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PRO/II Componentand ThermophysicalPropertiesReference Manual
The software described in this manual is furnished under a licenseagreement and may be used only in accordance with the terms of thatagreement.
Information in this document is subject to change without notice.Simulation Sciences Inc. assumes no liability for any damage to anyhardware or software component or any loss of data that may occur asa result of the use of the information contained in this manual.
Copyright Notice Copyright 1994 Simulation Sciences Inc. All Rights Reserved. Nopart of this publication may be copied and/or distributed without theexpress written permission of Simulation Sciences Inc., 601 S. ValenciaAvenue, Brea, CA 92621, USA.
Trademarks PRO/II is a registered mark of Simulation Sciences Inc.SIMSCI is a service mark of Simulation Sciences Inc.
Printed in the United States of America.
Credi ts Contributors:Althea Champagnie, Ph.D.J ohn CunninghamAllan Harvey, Ph.D.J ohn Tanger, Ph.D.
C.H. Twu, Ph.D.
Layout:Kris Oca
On-line Document Conversion:Mark NortonPeter StepmanAlthea Champagnie, Ph.D.
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Table of Contents
List of Tables TOC-5List of Figures TOC-6
Introduction Int-1
General Information Int-1
What is in This Manual? Int-1
Who Should Use This Manual? Int-1
Finding What you Need Int-1
1.1 Component Data I-3
1.1.1 Defined Components I-4
Component Libraries I-4
Using DATAPREPTM I-6Fixed Properties I-6
Temperature-dependent Properties I-6
Properties From Structure I-8
1.1.2 Petroleum Components I-9
General Information I-9
Property Generation--SIMSCI Method I-9
Property Generation--CAVETT Method I-13
Property Generation--Lee-Kesler Method I-16
1.1.3 Assay Processing I-18
General Information I-18
Cutpoint Sets (Blends) I-19
Interconversion of Distillation Curves I-21
Cutting TBP Curves I-25
Generating Pseudocomponent Properties I-30
Vapor Pressure Calculations I-30
1.2 Thermodynamic Methods I-37
1.2.1 Basic Principles I-38
General Information I-38
Phase Equilibria I-38
Enthalpy I-41
Entropy I-43
Density I-44
1.2.2 Appl ication Guidel ines I-45
General Information I-45
Thermodynamic Expert System (TES) I-45
Refinery and Gas Processes I-46
Natural Gas Processing I-49
Petrochemical Applications I-52
Chemical Applications I-54
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1.2.3 General ized Correlation Methods I-58
General Information I-58
Ideal (IDEAL) I-58
Chao-Seader (CS) I-60
Grayson-Streed (GS) I-61
Erbar Modification to Chao-Seader (CSE) andGrayson-Streed (GSE) I-61
Improved Grayson-Streed (IGS) I-62
Curl-Pitzer (CP) I-62
Braun K10(BK10) I-63
J ohnson-Grayson (J G) I-64
Lee-Kesler (LK) I-64
API I-65
Rackett I-65
COSTALD I-66
1.2.4 Equations of State I-69
General Information I-69
General Cubic Equation of State I-69
Alpha Formulations I-71Mixing Rules I-73
Soave-Redlich Kwong (SRK) I-74
Peng-Robinson (PR) I-74
Soave-Redlich-Kwong Kabadi-Danner (SRKKD) I-75
Soave-Redlich-KwongPanagiotopoulos-Reid(SRKP) and Peng-Robinson Panagiotopoulos-Reid (PRP) I-76
Soave-Redlich-Kwong Modified Panagiotopoulos-Reid (SRKM) and Peng-Robinson ModifiedPanagiotopoulos-Reid (PRM) I-77
Soave-Redlich-Kwong SimSci (SRKS) I-77
Soave-Redlich-Kwong Huron-Vidal (SRKH) andPeng-Robinson Huron-Vidal (PRH) I-79
HEXAMER I-80
UNIWAALS I-83
Benedict-Webb-Rubin-Starling I-84
Lee-Kesler-Plcker (LKP) I-85
1.2.5 Free Water Decant I-88
General Information I-88
Calculation Methods I-88
1.2.6 Liquid Activi ty Coeffi cient Methods I-90
General Information I-90
Margules Equation I-93
van Laar Equation I-94Regular Solution Theory I-95
Flory-Huggins Theory I-96
Wilson Equation I-97
NRTL Equation I-98
UNIQUAC Equation I-99
UNIFAC I-101
Modifications to UNIFAC I-104
Fill Methods I-107
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Henrys Law I-110
Heat of Mixing Calculations I-111
1.2.7 Vapor Phase Fugaci ties I-113
General Information I-113
Equations of State I-114
Truncated Virial Equation of State I-114
Hayden-OConnell I-116
1.2.8 Special Packages I-117
General Information I-117
Alcohol Package (ALCOHOL) I-117
Glycol Package (GLYCOL) I-120
Sour Package (SOUR) I-122
GPA Sour Water Package (GPSWATER) I-125
Amine Package (AMINE) I-127
1.2.9 Electrolyte Mathematical Model I-131
Discussion of Equations I-131
Modeling Example I-133
1. 2.10 Electrolyte Thermodynamic Equations I-135
Thermodynamic Framework I-135Equilibrium Constants I-135
Aqueous Phase Activities I-136
Vapor Phase Fugacities I-139
Organic Phase Activities I-143
Enthalpy I-143
Aqueous Liquid Phase I-144
Molar Volume and Density I-144
1.2.11 Sol id-Liquid Equi l ibria I-147
General Information I-147
vant Hoff Equation I-147
Solubility Data I-148Fill Options for Solubility Data I-148
1.2.12 Transport Properties I-150
General Information I-150
PURE Methods I-150
PETRO Methods I-151
TRAPP Correlation I-155
Special Methods for Liquid Viscosity I-157
Liquid Diffusivity I-159
Index Idx-1
PRO/II Component and Thermophysical Properties Table of Contents TOC-3Reference M anual
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List of Tables
1.1.1-1 PRO/II Library Component Properties . . . . . . . . . . . . . I-5
1.1.1-2 PRO/II Temperature-dependent Property Equations andExtrapolation Conventions . . . . . . . . . . . . . . . . . . . I-7
1.1.1-3 PRO/II Vapor Pressure Equations . . . . . . . . . . . . . . . . I-7
1.1.2-1 Values of Constants for Equations (14)-(17) . . . . . . . . . . I-11
1.1.3-1 Primary TBP Cutpoint Set . . . . . . . . . . . . . . . . . . . . I-19
1.1.3-2 Blending Example . . . . . . . . . . . . . . . . . . . . . . . . I-20
1.1.3-3 Values of Constants a, b, c . . . . . . . . . . . . . . . . . . . I-23
1.1.3-4 Values of Constants a, b . . . . . . . . . . . . . . . . . . . . . I-25
1.2.2-1 Methods Recommended for Low Pressure Crude Systems . . I-47
1.2.2-2 Methods Recommended for High Pressure Crude Systems . . I-47
1.2.2-3 Methods Recommended for Reformers and Hydrofiners . . . . I-48
1.2.2-4 Methods Recommended for Lube Oil and SolventDe-asphalting Units . . . . . . . . . . . . . . . . . . . . . . . I-48
1.2.2-5 Methods Recommended for Natural Gas Systems . . . . . . . I-50
1.2.2-6 Methods Recommended for Sour Water Systems . . . . . . . I-51
1.2.2-7 Recommended Ranges for Amine Systems . . . . . . . . . . . I-52
1.2.2-8 Methods Recommended for Light Hydrocarbons . . . . . . . . I-52
1.2.2-9 Methods Recommended for Aromatics . . . . . . . . . . . . . I-53
1.2.2-10 Methods Recommended for Aromatic/Non-aromaticSystems . . . . . . . . . . . . . . . . . . . . . . . . . . . . . I-54
1.2.2-11 Methods Recommended for Alcohol Systems . . . . . . . . . I-54
1.2.2-12 Methods Recommended for Non-ionic Chemical Systems . . . I-56
1.2.2-13 Methods Recommended for Ionic Chemical Systems . . . . . I-56
1.2.2-14 Methods Recommended for Environmental Applications . . . I-57
1.2.2-15 Methods Recommended for Solid Applications . . . . . . . . I-57
1.2.4-1 Some Cubic Equations of State . . . . . . . . . . . . . . . . . I-69
1.2.4-2 Constants for Two-parameter Cubic Equations of State . . . . I-70
1.2.4-3 Alpha Formulations . . . . . . . . . . . . . . . . . . . . . . . I-72
1.2.5-1 Components Available in the SIMSCI Water Solubility Method . I-89
1.2.6-1 Margules Equation . . . . . . . . . . . . . . . . . . . . . . . I-93
1.2.6-2 van Laar Equation . . . . . . . . . . . . . . . . . . . . . . . . I-94
1.2.6-3 Regular Solution Theory . . . . . . . . . . . . . . . . . . . . I-95
1.2.6-4 Flory-Huggins Theory . . . . . . . . . . . . . . . . . . . . . . I-96
1.2.6-5 Wilson Equation . . . . . . . . . . . . . . . . . . . . . . . . . I-97
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1.2.65 Wilson Equation . . . . . . . . . . . . . . . . . . . . . . . . . I-97
1.2.6-6 NRTL Equation . . . . . . . . . . . . . . . . . . . . . . . . . . I-98
1.2.6-7 UNIQUAC Equation . . . . . . . . . . . . . . . . . . . . . . . I-99
1.2.6-8 UNIFAC . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . I-101
1.2.8-1 Components Available for ALCOHOL Package . . . . . . . . . I-118
1.2.8-2 Components Available for GLYCOL Package . . . . . . . . . . I-120
1.2.8-3 Application Guidelines for Amine Systems . . . . . . . . . . . I-129
1.2.11-1 vant Hoff . . . . . . . . . . . . . . . . . . . . . . . . . . . . I-148
1.2.12-1 Transport Properties . . . . . . . . . . . . . . . . . . . . . . . I-150
1.2.12-2 Stream Average Properties . . . . . . . . . . . . . . . . . . . I-151
1.2.12-3 TRAPP Components (3.3 versions) . . . . . . . . . . . . . . . I-156
List of Figures1.1.3-1 Cutting TBP Curves . . . . . . . . . . . . . . . . . . . . . . . I-27
1.1.3-2 Matching Lightends to TBP Curve . . . . . . . . . . . . . . . . I-30
1.2.6-1 Flowchart for FILL Methods . . . . . . . . . . . . . . . . . . . I-109
1.2.8-1 Binary Interaction Data in the Alcohol Databank . . . . . . . . I-119
1.2.8-2 Binary Interaction Data in the Glycol Databank . . . . . . . . . I-121
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Introduction
GeneralInformation
The PRO/II Component and Thermophysical Properties Reference Manual
provides details on the basic equations and calculation techniques used in the
PRO/II simulation program. It is intended as a complement to the PRO/II
Keyword Input Manual, providing a reference source for the background behindthe various PRO/II calculation methods.
