Dear Masoumeh,
There are several ways, but all of them will require the use of a user
routine.
Probably the easiest is to use the existing scoring cards like USRTRACK,
USRBDX, USRCOLL, etc and activate the call to the routine fluscw.f with
the use of the USERWEIGht card. The FLUSCW will now be called for every
step during the simulation and for every detector. To distinguish the
scoring between the various heavy ion types, you will have to enable the
scoring by setting appropriately the LSCZER flag depending on the
contents of the IBARCH(IJ) baryon number and ICHRGE(IJ) for the charge
(from the (PAPROP) include) for each detector
A sample code for FLUSCW will be
INCLUDE (PAPROP)
* Check only for the first track length detector
IF (ISCRNG .EQ. 3 .AND. JSCRNG .EQ. 1) THEN
LSCZER = .NOT. (IBARCH(IJ) .EQ. 16 .AND. ICHRGE(IJ) .EQ. 8)
END IF
Regards
Vasilis
Alberto Fasso' wrote:
> I am forwarding your question to the Fluka discussion list.
> Please avoid sending your questions privately to me or to other
> members of the Fluka collaboration
>
> Alberto Fasso`
>
> On Sun, 20 Jul 2008, masoumeh jafari wrote:
>
>> Dear Dr.fasso
>> How can we obtain to energy distribution of secondary particle like O
>> or Be
>> (their flounce or flux) or at least their energy range? Thank for
>> answering
>> my emergency question.
>> M.Jafari
>>
>> Yours sincerely
>>
>
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