DESCRIPTION OF THE COMPUTER PROGRAM
Appendix F

of

Development of a Simulation Model
for Estimating Ground Level Concentrations
of Photochemical Pollutants
Prepared by

Systems Applications, Inc.
Beverly Hills, California  90212
for the

Air Pollution Control Office
of the Environmental Protection Agency
Durham, North Carolina  27701

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~ESCRIPTION OF THE COMPU'l'ER PROGRAM
Appendix F
of.
Development of a Simulation Model
for Estimating Ground Level Concentrations
of Photochemical Pollutants
Steven D. Reynolds
Report 71S2\I26
August 1971
Prepared by
Systems Applications, Inc.
Beverly Hills, California 90212
for the
Air Pollution Control Office
of the Environmental.protection Agency
Durham, North Carolina 27701
under Contract CPA 70-148

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ACKNOWLEDGlotENTS
.,
. We wish to acknowledge the contributions of Mr. Clarence L.
Nelson and Mr. Philip J. W. Roberts in the preparation of the
Aircraft Emissions Program and the subroutines UPWIND and PLUME
of: the Atmospheric Pollution Simulation Program respectively.

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CON'i'ENTS
'-'
INTRODU-::'l'IOH .
. . . . .
. . . . . . .
. . .
r.
THE ATMOSPHERIC POLLUTION SIMULATION P~OGf~
A".
~ne Structure of ths ~tmosphe~i~
Pollution Simulation Frog'ram ~ . . .
13.
Progrfu~ Operation.
. .
. . .
II.
THE A:.;(CHAFr E:l!SSIONS PROGRAM
. . . .
. . .
REFERENCES
. . . . .
. .
. . .
. .
. . .
p.age
. .
. F- 1
. F- 2
. . F- 3
. . . . .
F- 8
. . .
F-l8
. F-22

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INTRODUCTION
The purpose of this Appendix is to describe in. a general way
the various facets of the computer program that comprise the urban
airshed model. The development of this program is an involved
undertaking, as a wide variety of calculations are required both
in the numerical solution of the governing equations and in the
handling and manipulation of source .and meteorological data. .
Emphasis was placed on the preparation of an efficient program and
on insuring the applicability of the program in any urban airshed.
Computational efficiency is vital in hro respects. First, it
is important to minimize the number of calculations that must be carried'
out in any large-scale computing effort, particularly when these calcula-
tions are a part of iterative loops or are of a repetitive nature.
Second, the numerical solution of three dimensional, coupled, time
dependent partial differential equations is, apart from data input,
handling, and processing considerations, a very time consuming calcula-
tion, and efficiency is paramount. With regard to the general applica-
bility of the program, an airshed is essentially defined by its terrain,
meteorological, and source inputs. Since these parameters are all
treated as input data to the program, no difficulty should be encounter-
ed in applying the program in a variety of urban airsheds.
At this time, the most cumbersome aspect of program usage is the
large effort required in the preparation of the meteorological input
data (see Appendix C). Inccrporation of an interpolation scheme into
the program which automatically constructs wind and inversion maps from
the raw monitoring station data would alleviate this difficulty. Such
an addition to the existing program is required prior to the validation
of the model for a large number of different meteorological coni'.itions.
It is also worthwhile to remind the reader that, in general, a sizable
effort is needed for the preparation of the source emissions inventory
for any large urban area. Ho~.,ever" it should be noted that, while the spatial
and temporal distributions of pollutant emissions are generally the same
from day to day (with the exception of the weekend), the meteoro-
logy is likely to undergo daily variations. Thus, the emissions inven-
tory must be undertaken only once. If the model is to be used in
testing control strategies, it will become necessary to alter the source
input data. Such alterations should present few difficulties, however,
from the standpoint of program operation.
Two programs are currently being used in the Los Angeles Basin
simulation effort. The main program, the Atmospheric Pollution Simula-
tion Program, calculates pollutant concentrations as 'a function of space
and time using source and meteorological inputs. We discuss both the
structural and ele operational aspects of thi~ program in Section I of
this Appendix. Aircraft emissions are treated as input to this program
via magnetic tape. The computer program which generates this tape, The
Aircraft Emissions Program, is discussed in Section II.

