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group_secar2.0 [2018/09/11 13:44] plastun |
group_secar2.0 [2018/09/11 16:20] wagner |
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- | Group SECAR2.0 | + | ====== |
- | Reaction: < | + | -by Alex, Nadeesha and Louis- |
+ | |||
+ | ===== DAY1===== | ||
+ | ==== Getting started ===== | ||
+ | |||
+ | Choosen example reaction: < | ||
+ | ⇒important for < | ||
Beam: < | Beam: < | ||
{{ : | {{ : | ||
- | Matrix:\\ | + | ====Understanding COSY Matrix |
+ | Command: OV 1 1 0 ; {order 1, phase space dim 1 INCLUDING ENERGY, # of parameters 0}\\ | ||
+ | Output:\\ | ||
|1.0|0.0|0.0|0.0|-0.41| | |1.0|0.0|0.0|0.0|-0.41| | ||
|2.2|1.0|0.0|0.0|-0.35|\\ | |2.2|1.0|0.0|0.0|-0.35|\\ | ||
+ | Explaination: | ||
+ | |R< | ||
+ | |R< | ||
R< | R< | ||
R< | R< | ||
Line 28: | Line 39: | ||
{{ : | {{ : | ||
+ | **DAY2**\\ | ||
**Emittance measurement**\\ | **Emittance measurement**\\ | ||
+ | Distance between Q7 center and focal plane is 6.085 m. | ||
+ | {{ : | ||
+ | |||
+ | **Q7 strenght variation: | ||
+ | |B [T] |Xmax[m] |ap [m] |Brho* [Tm] |L [m] |K| | ||
+ | |0.02 |2.91E-03 |0.13 |0.8 |0.34 |0.065384615| | ||
+ | |0.01 |2.27E-03 |0.13 |0.8 |0.34 |0.032692308| | ||
+ | |0 |1.62E-03 |0.13 |0.8 |0.34 |0| | ||
+ | |-0.01 |1.20E-03 |0.13 |0.8 |0.34 |-0.032692308| | ||
+ | |-0.02 |9.08E-04 |0.13 |0.8 |0.34 |-0.065384615| | ||
+ | |-0.03 |6.23E-04 |0.13 |0.8 |0.34 |-0.098076923| | ||
+ | |-0.04 |9.54E-04 |0.13 |0.8 |0.34 |-0.130769231| | ||
+ | |-0.05 |1.60E-03 |0.13 |0.8 |0.34 |-0.163461538| | ||
+ | |-0.06 |2.26E-03 |0.13 |0.8 |0.34 |-0.196153846|\\ | ||
+ | |||
+ | *Brho the magnetic rigidity was extracted from COSY by comand CONS(CHIM)\\ | ||
+ | |||
+ | **Fit of the data to parabola** | ||
+ | {{ : | ||
+ | |||
+ | a = 0.000362572706 \\ | ||
+ | b = 0.0834414129893 \\ | ||
+ | c = 3.506973286e-07\\ | ||
+ | Double check for beam size calculation in Q7: X_calculated = 3.13mm, X_cosy_read_out = 3.16mm at the Q7 exit.\\ | ||
+ | Emittance = 3.045387898578198e-07 | ||
+ | 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. optics is non-linear.\\ | ||
+ | |||