2019-01-30-amp-evolv-paper » History » Version 4
Rogers, Chris, 08 February 2019 16:29
1 | 1 | Rogers, Chris | h1. 2019-01-30-amp-evolv-paper |
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3 | 2 | Rogers, Chris | 15:00 GMT |
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5 | 1 | Rogers, Chris | http://mice.iit.edu/phonebridge.html |
6 | 3 | Rogers, Chris | |
7 | h2. Notes |
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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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15 | observables (CR) |
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16 | introduce cooling formula; but phrased ito amplitude (FD) |
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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 |
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19 | Joining sentence between "observables" and "MICE" |
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21 | MICE |
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22 | (CR) contact Jason Tarrant and photo repro regarding image |
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23 | further KL edits |
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24 | (CR) remove phase space figure to MICE note; consider 2d amplitude plot instead a la Francois thesis figure 6.25 |
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26 | Results |
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27 | (CR) investigate the 17.5 mm bin issue esp at 10-140 |
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28 | (CR) investigate the scraping aperture; add a vertical line corresponding to the scraping aperture; comment in text |
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29 | (FD) fractional emittance is better than most significant bin as a table |
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30 | (FD) need to do the efficiency correction on density |
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31 | 4 | Rogers, Chris | (CR) Check apertures in lH2 vs None absorber; KL claims window aperture be mostly not there in "None" |
32 | 3 | Rogers, Chris | |
33 | Meet again next week - plan for Friday 15th 3 pm, KL to confirm by email |