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1:.
THE ATMOSPHERIC POLLUTION SIl.fiJLATION PROGRAM
The Atmospheric Pollution Simulation Program accepts source and
meteorological data as inputs to produce pollutant concentration/
time histories at discrete points distributed throughout the airshed.
The code consists of a MAIN program and several subroutines which
perform specialized tasks. In its present configuration, the program
utilizes two magnetic tape units and temporary disc storage. Current-
ly, the program size is approximately 350K bytes.
Inputs to the program are contained on cards and two magnetic
tap~s. The following information is supplied via punched cards:
.
the horizontal extent and topography of the airshed .
the time span over which the simulation is to take place
the spatial and temporal grid' ~ize "
the time interval for concentration'printout
the chemical species to be sinrolated
the maximum number of iterations allowed in Step I
. of the numerical solution of the governing equations
,freeway and non-frce""ay vehicle mileage distributions
fixed source emissions
the chemical reaction rate constants
the initial concentration distribution
.
.
.
.
.
.
.
Tbe two magnetic tapes mentioned above contain meteorological and
aircraft emissions data respectively. The meteorological data consists
of wind speed and direction, mixing depth, and temperature for each
colUmn of grid points. Each set of data is applicable for a certain
time interval (say, between 0630 and 0730 PST), and this time interval
is recorded on the tape immediately preceding each set of data. Before
~ simulation begins, the program reads the tape until it locates a set
of data applicable at the starting time of the simulation. Similarly,
the aircraft emissions tape contains sets of data preceded by a time
interval. This tape is also automatically positioned before the simu- .
tat ion begins. The aircraft emissions tape ,is generated by the Aircraft
Emissions Program, discussed in Section II, and consists of pollutant
emissions rates (ppm/minute) into each cell of the airshed.
The primary output of the program is a printout of the hourly-
~veraged ground-level concentration distribution for each chemical species
simulated. These concentration maps, in stan~ardized output format, ~an be
easily, compared with observed pollutant levels. It should be noted, how-
ever, that the number of concentration values that are computed is gen-
erally quite large. Thus, we do not attempt to display the entire con-
centration field at any time. It is felt that generally the ground-level
concentrations will be of most interest since measurements of pollutant
levels 'aloft are scarce. With this in mind, we have included an output
option which allows the user to monitor the ~rogress of the simul~tion
with an appropriate level of detail. The program prints the instantaneous
F-2

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"---
g~ound~level concentrations and user-selected vertical concentration
profiles at regular time intervals. The user chooses ground-level
coordinates of points of interest, and the program prints all concen-
trations between the ground and inversion base at those points. In
simulations performed thus far, we have sampled the instantaneous
concentrations every twenty minutes and have chosen to exanline the
vertical concentration profiles only above monitoring stations. We
have found this display of output to be quite satisfactory for this
phase of model development.
In future phases of progr~m development, we plan to investigate
alternative means of presenting the results of a simulation. Sucha
p~esentation will prob~ly include the use of graphical techniques to
disp~ay ground-level concentration conto~ maps and vertical concen-
tration profiles. Moreover, the present b;eatment of data input to
the program is by no means final, and, in fact, only represents a con-
venient means for satisfying current needs. When the model is com-
p~eted, treatment of input will be re-evaluated. At that time we will
be. able to make recommendations as to how the ,input should be handled.
A foreseeable change in the input structure will occur, for example,
if'we develop an 'interpolation scheme to construct the wind field
directly from the monitoring station dat~.
The remainder of this discussion will be segmented into two parts.
In Section A we describe the overall structure of the program and dis-
cuss the role played by each subroutine subprogram. Section B is
devoted to a genc~alized, step-by-step description of how the program
op~rates during a typical simulation run.
A'.
The Structure of the Atrnospheric Pollution Simulation Program
In this section we describe the various subprograms
the main program, giving details of how they operate and
appropriate portions of the main text and appendices for
cussions of the underlying concepts involved. In Figure
cate schematically the overall structure of the program,
Y-l:we list each subprogram and summarize its function.
that comprise
referring to
detailed dis-
F-l we indi-
and in Table
MAIN
MAIN is responsible for two aspects of a simulation:
(1)
(2)
the control of model initialization
the n~merical integration of the governing
air shed equations
Model initialization consists of defining the physical characteristics
of theairshed (horizontal ~xtent and topography), reading source
emissions data, positioning data tapes, est~lishing the grid on which
Figure F-l and Table F-l follo~'
. F-3