What is inThis Manual?
This manual contains the correlations and methods used to calculate thermo-
dynamic and physical properties, such as the Soave-Redlich-Kwong (SRK)
cubic equation of state for phase equilibria. This manual also contains infor-
mation on the definition of pure components and petroleum fractions.
For each method described, the basic equations are presented, and appropri-
ate references provided for details on their derivation. General application
guidelines are provided, and, for many of the methods, hints to aid solution
are supplied.
Who Should UseThis Manual?
For novice, average, and expert users of PRO/II, this manual provides a good
overview of the property calculation methods used to simulate a single unit
operation or a complete chemical process or plant. Expert users can find
additional details on the theory presented in the numerous references cited
for each method. For the novice to average user, general references are also
provided on the topics discussed, e.g., to standard textbooks.
Specific details concerning the coding of the keywords required for the
PRO/II input file can be found in the PRO/II Keyword Input Manual.
Detailed sample problems are provided in the PRO/II Application Briefs
Manual and in thePRO/II Casebooks.
Finding Whatyou Need
A Table of Contents and an Index are provided for this manual. Cross-
references are provided to the appropriate section(s) of the PRO/II Keyword
Input Manual for help in writing the input files.
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Symbols Used in This Manual
Symbol Meaning
Indicates a PRO/II input coding note. The number beside the
symbol indicates the section in the PRO/II Keyword Input
Manualto refer to for more information on coding the
input file.
Indicates an important note.
Indicates a list of references.
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Component Data
PRO/II allows the user to specify pure-component physical property data for agiven simulation. Pure component data are usually associated with either a prede-
fined component in a data library, a user-defined (non-library) component, or a
petroleum pseudocomponent.
Properties for defined components can be accessed in a variety of ways. They can be
retrieved from an on-line databank or library, estimated from structural or other
data, or input by the user as non-library components. User input can be used to
override properties retrieved from the libraries.
Properties for pseudo or petroleum components are derived from generalized
correlations based on minimal data, usually the normal boiling point, molecular
weight, and standard density. Hydrocarbon streams defined in terms of assay data
(including distillation data) can be converted to discrete pseudocomponents by a
number of assay processing methods.
1. 1
Section 1.1 Component Data
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Defined Components
ComponentLibraries
Table 1.1.1-1 lists the property data available in the built-in component libraries for
predefined components. These libraries include the PROCESS library (the physical
property library used as the default in PROCESS, PIPEPHASE, HEXTRAN, and
early versions of PRO/II), the SIMSCI library (a fully documented physical prop-
erty bank), the DIPPR (Design Institute for Physical Property Research) library
from the American Institute of Chemical Engineers, and the OLILIB library of
electrolyte species, which contains a subset of the library component properties
listed in the following sections.
Most of the fixed properties used in a simulation can be found in the input
reprint of the simulation. The coefficients of the correlations used for the
temperature-dependent properties stored in the libraries are not shown be-
cause they are usually covered by contractual agreements which disallowtheir display in a simulation.
References
1. PPDS, Physical Property Data Service, jointly sponsored by the National
Physical Laboratory, National Engineering Laboratory, and the Institution
of Chemical Engineers in the UK.
2. DIPPR, Design Institute for Physical Property Data, sponsored by the
American Institute of Chemical Engineers.
1.1.1
Component Data Section 1.1
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Table 1.1.1-1: PRO/II Library Component Properties
Fi xed Pr operti es and Constants Tem peratur e-dependent Pr operti es
Acentric Factor Enthalpy of Vaporization
Carbon Number Ideal Vapor Enthalpy
Chemical Abstract Number Liquid Density
Chemical Formula Liquid Thermal ConductivityCritical Compressibility Factor Liquid Viscosity
Critical Pressure Saturated Liquid Enthalpy
Critical Temperature Solid Density
Critical Volume Solid Heat Capacity
Dipole Moment Solid Vapor Pressure
Enthalpy of Combustion Surface Tension
Enthalpy of Fusion Vapor Pressure
Flash Point Vapor Thermal Conductivity
Free Energy of Formation Vapor Viscosity
Freezing Point (normal melting point)
Gross Heating Value
Heat of Formation
Hydrogen Deficiency Number
Liquid Molar Volume
Lower Heating Value
Molecular Weight
Normal Boiling Point
Rackett Parameter
Radius of Gyration
Solubility Parameter
Specific Gravity
Triple Point Temperature
Triple Point Pressure
UNIFAC Structure
van der Waals Area and Volume
Section 1.1 Component Data
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Using DATAPREPTM SimSci provides an interactive program, DATAPREP, for review and ma-nipulation of the pure component fixed and temperature-dependent proper-
ties available for defined components in libraries. DATAPREP is PC based.
Detailed descriptions for both the fixed and temperature-dependent library
properties mentioned above are contained in Appendix A of theDATAPREP
User Guide.
A comprehensive summary of the available data for each component, for any
release of the libraries, can also be generated by using DATAPREP.
DATAPREPs functionality also includes the ability to generate keyword
input file inserts containing component properties for non-library compo-
nents. Private pure component libraries can also be made using DATAPREP.
In addition to the USER.LB1 and USER.LB2 files that can be used directly
by PRO/II on a PC, ASCII input files are generated for input to the library
manager program for use on other platforms. Please refer to theDATAPREP
User Guidefor further information about its capabilities.
ReferenceDATAPREP User Guide, 1991, Simulation Sciences Inc.
Fixed Properties As explained in the above section, these properties are described in Appen-dix A of theDATAPREP User Guide. Some things to be aware of are that
the specific gravities of permanent gases are often given relative to air, with-
out any annotations in the output, and liquid molar volumes can be
extrapolated from a condition very different from 77F (25 C), if thecomponent doesnt naturally exist as a liquid at 77 F.
Temperature-
dependentProperties
The temperature-dependent correlations available for use in PRO/II are listed
in Section 17, Component Properties, of the PRO/II Keyword Input Manual.The equations that are typically used to represent a property are listed in Ta-
ble 1.1.1-2. While temperature-dependent library properties are fitted and are
usually very accurate at saturated, subcritical conditions, caution must be
used in the superheated or supercritical regions.
Because of the form of some of the allowable temperature-dependent equations,
extrapolation beyond the minimum and maximum temperatures is not done using
the actual correlation. PRO/II has adopted the rules shown in Table 1.1.1-2, based
on the property, for extrapolation of the temperature-dependent correlations.
