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group_secar2.0 [2018/09/11 16:52]
wagner
group_secar2.0 [2018/09/11 17:14]
wagner
Line 48: Line 48:
 === Quadrupole strenght variations for emittance measurment === === Quadrupole strenght variations for emittance measurment ===
  
-|B<sub>Q7</sub> [T] |X<sub>max</sub>[m] |ap [m] |Bρ* [Tm] |L<sub>Q7</sub> [m] |K| +|B<sub>Q7</sub> [T] |X<sub>max</sub>[m] |ap [m] |Bρ* [Tm] |L [m] |K| 
-|0.02 |2.91E-03 |0.13 |0.8 |0.34 |0.065384615| +|0.02 |2.91E-03 |0.13 |0.8 |6.085 |0.065384615| 
-|0.01 |2.27E-03 |0.13 |0.8 |0.34 |0.032692308| +|0.01 |2.27E-03 |0.13 |0.8 |6.085 |0.032692308| 
-|0 |1.62E-03 |0.13 |0.8 |0.34 |0| +|0 |1.62E-03 |0.13 |0.8 |6.085 |0| 
-|-0.01 |1.20E-03 |0.13 |0.8 |0.34 |-0.032692308| +|-0.01 |1.20E-03 |0.13 |0.8 |6.085 |-0.032692308| 
-|-0.02 |9.08E-04 |0.13 |0.8 |0.34 |-0.065384615| +|-0.02 |9.08E-04 |0.13 |0.8 |6.085 |-0.065384615| 
-|-0.03 |6.23E-04 |0.13 |0.8 |0.34 |-0.098076923| +|-0.03 |6.23E-04 |0.13 |0.8 |6.085 |-0.098076923| 
-|-0.04 |9.54E-04 |0.13 |0.8 |0.34 |-0.130769231| +|-0.04 |9.54E-04 |0.13 |0.8 |6.085 |-0.130769231| 
-|-0.05 |1.60E-03 |0.13 |0.8 |0.34 |-0.163461538| +|-0.05 |1.60E-03 |0.13 |0.8 |6.085 |-0.163461538| 
-|-0.06 |2.26E-03 |0.13 |0.8 |0.34 |-0.196153846|\\+|-0.06 |2.26E-03 |0.13 |0.8 |6.085 |-0.196153846|\\
  
 *Bρ the magnetic rigidity was extracted from COSY by comand CONS(CHIM)\\ *Bρ the magnetic rigidity was extracted from COSY by comand CONS(CHIM)\\
Line 73: Line 73:
 The consistency check for beam size calculation in Q7 shows:\\ The consistency check for beam size calculation in Q7 shows:\\
 X_calculated = 3.13mm, X_cosy_read_out = 3.16mm at the Q7 exit.\\ X_calculated = 3.13mm, X_cosy_read_out = 3.16mm at the Q7 exit.\\
-Emittance calculated from fit parameter  3.045387898578198e-07  π m rad0.3 π mm mrad.\\ +Emittance calculated from fit parameters ε<sqrt>ac</sqrt> / L<sup>2</sup> 37 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 by 3 orders 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 emittance 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