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"IJ
I
~
SOURCE
I
,
GJ
FI~URE F-l.
STRD~URE 9F THE ATMPSPHERIC P9LWTIPN snruLATION PROGRAM
BCCONC
AVCOOC
(
)
START
GJ
j
i
V
ICCONC
1 . 1
\ GUCOF (METEOR \
/ . - -r-1
SIMDIG
PLUME

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TABLE F-l.
ROUTINE
MAIN
AVCONC
BCCONC
DIFCOF
ICCONC
METEOR
PLUME
PRINTl
SIMDIG
SOURCE
UPWIND
SUMMARY OF SUBPROGRAMS AND THEIR FUNCTION
FUNCTION
initialization of the model and the numerical
solution of the governing airshed equations
calculates and prints hourly-averaged ground
level pollutant concentration maps
supplies boundary concentrations at points of
horizontal inflow into the model
calculates the turbulent eddy diffusivity at
each point in a given column of grid points
sets up the initial concentration distribution
reads lower wind field and inversion base
elevatioIE and alters the vertical concentration
distribution due to temporal changes in the
inversion base elevations
calculates the spatial distribution of power
plant et:\issions
prints instantaneous ground-level pollutant
concentration maps as well as user-selected
vertical concentration profiles
solves system of linear equations ~mose
coefficient matrix is tridiagonal
calculates automotive and fixed source pollutant
emissions (exc~pt power plants)
calculates the upper wind field
F-5

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. the nUInerical integration is to take place, and entering the initial
concentration distribution. However, not all of these functions take
place in MAIN. The sequencing involved in model initialization is
described in more detail in section B. When model initialization is
complete, the nUInerical integration procedure may be initiated.
Before an integration time step can be taken, source and meteoro-
logical variables. must be updated. Subroutines SOURCE, METEOR, 'and
PLUME are called to supply vehicular and fixed source emissions,
meteorological data, and power plant emissions respectively. Also,
aircraft emissions are obtained from the temporary disc area, and
subroutineDIFCOF is called to supply values of the eddy diffusivity.
The numerical integration now proceeds with the sequential solution of
Steps I, II, and III as described in Appendix.D. ..
,
When the simulation is complete, the program punches the final
concentration distribution onto cards. ,This enables the user to re-
start the integration at a later date. In early stages of model valida-
tion, we have found it convenient to divide a 12-hoursimulation into
three four-hour model runs, t~ereby allo~ring us to monitor the progress of
the simulation. If, after a four-hour segment, the predicted concen-
trations are found to be acceptable, we merely use the punched concen-
trations as initial conditions to continue the simulation further in time.
AVCONC
Subroutine AVCONC is called from MAIN after every integration time
step and is responsible for the calculation and printout of hourly- .
averaged ground level concentration maps. Each time AVCONC is entered,
an array is incremented by the current values of the ground level con-
centrations. After one hour, this array is divided by the n~ber of
time steps taken over that hour so as to produce an array of hourly-
averaged pollutant levels. By manually superposing the actual monitor-
ing station observations on these maps, one can easily evaluate the
model's performance.
BCCONC
Subroutine BCCONC .supplies pollutant levels at points on the air shed
boundary where horizontal inflow takes place. Generally, the actual con-
centrations are not known, and hence. the values used are merely educated
guesses. If levels were kno~m, then they could be input on cards or tape.
~n current simulation efforts involving CO, we have employed boundary con-
centrations of 3 ppm at all points of horizontal inflow.
DIFCOF
In Step I of the numerical integration and during the cubic spline
interpolation procedure, it is necessary to have values of the turbulent
eddy diffusivity. Subroutine DIFCOF supplies values of the diffusivity
F-6