Component Data Section 1.1
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Table 1.1.1-2: PRO/II Temperature-dependent Property Equations andExtrapolation Conventions
Temperature-dependentProperty
RecommendedEquations
ExtrapolationMethod
Vapor Pressure 14, 20, 21, 22 ln(Prop.) vs. 1/T
Liquid Density 1, 4, 16, 32 Prop. vs. T
Ideal Vapor Enthalpy 1, 17, 41 Prop. vs. T
Enthalpy of Vaporization 4, 15, 36, 43 Prop. vs. T
Saturated Liquid Enthalpy 1, 42, 35 Prop. vs. T
Liquid Viscosity 13, 20, 21 ln(Prop.) vs. 1/T
Vapor Viscosity 1, 19, 26, 27 Prop. vs. T
Liquid Thermal Conductivity 1, 4, 34 Prop. vs. T
Vapor Thermal Conductivity 1, 19, 33 Prop. vs. T
Surface Tension 1, 15, 30 Prop. vs. T
Solid Thermal Conductivity 1 Prop. vs. T
Solid Density 1 Prop. vs. T
Solid Cp or Enthalpy 1 Prop. vs. T
Solid Vapor Pressure 20 ln(Prop.) vs. 1/T
Another note of caution concerns the use of equations 20 and 21 in modeling
component vapor pressures. These equations are actually combinations of
two or more traditionally used vapor pressure equations (e.g., Antoine). It is
intended that the user apply only subsets of the available coefficients with
these equations corresponding to the more traditional equations. Table
1.1.1-3 gives some examples of this mapping.
Table 1.1.1-3: PRO/II Vapor Pressure Equations
Equation 20 / 21 Coefficients
Common VP Equations (#) C1 C2 C3 C4 C5 C6 C7
Clapeyron (20 or 21) x x
Antoine (21) x x x
Riedel (20) x x x x
Frost-Kalkwarf (21) x x x x
Reidel-Plank-Miller (20) x x x x
Section 1.1 Component Data
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Properties FromStructure
Properties for defined components, either library or non-library, may be
estimated if the user supplies a component structure and invokes the FILL
option in the component data category of input. This procedure primarily
uses the methods of Joback and is good for components with molecular
weights below 400 and components with less than 20 unique structural
groups. More accurate results are obtained for components containing just
one type of functional group. For example, amine properties would be moreaccurate than those predicted for an ethanol amine, which would contain
functional groups for both an alcohol and an alcohol amine. This feature is
available in DATAPREP and in PRO/II for all versions subsequent to v3.3.
Complete documentation of the estimation techniques used is contained in
Section 3.7, Prediction,of theDATAPREP User Guide.
Component Data Section 1.1
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Petrol eum Components
GeneralInformation
Petroleum components (often called pseudocomponents) are either defined
on a one-by-one basis on PETROLEUM statements or generated from one or
more streams given in terms of assay data. The processing of assays is de-
scribed in Section 1.1.3,Assay Processing. Each individual pseudocompo-
nent is typically a narrow-boiling cut or fraction. Component properties are
generated based on two of the following three properties:
Molecular weight.
Normal boiling point (NBP).
Standard liquid density.
If only two are supplied, the third is computed with the SIMSCI method (or
with another method if requested with the MW keyword). These methods are
described in the sections below.
From those three basic properties, the program estimates all other properties
needed for the calculation of thermophysical properties. Three different sets of
characterization methods are provided. These are known as the CAVETT, SIM-
SCI, and Lee-Kesler methods. The Cavett methods developed in 1962 have been
the default in all versions of PRO/II up to and including the 3.5 series. The SIM-
SCI methods use a combination of published (Black and Twu, 1983; Twu, 1984)
and proprietary methods developed by SimSci. These are the default for all
PRO/II versions subsequent to the 3.5 series. The LK option accesses methods
developed by Lee and Kesler in 1975 and 1976.
PropertyGeneration--
SIMSCI MethodCriti cal Properties and Acentric Factor
The SIMSCI characterization method was developed by Twu in 1984. It
expresses the critical properties (and molecular weight) of hydrocarbon com-
ponents as a function of NBP and specific gravity. The correlation is ex-
pressed as a perturbation about a reference system of normal alkanes. The
critical temperature (in degrees Rankine) is given by:
(1 )Tc=Tc
1 +2fT
1 2fT
2
(2 )fT=SGT0.362456
Tb12+0.03982850.948125
Tb12
SGT
1.1.2
Section 1.1 Component Data
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(3 )SGT=exp5
SG
SG
1
(4 )Tc=Tb(0.533272 +0.19101710
3Tb+0.77968110
7Tb
2
0.2843761010Tb3+0.9594681028Tb13)1
(5 )SG
=0.843593 0.1286243.36159
3
13749.512
where:
SG = specific gravity
Tb= normal boiling point, degrees Rankine
= 1 - Tb/ Tc
SG = specific gravity correctionf = correction factor
SG = specific gravity
subscript Trefers to the temperature
subscript crefers to the critical conditions
superscript refers to the reference system
The critical volume (in cubic feet per pound mole) and the critical pressure
(in psia) are given by similar expressions:
(6 )V
c=V
c
1+2f
V
1 2f
V
2
(7 )fV=SGV
0.466590
Tb12+0.182421+3.01721
Tb12
SGV
(8 )SGV=exp 4
SG
2SG2
1
(9 )Vc
=
1
0.419869 0.5058391.5643639481.7014
8
(10)Pc=Pc
Tc
TcVc
Vc
1+2fP
12fP
2
(11)f
P=SG
P[2.5326246.1955
Tb120.00127885T
b
+11.4277 +252.140Tb
12+0.00230535TbSGP]
(12)SGP=exp0.5
SG
SG
1
(13)Pc
=3.83354+1.19629
12+34.8888+36.19522+104.19342
where:
V = molar volume, ft3/lbmole
P = pressure, psia
subscripts Vand Prefer to the volume and pressure
Component Data Section 1.1
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The acentric factor for the SIMSCI method is estimated with the use of a gen-
eralized Frost-Kalkwarf vapor equation developed at SimSci. The equation is
given by:
(14)lnPR=A1+A4
+A2+A5
TR+A3+A6
lnTR+A7PRTR2
where:
A1toA7= constants given in Table 1.1.2-1
PR= reduced pressure (P/Pc)
TR= reduced temperature (T/Tc),
= a parameter evaluated at the NBP and given by:
(15)
=lnPR,bA7PR,b
TR,b2f
TR,bf
TR,b
where:
subscriptsR,bindicate reduced properties evaluated at the
normal boiling point
Functionsfandfare given by:
(16)f(TR)=A1+A2TR+A3lnTR
(17)f(TR)=A4+A5
TR+A6lnTR
The values of the seven constants in these equations are shown in Table 1.1.2-1.
Table 1.1.2- 1: Values ofConstants for Equations (14)-(17)
A1 10.2005
A2 -10.6317
A3-5.58058
A4 2.09167
A5 -2.09167
A6 1.70214
A7 0.4312
To compute the acentric factor, the parameter is determined using equation(15) and the known (or already estimated) values for the critical temperature
and pressure and the normal boiling point (NBP). This is then used in equation
(14) to compute the reduced vapor pressure at a reduced temperature of 0.7,
which is then used in the definition of the acentric factor:
(18)=log10PR,TR=0.71
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Other Fixed Properties
The heat of formation is computed from a proprietary correlation developed by
SimSci. The solubility parameter is estimated from the following equation:
(19)=
HVRT
VL
12
The molar latent heat of vaporization, HV, is computed from the Kistiakowsky-Watson method described later on in this section, while VLis the liquid molar
volume at 25 C.
Temperature-dependent Properties
The ideal-gas enthalpy (needed for equation-of-state calculations) is calcu-
lated from the method of Black and Twu developed in 1983. The method was
an extension of work done by Lee and Kesler and involved fitting a wide vari-
ety of ideal-gas heat capacity data for hydrocarbons from the API 44 project
and other sources. The equation (which produces enthalpies in Btu/lb and
uses temperatures in degrees Rankine) is as follows:
(20)H
=A1+A2T+
A32
T2+
A4
3T
3
(21)A2=C1+C7C4
(22)A3=C2+C7C5
(23)A4=C3+C7C6
(24)C1=0.33886 +0.02827K
(25)C2=(0.9291 1.1543K+0.0368K
2)104
(26)C3=1.665810
7
(27)C4=(0.26105 0.59332K)
(28)C5=4.9210
4
(29)C6=(0.536 0.6828K)107
(30)C7=[(12.8 K)(10 K)
10K]2
The Watson characterization factor, K, is defined as:
(31)K=NBP
13
SG
where:
NBP = normal boiling point in degrees Rankine
SG = specific gravity
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The constantA1in equation (20) is determined so as to give an enthalpy of zero
at the arbitrarily chosen zero for enthalpy, which is the saturated liquid at 0 C.The latent heat of vaporization as described below (to get from saturated liq-
uid to saturated vapor) and the SRK equation of state (to get from saturated
vapor to ideal gas) are used to compute the enthalpy departure between this
reference point and the ideal-gas state.
The vapor pressure is calculated from the reduced vapor-pressure equation(14) used above in the calculation of the acentric factor. The latent heat of
vaporization is also calculated from equation (14). The saturated liquid en-
thalpy is calculated by computing the departure from the ideal-gas enthalpy,
as a sum of the latent heat and the enthalpy departure (computed with the
SRK equation of state) for the saturated vapor. The saturated liquid density is
computed by applying the Rackett equation (see Section 1.2.3, Generalized
Correlation Methods) to saturated temperature and pressure conditions as
predicted from the vapor-pressure equation (14).
