*
* $Id: gprspe.inc,v 1.5 2009-06-12 18:39:54 pam-rm2 Exp $
*
* $Log: gprspe.inc,v $
* Revision 1.5  2009-06-12 18:39:54  pam-rm2
* - Introduced user-defined names of output files and random seeds number.
* Users can do it use options of PamVMCApplication constructor:
* PamVMCApplication(const char* name,  const char *title, const char*
* filename="pamtest", Int_t seed=0).
* The Random object that I use is TRandom3 object which has astronomical
* large period (in case of default initialization 0). All random generators
* in the code use this object by calling of gRandom singleton which keeps
* it.
*
* - Corrected TOF digitization routine. No problems with TDC hits due to
* hadronic interactions anymore.
*
* - Some small changes was done to compile code under Root 5.23. +
* geant4_vmc v. 2.6 without any warnings
*
* - Some classes of PamG4RunConfiguartion was changed for geant4_vmc v.
* 2.6.Some obsolete classes was deleted as soon as developers implemented
* regions.
*
* - Navigation was changed from "geomRootToGeant4" to "geomRoot", because on
* VMC web page written that as soon as Geant4 has no option ONLY/MANY
* translation of overlapped geometry to Geant4 through VGM could be wrong.
* I'd like to stay with Root navigation:
* http://root.cern.ch/root/vmc/Geant4VMC.html. This should be default
* option.
*
* - New Tracker digitization routine written by Sergio was implemented
*
* - PamVMC again became compatible with geant4_vmc v.2.5 and ROOT 5.20.
*  The problem was that ROOT developers introduced in TVirtualMC class a new
* method SetMagField and new base class:TVirtualMagField from which
* user-defined classes shoukd be derived
*
* Revision 1.1  2009-02-19 17:46:24  nikolas
* Cleaning up before releasing
*
* Revision 3.1  2005/12/06 01:08:13  cafagna
* Adding new magnetic field routines
*
* Revision 3.1.1.1  2002/07/11 16:01:59  cafagna
* First GPAMELA release on CVS
*
*
*
* gpdspe.inc
*
*CMZ :  2.01/00 05/04/2000  14.35.17  by  Marialuigia Ambriola
*-- Author :    Sergio Bottai   30/05/05
*
* Parameters for spe hit resolution
*
      INTEGER NDHIRES,NBINANG
      PARAMETER(NDHIRES=1000,NBINANG=11)
      REAL XMULT1_2,XMULT3,XRMSHMS,VANG,WX,WY,ANGLECUT
      COMMON/RESSPE/XMULT1_2(NBINANG),XMULT3(NBINANG),XRMSHMS(NBINANG),
     + VANG(12),WX(NDHIRES,NBINANG),WY(NDHIRES,NBINANG),ANGLECUT