2019-03-18 amp-evolv » History » Version 3
Rogers, Chris, 18 March 2019 17:25
1 | 1 | Rogers, Chris | h1. 2019-03-18 amp-evolv |
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3 | 17:00 GMT Monday 18th March |
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5 | http://mice.iit.edu/phonebridge.html |
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6 | |||
7 | h2. Actions |
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8 | |||
9 | intro (KL) |
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10 | -0th paragraph add section headings |
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11 | -1st paragraph needs revision; check historical details |
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12 | -3rd paragraph need caveat on e+e- |
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13 | 4th paragraph need frictional cooling |
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14 | |||
15 | observables (CR) |
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16 | -introduce cooling formula; but phrased ito amplitude (FD)- -_CR to integrate with paper (CR)_- |
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17 | -remove sentence regarding 9% centile just before eq 1- |
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18 | -Add a sentence regarding "human readable" what is kNN algorithm- -_FD to check CR's understanding (FD)_- |
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19 | -Joining sentence between "observables" and "MICE"- |
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20 | |||
21 | MICE |
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22 | (CR) -contact Jason Tarrant and photo repro regarding image- _for now keep working on it amongst ourselves_ |
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23 | (FD) -upload schematic latex to overleaf- |
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24 | (FD) -Add labels to schematic; make lH2 not LiH absorber; general "look and feel" stuff- |
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25 | (CR) -remove phase space figure to MICE note; consider 2d amplitude plot instead a la Francois thesis figure 6.25- |
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28 | Results |
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29 | (CR) francois asked by email - why is mc_reco sample size not same as reco sample size (they are supposed to be same sample _it is impurity at high radius (tracks in MC fiducial but not data fiducial); is impurity properly handled by correction mechanism? Need to check; relies on migration matrix non-unitary_ |
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30 | (CR) -investigate the 17.5 mm bin issue esp at 10-140- _could check rebinning but low priority for now_ |
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31 | (CR) -investigate the scraping aperture _looks like it is MC offset_-; add a vertical line corresponding to the scraping aperture; comment in text |
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32 | (FD) fractional emittance is better than most significant bin as a table |
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33 | (FD) -need to do the efficiency correction on fractional emittance- |
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34 | (FD) -need to do the efficiency correction on density- |
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35 | (CR) -Check apertures in lH2 vs None absorber; KL claims window aperture should be mostly not there in "None"- |
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36 | (CR/FD) *DONE* Check systematic for density plot in TKU 10 mm; why is SSU CC giving such large uncertainty? |
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37 | |||
38 | h2. Notes from CM53 |
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41 | Try Nature before Nature physics |
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43 | Fig. 1 - schematic |
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44 | (CR) -Preferably plot B_{z}, or introduce an arbitrary factor of -1 after the absorber, or label as |B|- |
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45 | (CR) -Note that the sigma(x) plot comes from linear beam optics calculation- |
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47 | Fig. 2 - phase space 2d plots |
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48 | (CR) Interesting that there is a cliff in the x-py and y-px plots. Is this diffuser aperture (or some other aperture) |
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49 | (CR) If show Phase space plots, put one beam ellipse on |
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51 | Fig. 3 - amplitude pdf |
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52 | (CR) Add the amplitude pdf plot without corrections to the supplementary information |
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53 | (CR) -Plot amplitude pdf as a histogram or without horizontal errors- |
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54 | (CR) Afterwards, JHC pointed out that log(n) vs sqrt(A) is linear for Gaussian beam. It might just confuse people to plot it. |
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55 | (CR) Vertical axis label is wrong. Normalisation needs to be explained. |
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57 | Fig. 4 - pdf ratio |
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58 | (CR) -Make MC less visible in pdf ratio plot - it tends to dominate- |
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59 | (CR) Increase the MC stats (implies going to production MC, it is time) |
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61 | Fig. 5 - cdf ratio |
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62 | (CR) -The number of significant figures in the table is too great. Need to understand the difference between the errors for different data- |
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63 | (CR) -John and KL asked for raw pdf numbers- |
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64 | (CR) -Discussion of which bin to choose and how to quantify the level at which we observe cooling- |
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65 | * Soler suggested CLS method |
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66 | * -Others suggested looking at significance of first bin rather than most significant bin- |
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68 | (CR) -Move the points to the bin edge, not bin centre; look and feel issues- |
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69 | (CR) Check systematic error correlations are handled correctly |
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71 | (CR) -General - check the systematic error is reasonable; e.g. do we need to include big error for SSU and for SSD; check we only use -ve error in SSU- |
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72 | (CR) General - move to production |
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74 | h2. Other jobs |
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76 | (CR) *DONE* Check - why is the systematic error so much higher on density plot than e.g. amplitude pdf plot? |
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77 | (CR) -Add labels to schematic- |
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78 | (CR) Fix or explain kink in 10-140 plot amplitdue pdf |
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79 | (CR) Write methods section |
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80 | (CR) Update MICE Note |
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81 | (FD) Add comment noting the beam used for the Poincare plot |
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82 | (FD) Add date to the schematic |
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83 | 3 | Rogers, Chris | (ALL) stats test for table |
84 | 2 | Rogers, Chris | (CR) data to francois for poincare section |