PropertyGeneration--
CAVETT Method
Critical Properties and Acentric Factor
Optionally, the user may choose to compute critical properties from the meth-
ods developed in 1962 by Cavett. This option is called the CAVETT method.
The equations are:
(32)Tc=768.07121 +1.7133693Tb0.0010834003Tb20.0089212579(API)Tb
+0.38890584106Tb3+0.5309492(API)Tb
2+0.327116107(API)2Tb
2
(33)log10Pc=2.8290406 +0.94120109103
Tb0.30474749105
Tb2
0.2087611104(API)Tb+0.15184103108T
b
3+0.11047899107(API)T
b
2
0.48271599107
(API)2
Tb+0.13949619109
(API)2
Tb2
where:
Tc= critical temperature in degrees Rankine
Pc= critical pressure in psia
Tb= normal boiling point in degrees Fahrenheit
API = API gravity
When the CAVETT characterization options are chosen, the acentric factor is
computed by a method due to Edmister (1958):
(34)=3
7
log10Pc
(Tc
Tb
)1
1
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In equation (34), Pcis in atmospheres. Finally, the critical volume is esti-
mated from the following equation:
(35)Zc=
PcVcRTc
=0.291 0.08
15 PRO/II Note: For more information on using the CAVETT characterizationmethod, see Section 15, Petroleum Component Properties, of the PRO/IIKeyword Input Manual.
Other Fixed Properties
When the CAVETT characterization option is chosen, the heat of formation
and solubility parameter are calculated exactly as in the SIMSCI method
above.
Temperature-dependent Properties
Ideal-gas enthalpies (in Btu/lb-mole) are computed with the following equations:
(36)H=A+BT+CT2+DT3
(37)A=a5MWa4+a0
(38)B=459.67 (1379.01a12a2)+a3
(39)C=a21379.01a1
(40)D=a1=9.17510
11API5.633108MW
(41)a2=3.10710
45.832108APIMW
(42)a3=
1.702510
6
1.489106
APIAPI2.85710
5API
+4.29310
33.084104KK+0.088)K0.819
MW
(43)a4=459.67
459.67
459.67a1a2
+a3
(44)a5=(0.351K8.953)K+43.402
K+188.25
+3.53510
4API0.053API5.95610
3K+3.544
API
where:
T = temperature in degrees Rankine
MW = molecular weight
API = API gravityK = Watson K-factor defined by equation (31)
The constant a0in equation (37) is determined so as to be consistent with the
arbitrary zero of enthalpy, which is the saturated liquid at 0 C.
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Vapor pressures (in psia) are computed from a generalized Antoine equation:
(45)ln P=A+ B
T80.0
(46)A=ln(14.696) B
Tb80.0
(47)B=
ln Pcln(14.696)1
Tc80.0 1
Tb80.0
Temperatures (including the critical temperatureTcand normal boiling point
Tb) are in degrees Rankine.
The saturated liquid density (in lb/ft3) is computed as follows:
(48)L
=A+BT+CT2
(49)A=1.328 L,60
(50)B=
0.3076 L,60Tc
(51)C=
0.3989 L,60Tc
2
where:
L,60
= liquid density at 60 F, calculated from the specific gravityand the density of water
Temperatures are in degrees Rankine
The latent heat of vaporization (in Btu/lb-mole) is calculated from a combina-
tion of the Watson equation (Watson, 1943, Thek and Stiel, 1966), for the tem-perature variation of the heat of vaporization, and the expression of
Kistiakowsky (1923), for the heat of vaporization at the normal boiling point:
(52)
Hvap
=H0
TcT
TcTb
0.38
(53)H0=Tb7.58 +4.571 lnTb
The critical temperature Tc, normal boiling point Tb, and temperature Tare
all in degrees Rankine.
The saturated liquid enthalpy is estimated with the correlation of Johnson
and Grayson. This method is discussed in Section 1.2.3, Generalized Correla-tion Methods. A constant is added so that the saturated liquid enthalpy is
zero at 0 C.
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PropertyGeneration--Lee-
Kesler Method
Criti cal Properties and Acentric Factor
Kesler and Lee used the following equations in 1976 to correlate critical tem-
peratures and critical pressures of hydrocarbons:
(54)
Tc
=341.7
+811SG
+
(0.4244
+0.1174 SG
)T
b
+
(0.4669
3.2623 SG
)10
5
T
b
(55)
lnPc=8.3634 0.0566SG0.24244 +2.2898SG+0.11857SG
210
3Tb+
1.4685 +3.648
SG+0.47227 SG210
7Tb
20.42019 +1.6977
SG210
10Tb
3
where:
Tc, Tb= critical and normal boiling temperatures (both in degrees
Rankine)
Pc= critical pressure in psia
SG = specific gravity
The acentric factor is estimated from an equation in an earlier work by Lee
and Kesler (1975):
(56)=
lnPR,b5.92714 +6.09648TR,b+1.28862lnTR,b0.169347TR,b6
15.251815.6875TR,b13.4721 lnTR,b+0.43577TR,b6
where:
subscriptsR,bindicate reduced properties evaluated at the normal
boiling point
The critical volume is then estimated from the following equation:
(57)Zc=
PcVcRTc
=0.29050.085
Other Fixed Properties
When the Lee-Kesler characterization option is chosen, the heat of formation
and the solubility parameter are calculated exactly as in the SIMSCI method
described previously.
Temperature-dependent Properties
Ideal-gas enthalpies (in Btu/lb-mole) are computed by integrating the follow-
ing equation for the ideal-gas heat capacity:
(58)
Cp
=0.33886 +0.02827K0.9291 1.1543K+0.0368K2
104
T1.6658107
T
2
(CF)0.26105 0.59332(4.56 9.48)104
T(0.536 0.6828)107T2
Component Data Section 1.1
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The factor CFis given by:
(59)CF=[(12.8 K)(10 K)(10)]
2
where:
K = Watson K-factor defined by equation (31)
T = temperature in degrees Rankine
= acentric factor as calculated by equation (56)
The constant of integration is determined so as to give an enthalpy of zero at the
arbitrarily chosen basis for enthalpy, which is the saturated liquid at 0 C.
When the Lee-Kesler characterization option is chosen, the vapor pressure,
saturated liquid density, saturated liquid enthalpy, and latent heat of vaporiza-
tion are all calculated by the methods used for CAVETT characterization, as
described in the previous section.
References
1. Black, C., and Twu, C.H., 1983, Correlation and Prediction ofThermodynamic Properties for Heavy Petroleum, Shale Oils, Tar Sands
and Coal Liquids, paper presented at AIChE Spring Meeting, Houston,
March 1983.
2. Cavett, R.H., 1962, Physical Data for Distillation Calculations -
Vapor-Liquid Equilibria, 27th Mid-year Meeting of the API Division of
Refining, 42[III], 351-357.
3. Edmister, W.C., 1958, Applied Hydrocarbon Thermodynamics, Part 4:
Compressibility Factors and Equations of State, Petroleum Refiner,
37(4), 173.
4. Kesler, M.G., and Lee, B.I., 1976, Improve prediction of enthalpy of
fractions,Hydrocarbon Proc., 53(3), 153-158.
5. Kistiakowsky, W., 1923,Z. Phys. Chem., 107, 65.
6. Lee, B.I., and Kesler, M.G., 1975, A Generalized Thermodynamic
Correlation Based on Three-Parameter Corresponding States,AIChE J.,
21, 510-527.
7. Thek, R.E., and Stiel, L.I., 1966, A New Reduced Vapor Pressure Equation,
AIChE J., 12, 599-602.
8. Twu, C.H., 1984, An Internally Consistent Correlation for Predicting the
Critical Properties and Molecular Weights of Petroleum and Coal-tar
Liquids, Fluid Phase Equil., 16, 137-150.
9. Watson, K.M., 1943,Ind. Eng. Chem., 35,398.
Section 1.1 Component Data
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Assay Processing
GeneralInformation
Hydrocarbon streams may be defined in terms of laboratory assay data. Typi-
cally, such an assay would consist of distillation data (TBP, ASTM D86,
ASTM D1160, or ASTM D2887), gravity data (an average gravity and possi-
bly a gravity curve), and perhaps data for molecular weight, lightends compo-
nents, and special refining properties such as pour point and sulfur content.
This information is used by PRO/II to produce one or more sets of discrete
pseudocomponents which are then used to represent the composition of each
assay stream.
The process by which assay data are converted to pseudocomponents can be ana-
lyzed in terms of several distinct steps. Before each of these is examined in de-
tail, it will be useful to list briefly each step of the process in order:
The user defines one or more sets of TBP cutpoints (or accepts the de-fault set of cutpoints that PRO/II provides). These cutpoints define the
(atmospheric) boiling ranges that will ultimately correspond to each
pseudocomponent. Multiple cutpoint sets (also known as blends) may
also be defined to better model different sections of a process.
Each set of user-supplied distillation data is converted to a TBP (True
Boiling Point) basis at one atmosphere (760 mm Hg) pressure.