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for.a vertical column of grid points. The coordinates of the column
are transferred to DIFCOF, and diffusivities are calculated from
knowledge of the meteorological conditions in the column (see Appendix
C for a discussion of the algorithm employed).
ICCONC
The initial concentration distribution is established through sub-
routine ICCONC. This subroutine assumes two forms, depending on the
mode of initial concentration input. In the first mode, the initial
ground-level concentrations are read from cards which were prepared
from ground-level concentration maps that are based on actual observed
pollutant levels. The values in the ground cells are extended verti-
cally to the inversion to complete the definition of the initial con-
centration field. The second mode of input a~ises when a simulation
begins at a point in time at which a previous simulation terminated.
As was mentioned in the discussion of the MAIN program, at the end of
a simulation the entire concentration field is punched onto cards. Thus
the second mode simply consists of a READ statement to read the punched
cards.
14ETEOR
The processing of the meteorological data is the domain of subroutine
METEOR. During model initialization, METEOR is called by ~~IN, and the
meteorological input tape is read until data applicable at the start of
the simulation are encountered. As the simulation progresses, the meteor~
ological variables are updated as necessary by reading the tape. See
Appendix C for a further discussion of the meteorological data. When
inversion elevations change, it beco~es necessary to transfer the concen-
tration field from the old grid to the new grid. A cubic spline proce-
dure is employed which requires values of the diffusivity as supplied by
DIFCOF. A system of linear equations must be solved, and subroutine
SIMDIG performs this task. Finally, subroutines UPWIND and PLUME are
called to supply the upper wind field and the spatial distribution of
power plant emissions, respectively.
PLUME
Subroutine PLUHE computes the spatial and temporal distribution of
p~1er plant emissions. Since the spatial distribution varies with
changes in meteorological variables (every hour in this case), it. was
convenient to call this subroutine from METEOR. A detailed discussion
of the method used to distribute the power plant emissions may be found.
in Section III of Appendix A.
PRINTl
The results of the numerical integration are printed in subroutine
PRINTI. User-selected vertical concentration profiles and ground-level
F-7

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concentration maps are printed at r,egular time intervals. 1'le have
found that an interval of 20 minutes petween printouts gives a good
indication of hourly trends and does not result in endless pages of
unused computer output. Predicted vertical concentration profiles
in the vicinity of monitoring stations are also printed out at the
option of the user.
SIMDIG
Subroutine SI~IDIG solves a system of linear equations whose co-
efficient matrix is tridiagonal. Thomas' algorithm is employed in
the solution (see von Rosenberg (1969) for details). The three bands
of the matrix and the y~own vector are transferred to the sQ~routine, and
the solution is returned upon completion.
, SOURCE
Auto:notive and fixed source emissions (\'ith the exception of pO\oler
plant emissions) are computed in subroutine SOURCE. All emissions are
treated as surface fluxes. See Appendix A for a complete discussion
of the source inventory.
UPWIND
Subroutine UPWIND computes the wind field aloft. ~~en the lower
wind field is completely defined in HETEOR, control is passed to UPWIND.
We refer the reader to Appendix C for a discussion of ,the algorithm
employed.
B.
Program Operation
In this section we discuss, in a general manner, the operation of
the program during a typical si~ulation. Since neither the model nor the
program have taken final form, a complete card-by-card description would
be lengthy and of no particular value at this juncture. Figure F-2
should be referred to throughout this discussion, as a schematic repre-
sentation of the order of the computational operations is shown
therein.
A simulation commences in ~~IN with the input of all information
contained on punched cards, with the exception of the initial concentra-
tion distribution, which is input later. The program then reads the
aircraft emissions tape until it encounters data applicable at the time
the simulation is to start. At this point the program calculates all
the'parameters that will be used in the numerical integration of the
governing airshed equations. For example, partial derivatives of the
terrain elevation
ah and ah
ax ay
 F-8 

-------
where h.(x,y) = terrain elevation at
x,y
are approximated by finite differences. After all necessary parameters
are calculated, subroutine METEOR is called to position the meteorolog-
ical data tape. As before, this is accomplished by reading the tape
until data applicable at th~ start of the simulation is encountered.
Control then passes to subroutine ICCONC where the initial conce~tra-
tion field is established. Finally, subroutine SOURCE is ~ntered, and
the automotive and fixed source emissions distributions are initialized
for future use. . Model initialization is now complete, and PRINTl is called to
print the initial concentration distribution.
The HAIN program now enters the "computational loop," in which the
governing partial differential equations are integrated numerically.
Each pass through this loop results in advancing the simulaticn time by
the value of one time step (1 to 5 minu~es). ;Before a forward step in
time can be made, however, photochemical, met~orological, and source
.variables must be updated. First, chemical reaction rate constants are
calculated. (See Section VI-A in Appendix B for a discussion of the
temporal variation of the photolysis rate constants.) Next, subroutine
METEOR is called to update the meteorological variables. If the current-
ly stored data are applicable at the time of the caJ.l, then control
immediately returns to ~~IN. Recall that the meteorological variables
are held constant for a period of one hour. If the data are no longer
current, then the meteorological data tap~ is read, and new values of
the meteorological variables are calculated. Upon return.from lI,ETEOR,
subroutine SOURCE is entered, and new values of the automotive and fixed
source emissions are computed. If the aircraft emissions rates stored in
the temporary disc area are no longer applicable, then the next set of
emissions is transferred from the tape to the disc area. This completes
the definition of the photochemical,. meteorological, and source variables.
We are now ready to proceed with the numerical integration of the govern-
ing air shed equations.
The numerical integration takes place in three sequential steps. In
step I we move from column to column solving the p-direction convection-
diffusion equation. The procedure followed in the solution of one
column of points (or nodes) will be described. Power plant and aircraft
emissions into the column are established first. The turbulent eddy
diffusivity at each point in the column is then calculated in DIFCOF.
Since Step I involves the iterative solution of implicit difference.
equations, the computation primarily involves solving systems of linear
equations of the form
Ax == Y
where A
x
y
= tridiagonal matrix
= solution vector
= kno\.m vector
F-9

