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gbeam.param.bak 3.6 KiB
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  • ;                    BPM calibration constants
    ;                    =========================
      guse_bpm_in_recon  = 0   ; if 1 use bpm information for reconstruction
      guse_bpmc = 1  ; if 1 use all 3 bpm info, if 0 use bpm A and B 
      gbpm_sample  = 500 ; number of events, which are used for average 
                         ; beam position ( <5000 ). Optimal value dep. on rate
    
    ; the names are based on Paul Gueye's 'Status of the actual Beam Position
    ;                   Monitors in the Hall C Beamline', December 1, 1995.
    ; (mkj) apr-4-03 kappa,alpha and off for 3rd bpm are guesses,
    ; need to find right values.
    ;
    ;  gbpm_kappa    = 1.85 ,1.85,1.85     ; sensitivity in cm
    gbpm_kappa    = 2.00 ,1.95,1.85  ; modified mkj 4/9/03
      gbpm_alpha_x = 1.8192,0.7330 ,0.7   ; calibration gain: we may get them from the
      gbpm_alpha_y = 1.0063,0.8935 ,0.7   ;  EPICS events, right now that's according to Paul's note
    
    ; the following offsets get added to the calculated positions
    ;  gbpm_x_off = -0.011,-0.004,0.      ; in cm: survey according to Paul's note
    ;  gbpm_y_off = +0.052,+0.056,0.
    ; From Dahlberg survey DT_C853 Apr 7, 2003
    gbpm_x_off = 0.017+.412,0.061-.353,0.037
    gbpm_y_off = 0.037+.381,-0.04-.211,0.028
    
    ; average beam positions: only used if 'guse_bpm_in_recon=0' 
    ;  gbeam_xoff  = +0.18
      gbeam_xoff  = +0.00
      gbeam_xpoff = +0.00
      gbeam_yoff  = +0.00
      gbeam_ypoff = +0.00
    
    ; spectrometers would like to see this positions (from optics studies) 
    ; we treat SOS and HMS the same, however, we may change this if necessary
    ;  gspec_xoff  = +0.18
      gspec_xoff  = +0.00
      gspec_xpoff = +0.00
      gspec_yoff  = +0.00
      gspec_ypoff = +0.00
    
    ; Pedestals for BPM ADCs: from cosmic run #10933, 10/3/96, book XI-137
      gbpm_xp_ped = 431.9,331.0,0.  ; these pedestals have to be determined
      gbpm_xm_ped = 514.7,350.6,0.  ; from runs with no beam in the cavities,
      gbpm_yp_ped = 406.9,358.8,0.  ; e.g. cosmic runs.
      gbpm_ym_ped = 499.7,292.7,0. ;
    
    ; positions of BPMs relative to target (from Paul's note)
      gbpm_zpos = 345.5,166.3,0.   ; cm
    
    
    ;             Fast Raster calibration constants
    ;             =================================
    
    ; Various fast raster quantities: gUse* are flags
    
      gusefr               = 1  ; if 1 correct for FRY in reconstruction
    
      guse_frdefault       = 1  ; if 1 do no phase correction (default)
    ;      gfr_cal_mom      = 3.245  ; = beam momnetum during calibration run 
    ;      gfrx_adcpercm    = 11328. ; = FR channels per cm deflection on target
    ;      gfry_adcpercm    = 10708. ; from run 9981, August 25, 1996, book X-22
    
          gfr_cal_mom      = 2.038  ; = beam momnetum during calibration run 
          gfrx_adcpercm    = 4364.7 ; = FR channels per cm deflection on target
          gfry_adcpercm    = 5471.9 ; from harp scan (H00A), June 19, 2004
    
    
                                ;if 0 apply phase correction 
          gfrx_dphase      = 0.0    ; phase shift (never measured for x so far) 
          gFrx_synccut     = 0.     ; should be zero if applied on centered distr.
          gfrx_adcmax      = 1000   ; ADC amplitude in channels.
          gfrx_maxsize     = 0.1    ; fast raster amplitude in centimeter.
    
          gfry_dphase      = 5.8    ; phase shift 
          gFry_synccut     = 0.     ; should be zero if applied on centered distr.
          gfry_adcmax      = 1000   ; ADC amplitude in channels.
          gfry_maxsize     = 0.1    ; fast raster amplitude in centimeter.
    
    ; The latest FR phase analysis from spring '96 showed, that there is no
    ; measurable phase shift. During early running (E91-13, E89-12) the FRY-phase
    ; was determined to be 5.8 degree.
    
    ; positions of FR magnets relative to target
      gfrx_dist  = 2111   ; cm
      gfry_dist  = 2071   ; cm