The resulting TBP data are fitted to a continuous curve and then the pro-
gram cuts each curve to determine what percentage of each assay
goes into each pseudocomponent as defined by the appropriate cutpoint
set. Gravity and molecular weight data are similarly processed so that
each cut has a normal boiling point, specific gravity, and molecular
weight. During this step, the lowest-boiling cuts may be eliminated ormodified to account for any lightends components input by the user.
Within each cutpoint set, all assay streams using that set (unless they are
explicitly excluded from the blending - this is described later) are com-
bined to get an average normal boiling point, gravity, and molecular
weight for each of the pseudocomponents generated from that cutpoint
set. These properties are then used to generate all other properties (criti-
cal properties, enthalpy data, etc.) for that pseudocomponent.
Note: Special refinery properties such as cloud point and sulfur content mayalso be defined within assays. The distribution of these properties into pseudo-
components and their subsequent processing by the simulator is outside thescope of this chapter but will be covered in a later document.
1.1.3
Component Data Section 1.1
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Cutpoint Sets(Blends)
Defining Cutpoints
In any simulation, there is always a primary cutpoint set, which defaults
as shown in Table 1.1.3-1.
Table 1.1.3-1: Prim ary TBP Cutpoint Set
TBP Range, oF Number ofComponents Width, oF
100-800 28 25
800-1200 8 50
1200-1600 4 100
The primary cutpoints shown in Table 1.1.3-1 may be overridden by supply-
ing a new set for which no name is assigned. In addition, secondary sets
of cutpoints may be supplied by supplying a set and giving it a name. The
blend with no name (primary cutpoint set) always exists (even if only named
blends are specifically given); there is no limit to the number of named
blends (secondary cutpoint sets) that may be defined. The user may designate
one cutpoint set as the default; if no default is explicitly specified, the pri-mary cutpoint set will be the default. Each cutpoint set (if it is actually used
by one or more streams) will produce its own set of pseudocomponents for
use in the flowsheet.
15 PRO/II Note: For more information on specifying TBP cutpoint sets, see Section15, Petroleum Component Properties, of thePRO/II Keyword Input Manual.
Association of Streams With Blends
Each assay stream is associated with a particular blend. By default, an assay
stream is assigned to the default cutpoint set. A stream may be associated
with a specific secondary cutpoint set by explicitly specifying the name of
that cutpoint set (blend) in association with the stream. If the assay stream is
associated with a blend name not given for any cutpoint set previously de-
fined, a new blend with that name is created using the same cutpoints as the
primary cutpoint set. The user may also specify that a stream use a certain set
of cutpoints but not contribute to the blended properties of the pseudocompo-
nents generated from that set (this might be appropriate if an estimate were
being supplied for a recycle stream, for example). This is done by selecting
the XBLEND option, which excludes the stream in question from the blend-
ing. The default is for the stream to be included in the blending for the pur-
poses of pseudocomponent property generation; this is called the BLEND
option. It is not allowed for the XBLEND option to be used on all streams as-
sociated with a blend, since at least one stream must be blended in to define
the pseudocomponent properties. The blending logic is best illustrated by an
example:
Section 1.1 Component Data
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Suppose that two secondary cutpoint sets A1 and A2 were defined, and that
A1 was designated as the default. This means that three sets actually exist,
since the primary cutpoint set supplied by PRO/II still exists (though it is no
longer the set with which streams will be associated by default). Now, sup-
pose the following streams (where extraneous information like the initial con-
ditions is not shown) are given:
Table 1.1.3-2: Blending Example
Stream Blend Option Blend Name
S1 none given(defaulted toBLEND)
none given(defaulted to A1)
S2 XBLEND none given(defaulted to A1)
S3 XBLEND A1
S4 BLEND A2
S5 BLEND B1
S6 XBLEND B1
S7 BLEND B2
Streams S1 and S2 will use the pseudocomponents defined by secondary cut-
point set A1, since it is the default. S3 will also use A1s pseudocomponents
since it is specified directly. The pseudocomponents in blend A1 will have
properties determined only by the cuts from stream S1, since the XBLEND
option was used for S2 and S3. Stream S4 will use the pseudocomponents de-
fined by cutpoint set A2. Streams S5 and S6 will go into a new blend B1
which will use the cutpoints of the primary cutpoint set. Since XBLEND is
used for stream S6, only stream S5s cuts will be used to determine the prop-
erties of the pseudocomponents in blend B1. Finally, stream S7 will use an-
other new blend, B2, also with the cutpoints from the primary cutpoint set.
Since it is a different blend, however, the pseudocomponents from blend B2
will be completely distinct (even though they will use the same cutpointranges) from those of blend B1.
15 PRO/II Note: For more information on blending options for assay streams, seeSection 15, Petroleum Component Properties, of the PRO/II Keyword Input
Manual.
Component Data Section 1.1
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Application Considerations
The selection of cutpoints is an important consideration in the simulation of
hydrocarbon processing systems. Too few cuts can result in poor repre-
sentation of yields and stream properties when distillation operations are
simulated; moreover, desired separations may not be possible because of
component distributions. On the other hand, the indiscriminate use of cuts
not needed for a simulation serves only to increase the CPU time unnecessar-
ily. It is wise to examine the cut definition for each problem in light of simu-
lation goals and requirements. The default primary cutpoint set in PRO/II
represents, in our experience, a good selection for a wide range of refinery
applications.
In some circumstances, it may be desirable to use more than one cutpoint set
in a given problem. This multiple blends functionality is useful when dif-
ferent portions of a flowsheet are best represented by different TBP cuts; for
example, one part of the process may have streams that are much heavier
than another and for which more cutpoints at higher temperatures would be
desirable. It is also useful when hydrocarbon feeds to a flowsheet differ in
character; for example, different blends might be used to represent an aro-
matic stream (producing pseudocomponents with properties characteristic of
aromatics) and a paraffinic stream feeding into the same flowsheet. The extra
detail and accuracy possible with this feature must be balanced against the in-
crease in CPU time caused by the increased number of pseudocomponents.
Interconversion ofDistillation Curves
Types of Distil lati on Curves
Assays of hydrocarbon streams are represented by distillation curves. A dis-
tillation curve represents the amount of a fluid sample that is vaporized as
the temperature of the sample is raised. The temperature where the first va-
porization takes place is referred to as the initial point (IP), and the tempera-
ture at which the last liquid vaporizes is called the end point (EP). Each data
point represents a cumulative portion (usually represented as volume per-
cent) of the sample vaporized when a certain temperature is reached.
Estimation of thermophysical properties for the pseudocomponents requires
(among other things) a distillation curve that represents the true boiling point
(TBP) of each cut in the distillation. However, rigorous TBP distillations are
difficult and not well standardized so it is common to perform some other
well-defined distillation procedure; standard methods are defined by the
American Society for Testing and Materials (ASTM). The ASTM procedures
most commonly used for hydrocarbons are D86, D1160, and D2887.
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ASTM D86 distillation is typically used for light and medium petroleum
products and is carried out at atmospheric pressure. D1160 distillation is
used for heavier petroleum products and is often carried out under vacuum,
sometimes at absolute pressures as low as 1 mm Hg. The D2887 method uses
gas chromatography to produce a simulated distillation curve; it is applicable
to a wide range of petroleum systems. D2887 results are always reported by
weight percent; other distillations are almost always reported on a volume
percent basis. More details on these distillation procedures may be found intheAPI Technical Data Book; complete specifications are given in volume 5
(Petroleum Products and Lubricants) of theAnnual Book of ASTM Standards.
Conversion of D1160 Curves
PRO/II converts D1160 curves to TBP curves at 760 mm Hg using the three-
step procedure recommended in theAPI Technical Data Book:
Convert to D1160 at 10 mm Hg using API procedure 3A4.1 (which in
turn references procedure 5A1.13). This procedure is expressed as a way
to estimate a vapor pressure at any temperature given the normal boiling
point, but the same equations may be solved to yield a normal boiling
temperature given the boiling temperature at another pressure. The equa-
tions used are as follows:
(1 )
(2 )log
10P=2663.129X5.994296
95.76X0.972546 0.0013X0.0022
(2P760 mmHg)
(3 )
where:
P* = vapor pressure in mm Hg at temperature T (in degrees
Rankine)
The parameterXis defined by:
(4 )
X=
Tb
T0.0002867Tb
748.1 0.2145Tb
where:
Tb= boiling point (in degrees Rankine) at a pressure of 760 mm
Hg
log10P=3000.538X6.76156
43X0.987672 forX>0.0022 (P
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For conversions where neither pressure is 760 mm Hg, the conversion may
be made by applying the above equations twice in succession, using 760 mm
Hg as an intermediate point:
Convert to TBP at 10 mm Hg using API Figure 3A2.1 (which has been
converted to equation form by SimSci).
Convert to TBP at 760 mm Hg using API procedure 3A4.1.
