Dear Haoyu,
Sender: owner-fluka-discuss_at_mi.infn.it
You can find in attach an example...
LINE 64, I write in a test file:
WRITE(LUNOUT,*)
CALL OAUXFI('testgek.dat',LUNRDB,'OLD',IERR)
OPEN(UNIT=3D89,FILE=3D"testsource.dat",STATUS=3D"UNKNOWN")
WRITE(LUNOUT,*)
DO I =3D 1, NLINES
READ(LUNRDB,*) ENRGY(I), XCOO(I), YCOO(I), ZCOO(I),
& UU(I), VV(I), WW(I), WEIGH(I)
*=09 ENRGY(I)=3DENRGY(I)
END DO
KOUNT =3D 0
END IF
Regards
Julien (CELIA FRANCE)
----- Mail original -----
De: "Haoyu Shi" <shihy_at_ihep.ac.cn>
=C3=80: "fluka-discuss" <fluka-discuss_at_fluka.org>
Envoy=C3=A9: Vendredi 24 Janvier 2020 20:03:04
Objet: [fluka-discuss]: How to output the source info?
Dear FLUKA Experts,
Sender: owner-fluka-discuss_at_mi.infn.it
I'm trying to study with external source file. The source file contains=20
the x,y,z,cosx,cosy and energy. Since I always get strange results, I=20
want to let the program output the source information, to whether the=20
LUNOUT or user-defined file.
For example, I read =E2=80=9CX,COSX,Y,COSY,Z,DE=E2=80=9D from one file open=
ed by=20
OPEN card, and then let
TKEFLK (NPFLKA) =3D (1.0D0+DE)*10.0D0
TXFLK (NPFLKA) =3D COSX
TYFLK (NPFLKA) =3D COSY
TZFLK (NPFLKA) =3D SQRT ( ONEONE - TXFLK (NPFLKA)**2
& - TYFLK (NPFLKA)**2 )
XFLK (NPFLKA) =3D X*100.0D0
YFLK (NPFLKA) =3D Y*100.0D0
ZFLK (NPFLKA) =3D Z*100.0D0
And I just want to write all these infos to the LUNOUT or some other=20
file using same variable name(TKEFLK,TXFEK=E2=80=A6etc). I tried to add=20
=E2=80=9Cwrite=E2=80=9D command within source.f, or in USROUT routine, but =
all failed.
How could I do this? Or is there any other way to check my source input?
Thank you very much.
Best Regards,
Haoyu
__________________________________________________________________________
filename=source.f
*$ CREATE SOURCE.FOR
*COPY SOURCE
*
*=== source ===========================================================*
*
SUBROUTINE SOURCE ( NOMORE )
INCLUDE '(DBLPRC)'
INCLUDE '(DIMPAR)'
INCLUDE '(IOUNIT)'
*
*----------------------------------------------------------------------*
* *
* Copyright (C) 1990-2006 by Alfredo Ferrari & Paola Sala *
* All Rights Reserved. *
* *
* *
* New source for FLUKA9x-FLUKA200x: *
* *
* Created on 07 january 1990 by Alfredo Ferrari & Paola Sala *
* Infn - Milan *
* *
* Last change on 03-mar-06 by Alfredo Ferrari *
* *
* This is just an example of a possible user written source routine. *
* note that the beam card still has some meaning - in the scoring the *
* maximum momentum used in deciding the binning is taken from the *
* beam momentum. Other beam card parameters are obsolete. *
* *
*----------------------------------------------------------------------*
*
INCLUDE '(BEAMCM)'
INCLUDE '(FHEAVY)'
INCLUDE '(FLKSTK)'
INCLUDE '(IOIOCM)'
INCLUDE '(LTCLCM)'
INCLUDE '(PAPROP)'
INCLUDE '(SOURCM)'
INCLUDE '(SUMCOU)'
*
LOGICAL LFIRST
INTEGER IJBEAM
PARAMETER(NLINES = 33000)
DIMENSION ENRGY(NLINES), XCOO(NLINES), YCOO(NLINES),
& ZCOO(NLINES), UU(NLINES), VV(NLINES), WW(NLINES),
& WEIGH(NLINES)
SAVE LFIRST, KOUNT
DATA LFIRST / .TRUE. /
*======================================================================*
* *
* BASIC VERSION *
* *
*======================================================================*
NOMORE = 0
IJBEAM=1
* +-------------------------------------------------------------------*
* | First call initializations:
IF ( LFIRST ) THEN
* | *** The following 3 cards are mandatory ***
TKESUM = ZERZER
LFIRST = .FALSE.
LUSSRC = .TRUE.