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tie thus compute A and y, and then call SIMDIC: . which returns x. Each
component of the solution vector represents th9' concentration' at one
point in the colunm. ~nen the .iteration has converged at a given
column, we repeat the calculation for the n~xt column. Step I is
complete when these computations have been carried out for all
columns. .
Before Step II can be initiated, subroutine BCCONC must be
called to provide pollutant concentration levels at points of
horizontal inflow on east and west boundaries. upon return from
BCCONC, Step II proceeds as described in Appendix D. When Step II
is complete, BCCONCis again called,'Dut this time to supply con-
centration levels for the north and sou~h boundaries. The compu-
tation of Step III then follows. . At th~ conq~.usion of Step III,
the numerical integration. procedure is compldted for a single t~e
step. ..'
Subroutine AVCONC is now entered, and the hourly-averaged ground-
level .concentration array is incremented by the' ne\'l ground-level
concentrations. If an hour has elapsed, then the array is divided
by the number of time steps taken over that hour. AVCONC then pro-
ceeds to print an average concentration map for each chemical species.
Instantaneous ground-level concentration maps and
vertical concentration profiles are printed at regular
(say, every 20 minutes). The,program checks to see if
be called to perform the output task.
user-selected
time intervals
PlUNTl should
We have no,'! made one .complete pass through the "coIi\putational
loop." If the simulation is to be continued, then control passes to
the beginning of the "loop," and the process described above is
repeated. When the simulation is terminated, the entire concentra- .
t~.on field .is punched onto cards~ This enables the user to re-start
a simulation at some later time.
F-lO

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FIGURE F-2.
Calculate
Operating
Parameters
i
f.1ETEOR
FLOW DIAGRAM OF THE ATMOSPHERIC
POLLUTION SIMULATION PRQGRN1
PRINTl
Calculate
Reaction
.Rate
Constants
0--
'-'''''~ .
F-ll
t40ve to
Next
Column.
., OC>I"'.
. Input
Aircraft
Emissions
(Tape)
Output
Air9raft
. 'Emissions
. (Disc)

-------
.~
Set Up
Linear
Systems
SnmIG
No
No
F-12
Step II -
Integrate
in t-Dir.
Step III -
Integrate
in T\-Dir.
No
No
e

-------
Stop
'"
Start
AVCONC
Increment
Ave. Conc.
Array
Yes
.
Compute
Average
Cone.
Output
Ave.
Cone.
Start
BCCONC

1 .
procflss
Inflow
Cone.
Return
MAIN
Start
DIFCOF

l-


calCUlatle
Vertical
Diffusivity.
'Return
F-13

-------
Return
!-IAIN
Reter." )
MAIN. .
-~--
\.F-14
r;:-k. : Yes

.~_.
(0--
"j-----------~

I Cubic I
: Spline I
: Procedure:
I Fol1m~s :
L - -.- - _. - - - - - -
Move to
Next
Colu:,\n
Calculate
Coefficient
Matrix &
Kno.,rn
Vector
SHIDIG
Assign
Cone. to
New Grid.