Conversion of D2887 Curves
PRO/II converts D2887 simulated distillation data to TBP curves at 760 mm Hg
using the two-step procedure recommended in theAPI Technical Data Book:
Convert to D86 at 760 mm Hg using API procedure 3A3.1. This procedure
converts D2887 Simulated Distillation (SD) points (in weight percent) to
D86 points (in volume percent) using the following equation:
(5 )D86 =a(SD)bFc
where:
D86 and SD = the ASTM D86 and ASTM D2887 temperatures in de-
grees Rankine at each volume percent (for D86) and thecorresponding weight percent (for SD), and a, b, and c
are constants varying with percent distilled according
to Table 1.1.3-3.
Table 1.1.3-3: Values of Constants a, b, c
PercentDistilled a b c
0 6.0154 0.7445 0.2879
10 4.2262 0.7944 0.2671
30 4.8882 0.7719 0.3450
50 24.1357 0.5425 0.713270 1.0835 0.9867 0.0486
90 1.0956 0.9834 0.0354
100 1.9073 0.9007 0.0625
The parameterFin equation (5) is calculated by the following equation:
(6 )F=0.009524(SD10%)0.05434(SD50%)0.6147
where:
SD10% and SD50% = D2887 temperatures in degrees Rankine at the 10% and
50% points, respectively
Section 1.1 Component Data
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Convert to TBP at 760 mm Hg using API procedure 3A1.1, which is
described in the section Conversion of D86 Curves with New (1987) API
Methodbelow.
Conversion of D86 Curves
PRO/II has three options for the conversion of D86 curves to TBP curves at 760
mm Hg. These are the currently recommended (1987) API method, the older
(1963) API method, and the Edmister-Okamoto correlation. In addition, a correc-
tion for cracking may be applied to D86 data; this correction was recommended
by the API for use with their older conversion procedure, but is not recom-
mended for use with the current (1987) method. The conversion of D86
curves takes place in the following steps:
If a cracking correction is desired, correct the temperatures above 475 F asfollows:
(7 )Tcorr=Tobs+D; log10D= 1.587 +0.00473Tobs
where:
Tcorr, Tobs= the corrected and observed temperatures, respectively,
in degrees Fahrenheit.If necessary, convert the D86 curve at pressure Pto D86 at 760 mm Hg
with the standard ASTM correction factor:
(8 )T760=TP+0.00012(760 P)(460 +TP)
where:
TP= D86 temperature in Fahrenheit at pressure P
T760= D86 temperature in Fahrenheit at 760 mm Hg
Convert from D86 at 760 mm Hg to TBP at 760 mm Hg using one of the
three procedures below.
a) Conversion of D86 Curves with New (1987) API MethodBy default, PRO/II converts ASTM D86 distillation curves to TBP curves
at 760 mm Hg using procedure 3A1.1 (developed by Riazi and Daubert in
1986) recommended in the 5th edition of theAPI Technical Data Book.
The equation for this procedure is as follows:
(9 )TBP=a(D86)b
where aand bare constants varying with percent of liquid sample distilled
as given in Table 1.1.3-4:
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Table 1.1.3-4: Values of Constants a, b
Percent Distilled a b
0 0.9167 1.0019
10 0.5277 1.0900
30 0.7429 1.0425
50 0.8920 1.0176
70 0.8705 1.0226
90 0.9490 1.0110
100 0.8008 1.0355
b) Conversion of D86 Curves with Old (1963) API Method
This method, while no longer the default, is still available for users whose
flowsheets may be tuned to the results using the old method. This method
was recommended (and shown in graphical form) in older editions of the
API Technical Data Book. The graphical correlation has been converted to
equation form by SimSci.
c) Conversion of D86 Curves with Edmister-Okamoto Method
Edmister and Okamoto (1959) developed a method which is still widelyused for converting ASTM D86 curves to TBP curves. If the Edmister-
Okamoto method is specified as the conversion method, their procedure
(converted from the original graphical form to equations by SimSci) is
used for conversion of D86 to TBP curves.
Cutting TBP Curves Fitting of Distill ation Curves
Before a curve is cut into pseudocomponents, the distillation data must be fit-
ted to a continuous curve. This is necessary because the supplied data points
will not in general correspond to the desired cutpoints. PRO/II offers three
methods for fitting distillation curves.
The default is the cubic spline method (known as the SPLINE option). A cu-
bic spline function is used to fit all given volume percents between the first
and last points. Beyond those bounds, points 1 and 2 and points N and N-1
are used to define a normal distribution function to extrapolate to the 0.01%
and 99.99% points, respectively. If only two points are supplied, the entire
curve is defined by the distribution function fit. This extrapolation feature is
particularly valuable when extrapolating heavy ends distillations which often
terminate well below 50 volume percent. This method in general results in an
excellent curve fit. The only exception is when the distillation data contain a
significant step function (such a step is often the unphysical result of an error
in obtaining or reporting the data); in that case, the step creates an instability
that tends to propagate throughout the entire length of the curve. Should this
happen, the input data should be checked for validity.
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The quadratic fit method (known as the QUADRATIC option) provides a suc-
cessive quadratic approximation to the shape of the input assay curve. This
method is recommended in the rare case (see above) where a cubic spline fit
is unstable.
The Probability Density Function (PDF) method (known as the PDF option)
is different in that it does not necessarily pass through all the points input by
the user. Instead, it fits a probability density function to all points supplied.
The resulting curve will maintain the probability-curve shape characteristic
of petroleum distillations, while minimizing the sum of the squares of the dif-
ferences between the curve and the input data. If desired, the curve may be
constrained to pass through either or both of the initial point and end point.
The PDF method is recommended whenever it is suspected that the distilla-
tion data are noisy, containing significant random errors.
It is worth noting that the choice of curve-fitting procedure will also have a
slight impact on the distillation interconversions described in the previous sec-
tion. That is because most of the conversion procedures work by doing the
conversion at a fixed set of volume percents, which must be obtained by interpo-
lation and sometimes extrapolation, using some curve-fitting procedure.
Division into Pseudocomponents
Once a smooth distillation curve is obtained, the volume percent distilled at each
cutpoint is determined. The differences between values at adjacent cutpoints de-
fine the percent of the streams volume that is assigned to the pseudocomponent
defined by the interval between two adjacent cutpoints. For example, using the
default set of cutpoints shown in Table 1.1.3-1, the first pseudocomponent would
contain all material boiling between 100 F and 125 F, the second would con-tain the material boiling between 125 F and 150 F, and so forth. Material boil-ing above the last cutpoint (1600 F) would be combined with the last(1500-1600) cut, while (with the exception of lightends as discussed below)
material boiling below 100 F would be combined with the first cut. If the distil-lation data do not extend into all of the cut ranges (in this example, if the initial
point were higher than 125 F or if the end point were lower than 1500 F), theunused cuts are omitted from the simulation.
The normal boiling point (NBP) of each cut is determined as a volume-frac-
tion average (or, in rare cases where TBP, D86, or D1160 distillations are
entered on a weight basis, as a weight-fraction average) by integrating across
the cut range. For small cut ranges, this will closely approach other types of
average boiling points. These average boiling points are used (possibly after
blending with cuts from other assay streams in the flowsheet) as correlating
parameters when calculating other thermophysical properties for each
pseudocomponent.
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These procedures are demonstrated in Figure 1.1.3-1 for a fictitious assay
with an IP of 90 F being cut according to the default cutpoint set (Table1.1.3-1); for simplicity only the first ten percent of the curve is shown. In ad-
dition to its range, the first cut picks up the portion boiling below 100 F, andits average boiling point (about 110 F in this case) is determined by integrat-ing the curve from the IP to the 125 F point. The second cut is assigned thematerial boiling from 125 F to 150 F, which is integrated to get a NBP ofapproximately 138 F. The third and subsequent cuts are generated in a simi-lar manner.
Figure 1.1.3-1 :Cutting TBP Curves
Gravity Data
PRO/II requires the user to enter an average gravity (either as a Specific
Gravity, API Gravity, or Watson K-factor) for each assay. If a Watson K isgiven, it is converted to a gravity using the TBP data for the curve. Entry of a
gravity curve is recommended but not required.
If a user-supplied gravity curve does not extend to the 95% point, quadratic
extrapolation is used to generate an estimate for the gravity at the 100%
point. A gravity for each cut is determined at its mid-point, and an average
gravity for the stream is computed. If this average does not agree with the
specified average, the program will either normalize the gravity curve (if
data are given up to 95%) or adjust the estimated 100% point gravity value to
force agreement. Since the latter could in some cases result in unreasonable
gravity values for the last few cuts, the user should consider providing an es-
timate of the 100% point gravity value and letting the program normalize the
curve, particularly when gravity data are available to 80% or beyond.
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If no gravity curve is given, the program will generate one from the specified
average gravity. The default method for doing this is referred to as the WAT-
SONK method. For a pure component, the Watson K-factor is defined by the
following equation:
(10)K=
NBP13
SG
where:
NBP = normal boiling point in degrees Rankine
SG = specific gravity at 60 F relative to H2O at 60 F
For a mixture (such as a petroleum cut), the NBP is traditionally replaced by a
more complicated quantity called the mean average boiling point (MeABP). For
this purpose, however, it is sufficient to simply use the volume-averaged boil-
ing point computed from the distillation curve. The gravity curve is gener-
ated by assuming a constant value of the Watson K, applying equation (10)
to each cut to get a gravity, averaging these values, and then adjusting the as-
sumed value of the Watson K until the resulting average gravity agrees with
the average gravity input by the user.