* | *** User initialization ***
WRITE(LUNOUT,*)
CALL OAUXFI('testgek.dat',LUNRDB,'OLD',IERR)
OPEN(UNIT=89,FILE="testsource.dat",STATUS="UNKNOWN")
WRITE(LUNOUT,*)
DO I = 1, NLINES
READ(LUNRDB,*) ENRGY(I), XCOO(I), YCOO(I), ZCOO(I),
& UU(I), VV(I), WW(I), WEIGH(I)
* ENRGY(I)=ENRGY(I)
END DO
KOUNT = 0
END IF
* |
* +-------------------------------------------------------------------*
KOUNT = KOUNT + 1
* Sample a line from the file
XI = FLRNDM(DUMMY)
LINE = INT(XI * DBLE(NLINES)) + 1
IF(KOUNT .LE. 100) THEN
WRITE(89,*) LINE,ENRGY(LINE),XCOO(LINE),YCOO(LINE),
& ZCOO(LINE),UU(LINE),VV(LINE),WW(LINE),WEIGH(LINE)
END IF
* Push one source particle to the stack. Note that you could as well
* push many but this way we reserve a maximum amount of space in the
* stack for the secondaries to be generated
* Npflka is the stack counter: of course any time source is called it
* must be =0
NPFLKA = NPFLKA + 1
* Wt is the weight of the particle
WTFLK (NPFLKA) = WEIGH(LINE)
WEIPRI = WEIPRI + WTFLK (NPFLKA)
* Particle type (1=proton.....). Ijbeam is the type set by the BEAM
* card
* +-------------------------------------------------------------------*
* | (Radioactive) isotope:
IF ( IJBEAM .EQ. -2 .AND. LRDBEA ) THEN
IARES = IPROA
IZRES = IPROZ
IISRES = IPROM
CALL STISBM ( IARES, IZRES, IISRES )
IJHION = IPROZ * 1000 + IPROA
IJHION = IJHION * 100 + KXHEAV
IONID = IJHION
CALL DCDION ( IONID )
CALL SETION ( IONID )
* |
* +-------------------------------------------------------------------*
* | Heavy ion:
ELSE IF ( IJBEAM .EQ. -2 ) THEN
IJHION = IPROZ * 1000 + IPROA
IJHION = IJHION * 100 + KXHEAV
IONID = IJHION
CALL DCDION ( IONID )
CALL SETION ( IONID )
ILOFLK (NPFLKA) = IJHION
* | Flag this is prompt radiation
LRADDC (NPFLKA) = .FALSE.
* |
* +-------------------------------------------------------------------*
* | Normal hadron:
ELSE
IONID = IJBEAM
ILOFLK (NPFLKA) = IJBEAM
* | Flag this is prompt radiation
LRADDC (NPFLKA) = .FALSE.
* | Group number for "low" energy neutrons, set to 0 anyway
IGROUP (NPFLKA) = 0
END IF
* |
* |
* +-------------------------------------------------------------------*
* From this point .....
* Particle generation (1 for primaries)
LOFLK (NPFLKA) = 1
* User dependent flag:
LOUSE (NPFLKA) = 0
* User dependent spare variables:
DO 100 ISPR = 1, MKBMX1
SPAREK (ISPR,NPFLKA) = ZERZER
100 CONTINUE
* User dependent spare flags:
DO 200 ISPR = 1, MKBMX2
ISPARK (ISPR,NPFLKA) = 0
200 CONTINUE
* Save the track number of the stack particle:
ISPARK (MKBMX2,NPFLKA) = NPFLKA
NPARMA = NPARMA + 1
NUMPAR (NPFLKA) = NPARMA
NEVENT (NPFLKA) = 0
DFNEAR (NPFLKA) = +ZERZER
* ... to this point: don't change anything
* Particle age (s)
AGESTK (NPFLKA) = +ZERZER
AKNSHR (NPFLKA) = -TWOTWO
* Group number for "low" energy neutrons, set to 0 anyway
IGROUP (NPFLKA) = 0
* Kinetic energy of the particle (GeV)
TKEFLK (NPFLKA) = ENRGY(LINE)
* Particle momentum
PMOFLK (NPFLKA) = SQRT ( TKEFLK (NPFLKA) * ( TKEFLK (NPFLKA)
& + TWOTWO * AM (ILOFLK(NPFLKA)) ) )
* Cosines (tx,ty,tz)
TXFLK (NPFLKA) = UU(LINE)
TYFLK (NPFLKA) = VV(LINE)
TZFLK (NPFLKA) = SQRT ( ONEONE - TXFLK (NPFLKA)**2
& - TYFLK (NPFLKA)**2 )
* Polarization cosines:
TXPOL (NPFLKA) = -TWOTWO
TYPOL (NPFLKA) = +ZERZER
TZPOL (NPFLKA) = +ZERZER
* Particle coordinates
XFLK (NPFLKA) = XCOO(LINE)
YFLK (NPFLKA) = YCOO(LINE)
ZFLK (NPFLKA) = ZCOO(LINE)
* Calculate the total kinetic energy of the primaries: don't change
IF ( ILOFLK (NPFLKA) .EQ. -2 .OR. ILOFLK (NPFLKA) .GT. 100000 )
& THEN
TKESUM = TKESUM + TKEFLK (NPFLKA) * WTFLK (NPFLKA)
ELSE IF ( ILOFLK (NPFLKA) .NE. 0 ) THEN
TKESUM = TKESUM + ( TKEFLK (NPFLKA) + AMDISC (ILOFLK(NPFLKA)) )
& * WTFLK (NPFLKA)
ELSE
TKESUM = TKESUM + TKEFLK (NPFLKA) * WTFLK (NPFLKA)
END IF
RADDLY (NPFLKA) = ZERZER
* Here we ask for the region number of the hitting point.
* NREG (NPFLKA) = ...
* The following line makes the starting region search much more
* robust if particles are starting very close to a boundary:
CALL GEOCRS ( TXFLK (NPFLKA), TYFLK (NPFLKA), TZFLK (NPFLKA) )
CALL GEOREG ( XFLK (NPFLKA), YFLK (NPFLKA), ZFLK (NPFLKA),
& NRGFLK(NPFLKA), IDISC )
* Do not change these cards:
CALL GEOHSM ( NHSPNT (NPFLKA), 1, -11, MLATTC )
NLATTC (NPFLKA) = MLATTC
CMPATH (NPFLKA) = ZERZER
CALL SOEVSV
RETURN
*=== End of subroutine Source =========================================*
END
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Received on Mon Jan 27 2020 - 12:34:37 CET