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group_secar2.0 [2018/09/11 16:40]
wagner
group_secar2.0 [2018/09/11 16:50]
wagner
Line 1: Line 1:
 ====== Group SECAR2.0 ====== ====== Group SECAR2.0 ======
  
--by Alex, Nadeesha and Louis-+-- by Alex, Nadeesha and Louis --
  
 ===== DAY1===== ===== DAY1=====
Line 64: Line 64:
  
 {{ :plot.png?400 |}} {{ :plot.png?400 |}}
 +
 +Fit result for parabola X<sub>max</sub><sup>2</sup> = σ<sub>11</sub> = a·K<sup>2</sup> - 2ab·K + ab<sup>2</sup> + c is:\\
  
 a = 0.000362572706 \\ a = 0.000362572706 \\
 b = 0.0834414129893 \\ b = 0.0834414129893 \\
 c = 3.506973286e-07\\ c = 3.506973286e-07\\
 +
 The consistency check for beam size calculation in Q7 shows: X_calculated = 3.13mm, X_cosy_read_out = 3.16mm at the Q7 exit.\\ The consistency check for beam size calculation in Q7 shows: X_calculated = 3.13mm, X_cosy_read_out = 3.16mm at the Q7 exit.\\
-Emittance = 3.045387898578198e-07  π m rad= 0.3 π mm mrad.\\+Emittance calculated from fit parameter  = 3.045387898578198e-07  π m rad= 0.3 π mm mrad.\\
 Start beam emittance= XX * AX= 0.2 π mm mrad, so the emittance grows from the start to the focal point.\\ Start beam emittance= XX * AX= 0.2 π mm mrad, so the emittance grows from the start to the focal point.\\
 This rmittance grow is possibly due to the optics aberrations. Input COSY file does a 4th-order-calculation. Also the measured points don't fit the parabola ideally, i.e. the optics is non-linear.\\ This rmittance grow is possibly due to the optics aberrations. Input COSY file does a 4th-order-calculation. Also the measured points don't fit the parabola ideally, i.e. the optics is non-linear.\\
  
  
/srv/thewikis/JIOSS/data/pages/group_secar2.0.txt · Last modified: 2018/09/13 16:49 by plastun