Another method (known as the PRE301 option) is available primarily for com-patibility with older versions. It is similar to the preferred method described
above, except that the average Watson K is estimated from the 10, 30, 50, 70,
and 90 percent points on a D86 curve (which can be obtained from the TBP
curve by reversing one of the procedures in the previous section) and then
applied to the NBP of each TBP cut to generate a gravity curve. This curve is
then normalized to produce the specified average gravity.
The preferred method (constant Watson K applied to TBP curve) is justified
by the observation that, for many petroleum crude streams, the Watson K of
various petroleum cuts above light naphtha tends to remain fairly constant.
For other types of petroleum streams, however, this assumption is often incor-
rect. Hence, for truly accurate simulation work, the user is advised to supply
gravity curves whenever possible.
Molecular Weight Data
In addition to the NBP and specific gravity, simulation with assays requires
the molecular weight of each cut. These may be omitted completely by the
user, in which case they are estimated by the program.
The user may supply a molecular weight curve, which is quadratically inter-
polated and extrapolated to cover the entire range of pseudocomponents. Op-
tionally, the user may also supply an average molecular weight. In that case,
the molecular weight value for the last cut is adjusted so that the curve
matches the given average, or if the 100% value is provided, the entire mo-
lecular weight curve is normalized to match the given average.
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If no molecular-weight data are supplied, the molecular weights are esti-
mated; the default method is a proprietary modification (known as the SIM-
SCI method) of the method developed by Twu (1984). This method is a
perturbation expansion with the normal alkanes as a reference fluid. Twus
method was originally developed to be an improvement over Figure 2B2.1 in
older editions of theAPI Technical Data Book. That figure relates molecular
weight to NBP and API gravity for NBPs greater than 300 F. The SIMSCI
method matches that data between normal boiling points of 300 F and 800F, and better extrapolates outside that temperature range.
The unaltered old API method is (API63) is also available.
A newer API method, called the extended API method (known as the EXTAPI
option), is also available. This is API procedure 2B2.1, and it is an extension of
the earlier API method which better matches known pure-component data below
300 F. The equation is as follows:
(11)
MW=20.486 exp(1.16510
4Tb7.78712 SG+1.158210
3TbSG)
Tb
1.26007SG
4.98308
where:
SG = specific gravity of the pseudocomponent
Tb= normal boiling point in degrees Rankine
Lightends Data
Hydrocarbon streams often contain significant amounts of light hydrocarbons
(while there is no universal definition of light, C6 is a common upper limit).
Simulation of such systems is more accurate if these components are considered
explicitly rather than being lumped into pseudocomponents. If the distillation
curve is reported on a lightends-free basis, the light components can be fed to
the flowsheet in a separate stream and handled in a straightforward manner. Typi-
cally, however, the lightends make up the initial part of the reported distillation
curve, and adjustment of the cut-up curves is required to avoid double-counting
the lightends components.
By default, the program matches user-supplied lightends data to the TBP curve.
The user-specified rates for all lightends components are adjusted up or down, all
in the same proportion, until the NBP of the highest-boiling lightends component
exactly intersects the TBP curve. All of the cuts from the TBP curve falling into the
region covered by the lightends are then discarded and the lightends components
are used in subsequent calculations. This procedure is illustrated in Figure 1.1.3-2,
where lightend component flows are adjusted until the highest-boiling lightend
(nC5 in this example) has a mid-volume percent (point a) that exactly coincides
with the point on the TBP curve where the temperature is equal to the NBP of nC5.
The cumulative volume percent of lightends is represented by point b, and the
cuts below point b (and the low-boiling portion of the cut encompassing that point)
are discarded.
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Figure 1.1.3-2 :Matching Lightends
to TBP Curve
Alternatively, the lightends may be specified as a fraction or percent (on a
weight or liquid-volume basis) of the total assay or as a fixed lightends flowrate.In these cases, the input numbers for the lightends components can be normal-
ized to determine the individual component flowrates. A final alternative is to
specify the flowrate of each lightends component individually.
GeneratingPseudocomponent
Properties
Once each curve is cut, the program processes each blend to produce average
properties for the pseudocomponents from each cutpoint interval in that
blend. All the streams in a given blend (except for those for which the
XBLEND option was used) are totaled to get the weights, volumes, and
moles for each cutpoint interval. Using the above totals, the average molecu-
lar weight and gravity are calculated for each cut range. Finally, the normal
boiling point for each pseudocomponent is calculated by weight averaging
the individual values from the contributing streams.
Once the normal boiling point, gravity, and molecular weight are known for
each pseudocomponent, all other properties (critical properties, enthalpies,
etc.) are determined according to the characterization method selected by the
user (or defaulted by the program). These methods are described in Section
1.1.2,Petroleum Components.
Vapor PressureCalculations
While not a part of the programs actual processing of assay streams, many
problems involving hydrocarbon systems will involve a specification on
some vapor pressure measurement. The two most common of these are the
True Vapor Pressure (TVP) and the Reid Vapor Pressure (RVP). PRO/II al-
lows specification of these quantities from several unit operations, and they
may be reported in output in the Heating/Cooling Curve (HCURVE) utilityor as part of a user-defined stream report.
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True Vapor Pressure (TVP) Calculati ons
The TVP of a stream is defined as the bubble-point pressure at a given refer-
ence temperature. By default, that reference temperature is 100 F, but thismay be overridden by the user. The user may specify a specific thermody-
namic system to be used in performing all TVP calculations in the flowsheet;
by default, the calculation for a stream is performed using the thermody-
namic system used to generate that stream.
Reid Vapor Pressure (RVP) Calculations
The RVP laboratory procedure provides an inexpensive and reproducible meas-
urement correlating to the vapor pressure of a fluid. The measured RVP is usu-
ally within 1 psi of the TVP of a stream. It is always reported as psi, although
the ASTM test procedures (except for D5191 which, as mentioned below, uses
an evacuated sample bomb) actually read gauge pressure. Since the air in the
bomb accounts for approximately 1 atm, the measured gauge pressure is a rough
measure of the true vapor pressure. Six different calculation methods are avail-
able. Within each calculation method, the answer will depend somewhat on the
thermodynamic system used. As with the TVP, the thermodynamic system for
RVP calculations may be specified explicitly or, by default, the thermodynamic
system used to generate the stream will be used.
The APINAPHTHA method calculates the RVP from Figure 5B1.1 in theAPI
Technical Data Book, which represents the RVP as a function of the TVP and
the slope of the D86 curve at the 10% point. The graphical data have been con-
verted to equation form by Simsci. This method is the default for PRO/IIs RVP
calculations. It is useful for many gasolines and other finished petroleum prod-
ucts, but it should not be used for oxygenated gasoline blends.
The APICRUDE method calculates the RVP from Figure 5B1.2 in theAPI
Technical Data Book, which represents the RVP as a function of the TVP and
the slope of the D86 curve at the 10% point. The graphical data have been
converted to equation form by SimSci. It is primarily intended for crude oils.
The ASTM D323-82 method (known as the D323 method) simulates a stand-ard ASTM procedure for RVP measurement. The liquid hydrocarbon portion
of the sample is saturated with air at 33 F and 1 atm pressure. This liquid isthen mixed at 100 F with air in a 4:1 volume ratio. Since the test chamber isnot dried in this procedure, a small amount of water is also added to simulate
this mixture. The mixture is flashed at 100 F at a constant volume (corre-sponding to the experiment in a sealed bomb), and the gauge pressure of the
resulting vapor-liquid mixture is reported as the RVP. Both air and water
should be in the component list for proper use of this method.
The obsolete ASTM D323-73 method (known as the P323 method) is avail-
able for compatibility with earlier versions of the program.
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The ASTM D4953-91 method (known as the D4953 method) was developed
by the ASTM primarily for oxygenated gasolines. The experimental method
is identical to the D323 method, except that the system is kept completely
free of water. The algorithm for simulating this method is identical to that for
D323, except that no water is added to the mixture. Air should be in the com-
ponent list for proper use of this method.
The ASTM D5191-91 method (known as the D5191 method) was developed as an
alternative to the D4953 method for gasolines and gasoline-oxygenate blends. In
this method, the air-saturated sample is placed in an evacuated bomb with five
times the volume of the sample, and then the total pressure of the sample is meas-
ured. In the simulator, this is accomplished by flashing, at constant volume, a mix-
ture of 1 part sample (at 33 F and 1 atm) and 4 parts air (at the near-vacuumconditions of 0.01 psia and 100 F). The resulting total pressure is then con-verted to a dry vapor pressure equivalent (DVPE) using the following equation:
(12)DVPE=0.965XA
where:
X = the measured total pressure
A = 0.548 psi (3.78 kPa)This number is then reported as the RVP. Air should be in the component list
for proper use of this method.
