/[PAMELA software]/gpamela/gpspe/gpdspe.F
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revision 3.3 by pam-ba, Mon Dec 5 12:15:21 2005 UTC revision 3.7 by bottai, Tue Feb 7 11:38:52 2006 UTC
# Line 1  Line 1 
1  *  *
2  * $Id: gpdspe.F,v 3.2 2005/07/25 11:53:21 cafagna Exp $  * $Id: gpdspe.F,v 3.6 2006/02/06 14:17:21 bottai Exp $
3  *  *
4  * $Log: gpdspe.F,v $  * $Log: gpdspe.F,v $
5    * Revision 3.6  2006/02/06 14:17:21  bottai
6    *  adapt again the resolution simulation to the ITRPB volume identification
7    *
8    * Revision 3.5  2006/01/24 13:52:01  bottai
9    * prepare to store the x and y multiplicity of the hit
10    *
11    * Revision 3.4  2006/01/18 09:41:33  bottai
12    *  Some correction to the spe plane ID due to the new geometry tree
13    *
14    * Revision 3.3  2005/12/05 12:15:21  pam-ba
15    * new spectrometer geometry and internal magnetic field
16    *
17  * Revision 3.2  2005/07/25 11:53:21  cafagna  * Revision 3.2  2005/07/25 11:53:21  cafagna
18  * Several updates. See history for details  * Several updates. See history for details
19  *  *
# Line 16  Line 28 
28  *CMZ :  1.00/02 27/03/96  18.35.42  by  Francesco Cafagna  *CMZ :  1.00/02 27/03/96  18.35.42  by  Francesco Cafagna
29  *-- Author :    Francesco Cafagna   23/02/96  *-- Author :    Francesco Cafagna   23/02/96
30        SUBROUTINE GPDSPE        SUBROUTINE GPDSPE
31  ************************************************************************  *************************************************************************
32  *                                                                      *  *                                                                       *
33  * To perform SPE digitization                                          *  * To perform SPE digitization                                           *
34  *                                                                      *  *                                                                       *
35  * Called by: GUDIGI                                                    *  * Called by: GUDIGI                                                     *
36  * Author: Francesco Cafagna, 23/02/96 12.50.38                         *  * Author: Francesco Cafagna, 23/02/96 12.50.38                          *
37  *                                                                      *  *                                                                       *
38  ************************************************************************  *************************************************************************
39  #include "gcunit.inc"  #include "gcunit.inc"
40  #include "gpphit.inc"  #include "gpphit.inc"
41        PARAMETER (RADDEG=57.295779)        PARAMETER (RADDEG=57.295779)
# Line 161  C       Line 173  C      
173    
174           CALL GPRSPE(ANGLEX,ANGLEY,BMAGNET,XMULT,YMULT,DXPOS,DYPOS)           CALL GPRSPE(ANGLEX,ANGLEY,BMAGNET,XMULT,YMULT,DXPOS,DYPOS)
175    
176             NXMULT(I)=INT(XMULT)
177             NYMULT(I)=INT(YMULT)
178    
179           XAVSPE(I) = XAVSPE(I) + DXPOS           XAVSPE(I) = XAVSPE(I) + DXPOS
180           YAVSPE(I) = YAVSPE(I) + DYPOS           YAVSPE(I) = YAVSPE(I) + DYPOS
181    
182  C  C
183  C ADD RESOLUTION OF THE SHIFT INDUCED BY THE MAG. FIELD  C ADD THE SHIFT INDUCED BY THE MAG. FIELD
184  C  C
185    
186           IF(ITRPB(I).LT.6) THEN           IF(ITRPB(I).LT.6) THEN
# Line 176  C Line 191  C
191    
192        ENDDO        ENDDO
193  *  *
194  * Loop on the hits retrived to fill the CWN common and the DIGI bank  * Loop on the hits retrived to fill the CWN common and the DIGI b
195  *  *
196  C fc       IF (HF) NTHSPE = NHITS  C fc       IF (HF) NTHSPE = NHITS
197  C fc       DO I=1,NHITS  C fc       DO I=1,NHITS
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