-~

-------
&
0--
Calculate
Wind
Components
in Lm'ler
t'lind Field
Calculate.
Vertical
t1ind .
Component
PLUME
F-15
start
PLUME
--- ...--
Advance
to Next
Power PUn t
Calculate
Amount
& Spatial
Dist. of
Emissions
No
Return
r-~ETEOR
S,tart
PRINTl

-------
.C?
Output
vertical
Profiles
~-
Return
HAIN
Compute
Temporal
Distributions
of Autos
star;'
SIMDI0
>J.I
Conpute
Auto
Emissions
1
Compute
Fixed
Source
Emissions
Solve
System of
Linear
Equations
Return
I4AIN
( R:urn)
F-16

-------
./
Sf~
Advance
to Next
Cell .
Calculate
Air Inputs
to Cell
L
'if .
calCUlate]
Air Outlet
Velocities
from Cell
Return
UETEOR
(
F-17
no

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II.
THE AIRCRAFT EMISSIONS PROGRAM
. The Atrnospheric Pollution Simulation Program, described in Section
II reads aircraft emissions from a magnetic tape created by the Aircraft
Emissions. Program. The a.ircraft emissions model .consists of two major
p~rtsi ground operations and airborne operations. Emissions from these
operations are treated as lumped volume sources, generated in the cell
into which they are injected. We refer the reader to Section II of
Appendix A for a discussion of the gove~ning model.
.. The Aircraft
subroutine AIRI.
flight and ground
ferred from MAIN.
Emissions Program consists of a MAIN program and a ,
Subroutine AIRl calculates emissions for both the
operation modes from aircraft and airport data trans-
Input to the program:consists ofl
.
terrain elevations
emissions rates tabulated accord~ngto aircraft class,
opr.rating,mode,and chemical species
the time spent by each class of aircraft in each
operating mode
individ~al airport data, including location of the
airport on the grid and ground and flight operation
characteristics
meteorological data, such as inversion base elevations
.
.
.
The program uses this information to calculate aircraft emissions into
those cells in which airplanes operate. The output of the program, i.e.,
the pollutant emissions rates'into each cell of the airshed, is recorded
on the aircraft emissions tape for use by the Atmospheric Pollution
Simulation Program. .
Program operation starts in MAIN with the input of the first four
items listed in the preceding paragraph, all of which are contained on
p~nched cards. (See the schematic flow chart in Figure F-3.) We then
begin the calculation of the aircraft emissions ~or each hour or, for
that matter, for any other time interval of the simulated day. The
emissions into each cell are stored in a large a.rray, which must be
initialized to zero. The inversion base elevations are obtained from
the meteorological data tape, and cell heights are calculated from
(inversion base elevation - terrain elevation)/lO, where 10 is equal to
the number of horizontal strata. We now calculate the emissions from
each airport ,due to both ground and flight operations. Pertinent infor-
mation about each mode of operation (e.g., take-off, taxi, landing, etc.)
is transferred to AI~l, and the source array is incremented appropriately.
After the emissions from each airport have been computed, the time of day
and the source values are written on the magnetic tape. If fur tiler cal-
culations are to be made, then the source array is again initialized,
and the above sequence takes place for another time interval.
F-IS

-------
/
It should be noted that this program can also function as a
subroutine in the Atmospheric Pollution Simulation Program. We have
operated the aircraft program separately to minimize the storage
requirements for the Atmospheric Pollution Sinrolation Program. In
future program developmentI efforts, we will investigate further the.
question of integrating the Aircraft Emissions Program with the main
simulation program.
F-19

-------
FIGURE
F-3.
Start
l-IAIN
\!I.
Input
Airport
Data
Initialize
Source
Array to
ro
THE AIRCRAFT EMISSIONS PROGRM1
o
F-20
(0
Calculate
Cell
Heights
1B
Advan~e
to Next
Airport .
l
AJ:RL -
Landing
Mode
o

-------
(0
!

AIRl
~~~'p;Jt -.
Time
(Tape)

J
Output
Emissions
(Tape)
)
eSTOP
Ito Q

~v
~
V
~.NO
~~--
F-21
(
Start
AIRl
)
Yes
calc~late J .
Approach/
Take-off
Emissions
Ret urn
MAIN
G
Calculate
Ground
Ope ra ti ons
Emissions
Return
MAIN

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. REFERENCES
von Rosenberg, D. U.., "Methods for the Numerical Solution of Partial
Differential Equations, II American .Elsevier Publishing' Company,
NeW York (1969).' . . .
J
F-22
. .
"

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