Comments on RVP and TVP Methods
Because of the sensitivity of the RVP (and the TVP) to the light components
of the mixture, these components should be modeled as exactly as possible if
precise values of RVP or TVP are important. This might mean treating more
light hydrocarbons as defined components rather than as pseudocomponents;
oxygenated compounds blended into gasolines should also be represented as
defined components rather than as part of an assay. It is also important to ap-
ply a thermodynamic method that is appropriate for the stream in question
(see Section 1.2.2,Application Guidelines). The thermodynamics becomesparticularly important for oxygenated systems, which are not well-modeled
by traditional hydrocarbon methods such as Grayson-Streed. These systems
are probably best modeled by an equation of state such as SRK with the Sim-
Sci alpha formulation and one of the advanced mixing rules (see Section
1.2.4,Equations of State). It is important to have binary interaction parame-
ters between the oxygenates and the hydrocarbon components of the system.
PRO/IIs databanks contain many such parameters, but others may have to be
regressed to experimental data or estimated.
One should not be too surprised if calculated values for RVP differ from an
experimental measurement by as much as one psi. Part of this is due to the
uncertainty in the experimental procedure, and part is due to the fact that the
lightends composition inside the simulation may not be identical to that ofthe experimental sample.
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One of the less appreciated effects in experimental measurements is the pres-
ence of water, not only in the sample vessel, but also in the air in the form of
humidity. The difference between the D323 (a wet method) RVP and the
D4953 (a dry method) RVP will be approximately the vapor pressure of
water at 100 F (about 0.9 psi), with the D323 RVP being higher. Both ofthese calculations assume that dry air is used in the procedure. The presence
of humidity in the air mixed with the sample can alter the D323 results, low-
ering the measured RVP because of the decreased driving force for vaporiza-tion of the liquid water. In the extreme case of 100% humidity, the D323
results will be nearly identical with the D4953 results. Therefore, a wet
test performed with air that was not dry would be expected to give results in-
termediate between PRO/IIs D323 and D4953 calculations. The results from
the D5191 method (both in terms of the experimental and calculated num-
bers) should in general be very close to D4953 results.
The primary application guideline for which RVP calculational model to use
is, of course, to choose the one that corresponds to the experimental proce-
dure applied to that stream. Secondary considerations include limitations of
the individual methods. The APINAPHTHA and APICRUDE methods are
good only for hydrocarbon naphtha and crude streams, respectively. The
D323 method (and its obsolete predecessor, P323) is intended for hydrocar-bon streams; the presence of water makes it less well-suited for use with
streams containing oxygenated compounds. The D4953 and D5191 methods
are both better suited for oxygenated systems, and calculations with these
methods should give similar results.
References
1. American Petroleum Institute, 1988, Technical Data Book - Petroleum
Refining, 5th edition (also previous editions), American Petroleum
Institute, Washington, DC.
2. American Society for Testing of Materials,Annual Book of ASTM
Standards, section 5 (Petroleum Products, Lubricants, and Fossil Fuels),ASTM, Philadelphia, PA (issued annually).
3. Edmister, W.C., and Okamoto, K.K., 1959, Applied Hydrocarbon
Thermodynamics, Part 12: Equilibrium Flash Vaporization Calculations
for Petroleum Fractions, Petroleum Refiner, 38(8), 117.
4. Twu, C.H., 1984, An Internally Consistent Correlation for Predicting the
Critical Properties and Molecular Weights of Petroleum and Coal-tar
Liquids, Fluid Phase Equil., 16, 137-150.
Section 1.1 Component Data
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Thermodynamic Methods
PRO/II offers numerous methods for calculating thermodynamic properties such
as K-values, enthalpies, entropies, densities, gas and solid solubilities in liquids,
and vapor fugacities. These methods include:
Generalized correlations, such as the Chao-Seader K-value method and the API
liquid density method.
Equations of state, such as the Soave-Redlich-Kwong method for calculating
K-values, enthalpies, entropies, and densities.
Liquid activity coefficient methods, such as the Non-Random Two-Liquid
(NRTL) method for calculating K-values.
Vapor fugacity methods, such as the Hayden-OConnell method for dimerizing
species.Special methods for calculating the properties of specific systems of compo-
nents such as alcohols, glycols, and sour water systems.
Solid-liquid equilibria methods such as the vant Hoff method for calculating
the solubility of a solid in a liquid.
In addition, the electrolyte version of PRO/II contains a number of thermody-
namic methods to handle systems containing aqueous ionic species.
1. 2
Section 1.2 Thermodynamic Methods
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Basic Principl es
GeneralInformation
When modeling a single chemical process or an entire chemical plant, the use of
appropriate thermodynamic methods and precise data is essential in obtaining a
good design. PRO/II contains numerous proven thermodynamic methods for the
calculation of the following thermophysical properties:
Distribution of components between phases in equilibrium (K-values).
Liquid-phase and vapor-phase enthalpies.
Liquid-phase and vapor-phase entropies.
Liquid-phase and vapor-phase densities.
PhaseEquilibria When two or more phases are brought into contact, material is transferredfrom one to another until the phases reach equilibrium, and the compositionsin each phase become constant. At equilibrium for a multicomponent system,
the temperature, pressure, and chemical potential of component iis the same
in every phase, i.e.:
(1 )T=T==T
(2 )P
=P==P
(3 )i
=i
==i
where:
T = system temperature
P = system pressure
= the chemical potential
,, ..., represent the phasesThe fugacity of a substance is then defined as:
(4 )ii
0=RTln
f
i/fi
0
where:
fi= fugacity of component i
fi0= standard-state fugacity of component iat T, P
i0= standard-state chemical potential of component iat T,P
1.2.1
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It follows from (3) and (4) that the fugacities in each phase must also be equal:
(5 )fi
=fi
==f
i
, i=1,2, n
The fugacity of a substance can be visualized as a corrected partial pres-
sure such that the fugacity of a component in an ideal-gas mixture is equal
to the component partial pressure.
For vapor-liquid equilibrium calculations, the ratio of the mole fraction of a com-
ponent in the vapor phase to that in the liquid phase is defined as the K-value:
(6 )Kiyi/xi
where:
Ki= K-value, or equilibrium ratio
yi= mole fraction in the vapor phase
xi= mole fraction in the liquid phase
For liquid-liquid equilibria, a corresponding equilibrium ratio or distribution
coefficient is defined:
(7 )KDi
xi
I/xi
II
where:
KDi= liquid-liquid distribution coefficient
I,IIrepresent the two liquid phases
The vapor-phase fugacity coefficient of a component, iV, is defined as the
ratio of its fugacity to its partial pressure, i.e.:
(8 )iVfi
V/yiP
where:
iV= vapor-phase fugacity coefficient of component i
If a liquid activity coefficient method is used in the liquid phase calculation,
then the activity coefficient of the liquid phase can be related to the liquid
fugacity by the following relationship:
(9 )fiL
=iL
xifiOL
where:
i
L= liquid-phase activity coefficient
fi0L
= standard-state fugacity of pure liquidi
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With this definition of liquid fugacity, iL1 asxi1. The standard-statefugacity is as follows:
(10)f
i
0L=P
i
sat
i
satexp
Pi
sat
P
vi
L/RTdP
where:
Pisat= saturated vapor pressure of component iat T
R = gas constant
viL
= liquid molar volume of component iat Tand P
isat= fugacity coefficient of pure componentiat Tand Pi
sat
Equation (10) provides two correction factors for the pure liquid fugacity. The
fugacity coefficient, isat, corrects for deviations of the saturated vapor fromideal-gas behavior. The exponential correction factor, known as the Poynting cor-
rection factor, corrects for the effect of pressure on the liquid fugacity. The
Poynting correction factor is usually negligible for low and moderate pressures.
Combining equations (6), (8), and (9) yields:
(11)Ki=
i
Lf
i
OL/Pi
V
Combining equations (7) and (9) yields:
(12)KDi
=i
LII/i
LI
If an equation of state is applied to both vapor and liquid phases, the vapor-
liquid K-values can be written as:
(13)Ki=iL
/iV
The liquid-liquid equilibria can be written as:
(14)K
Di=
i
LII
iL
I
Equations (11), (12), (13), and (14) are used to calculate the distribution of
components between phases.
For vapor-liquid equilibria, equation-of-state methods may be used to calculate
the fugacity coefficients for both liquid and vapor phases using equation (13).
One important limitation of equation-of-state methods is that they have to be ap-
plicable over a wide range of densities, from near-zero density for gases to high
liquid densities, using constants obtained from pure-component data. Equations
of state are not very accurate for nonideal systems unless combined with compo-nent mixing rules and alpha formulations (see Section 1.2.4,Equations of State)
appropriate for those components.
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Equation (11) may be solved by using equation-of-state methods to calculate va-
por fugacities combined with liquid activity methods to compute liquid activity
coefficients (see Section 1.2.6,Liquid Activity Methods). Liquid activity met