p, k) that minimizes

    F[X(k)] =

    1 2

    [f(k)

    +

    p, (k) J(k)p(k)] T

    . [f(k)

    +p,(k)J(k)P(k)]

    (C-7)

    is given by

    . . . . . . . . . . . . . . . . . . . . . C-8)

    Although the steepest-descent method avoids

    divergence, it converges very slowly near the solution.

    Powell's hybrid method is a combination of a Newton

    like method and the steepest-descent method. It has the

    divergence-avoiding characteristic of steepest-descent

    method and the rapidly converging property of the

    Newton-like method near the solution.

    Powell's algorithm computes a scalar e k), o ~ e k )

    1, that is used to define the step (k) =x(k+ 1) - x (k ) as

    follows.

    where elk)

    =

    1 corresponds to the Newton-like method

    and elk) =0 corresponds to the steepest-descent method.

    The Jacobian matrix J and its inverse H are computed

    numerically at the beginning of the iteration and updated

    at each step using rank-one matrices according to

    Broyden.

    I2

    [

    f (k+I) _f k ) _J(k) (k) T(k)

    J(k+I) =J(k)

    + .

    T(k) (k)

    C-IO)

    530

    H(k+I )

    =H(k)

    [ (k+

    1)

    _ H(k)[f(k+ I - f (k )J j

    T(k)Hlk)

    ~ ~ ~ ~ ~

    T(k)H(k)[f(k+I) _f lk ) ]

    C-ll)

    A method using this updating scheme is called quasi

    Newton, and the final convergence is superlinear rather

    than quadratic .

    The computation

    of

    e

    n

    Eq. C-9 is given in the follow

    ing. Let be the maximum norm of the correction vector

    . Therefore, if

    I l a k ) I I ~ ~ , ........................... C-12)

    e k) is set to unity (a quasi-Newton step). Otherwise a

    multiple of p is included in in order to satisfy

    I l e a + l - e ) P I I = ~

    ..................... C-13)

    Straightforward algebra gives for j the expression

    e ~

    2

    -IIPI1

    2

    /[ra-p) Tp + a Tp _ ~ 2 ) 2

    + llaI1

    2

    _ ~ 2 ) ~ 2

    -IIPI12)]'12).

    .

    .......

    C-14)

    The = 5 in all examples.

    SI

    Metric onversion Factors

    O OF-32)/1.8

    psi x 6.894 757

    onversion

    factor

    is

    exact

    C

    E+OO = kPa

    SP J

    Original manuscript received in Society of Petroleum Engineers office July 31,1979

    Paper accepted for publication Aug. 19, 1982. Revised manuscripl received Feb. 7,

    1983. Paper SPE 8285) first presented at the 1979 SPE Annual Technical Can

    ference and Exhibition held in Las Vegas, Sept. 23-26.

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