Re: FLUKA error in Ubuntu

Dear Ariel,

I have tested your source routine and it seems fine.
Please understand that it is difficult to help you when we are not able
to reproduce the crash on our own computers.
If you don't want to send your input to test your problem on Ubuntu then
try to answer the following questions:
Did you ever run successfully a FLUKA simulation on your machine?
Did you you observe any messages related to the crash in the *err, *out
and log file?
How many particles where simulated before the crash occurred?
Was a core file produced?
Does the same simulation run without the source routine?
Are you sure you are creating the executable correctly? If I understand
correctly you are overwriting the default source.f in the usermvax
directory. If you have done similar things already in the past it can be
  that you are linking modified user routines to your executable.
Do you have other FLUKA installations on your machine and the FLUPRO
variable is not set to the right one?
Do you have a problem with DOS like line endings?
Are you sure you don't have tabs in your source.f file? The file you
send arrived as quote in the mail and not as attachment so I cannot
check this.

Cheers, Florian

Ariel Shnitzer wrote:
> OK, in response to the replies, I am posting my source file. I wouldn't
> understand however, how it would run on my associate's computer but not
> on mine. To check, I had her email me the source file and input file,
> and it still gave me the same error. Thanks for looking,
> Ariel
>
>
> *$ 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
>
> *
>
> SAVE LFIRST
>
> DATA LFIRST / .TRUE. /
>
>
>
> PARAMETER (COEFC = 1.230E+12)
>
> PARAMETER (COEFK = 2.115E+00)
>
> PARAMETER (ALPHA = 0.2815E+00)
>
> PARAMETER (IBNUM = 999) ! number of energy bins
>
>
>
> DIMENSION ENERGY(0:IBNUM) ! Initial Energy Of Each Bin
>
> DIMENSION SPECTR(0:IBNUM) ! differential fluence function
>
> DIMENSION CUMUL(0:IBNUM) ! Cumulative function
>
> *======================================================================*
>
> * *
>
> * BASIC VERSION *
>
> * *
>
> *======================================================================*
>
> NOMORE = 0
>
> * +-------------------------------------------------------------------*
>
> * | First call initializations:
>
> IF ( LFIRST ) THEN
>
> * | *** The following 3 cards are mandatory ***
>
> TKESUM = ZERZER
>
> LFIRST = .FALSE.
>
> LUSSRC = .TRUE.
>
> * | *** User initialization ***
>
> WRITE(*,*)
>
> WRITE(*,*) "source foror Al slab/ monodirectional beam"
>
> WRITE(*,*) "Version 1 called"
>
> WRITE(*,*)
>
>
>
>
>
> DO I = 0, IBNUM
>
> ! WRITE(*,*) I
>
> ENERGY(I) = 1.0E-3 + 1.0E-3 * I
>
> ! WRITE(*,*) I, ENERGY(I)
>
> SPECTR(I) = COEFC * COEFK * ALPHA *
>
> & EXP(-COEFK * (ENERGY(I) ** ALPHA))*
>
> & ENERGY(I) ** (ALPHA - 1.D0)
>
> WRITE(*,*) I, ENERGY(I), SPECTR(I)
>
> END DO
>
>
>
> ! WRITE(*,*) "enegry, spectr initialized"
>
> CUMUL(0) = ZERZER
>
>
>
> * calculate the cumulative function
>
>
>
> DO I = 1, IBNUM
>
> CUMUL(I) = CUMUL(I-1) + HLFHLF * (SPECTR(I) + SPECTR(I-1))
>
> & * (ENERGY(I) - ENERGY(I-1))
>
> WRITE(*,*) I, ENERGY(I), CUMUL(I)
>
> END DO
>
> ! WRITE(*,*) "cumulative function initialized", CUMUL(IBNUM)
>
> * normalize the cumulative function to 1
>
>
>
> SUM = CUMUL(IBNUM)
>
> DO I = 1, IBNUM
>
> CUMUL(I) = CUMUL(I)/SUM
>
> WRITE(*,*) I, ENERGY(I), CUMUL(I)
>
> END DO
>
>
>
> ! WRITE(*,*) "cumulative function norm", CUMUL(IBNUM)
>
>
>
> END IF
>
>
>
> * IJBEAM = 1
>
>
>
> * |
>
> * +-------------------------------------------------------------------*
>
> * 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) = ONEONE
>
> 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.
>
> 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) = SQRT ( PBEAM**2 + AM (IONID)**2 ) - AM (IONID)
>
> !
>
> ! Sampling from the distribution
>
> !
>
> XI = FLRNDM(DUMMY)
>
> WRITE(*,*) " XI", XI
>
> DO 111 I = 0, IBNUM - 1
>
> IF ( XI .LT. CUMUL(I+1) ) THEN
>
> * come here when cumul(i) =< xi < cumul(i+1). Interpolate
>
> write(*,*) ENERGY(I), ENERGY(I+1)
>
> SAMPLE = ENERGY(I) + (ENERGY(I+1) - ENERGY(I))
>
> & * (XI - CUMUL(I)) / (CUMUL(I+1) - CUMUL(I))
>
> WRITE(*, *) "Sample", SAMPLE
>
> GO TO 222
>
> END IF
>
> 111 CONTINUE
>
> 222 CONTINUE
>
> TKEFLK (NPFLKA) = SAMPLE
>
>
>
> !
>
> !
>
> * Particle momentum
>
> * PMOFLK (NPFLKA) = PBEAM
>
> !
>
> PMOFLK (NPFLKA) = SQRT ( TKEFLK (NPFLKA) * ( TKEFLK (NPFLKA)
>
> & + TWOTWO * AM (IONID) ) )
>
> WRITE(*, *) " momentum", PMOFLK (NPFLKA)
>
> !
>
> * Cosines (tx,ty,tz)
>
> ! TXFLK (NPFLKA) = UBEAM
>
> ! TYFLK (NPFLKA) = VBEAM
>
> ! TZFLK (NPFLKA) = WBEAM
>
>
>
> TXFLK (NPFLKA) = 0.D0
>
> TYFLK (NPFLKA) = 0.D0
>
> TZFLK (NPFLKA) = SQRT ( ONEONE - TXFLK (NPFLKA)**2
>
> & - TYFLK (NPFLKA)**2 )
>
> WRITE(*, *) " cos z", TZFLK (NPFLKA)
>
> !
>
> * Polarization cosines:
>
> TXPOL (NPFLKA) = -TWOTWO
>
> TYPOL (NPFLKA) = +ZERZER
>
> TZPOL (NPFLKA) = +ZERZER
>
> * Particle coordinates
>
> ! XFLK (NPFLKA) = XBEAM
>
> ! YFLK (NPFLKA) = YBEAM
>
> ! ZFLK (NPFLKA) = ZBEAM
>
>
>
> XFLK (NPFLKA) = -40.D0 + 80.D0 * FLRNDM(DUMMY)
>
> YFLK (NPFLKA) = -40.D0 + 80.D0 * FLRNDM(DUMMY)
>
> ZFLK (NPFLKA) = -10.D0
>
> WRITE(*, *) " cordinates",XFLK(NPFLKA),YFLK(NPFLKA),ZFLK (NPFLKA)
>
> WRITE(*, *) "***************************************************"
>
> * 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
>
> WRITE(*, *) " total kinetic energy", TKESUM
>
> 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
>
> * WRITE(*, *) " just before exiting tracker"
>
> RETURN
>
> *=== End of subroutine Source =========================================*
>
> END
>
>

-- 
###########################################
Florian Sommerer
European Organization for Nuclear Research
CERN AB-ATB-EET
Mailbox Z04500
Geneve 23
CH-1211 Switzerland
Tel : +41 2276 75582
Fax : +41 2276 77555
###########################################